AAS Job Register Editorial

Job Register Fee Change

The AAS Job Register has always had a 250 word limit per job announcement. This limit encourages the brief and informative description of jobs and greatly aids job seekers by limiting announcements to a reasonable length. In the past, we worked with institutions to edit their announcements to meet this limit, but this was always an inconvenience for both the AAS and the publishing institution.

Announcements beyond the 250 word limit can now appear, but will incur a $0.25 per word surcharge. It is understood that some announcements must be longer than 250 words and this fee was set low so as not to incur an undue financial penalty on these lengthy announcements.

The Job Register announcement base rate remains at a very low rate compared to comparable services provided by other professional societies. The AAS will continue to strive to maintain a low rate for the announcement of employment opportunities, which we feel is of significant benefit to the astronomical community and continues to secure the AAS Job Register's position as the number one source for astronomical employment opportunities.

Kevin B. Marvel
Executive Officer

Publication Policy for the AAS Job Register

Deadlines for submission

Job announcements may be submitted at any time and should be submitted well before the deadline so that any errors or difficulties can be resolved efficiently.

Job announcements must be received by the 15th and paid for by the 25th of each month for publication in the subsequent issue of the Job Register.

If payment is not received, then the announcement will not run in the next month's issue, but in the subsequent month's issue. We recommend that submission and payment be made well in advance of the monthly deadline.

Examples

Submit and pay by 15 October - Announcement will appear in the November Job Register
Submit and pay by 19 October - Announcement will appear in the December Job Register
Submit by 15 October, but pay after that date but before December 1 - Announcement will appear in the December Job Register.

Rate Sheet

For rate information please see the job register submission form.

Employers must indicate how they will pay for their announcement at the time of submission.

We accept payment by:

Check, in US currency drawn on a US bank. VISA and MasterCard be sure to include expiration date.

Checks should be made payable to American Astronomical Society and sent to:

American Astronomical Society
Attention Job Register Payment
2000 Florida Ave., NW Suite 400
Washington, DC 20009-1231, USA

Phone: 202-328-2010
FAX: 202-234-2560

The AAS is a small, scientific, non-profit organization. The AAS Federal Identification number is 21-0735173.

In very rare circumstances a discount may be available for insitituions from developing countries. In all cases, a formal petition for a reduced fee must be sent by email or FAX to the Deputy Executive Officer, Dr. Kevin B. Marvel requesting a discount and justifying the request.

In no case will the discount exceed a 50% reduction in the publishing fee or will discounts be available for more than one announcement per year.

Announcement Requirements

The word count limit per listing is 250 words. For longer ads, a $0.25 per word charge will be applied.

Jobs will not be published without the following:

Indication that the vacancy is bona fide and that the position has not been promised to anyone;
for first time publication, an application closing date that falls no earlier than the last day of the month of publication; and
a check or appropriate billing information as described above.

We encourage advertisers to provide URLs to relevant web sites with their job announcements or additional information (e.g. department homepage).

We also STRONGLY encourage employers to include in the postings information about benefits offered or to link to this information. This is especially important to clarify for post-doctoral or other non-permanent positions. We also encourage applicants to inquire and obtain a clear picture of the benefits at the time any offer is proffered.

Previously published position announcements may be re-published for additional months as long as the closing date is one month or more from the initial publication date of the job. Example: A job initially published in the January issue may be republished in the February issue and have a closing date in February.

The AAS Job Register cannot require overseas employers to comply with any U.S. regulations regarding employment discrimination.

Submission

All jobs should be submitted using the Web Submission Form or, if necessary, send your advertisement by electronic mail to jobs@aas.org. If electronic mail is not available, job announcements, with payment are also accepted by US mail, and by FAX at 202-234-2560.

AAS Postdoctoral Position Policy

The AAS Council has passed (1988) and reaffirmed (2003) a resolution stating that no postdoctoral position should require a candidate response prior to February 15 of each year. This policy applies to postdoctoral positions whose recruitment cycles follow the normal academic search timeline (offers in early spring to begin summer or fall of the same year). The text of this resolution is available on the Council Resolution webpage.

Employers should take this policy into account in their recruitment process.

Frequency and Circulation

The Job Register is published monthly. On the average, 60 new jobs are announced in each issue. Since the Job Register is freely available to anyone with Internet access, circulation numbers are hard to estimate. In February 2001, over 6,000 unique IP addresses accessed the Job Register.

Job Register statistics are published on the Career webpages and in the Annual Report of the Society in the Bulletin of the American Astronomical Society.

The Job Register is published on the Web at: http://members.aas.org/JobReg/JobRegister.cfm.

Member Notification

The AAS maintains a list of members that like to be notified when a New Job Register is posted. Members may be added to the Job Register email notice list by sending a message to address@aas.org.

Recent Job Postings

Notes

Some jobs reposted from prior months may have closing dates during the current month. Readers shoud pay careful attention to the posted closing dates.
Jobs marked as new were posted this month.

No. 26658 (New)
Post-doctoral fellowship in X-ray studies of galaxies
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
Tel:
Email Submission Address: gfabbiano@cfa.harvard.edu
Email Inquiries: gfabbiano@cfa.harvard.edu

Attention: Dr. G. Fabbiano
Applications are invited for a post-doctoral opening in the High Energy Astrophysics Division of the Harvard-Smithsonian Center for Astrophysics for a recent recipient of the Ph.D. degree with expertise and interests in the study of galaxies in X-rays. The position involves analysis, interpretation, and modeling of data principally from Chandra and comparison with data at different wavelengths and with models as appropriate. The successful applicant will work with Dr. G. Fabbiano on a variety of projects, including the study of AGN-galaxy feedback using high resolution Chandra observation of AGNs, and X-ray binary populations in nearby galaxies.

Candidates must possess: a Ph.D. or equivalent in astronomy, physics, or a closely related field; experience in observational research related to XRBs, ISM, or AGN and in the analysis and modeling of data; experience with data from X-ray missions is desirable. To carry out the required research tasks successfully, candidates must have familiarity with modern computer techniques as well as demonstrated ability to communicate and work with other scientists and to prepare material for publication and presentation at meetings.

The initial appointment will be for one year, beginning as soon as possible, at an initial stipend of about $56,000, with renewal for a second and possible third year subject to satisfactory performance and funding. Interested applicants should send electronically a CV, statement of research interests, and the names of three references to gfabbiano@cfa.harvard.edu.

For further information please contact Dr. G. Fabbiano (gfabbiano@cfa.harvard.edu)

No. 26696 (New)
Assistant Research Fellow in Astronomy at East Asian ALMA Regional Center
ALMA-J PROJECT OFFICE, NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN
2-21-1
Osawa
Mitaka, Tokyo 181-8588
JAPAN
Tel:
Email Inquiries: sachiko.k.okumura@nao.ac.jp

Attention: Ken’ichi Tatematsu, ALMA-J Project Director
ALMA is a partnership of Europe, North America and East Asia in cooperation with the Republic of Chile.

Applications are invited for the position of an Assistant Research Fellow at East Asian ALMA Regional Center (EA-ARC) of ALMA-J Project Office, as an ARC scientist. The responsibilities include: Science promotion related to ALMA; User support (face-to-face, helpdesk and so on) for ALMA users; Participation in Commissioning and Science Verification at OSF (2,900m elevation) in Chile with regular trips to serve as Astronomer on Duty.

The ARC scientist spends 75 % of his/her time for the above duties, and 25 % of the time is for own scientific research. The successful candidate is expected to conduct astronomical research which areas will be directed towards use of ALMA.

Professional requirements/Qualifications: An astronomer with a PhD and much interest in millimeter and/or submillimeter observations with ALMA as well as a proven track record of scientific research. A good command of English language is essential. Fluency in Japanese will be preferable.

Duty station: Mitaka, Tokyo, Japan.

Starting date: 1 December 2010

Appointment: Full-time academic position for 5 years. (This is not a tenure-track.)

Application: CV, research experience, list of publications (separate refereed and non-refereed papers), statement of research interest, and names and contact details of two references should be sent to Dr. Ken’ichi Tatematsu, ALMA-J project Director by regular mail, by September 30, 2010 The application package should arrive on or before this date by the registered post. We cannot receive the package by e-mail.

No. 26626 (New)
Faculty Position in Astrophysics
UNIVERSITY OF PITTSBURGH
3941 O'Hara Street
100 Allen Hall
Pittsburgh, PA 15260
Tel: 412-624-6381
FAX: 412-624-9163
Email Submission Address: pasearch+cosmo@pitt.edu

Attention: Cosmo Search Committee, Dept. of Physics and Astronomy
Faculty Position in Astrophysics University of Pittsburgh Department of Physics and Astronomy

The Department of Physics and Astronomy at the University of Pittsburgh ( http://www.physicsandastronomy.pitt.edu/ ) invites applications for a new tenure-stream faculty member in astrophysics. The appointment, which is subject to budgetary approval, will be at the assistant professor level and would begin in the Fall Term of 2011 or thereafter. We are especially interested in candidates with strong physics backgrounds who will complement current research strengths in astrophysics, particularly in cosmology and extragalactic astronomy. In addition to research accomplishments and future promise, candidates must show potential for a high degree of teaching effectiveness at both the graduate and undergraduate levels.

Current faculty research interests include cosmology, galaxy evolution, quasars, supernovae, and stellar atmospheres. Faculty use theoretical, observational, and numerical techiques. The Department is a member of the Sloan Digital Sky Survey (SDSS) and Large Synoptic Survey Telescope (LSST) collaborations, and has close ties to the Pittsburgh Supercomputer Center, the Pittsburgh Computational Astrostatistics group, and the McWilliams Center for Cosmology at neighboring Carnegie Mellon University. Faculty participate in the Atacama Cosmology Telescope (ACT), Pan-STARRS, SDSS-III, and the CANDELS multiwavelength survey, among other projects.

To ensure full consideration, complete applications should be received by November 15, 2010. However, applications will be accepted until the position is filled. Applicants should email a cover letter, curriculum vitae, bibliography, statement of research interests, and brief teaching statement in PDF format to pasearch+cosmo@pitt.edu (a single, combined file is preferable). In addition, applicants should arrange for at least three letters of reference sent via email to pasearch+cosmo@pitt.edu (preferred) or else mailed to: Cosmo Search Committee, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260. The University of Pittsburgh is an Affirmative Action, Equal Opportunity Employer. Women and members of minority groups under-represented in academia are especially encouraged to apply.

No. 26633 (New)
Assistant Professor in Astronomy
DARTMOUTH COLLEGE
Dept. of Physics & Astronomy
6127 Wilder Laboratory
Hanover, NH 03755-3528
United States
Tel:
URL1: www.dartmouth.edu/~physics

Attention: Astronomy Search Committee
Tenure Track Assistant Professor in Astronomy Dartmouth College

The Department of Physics and Astronomy at Dartmouth College invites applications for an Assistant Professorship in the ?eld of astronomy to begin in July, 2011. The successful candidate will be expected to establish a vigorous research program involving undergraduate and graduate students, and to have a strong commitment to excellence in teaching. The Department of Physics and Astronomy has 17 faculty members and approximately 50 PhD students, with research interests in condensed matter physics, space physics, cosmology, and astronomy. We are seeking candidates who will enhance and complement our existing research programs and utilize the MDM and SALT observatories. Current astronomy research at Dartmouth is in the ?elds of stellar evolution, stellar populations, close binary stars, supernova, supernova remnants, galaxy populations, galaxy dynamics and astrometry. A PhD and post-doctoral experience in astronomy or astrophysics is required along with a strong record of published research.

Applicants should send a curriculum vitae, bibliography, the names and contact information of three references, and brief statements of research and teaching interests to:

Astronomy Search Committee Department of Physics and Astronomy 6127 Wilder Laboratory Dartmouth College Hanover NH 03755-3528

For full consideration, hard copy applications should arrive by November 22, 2010. Dartmouth College is committed to diversity and strongly encourages applications from women and minorities.

No. 26644 (New)
Faculty Opening in Astronomy & Astrophysics
UNIVERSITY OF UTAH, PHYSICS & ASTRONOMY
115 S 1400 E #201
Salt Lake City, UT 84112
USA
Tel: 801-581-5697
FAX: 801-581-4801
URL1: http://www.physics.utah.edu/on/Astronomy_Search.pdf
Email Submission Address: heidi@physics.utah.edu
Email Inquiries: heidi@physics.utah.edu

Attention: Heidi Frank, Administrative Officer
As part of our ongoing expansion, the Department of Physics and Astronomy at the University of Utah in Salt Lake City invites applications from outstanding candidates for a tenure-track faculty position in astronomy and astrophysics. We are particularly interested in enhancing our strength in the area of theoretical astrophysics and/or cosmology, and seek candidates whose work would benefit from the University's full institutional participation in the Sloan Digital Sky Survey III and the University's Center for High Performance Computing. The appointment may be made at the level of assistant, associate, or full professor depending upon the qualifications of the successful applicant. The expected start date is August 2011.

The successful applicant will be expected to establish an active research program involving undergraduate and Ph.D. students, to teach two courses per year, and to take an active role in furthering the University’s Astronomy and Astrophysics initiative. Current astronomy and astrophysics research in the Department includes: observational cosmology; galaxy formation, structure, and evolution; Galactic archaeology and chemodynamics; planet formation; astronomical instrumentation; theoretical gravitational dynamics; theoretical particle astrophysics; experimental cosmic ray physics; and gamma-ray astronomy.

This position offers competitive pay and benefits. Applicants should submit a letter of application, curriculum vitae, a statement of research interests, and the names of at least three professional referees who have been asked by the applicant to submit letters of recommendation or appraisal directly to the search committee. Early applications are encouraged as completed applications will be reviewed and interviews scheduled on a rolling basis. First priority will be given to applications received before November 15, 2010.

Electronic applications may be sent to heidi@physics.utah.edu with the subject line "Astrophysics Search". Hard copy submissions can be sent to:

Astrophysics Search Committee The University of Utah Department of Physics and Astronomy 115 South 1400 East #201 Salt Lake City, UT 84112-0830

URLs of interest: http://www.physics.utah.edu/on/jobs.html http://www.utah.edu/ http://www.sdss3.org/

The University of Utah is fully committed to affirmative action and to its policies of nondiscrimination and equal opportunity in all programs, activities, and employment. Employment decisions are made without regard to race, color, national origin, sex, age, status as a person with a disability, religion, sexual orientation, gender identity or expression, and status as a protected veteran. The University seeks to provide equal access for people with disabilities. Reasonable prior notice is needed to arrange accommodations. Evidence of practices not consistent with these policies should be reported to: Director, Office of Equal Opportunity and Affirmative Action, (801) 581-8365 (V/TDD).

The University of Utah values candidates who have experience working in settings with students from diverse backgrounds, and possess a [strong or demonstrated] commitment to improving access to higher education for historically underrepresented students.

No. 26646 (New)
Facility Centre Astronomer
ESO - EUROPEAN ORGANISATION FOR ASTRONOMICAL RESEARCH IN THE SOUTHERN HEMISPHERE
Karl-Schwarzschild-Str. 2
Garching near Munich, Bavaria 85748
Germany
Tel: +49 89 3200 6865
FAX: +49 89 3200 6497
URL1: https://jobs.eso.org/ESOCP370/default.asp?PageNo=DEFAULT
URL2: http://www.eso.org/public/
Email Submission Address: vacancy@eso.org
Email Inquiries: vacancy@eso.org

Attention: Human Resources, Human Resources
Applications are invited for a Facility Centre Astronomer in the Data Management & Operations Division at the ESO Headquarters in Garching (Munich), Germany.

ESO is part of a coordinated effort in collaboration with other partners in Europe known as Euro-VO (Virtual Observatory).

The Euro-VO Facility Centre hosted at ESO, provides the Euro-VO with a centralized organization for resources, standard, and certification mechanisms. It also provides community support for scientific programs using VO tools and resources, with a strong focus on the exploitation of the resources in the ESO Science Archive.

Within the VO Project Office, you will be the main contact point of the Euro-VO Facility Centre and will interact with the astronomical community on a variety of VO related tasks, participating in the strategic development of the ESO science archive. A detail of the main tasks is available on the vacancy posted on the ESO web.

As an astronomer and member of the ESO Science Faculty you will be expected to conduct astronomical research directed towards the effective exploitation of the ESO Science Archive and VO tools and participate actively in the scientific life of ESO.

Further information about VO activities are on the ESO web.

The position requires a PhD in Astronomy, Physics or equivalent.

You should have at least 3 years of experience of research in astronomy and should be familiar with the use of large astronomical databases, archival data, and VO software and tools. Experience with a broad range of instrumental, data analysis, and observational techniques will be an important asset. A strong record of multi-wavelength astronomical research is highly desirable.

No. 26660 (New)
Professor of Astronomy
CORNELL UNIVERSITY
Dept. of Astronomy
610 Space Sciences Building
Ithaca, NY 14853
USA
Tel: 607-255-6920
FAX: 607-255-6918
Email Submission Address: sjf5@cornell.edu
Email Inquiries: ira@astro.cornell.edu

Attention: Sharon Falletta, Admin. Assistant
Faculty Position in Astronomy, Cornell University

The Cornell University Astronomy Department invites applications for a tenured full professor position in Planetary Astronomy, including both solar system and extrasolar planetary astronomy. Applications at the tenured associate professor and tenure-track assistant professor level will also be considered. Cornell Astronomy faculty and research staff are involved in a wide range of research in planetary astronomy, including active participation in space missions such as MER, Cassini and StardustNExt, as well as observational and theoretical studies of exoplanets.

Applicants should send a CV, list of publications, statement of research interests, and the names of three individuals who may be contacted for references to:

Sharon Falletta 610 Space Sciences Building Cornell University Ithaca, NY 14853 EMAIL: falletta@astro.cornell.edu

Inquiries may be sent to Steven Squyres (squyres@astro.cornell.edu), chair of the search committee, or Ira Wasserman (ira@astro.cornell.edu), chair of the department.

We will begin reviewing applications November 15, 2010, anticipating a start date of approximately July 1, 2011.

Cornell University is an Equal Opportunity/Affirmative Action Employer and Educator.

No. 26668 (New)
Tenure Track Faculty Position in Astronomy
UNIVERSITY OF WYOMING
Dept 3905
1000 E. University
Laramie, WY 82071
USA
Tel: 307-766-6150
FAX: 307-766-2652
Email Submission Address: physics@uwyo.edu
Email Inquiries: physics@uwyo.edu

Attention: Faculty Search Chair
Tenure Track Faculty Position in Astronomy University of Wyoming Department of Physics and Astronomy, #3905 Laramie, WY 82071

Attention: Chair, Faculty Search Committee Email Inquiries: Mike Brotherton (mbrother@uwyo.edu)

The Department of Physics and Astronomy at the University of Wyoming is seeking highly qualified candidates for an assistant professorship in astronomy beginning the fall semester of 2011. Our research facilities include a 2.3 m optical/infrared telescope (WIRO), a 24 inch telescope (Red Buttes Observatory), and the NCAR-Wyoming Supercomputing Center. The successful candidate should demonstrate commitment to teaching and ability to develop a vigorous funded research program that involves graduate and undergraduate students. Minimum requirements: a Ph.D in physics, astronomy, or closely related subject, plus two years post-doctoral experience. For full consideration, applications should be received no later than October 15, 2010. Additional information about the Department is available at http://faraday.uwyo.edu . Applications or inquiries should be addressed to Chair, Faculty Search Committee, at the above address. Completed applications will include a vita, three letters of reference, and statements of teaching philosophy and research interests. Persons seeking admission, employment or access to programs of the University of Wyoming shall be considered without regard to race, color, religion, sex, national origin, disability, age, veteran status, sexual orientation or political belief. The University of Wyoming is committed to diversity and endorses principles of affirmative action. We acknowledge that diversity enriches and sustains our scholarship and promotes equal access to our educational mission. We seek and welcome applications from individuals of all backgrounds, experiences and perspectives.

No. 26673 (New)
Assistant Professor in Experimental Astrophysics or Observational Astronomy
UNIVERSITY OF TORONTO
Tel:
URL1: www.astro.utoronto.ca (Department of Astronomy and Astrophysics)
URL2: www.di.utoronto.ca (Dunlap Institute for Astronomy and Astrophysics)
Email Submission Address: astrochair@astro.utoronto.ca
Email Inquiries: chair@astro.utoronto.ca or director@di.utoronto.ca

Attention: Professor Howard K.C. Yee, Chair
The Dunlap Institute for Astronomy and Astrophysics (DI) and the Department of Astronomy and Astrophysics (DAA) at the University of Toronto invite applications for a tenure-stream faculty appointment at the rank of Assistant Professor to commence July 1, 2011.

The successful applicant will hold a joint appointment between the DAA and the newly founded and rapidly growing DI. The Dunlap Institute's expansion plans include a significant increase in our complement of faculty and postdoctoral fellows over the next few years. We seek candidates in experimental astrophysics or observational astronomy, and encourage applicants with experience and interest in developing innovative astronomical instrumentation and advanced observing techniques, for instance those applicable to large and very large optical, infrared, or sub-mm telescopes.

The successful applicant will have an outstanding research record and potential to lead the development of the DI, augment the present research strength of DAA, and have a demonstrated excellence in teaching and research. The DI also welcomes candidates who will advance its commitment to education and community outreach. Salary to be commensurate with qualifications and experience. DAA and DI enjoy access to national facilities including the CFHT, the Gemini Observatory, and ALMA. Canada isalso a partner in the Thirty Meter Telescope consortium. DAA is active in the BLASTpol and SPIDER balloon telescopes, the MOST and BRITE satellites, the Herschel Space Observatory, and the Planck Mission, as well as planning for the TMT. DAA and DI have strong ties with the Canadian Institute for Theoretical Astrophysics (CITA), which is hosted by the University of Toronto. The University of Toronto ( http://www.utoronto.ca ) offers the opportunity to teach, conduct research, and live in one of the most diverse cities in the world.

The University of Toronto is strongly committed to diversity within its community and especially welcomes applications from visible minority group members, women, Aboriginal persons, persons with disabilities, members of sexual minority groups, and others who may contribute to the further diversification of ideas.

All qualified candidates are encouraged to apply; however, Canadians and permanent residents will be given priority.

We encourage you to submit your application online by clicking on the link below. If you are unable to apply online please submit your application and other materials to the following address via email at astrochair@astro.utoronto.ca:

Professor H.K.C. Yee, Chair,Department of Astronomy and Astrophysics, University of Toronto,Toronto, Ontario, Canada. Applications should include a curriculum vitae and a statement of current research interests with future plans. Applicants should also ask at least three referees to send letters directly to the above departmental address via e-mail at astrochair@astro.utoronto.ca, by November 1, 2010.

Closing date for this position is November 1, 2010.

To Apply Online please click: https://utoronto.taleo.net/careersection/10050/jobdetail.ftl?lang=en&job=1000743

No. 26681 (New)
Assistant Professor
PRINCETON UNIVERSITY
Tel:
URL1: https://jobs.princeton.edu (Web submission)
URL2: http://www.princeton.edu/astro/ (Department of Astrophysical Sciences)
Email Inquiries: lipman@princeton.edu

Attention: Web submissions only: https://jobs.princeton.edu
Princeton University is searching for a tenure-track Assistant Professor in the Department of Astrophysical Sciences, to begin in September 2011. The primary selection criteria will be achievement, promise and breadth in astrophysics research, as well as the ability to teach a broad range of courses and to supervise undergraduate and graduate student research projects. While the initial focus of this search is in observational and/or instrumental astrophysics, especially in the context of the department's leadership position in astronomical surveys, outstanding candidates in all fields of astrophysics are encouraged to apply for the position.

Information on departmental resources and research programs can be found at http://www.princeton.edu/astro , or by directly contacting departmental faculty.

Applicants should apply via the web at: http://jobs.princeton.edu . The application should include curriculum vitae, bibliography, a description of past research and future plans, and contact information for three references.

Applications will be accepted until the position is filled. Review of applications will start on November 15, 2010.

Princeton University is an equal opportunity employer and complies with applicable EEO and affirmative action regulations.

No. 26683 (New)
William Band Chair of Theoretical Physics
WASHINGTON STATE UNIVERSITY
Tel:
URL1: http://www.physics.wsu.edu/ (Department of Physics and Astronomy Website)
Email Submission Address: sabreen@wsu.edu
Email Inquiries: sabreen@wsu.edu

Attention: Sabreen Dodson
William Band Chair of Theoretical Physics Washington State University Pullman, Washington

The Department of Physics and Astronomy invites applications and nominations for the endowed William Band Chair of Theoretical Physics. Research specialties within theoretical physics, including astrophysics, atomic-molecular-optical physics, condensed matter physics, materials science, and emerging fields of physics such as biophysics, will be given consideration. Preference will be given to applicants whose specialties complement and enhance current research in the department. This is a permanent, full-time position at the rank of full Professor with tenure beginning August 16, 2011. The Department of Physics and Astronomy is actively committed to diversity within our community.

The successful candidate must have an internationally recognized record of significant theoretical physics research accomplishments, a demonstrated ability of establishing and maintaining an internationally competitive research program, and a strong commitment to teaching at the graduate and undergraduate levels. Applicants must have a Ph.D. in physics or related field, with at least five years of relevant experience past the awarding of the degree, and have demonstrated a strong track record of extramural funding. Applicants located outside the US must provide a detailed strategy for obtaining funding. For additional details, please see the Notice of Vacancy at http://www.physics.wsu.edu .

Applicants should submit a letter of application, a detailed curriculum vitae including a complete list of publications, a statement of research goals, and the names and contact information of at least three references. Please also include a very brief biography of the references and their connection to the applicant.

It is preferable that application materials be submitted electronically in pdf format to sabreen@wsu.edu. For further information, please contact Sabreen Dodson, phone (509) 335-9532, FAX (509) 335-7816. Alternatively, materials can be submitted in writing to: William Band Search Committee, Department of Physics and Astronomy, Washington State University, Pullman, WA 99164-2814.

Screening of completed applications will begin January 1, 2011 EE0/AA/ADA

No. 26690 (New)
Professor in Astrophysics
NORTH-WEST UNIVERSITY
North-West University
Private Bag X6001
South Africa
Tel: +27-18-299-2409/2423
FAX: +27-18-299-2421
URL1: http://www.nrf.ac.za/projects.php?pid=33
URL2: http://www.nwu.ac.za/vacancies/index.html
Email Submission Address: adri.burger@nwu.ac.za
Email Inquiries: adri.burger@nwu.ac.za

Attention: Adri Burger, Director
The Unit for Space Physics of the Potchefstroom Campus of North-West University is inviting applications for a professorship. This is a permanent position, created to support our NRF/DST Research Chair in Astrophysics and Space Physics, Prof Okkie de Jager, and to strengthen the Astrophysics Group in general. We require a PhD in Astrophysics or a related field, and a current B rating by the NRF or an equivalent research profile (see http://www.nrf.ac.za/projects.php?pid=33 Rating categories). We also require eight years’ research experience relevant to the HESS/CTA project after PhD and the ability to provide research guidance to graduate students up to PhD level. The successful candidate must be able to function independently but also as part of a team, and be able to provide leadership. The university requires a demonstration of language proficiency in order to function optimally in the multilingual environment of the NWU. The composition of our student body in the Unit requires a good command of English. Experience in research and knowledge of the use of, and programming for, high-performance computers may serve as a recommendation.

The University subscribes to and applies the principles of the South African Employment Equity Act, and is committed to transformation. All applications will be considered. Inquiries can be addressed to the Director (adri.burger@nwu.ac.za, phone +27-18-299-2409/2423).

Information about how to apply can be found at http://www.nwu.ac.za/vacancies/index.html . The advertisement for this position will only appear on that website around 19 September.

No. 26701 (New)
Faculty Position in Astronomy
UNIVERSITY OF CALIFORNIA, BERKELEY
601 Campbell Hall
MC4311
Berkeley, CA 94720-4311
USA
Tel:

Attention: Karen Wang, Extragalactic Astronomy Search Committee
Faculty Position in Astronomy

Joint Appointment between the University of California, Berkeley, and Lawrence Berkeley National Laboratory

The Astronomy Department of the University of California, Berkeley and the Physics Division of Lawrence Berkeley National Laboratory intend to make a joint faculty appointment effective July 1, 2011. This position is targeted for Extragalactic Astronomy and Cosmology, with preference for an observer and/or instrumentalist. The search will be at a junior tenure-track level, though an appointment at a senior tenured level is possible if a candidate with outstanding breadth and record is identified.

All qualified candidates are invited to apply. Applications from minority and women candidates are especially encouraged, since the UC campus is committed to a strategic plan for equity and inclusion. A curriculum vitae, bibliography, statement of research interests, and a list of at least 6 references (names and complete addresses including email) are required for consideration. UC Berkeley’s Statement of Confidentiality can be found at: http://apo.chance.berkeley.edu/evalltr.html .

Online applications are strongly preferred. Please go to http://apptrkr.com/156398 and click on the “Faculty Job Listing” link located in the right side bar. Follow the directions for self-registration, uploading of PDF’s, and obtaining the URL for your letters of reference writers. For applicants at the assistant professor level, give this URL to at least 3 references and have them upload their letter. If online application is not possible, mail curriculum vitae, bibliography, statement of teaching and research interests, and arrange to have at least 3 references mailed to:

Attention: Karen Wang Extragalactic Astronomy Search Committee University of California, Berkeley 601 Campbell Hall MC4311 Berkeley, CA 94720-4311

For applicants who wish only to be considered at the associate or full professor level, it is sufficient to provide names and addresses in the initial application; the search committee will contact these references only after the applicant is selected for further consideration.

Applications by E-mail or FAX will not be accepted. Applications must be received by January 14, 2011, at which time interviews will begin. The University of California and the Lawrence Berkeley National Laboratory are Equal Opportunity, Affirmative Action Employers.

No. 26553
Faculty Openings for McWilliams Center for Cosmology
CARNEGIE MELLON UNIVERSITY
5000 Forbes Avenue
Dept. of Physics, WEH 6325
Pittsburgh, PA 15213
USA
Tel: 412-268-8367
FAX: 412-681-0648
Email Submission Address: donnat@andrew.cmu.edu
Email Inquiries: donnat@andrew.cmu.edu

Attention: Donna Thomas, Secretary
Faculty Openings Carnegie Mellon University McWilliams'Center for Cosmology

The Department of Physics at Carnegie Mellon University invites applications for tenure-track faculty positions at the junior or senior levels associated with the Bruce and Astrid McWilliams Center for Cosmology. The McWilliams Center, which has benefited from a major endowment gift to the university, joins efforts in particle physics and astrophysics within the Department of Physics at Carnegie Mellon. Historically, the Department has had a strong effort in particle theory and high-energy experiment. More recently, the Department has built up a theoretical and observational cosmology group, much of whose research is related to uncovering the nature of the dark part of the universe. The McWilliams' Center synergizes these efforts within Physics and capitalizes on unique collaborative opportunities both within and outside Carnegie Mellon. Powerful computing clusters have been created both within the McWilliams Center and in collaboration with the Department of Computer Science. Carnegie Mellon joined the LSST collaboration, has faculty working on BOSS in SDSS-III, and is engaged in trying to build a new type of radio telescope to explore the universe using the 21 cm radiation of neutral Hydrogen. Physical space for the McWilliams'Center has been expanded and renovated within the Department of Physics. The first two McWilliams Postdoctoral Fellows are at the Center, and the first of several new faculty members has been hired. Please visit the Center’s website at www.cmu.edu/cosmology for more details.

The research areas for the search include: theoretical astrophysics, with emphasis on computation and simulation; experimental astrophysics, with emphasis on the dark part of the universe and data mining; and theoretical particle physics as related to understanding dark matter and dark energy. We seek candidates with significant accomplishments and promise for further achievement in exploring the nature of dark matter and dark energy. Tenure-track appointments at the junior or senior level will be considered. Successful candidates are encouraged to enhance links between the Department of Physics and the School of Computer Science and the Department of Statistics at Carnegie Mellon, the Pittsburgh Supercomputing Center, and the Department of Physics and Astronomy at the University of Pittsburgh.

Candidates should submit a curriculum vitae, publication list, statement of research plans, and arrange for three letters of recommendation sent to

Cosmology Search Committee, Department of Physics, Carnegie Mellon University, 5000 Forbes Avenue, Pittsburgh, PA 15213.

For full consideration, all materials should be received by October 15, 2010.

Carnegie Mellon University is an Equal Opportunity/Affirmative Action Employer.

No. 26495
Tenure-Track Faculty Position in Astrophysics
WEST VIRGINIA UNIVERSITY
Tel:
URL1: http://www.wvu.edu (West Virginia University)
URL2: http://physics.wvu.edu (Physics Department)
URL3: http://astro.wvu.edu (Astrophysics Group)
Email Submission Address: duncan.lorimer@mail.wvu.edu
Email Inquiries: duncan.lorimer@mail.wvu.edu

Attention: Dr. Duncan Lorimer
The Department of Physics at West Virginia University invites applications for a faculty position in astrophysics. The astrophysics group at WVU consists of three professors, one post-doc, ten graduate students, and three undergraduate students. The group specializes in studies of compact objects and galaxy formation and evolution in the local universe (see the astrophysics group website for a description of our current activities) and works in close collaboration with the National Radio Astronomy Observatory, and in particular is a major user of the observatory facilities in Green Bank, WV.

Qualified candidates in any area of astronomy and astrophysics are encouraged to apply; a preference will be given to observational astronomers with postdoctoral experience and at least some experience in radio astronomy. Minimum requirements are a Ph.D. in physics, astronomy, or astrophysics; a commitment to teaching astronomy and astrophysics at both the undergraduate and graduate levels; and evidence of potential to achieve a record of excellence in research and teaching. The successful candidate is expected to obtain external funding and develop a nationally recognized research program. The WVU Physics Department consists of 18 tenured and tenure-track faculty, three research faculty, seven postdoctoral researchers, and 62 graduate students. The largest research areas are condensed matter physics, astrophysics, and plasma physics. The departmental website contains information about the course offerings in undergraduate and graduate astronomy/astrophysics.

To apply, send (1) a curriculum vitae including a full list of publications and relevant teaching experience, (2) a research plan for the next five years, and (3) a statement of teaching philosophy and experience. Please arrange for three letters of recommendation to be sent separately. E-mail applications consisting of a single file in PDF format can be sent to Duncan Lorimer at Duncan.Lorimer@mail.wvu.edu. Review of applications will begin October 1, 2010 and continue until the position is filled. West Virginia University is an affirmative action, equal opportunity employer. Applications are encouraged from women and members of historically underrepresented groups. WVU provides support for dual career couples (see http://dualcareer.wvu.edu ).

No. 26598 (New)
CITA Research Associate
CANADIAN INSTITUTE FOR THEORETICAL ASTROPHYSICS
Tel:
URL1: www.cita.utoronto.ca (check under working at CITA)

Attention: CITA
CITA is a national centre for theoretical astrophysics located at the University of Toronto. CITA expects to offer one or more Research Associate positions of three to five years duration. The start date will be September 1, 2011. Applicants should have an excellent research record in astrophysics and postdoctoral experience. Funds will be available for travel and other research expenses. The primary duty is to carry out original research in theoretical astrophysics, but Research Associates are also expected to work with postdoctoral fellows and to assist with administration of the Institute. All applicants for these positions are also considered automatically for postdoctoral fellowships.

We only accept electronic submissions. See the CITA website: http://www.cita.utoronto.ca for instructions. Applicants will be asked to submit a curriculum vitae; statement of research interests; and arrange for three letters of recommendation. Deadline for applications and all letters of recommendation is November 15, 2010.

All qualified candidates are encouraged to apply; although Canadians and permanent residents will be given priority. In accordance with its Employment Equity Policy, the University of Toronto encourages applications from qualified women and men, members of visible minorities, aboriginal peoples and persons with disabilities.

No. 26603 (New)
Director, Department of Terrestrial Magnetism
CARNEGIE INSTITUTION FOR SCIENCE
Tel:
Email Submission Address: search@carnegiescience.edu
Email Inquiries: MaryLou.Zoback@rms.com

Attention: Search Committee
Director, Department of Terrestrial Magnetism Carnegie Institution for Science

The Carnegie Institution for Science seeks a Director for the Department of Terrestrial Magnetism to lead the department in a multidisciplinary program of basic research in Earth and planetary science. Applicants should have a record of excellence in research on scientific problems in this area. The successful candidate will be expected to carry out an active scientific program and provide general scientific leadership for the staff, which currently includes groups in geochemistry and cosmochemistry, planetary and stellar astronomy, and geophysics and planetary physics.

Founded in 1902 as an organization for scientific discovery, the Carnegie Institution hosts scientists who are leaders in the fields of plant biology, developmental biology, Earth and planetary sciences, astronomy, and global ecology. Situated in a park-like setting in Washington, D.C., the Department of Terrestrial Magnetism has 15 staff scientists, 15-20 postdoctoral fellows, and a supporting technical staff. A significant portion of scientific and technical staff salaries, several postdoctoral fellows, and a major part of the research program are covered by endowment funds. Research grants make up the balance of the funding. It is collocated with the Geophysical Laboratory, which carries out independent research programs in rock and mineral physics, geochemistry, and geo- and astrobiology.

The Carnegie Institution is an Equal Opportunity Employer and encourages applications from women and minorities. Potential candidates should send a CV and letter of interest to search@carnegiescience.edu. If you have questions or would like further information, please contact the chair of the search committee, Dr. Mary Lou Zoback, at MaryLou.Zoback@rms.com.

No. 26613 (New)
Teaching & Research Support Technician
COLGATE UNIVERSITY
Hamilton, New York 13346
USA
Tel:
URL1: http://www.apply-for-job.net/c/jobclick.cfm?site=2867&job=7036185 (Apply Here)

Attention: Human Resources
Job Description: Provide technical support for the teaching and research mission of the department, reporting to the Chair of the Department of Physics and Astronomy.

Essential Functions: Support teaching laboratories and demonstrations: set up, test, and take down apparatus used in teaching laboratories and classroom demonstrations; purchase, maintain, and replace/upgrade teaching apparatus and software as needed, including the observatory; work with faculty to develop new laboratory and lecture demonstration apparatus; and maintain teaching laboratory computers that use specialized software and data collection boards. Provide technical support for student/faculty research: train students in safe and correct machine shop practice; assist in laboratory assembly and the purchase and installation of equipment; purchase research supplies and monitor their inventory, anticipating the needs of faculty (compressed gases and cryogenic fluids, chemicals, glassware, gloves); handle the delivery, storage, and distribution of gases and cryogens; maintain and effect repairs on laboratory apparatus such as vacuum systems, ovens, telescopes; troubleshoot and effect minor repairs on electronic apparatus; and maintain the department machine shop, replenishing supplies and tools as needed.

Qualifications: Bachelor's (or higher) degree in physics, astronomy, or engineering, or a combination of education and experience from which comparable skills are attained. The ideal candidate will have an avid interest or background in physics or astronomy, and a sufficient understanding of concepts at an undergraduate level to be able to design demonstrations and laboratories that will illustrate these concepts. The following skills are all highly desirable. Electronics: an understanding of basic circuitry, with the ability to design and troubleshoot simple circuits; familiarity with digital and analog devices sufficient to order components for courses, especially our electronics course. Machine shop: ability to use machine and hand tools effectively and safely, including the lathe, milling machine, drill press, soldering apparatus, welding, and common tools (hammer, saw, etc.); skills should be sufficient to construct small parts from shop drawings, and to teach safe and effective shop practice to undergraduates. Cryogenics and vacuum systems: familiarity with techniques used for laboratory research and ability to troubleshoot problems such as leak checking. Information technology: familiarity with computer systems sufficient to install new software, maintain computers having specialized software and hardware for data collection and analysis, and troubleshoot software or computer interface problems. The candidate must be self-motivated, able to prioritize and balance many ongoing projects and anticipate departmental needs, and capable of working without close supervision. Must be capable of working collegially with a diverse group of students, faculty, staff, and visitors on a daily basis.

Special Instructions to Applicants: Review of application material will begin immediately and continue until the position is filled. Colgate, an Affirmative Action and Equal Opportunity Employer, is committed to developing and sustaining a diverse faculty, student body, and staff to further the university's academic mission. Minorities are encouraged to apply.

Apply Here: http://www.apply-for-job.net/c/jobclick.cfm?site=2867&job=7036185

No. 26637 (New)
Editor, The Astrophysical Journal Letters
THE AMERICAN ASTRONOMICAL SOCIETY
2000 Florida Avenue NW, Suite 400
Washington, DC 20009-1231
Tel:
Email Submission Address: search@aas.org

Attention: Paul Vanden Bout, Chair, ApJL Search Committee
Editor, The Astrophysical Journal Letters

The American Astronomical Society is soliciting applications and nominations of candidates to become Editor of The Astrophysical Journal Letters (ApJL) following the retirement of the current Editor at the end of 2012. The ApJ Letters office receives over 1200 short papers each year and works closely with the editorial office of the Astrophysical Journal (Part I), EJPress, and IOP rapidly to process and publish the most important astronomical discoveries and ideas of our time.

The Society seeks an individual with stature and achievement in the field of astronomy and with a reputation for fairness, honesty, and consistency. The Editor will be expected to manage an office of clerical and technical staff and to be able to work with the AAS, the Editor in Chief of the ApJ, EJPress, and IOP on the management and production of the journal. Previous editorial experience is an asset, but not required. An essential requirement for rapid publication is that the Editor has the time and ability each day to process promptly articles when they are submitted.

The Editor of the ApJ Letters receives manuscripts for publication, decides on their suitability for rapid publication, assures their brevity and conciseness, assigns them to referees and tracks the refereeing process for timeliness and fairness, makes judgments on the suitability of manuscripts for publication based on the referee's reports and on the authors' revisions, and submits the accepted papers to the publisher. The Editor is also required to report on the state of the Journal at AAS Council and Publications Board meetings. While the overall operation and editorial standards of the ApJ are the responsibility of the Editor in Chief, Dr. E. Vishniac, the ApJ Letters Editor operates independently in accepting or declining Letters to the journal and in setting the requirements for style and length. Confidentiality of all reports and communications is of the highest importance.

The AAS expects to compensate the Editor at roughly a half-time level and will negotiate the level of effort for any other staff with the successful candidate. The current operating structure includes an Editor and a Deputy. A small staff at the Editor’s location provides managerial and clerical support.

Candidates for this position should submit a cover letter, curriculum vitae, explanation of previous editorial experience, if any, and bibliography, either by regular mail or email to:

Paul Vanden Bout Chair, ApJL Search Committee American Astronomical Society 2000 Florida Avenue NW, Suite 400 Washington, DC 20009-1231 USA

search@aas.org

Nominations for the position should be sent to the same address.

Selected candidates will be asked to provide evidence of institutional support for their taking on editorial responsibilities and the associated infrastructure requirements (office space, Internet connections, etc.). If information relevant to such support is known, candidates are encouraged to mention this in their cover letters. The cover letter should also include plans for running the ApJ Letters office, including requirement for support personnel and assistant editors, if desired.

In accordance with the Bylaws of the Society, the AAS Publications Board will make recommendations to the AAS Council. The final selection will be made by the Council. Applications and nominations received before December 31, 2010 will be given full consideration.

The AAS is an equal opportunity employer.

No. 26639 (New)
Research Astronomer
SOUTH AFRICAN ASTRONOMICAL OBSERVATORY
P O Box 9
Observatory
Cape Town, Western Cape 7935
South Africa
Tel: +27 21 447 0025
FAX: +27 21 447 3639
URL1: http://www.saao.ac.za (South African Astronomical Observatory)
URL2: http://www.salt.ac.za (Southern African Large Telescope)
Email Submission Address: linda@saao.ac.za
Email Inquiries: linda@saao.ac.za

Attention: Ms Linda Tobin, HR Manager
Research Astronomer

Applications are invited for a Research astronomer at the South African Astronomical Observatory (SAAO). The appointment will initially be for two years, with the possibility of tenure.

Candidates must have experience with the use of large telescopes and specific experience with the design and/or construction of optical or infrared astronomical instrumentation will be a great advantage. Candidates should have research interests that are relevant to South Africa's exploitation of SALT.

The SAAO is the National Facility for optical/IR astronomy in South Africa. Its headquarters are in Cape Town where the successful applicant will be based. Observing facilities, situated 360 km away at Sutherland, comprise six telescopes with apertures ranging from 0.5 to 1.9m, plus the 10-m class Southern African Large Telescope (SALT), currently in the final stages of commissioning. SALT is operated by SAAO on behalf of an international consortium and about 1/3 of its observing time is available to the South African research community.

The successful applicant will spend about half her/his time on research, and will also be expected to contribute to some combination of instrumentation and software development as well as to postgraduate teaching and supervision.

More details of SAAO and SALT are available through www.saao.ac.za.

Applicants must have a PhD in astrophysics or a related subject. They should submit a CV, with a statement of research and relevant background interests to: The HR Manager, Ms Linda Tobin, SAAO, P O Box 9, Observatory, 7935, South Africa, phone: +27 21 447 0025; fax: +27 21 447 3639; email: linda@saao.ac.za. Applicants should arrange for three professional referees to supply letters of recommendation by the due date of 1 October 2010. SAAO is committed to equity.

No. 26648 (New)
Data Mining Analyst
WATERFRONT INTERNATIONAL LTD
95 Wellington St West, Suite 1900
Toronto, Ontario M5J 2N7
Canada
Tel:
Email Submission Address: recruiting@wil.com

Attention: WIL Recruiter
Waterfront International is a Toronto-based financial consulting firm, specializing in developing computer based statistical trading strategies. Waterfront’s selective hiring process considers only highly talented individuals with a history of exceptional professional and academic achievement, and solid real-world experience.

Primary Responsibilities: - Perform financial market data research and analysis to identify and resolve data issues using advanced data mining techniques. - Develop proprietary data mining tools and applications. - Develop predictive models.

Requirements of the Candidate include: - PhD or Masters in mathematics, statistics or computer science specializing in data mining. - Experience with machine learning and knowledge discovery techniques. - Solid quantitative background with excellent analytical skills. - Strong working knowledge of data mining and statistics. - Must possess expert level C/C++ programming skills. - Some financial experience desired but not required. - Must be a strong self-starter and able to work well independently.

No. 26670 (New)
Observing Support Scientist Ref: LSR04_10
ISAAC NEWTON GROUP OF TELESCOPES
Alvarez de Abreu 68
S/C de la Palma, S/C de Tenerife 38700
Spain
Tel: +34 922 42 54 10
URL1: http://www.ing.iac.es/About-ING/Vacancies/vacancies1.html
Email Submission Address: recruit@ing.iac.es

Attention: Juan Martinez, Mr
The Isaac Newton Group of Telescopes (ING) invites applications for two openings in the Observing Support Scientist group. We expect to offer one long-term post, and one 1-year post to cover a maternity leave. Approval for these posts is currently in process.

ING ( http://www.ing.iac.es ) is based on the island of La Palma in the Canaries and is responsible for the operation of the 4.2-m William Herschel Telescope (WHT) and the 2.5-m Isaac Newton Telescope. The WHT is one of the largest and most-advanced optical telescopes in Europe. The telescopes are located in the Observatorio del Roque de los Muchachos (ORM), 2400 metres above sea level, and are operational every day of the year in support of astronomical research programmes. ING is funded by a partnership of agencies from the UK, Netherlands and Spain.

ING’s strategic plan for the coming decade,

http://www.ing.iac.es/About-ING/Strategy/decadal_strategy_2010_2020.html

calls for an increased focus on wide-field astronomy, and a progressive increase of the time devoted to large-scale surveys, while maintaining classical observing and the visitor instrument program. The prospects for a wider operational integration of the various telescopes at ORM will open up exciting opportunities at ING in the near future.

ING pursues a vigorous instrument-development programme. Development work currently focuses on designing a wide-field, highly-multiplexed spectrograph for WHT prime focus, in consortium with UK, Dutch and Spanish institutes, to start operating in ~2015.

In support of its operational activities, ING seeks two Observing Support Scientists.

Qualifications, knowledge and skills

Applicants must have a PhD in astronomy together with a good understanding of astronomical instrumentation, and a strong track record in research, in instrument development or in observatory operations. A good working knowledge of computer systems, in particular the Unix/Linux operating system, is essential, as is familiarity with astronomical data reduction tools (e.g. IRAF, IDL). Applicants must be able to communicate effectively in English (and in Spanish would be an advantage), be self-motivated, be good team players with effective problem-solving and inter-personal skills and be capable of working in a multi-disciplinary team.

Duties

The successful candidates will spend the majority of their time in support of ING's operational activities and they are expected to spend approximately 50% of their working hours on activities directly related to the night-time support of the telescope. The main night-time responsibilities will be service-observing, and scientific support of visiting astronomers. Support activities include preparation of instrumentation and the observing programme for the night, and ensuring the quality of data taken during the night. Work activities may include fault finding and assisting in resolving such faults. The observing support scientists will also act as a point-of-contact for external scientists.

The post holders may be given responsibility for the operation of an individual scientific instrument or for other operational activities carried out within ING’s astronomy group.

Approximately 25% of the post-holders' time will be available to pursue personal research activities in a dynamic environment of forefront research and technical developments. Applications from candidates with an interest in the planned wide-field spectrograph are especially welcome.

The work will be carried out at two locations: the telescopes at the Observatory; and the ING's sea-level base in the island's capital, Santa Cruz de la Palma. The post holder will be available for night-time support on a rostered basis. A full, current, driving licence is essential, as is the ability to work at an altitude of 2400m. The successful candidates will join ING’s astronomy group and report to the Head of Astronomy.

Contractual information Starting gross annual salary will be 41059 Euros rising to 43223 Euros after one year (Grade E). An additional 20% of salary will be paid as a bonus for night work. The salary is subject to ~ 25% Spanish income tax and social-security payments. Medical cover under the Spanish National Health Service will be available to the appointee, spouse and accompanying children. A relocation package is available.

For the long-term contract, duration is expected to be at least two years. Potential applicants may seek further information from ING’s Head of Administration (contact details below).

ING will assist those coming from abroad in registering with the Social Security and Health Service, and will offer financial support for Spanish lessons.

The terms and conditions of these appointments will be in accordance with the Convenio Colectivo, the bargaining agreement between the Science and Technology Facilities Council and ING's Staff.

Applicants from outside the EU need to be in possession of both residence and work permits, valid in Spain.

Applications To apply, please send a completed application form, available at http://www.ing.iac.es/About-ING/Vacancies/vacancies1.html by email to recruit@ing.iac.es. The closing date for applications is 30 September 2010.

Applications should be accompanied by a brief description of research interests (not more than two pages) and a list of publications. Applicants should indicate which three of their publications they consider to be the most important.

Two letters of recommendation should be sent to the email address above, from referees familiar with the candidate's work.

Information related to the terms and conditions of this post is available from the Head of ING’s Administration, Mr. Juan Martinez.

Email: juan@ing.iac.es Tel: + 34 922 425414 Fax: + 34 922 425401

ING is fully committed to equality of opportunity in the workplace.

Further information

Further information on this position is available from ING's Head of Astronomy, Dr. Chris Benn: Tel: + 34 922 425432 or email crb@ing.iac.es.

No. 26720 (New)
Director of IAU Office for Astronomy Development
INTERNATIONAL ASTRONOMICAL UNION
98bis bd Arago
Paris, Ile-de-France 75014
France
Tel: +33143258358
FAX: +33143252616
URL1: www.iau.org (Website of the International Astronomical Union)
Email Submission Address: iau@iap.fr
Email Inquiries: iau@iap.fr

Attention: Ian F Corbett, General Secretary
DIRECTOR OF IAU OFFICE FOR ASTRONOMY DEVELOPMENT

The International Astronomical Union will locate the Office for Astronomy Development (OAD) at the South African Astronomical Observatory in Cape Town. A joint venture between the IAU and the SAAO, the OAD will lead and coordinate the global development activities of the IAU in implementing the decadal strategic plan “Astronomy for the Developing World – Building from the IYA2009.”

We now seek an outstanding individual, meeting the following requirements, to provide leadership to the OAD: - An honours degree or equivalent in astronomy or a closely related field. - Proven track record in education and capacity building at an international level. - Demonstrable strategic vision and experience of change management. - Managerial experience, including people and finances. - Record of leadership and achievement, as well as a strong international reputation. Experience in fundraising will be a significant advantage.

The Director will be appointed according to normal conditions of service of NRF employees and report to the OAD Steering Committee. This is a contract position for 5 years. Interested candidates should send a cover letter and full CV, including the contact details of at least 3 references, by email to both the IAU General Secretary, Ian Corbett (iau@iap.fr), and SAAO HR Manager, Linda Tobin (linda@saao.ac.za). The selection process will begin after 30 September 2010.

For further information please consult the IAU website at www.iau.org

No. 26554 (New)
2011 Henri Poincaré Fellowship
OBSERVATOIRE DE LA CÔTE D'AZUR
Tel:
URL1: http://www.oca.eu/poincare (Henri Poincaré Fellowship webpage)
URL2: http://www.oca.eu/poincare/faq.html (Frequently Asked Questions)
URL3: http://www.oca.eu/poincare/factsheet.html (Electronic Application Factsheet)
Email Submission Address: cpoca@oca.eu
Email Inquiries: cpoca@oca.eu

Attention: Dr. Fathi Namouni
The Observatoire de la Côte d'Azur (OCA) offers a postdoctoral fellowship in various research areas related to astronomy and geophysics including: astrometry, coronography, gravitational waves, image and signal processing, observational cosmology, optical interferometry, planetary science, space geodesy, stellar astrophysics, turbulence and space plasmas, geochemistry, geochronology, marine geology, petrology, rock mechanics, seismology and tectonics. The position is for one to two years. The fellowship monthly stipend ranges from 2000 to 2400 euros. Applicants must have obtained their PhD outside the OCA. Applications are reviewed internally, before a final selection by the Henri Poincaré Committee, comprising representatives of Conseil Général des Alpes-Maritimes, Académie des Sciences, Collège de France and funding agencies. The start date is between September 1, 2011 and December 1, 2012

Applicants should fill in the electronic Application Factsheet and submit their applications electronically as a single PDF file to cpoca@oca.eu. Applications (no special format) should include a CV, a description of research work, the names and contact details of (no more than) three referees and three key publications. The overall size of the application should not exceed 10Mbytes. Reference letters may be sent electronically to Dr. Fathi Namouni (cpoca@oca.eu) or by standard mail to Dr. Fathi Namouni, Observatoire de la Côte d'Azur, BP 4229, 06304 Nice cedex 4 France. Reference letters must be received no later than two weeks after the closing date, November 15, 2010.

For further information, please see the Frequently Asked Questions webpage or contact Dr. Fathi Namouni (phone: +33492003023, fax: +33492003118, email: cpoca@oca.eu)

No. 26555 (New)
2011 Henri Poincaré Fellowship
OBSERVATOIRE DE LA CÔTE D'AZUR
Tel:
URL1: http://www.oca.eu/poincare (Henri Poincaré Fellowship webpage)
URL2: http://www.oca.eu/poincare/faq.html (Frequently Asked Questions)
URL3: http://www.oca.eu/poincare/factsheet.html (Electronic Application Factsheet)
Email Submission Address: cpoca@oca.eu
Email Inquiries: cpoca@oca.eu

Attention: Dr. Fathi Namouni
The Observatoire de la Côte d'Azur (OCA) offers a postdoctoral fellowship in various research areas related to astronomy and geophysics including: astrometry, coronography, gravitational waves, image and signal processing, observational cosmology, optical interferometry, planetary science, space geodesy, stellar astrophysics, turbulence and space plasmas, geochemistry, geochronology, marine geology, petrology, rock mechanics, seismology and tectonics. The position is for one to two years. The fellowship monthly stipend ranges from 2000 to 2400 euros. Applicants must have obtained their PhD outside the OCA. Applications are reviewed internally, before a final selection by the Henri Poincaré Committee, comprising representatives of Conseil Général des Alpes-Maritimes, Académie des Sciences, Collège de France and funding agencies. The start date is between September 1, 2011 and December 1, 2011.

For further information, please see the Frequently Asked Questions webpage or contact Dr. Fathi Namouni (phone: +33492003023, fax: +33492003118, email: cpoca@oca.eu)

No. 26557 (New)
Vaidya-Raychaudhuri Post-doctoral Positions
INTER-UNIVERSITY CENTRE FOR ASTRONOMY AND ASTROPHYSICS
Post Bag 4, Ganeshkhind,
Pune University Campus,
Pune, Maharashtra 411007
India
Tel: +91-20-25604100
FAX: +91-20-25604699
URL1: http://www.iucaa.ernet.in/Openings.html (Openings for positions at IUCAA)
URL2: http://www.iucaa.ernet.in/ (IUCAA Home Page)
Email Submission Address: snk@iucaa.ernet.in
Email Inquiries: snk@iucaa.ernet.in

Attention: Santosh Khadilkar, Mr.
Applications are invited from researchers with outstanding track record for newly constituted Vaidya-Raychaudhuri Post-doctoral Fellowships in Astronomy and Astrophysics. The duration of the fellowship is typically for 2-3 years, but is extendable up to a maximum period of five years based on performance. The fellowship will carry a remuneration of Indian Rs.40,000/- per month for the first two years and Indian Rs.45,000/- per month in the subsequent years. There will be a contingency grant of Indian Rs.1,50,000/- per year throughout the tenure. Facilities required for research are provided institutionally. A post-doctoral fellow with excellent performance will be considered for a tenured position.

Research areas at IUCAA:

* Cosmology and large scale structure * Galactic and extragalactic astronomy * General relativity * Gravitational waves * High energy astrophysics * Instrumentation for astronomy * Optical, UV, X-ray, and radio astronomy * Quantum gravity, including string theory * Solar astronomy * Virtual observatory

Facilities at IUCAA include a network of state-of-the-art computers, high performance computing clusters, high speed internet connections, mirror sites of important databases, a very well equipped instrumentation laboratory, and a library with exhaustive collection of books and periodicals.

A 2 m optical telescope, IUCAA Girawali Observatory (IGO), has been installed at a site, which is about 80 km from IUCAA campus. IUCAA is a partner in the Southern African Large Telescope (SALT), which is suited to imaging of high redshift galaxies and the spectroscopy of faint objects. Support is also available for guest observing from other international facilities.

Applicants should send a curriculum vitae, list of publications, and research plans, and arrange for three confidential reference letters to be sent independently.

All the relevant material should reach IUCAA by September 30, 2010. Candidates will be informed of the result by the end of November 2010. Successful candidates are normally expected to commence their fellowship during 2011.

No. 26576 (New)
CfA Postdoctoral Fellowship 2011
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
60 Garden Street, MS 67
Cambridge, MA 02138
USA
Tel: 617-495-7103
FAX: 617-496-7589
URL1: http://www.cfa.harvard.edu/postdoc/
Email Submission Address: postdoc@cfa.harvard.edu
Email Inquiries: postdoc@cfa.harvard.edu

Attention: Fellowship Program Coordinator
Harvard-Smithsonian Center for Astrophysics CfA Postdoctoral Fellowship 2011

The Harvard-Smithsonian Center for Astrophysics invites applications for the 2011 CfA Postdoctoral Fellowship. Intended for recent Ph.D. recipients who do not already have extensive postdoctoral experience, one or more of these appointments will be made to an outstanding researcher–or researchers–displaying significant promise in theory, observation, instrumentation, and/or laboratory experiment.

The CfA combines the resources and research facilities of the Harvard College Observatory and the Smithsonian Astrophysical Observatory under a single director. Now organized in six research divisions–Atomic and Molecular Physics; High Energy Astrophysics; Optical and Infrared Astronomy; Radio and Geoastronomy; Solar, Stellar, and Planetary Sciences; and Theoretical Astrophysics–nearly 350 Smithsonian and Harvard scientists work cooperatively in an environment that welcomes the ideas and contributions of young scientists.

The facilities include the MMT (Fred Lawrence Whipple Observatory, Arizona), Magellan (Las Campanas Observatory, Chile), and other optical and infrared telescopes; radio telescopes, especially the Submillimeter Array on Mauna Kea, Hawaii; a large Beowulf cluster and network of workstations; a number of specialized laboratories; an outstanding library; and access to data from a wide range of space missions, especially the Chandra X-ray Observatory and the Spitzer Space Telescope.

Appointments are for 2 years, with renewal for a third year likely, contingent upon satisfactory progress. The stipend for 2011–2012 will be approximately $62,500 with a research budget of $16,000. Funds are also provided for health benefits and relocation expenses. Only applicants who receive their degrees between July 1, 2010, and September 1, 2011, will be considered.

Application forms and instructions are available at http://www.cfa.harvard.edu/postdoc/ . Applications are due by October 29, 2010. Offers will be made by December 17, 2010.

The Harvard-Smithsonian Center for Astrophysics is an Equal Opportunity/Affirmative Action Employer where all qualified applicants receive consideration for employment without regard to race, creed, color, sex or national origin.

No. 26585 (New)
Izaak Walton Killam Memorial Postdoctoral Fellowship in Stellar & High Energy Astrophysics
UNIVERSITY OF ALBERTA
Tel:
URL1: http://www.postdoc.ualberta.ca/fundingfellowship/uofafellowships.htm
URL2: http://www.ualberta.ca/~ivanova1/postdoc_2010.html
Email Submission Address: nata.ivanova@ualberta.ca

Attention: Natalia Ivanova, Professor
Applications are invited for the Izaak Walton Killam Memorial Postdoctoral Fellowship to be held at the University of Alberta with starting dates in the Fall of 2011. Applicants with experience and interests in theoretical and/or observational studies of stellar and high-energy astrophysics (stellar evolution, X-ray binaries - theory and observations, compact objects) are encouraged to apply. The University of Alberta is a top ranked university in Canada and internationally. The Astrophysics group at the U of A includes 13 active faculty (including 4 in stellar high energy astrophysics), 14 postdocs and more than twenty graduate students, and has research interests in binary stars, compact objects, high energy astrophysics, gravity, cosmology, the CMB, fluid dynamics and space plasma physics. The successful applicant(s) will have access to WestGrid supercomputing facilities, and can apply for time on the Gemini telescopes, the Canada-France-Hawaii telescope, and most space-based astronomy facilities (e.g. Chandra, Hubble, XMM). The appointment would be for two years with competitive salary and travel support, likely supplemented by a supervising professor. The applicants must have completed a doctoral degree within the previous 3 years before the application submission.

Applicants are required to first contact a proposed hosting professor at the UofA to find out if he/she will be nominated: Natalia Ivanova (nata.ivanova@ualberta.ca), Craig Heinke (heinke@ualberta.ca), Gregory Sivakoff (grs8g@virginia.edu) or Sharon Morsink (morsink@ualberta.ca). For this send a CV, a publication list, and a statement of research interests -- proposed research (limited to one page) and research experience (limited to two pages) -- and arrange for 3 signed letters of recommendation to be sent only electronically (PDF) by November 1.

In case of nomination, make sure that all forms required for the fellowships ( http://www.postdoc.ualberta.ca/fundingfellowship/apply.htm ) can be filled and submitted before or on November 29, 2010.

No. 26586 (New)
Banting Fellowship in Stellar & High Energy Astrophysics
UNIVERSITY OF ALBERTA
Tel:
URL1: http://www.nserc-crsng.gc.ca/Students-Etudiants/PD-NP/Banting-Banting_eng.asp
URL2: http://www.ualberta.ca/~ivanova1/postdoc_2010.html
Email Submission Address: nata.ivanova@ualberta.ca

Attention: Natalia Ivanova, Professor
Applications are invited for the Banting Postdoctoral Fellowship to be held at the University of Alberta with starting dates in the Fall of 2011. Applicants with experience and interests in theoretical and/or observational studies of stellar and high-energy astrophysics (stellar evolution, X-ray binaries - theory and observations, compact objects) are encouraged to apply. The University of Alberta is a top ranked university in Canada and internationally. The Astrophysics group at the U of A includes 13 active faculty (including 4 in stellar high energy astrophysics), 14 postdocs and more than twenty graduate students, and has research interests in binary stars, compact objects, high energy astrophysics, gravity, cosmology, the CMB, fluid dynamics and space plasma physics. The successful applicant(s) will have access to WestGrid supercomputing facilities, and can apply for time on the Gemini telescopes, the Canada-France-Hawaii telescope, and most space-based astronomy facilities (e.g. Chandra, Hubble, XMM). The appointment(s) would be for two years with very competitive salary (fellowship is valued at 70,000CAD/year, taxable). The applicants must have completed a doctoral degree within the eligibility window of November 3rd, 2007 through December 31, 2010.

Applicants are required to first contact a proposed hosting professor at the UofA to find out if he/she will be nominated: Natalia Ivanova(nata.ivanova@ualberta.ca), Craig Heinke (heinke@ualberta.ca), Gregory Sivakoff (grs8g@virginia.edu) or Sharon Morsink (morsink@ualberta.ca). For this send a CV, a publication list, and a statement of research interests -- proposed research (limited to one page) and research experience (limited to two pages) -- and arrange for 3 signed letters of recommendation to be sent only electronically (PDF) by October 1, 2010.

No. 26594 (New)
KVN Postdoctoral Fellow and Radio Astronomer
KOREA ASTRONOMY AND SPACE SCIENCE INSTITUTE
P.O. Box 88, Yonsei University,
134 Shinchon-dong, Seodaemun-gu,
Republic of Korea
Tel: +82-2-2012-7523
FAX: +82-2-2012-7501
URL1: http://www.kasi.re.kr/english
URL2: http://kvn-web.kasi.re.kr/en/en_index.php
Email Submission Address: ktkim@kasi.re.kr
Email Inquiries: ktkim@kasi.re.kr

Attention: Kee-Tae Kim
Korean VLBI Network (KVN) is the only VLBI facility in Korea being developed by Korea Astronomy and Space Science Institute (KASI). KVN consists of three 21 m radio telescopes, which are equipped with multi-frequency band receiver systems for simultaneous VLBI observations at four (22, 43, 86, 129 GHz) different frequencies. KVN will be frequently operated in combination with Japanese and Chinese VLBI networks to form so-called East Asian VLBI network (EAVN), which is expected to be comparable to VLBA and EVN in spatial resolution, sensitivity, and imaging fidelity. The KVN telescopes are now equipped with 22/43 GHz receivers and will be with 22/43/86/129 GHz receivers in 2011.

Applications are invited for a postdoctoral position and a radio astronomer position in the KVN group at KASI. These positions are aimed chiefly at research in radio interferometry, and the successful applicants will propose and participate in science with KVN and EAVN. Applicants must have a PhD in astronomy or a related field, and experience with VLBI observations and data analysis.

The appointment is initially for one year and can be renewed based on satisfactory performance. The starting stipend of the postdoctoral position is approximately US$25,000(KRW30,000,000) with health insurance, while the stipend of the radio astronomer position is commensurate with research experience and accomplishments. These positions include expenses for publication charges, travel support, and computing. Applicants should submit a curriculum vita, a bibliography, and a statement of research interest, and should arrange for two letters of recommendation to be sent to the above address. Applications received by October 15, 2010 will receive full consideration.

No. 26597 (New)
CITA Postdoctoral Fellowship
CANADIAN INSTITUTE FOR THEORETICAL ASTROPHYSICS
Tel:
URL1: www.cita.utoronto.ca (check under working at CITA)

Attention: CITA
CITA is a national centre for theoretical astrophysics located at the University of Toronto. The Institute expects to offer several postdoctoral fellowships of two to three years. The starting date will be 1 September, 2010. Funds will be available for travel and other research expenses. A Ph.D. in any field of theoretical astrophysics is required. Fellows are expected to carry out original research in theoretical astrophysics under the general supervision of the permanent faculty whose interests include: cosmology, interstellar matter, nuclear and relativistic astrophysics, solar physics, star and planet formation, high energy astrophysics.

See the CITA web page at: http://www.cita.utoronto.ca for instructions. We only accept electronic submissions. Applicants will be asked to submit a curriculum vitae, statement of research interests, and arrange for three letters of recommendation. The deadline for applications and letters of recommendation is November 15, 2010.

No. 26599 (New)
CITA National Fellowship
VARIOUS CANADIAN UNIVERSITIES
Tel:
URL1: www.cita.utoronto.ca (check under working at CITA)

Attention: CITA
CITA is a national centre for theoretical astrophysics located at the University of Toronto. As part of its mandate to promote research throughout Canada, the Institute provides partial support for postdoctoral fellows working in theoretical astrophysics or closely related fields at Canadian universities other than the University of Toronto, through its National Fellows program.

The responsibility for identifying and nominating potential CITA National Fellows who will work at a given university lies with the faculty at that university. Only faculty at Canadian universities may submit nominations. The deadline for these nominations is November 15, 2010 for fellowships to start in September 2011.

If you are interested in applying for National fellowships at other universities in Canada, please contact any of the following faculty by e-mail or check department websites for further research and application details:

Professor Andrew Cumming, McGill University, http://www.physics.mcgill.ca ; Professor Julio Navarro, University of Victoria http://www.phys.uvic.ca ; Professor Natalia Ivanova, University of Alberta, http://www.ualberta.ca/~ivanova1/ ; Professor Shantanu Basu, University of Western Ontario, basu@uwo.ca; Dr. Robert Thacker, Saint Mary’s University, thacker@ap.stmarys.ca ; Various opportunities at the University of British Columbia, http://www.astro.ubc.ca/citafellow.html , Professor Paul Wiegert, University of Western Ontario, pwiegert@uwo.ca; Various opportunities at the University of Waterloo, http://astro.uwaterloo.ca/citafellow.html

No. 26602 (New)
Postdoctoral Position in Galactic Infrared Astronomy
MAX-PLANCK-INSTITUT FUER RADIOASTRONOMIE
Auf dem Huegel 69
Germany
Tel: +49228525297
FAX: +49228525435
URL1: http://www.mpifr-bonn.mpg.de/div/mm/
Email Submission Address: kmenten@mpifr-bonn.mpg.de
Email Inquiries: kmenten@mpifr-bonn.mpg.de

Attention: Karl M. Menten, Professor
Postdoctoral Position in Galactic Infrared Astronomy - MAX-PLANCK-INSTITUT FUER RADIOASTRONOMIE

For the major project "A Global View of Star Formation in the Milky Way (GLOSTAR)" financed by an Advanced Investigator Grant of the European Research Council (ERC), the Max Planck Institute fuer Radioastronomie (MPIfR) in Bonn, Germany, is seeking a motivated, independent, and highly qualified postdoctoral researcher with excellence in observational infrared astronomy, resolved stellar populations, stellar clusters, massive stars, and star forming regions.

The successful applicants will work with Prof. Karl M. Menten's group and international collaborators on GLOSTAR using a powerful multi-pronged approach:

1) Using VLBI observations of maser sources GLOSTAR will measure distances by trigonometric parallax to most of the dominant star forming regions in the Galaxy, which will reveal its spiral structure as well as faithfully represent the luminosity and masses of its constituents.

2) Very sensitive observations of the Galactic plane with the newly Expanded Very Large Array are planned to find masers and hyper- and ultracompact HII regions, pinpointing the very centers of the earliest star-forming activity. Furthermore, follow-up observations of pre-star cluster clumps found in the APEX ATLASGAL submillimeter dust continuum survey are foreseen in ALMA early science.

3) By performing infrared studies of giant HII regions, which host a population of infrared candidate clusters, GLOSTAR will identify the ionizing stars, derive spectro-photometric distances, and characterize the star formation of each cloud in time and space. Spectro-photometric distance methods will be calibrated with the trigonometric parallaxes.

All together, GLOSTAR aims at building a unique dataset with true legacy value for a global perspective on star formation in our Galaxy.

The selected candidate should work on the third part of the GLOSTAR project. He is expected to conduct frontline research using existing data of candidate stellar clusters from VLT, VISTA, UKIDSS, GLIMPSE, reducing and analyzing the datasets, writing papers, presenting the results at conferences. The candidate should be active in proposing further observations with ground-based and/or satellite facilities.

The MPIfR offers a vibrant research environment with a strong expertise in star formation and interferometry. It is the leading radioastronomical institute in Germany, operates the 100-m radio telescope at Effelsberg, which is a key element of the European VLBI Network, holds a 50% share of the observing time with the APEX telescope in Chile and offers access to the IRAM instruments. The applicant will have direct access to ESO telescopes, the Large Binocular Telescope, and the Calar Alto Observatory. Other facilities are accessible using the OPTICON network.

Salaries are paid at German civil service rates according to TvÃ–D 14 (gross annual pre-tax income including health insurance contributions and social security currently in the range 40.000 EUR to 50.000 EUR, depending on experience).

Applicants must have a PhD in astronomy, astrophysics, or a closely related field. Interested candidates should send application materials including curriculum vitae, list of publications, a two-page summary of relevant experience and plans, and the names of three professional referees who have been asked by the applicant to be willing to submit letters of recommendation by email to kmenten@mpifr-bonn.mpg.de. Initial review of applicants will begin on October 1st, 2010; however, applications will be accepted until the position is filled.

Max-Planck-Institut fuer Radioastronomie Prof. Karl M. Menten Auf dem HÃ¼gel 69 D-53121 Bonn Germany

E-Mail submission: kmenten@mpifr-bonn.mpg.de

The Max Planck Society is an equal opportunity employer. Applications from women, disabled people and minority groups are particularly welcome. The MPIfR supports its employees in their search for suitable child care.

No. 26604 (New)
Sagan Postdoctoral Fellowship Program
NASA EXOPLANET SCIENCE INSTITUTE/CALIFORNIA INSTITUTE OF TECHNOLOGY
Tel:
URL1: http://nexsci.caltech.edu/sagan/fellowship.shtml
Email Inquiries: saganfellowship@ipac.caltech.edu

Attention: Sagan Fellowship (Web submissions only)
The NASA Exoplanet Science Institute announces the 2011 Sagan Postdoctoral Fellowship Program and solicits applications for fellowships to begin in the fall of 2011.

The Sagan Fellowships support outstanding recent postdoctoral scientists to conduct independent research that is broadly related to the science goals of the NASA Exoplanet Exploration area. The primary goal of missions within this program is to discover and characterize planetary systems and Earth-like planets around nearby stars.

The proposed research may be theoretical, observational, or instrumental. This program is open to applicants of any nationality who have earned (or will have earned) their doctoral degrees on or after January 1, 2008, in astronomy, physics, or related disciplines. The fellowships are tenable at U.S. host institutions of the fellows' choice, subject to a maximum of one new fellow per host institution per year. The duration of the fellowship is up to three years: an initial one-year appointment and two annual renewals contingent on satisfactory performance and availability of NASA funds.

The Announcement of Opportunity, which includes detailed program policies and application instructions is available at the web site: http://nexsci.caltech.edu/sagan/fellowship.shtml Applicants must follow the instructions given in this Announcement. Applications must be submitted electronically through the above website. Inquiries about the Sagan Fellowships may be directed to saganfellowship@ipac.caltech.edu.

The deadline for both applications and letters of reference is Thursday, November 4, 2010. Offers will be made before February 1, 2011, and new appointments are expected to begin on or about September 1, 2011.

No. 26605 (New)
ESO Fellowship Programme 2010/2011
ESO - EUROPEAN ORGANISATION FOR ASTRONOMICAL RESEARCH IN THE SOUTHERN HEMISPHERE
Karl-Schwarzschild-Str. 2
Garching near Munich, Bavaria 85748
Germany
Tel: +49 89 3200 6865
FAX: +49 89 3200 6497
URL1: https://jobs.eso.org/ESOCP370/documents/DOC0000285.PDF
URL2: http://www.eso.org/sci/activities/ESOfellowship.html
Email Submission Address: vacancy@eso.org
Email Inquiries: vacancy@eso.org

Attention: Human Resources, Human Resources
The European Organisation for Astronomical Research in the Southern Hemisphere awards several postdoctoral fellowships each year. The goal of these fellowships is to offer young outstanding scientists opportunities and facilities to enhance their research programmes in close contact with the activities and staff at one of the world's foremost observatories.

In addition to pursuing independent research, all fellows have ample opportunities for scientific collaboration both in Garching and Santiago.

In Garching, the fellowships start with an initial contract of one year followed by a two-year extension (3 years total). The ESO Headquarters in Garching near Munich, Germany, is located in one of the most active research areas with among the highest concentration of astronomers in Europe. Furthermore, ESO is currently participating in the newly formed Excellence Cluster on Astrophysics with the Max Planck Institute at the Garching Campus.

In addition to the excellent scientific environment that will allow to develop their scientific skills, as part of the diverse training ESO offers, fellows are encouraged to take part for up to 25% of their time in some functional work related to instrumentation, operations support, archive/virtual observatory, VLTI, ALMA, ELT, public affairs, or science operations at the Observatory in Chile.

In Chile, the fellowships are granted for one year initially with an extension of three additional years (4 years total). During the first three years, the fellows are assigned to one of the operations groups on Paranal, ALMA or APEX. Fellows contribute to the operations at a level of 80 nights per year at the Observatory.

Apart from opportunities for scientific interactions within ESO, fellows have the opportunity to collaborate with the rapidly growing Chilean astronomical community as well as with astronomers at other international observatories located in Chile. The anticipated 2010 completion of the new ALMA building next to ESO's Santiago offices will further enhance the stimulating scientific environment available to ESO Chile fellows.

During the fourth year there is little or no functional work and several options are provided. The fellow may be hosted by a Chilean institution (and will thus have access to all telescopes in Chile via the Chilean observing time). Alternatively, she/he may choose to spend the fourth year either at ESO's Astronomy Centre in Santiago, or at the ESO Headquarters in Garching, or at any institute of astronomy/astrophysics in an ESO member state.

The programme is open to applicants who will have achieved their PhD in astronomy, physics or related discipline before 1 November, 2011. Young scientists from all astrophysical fields are welcome to apply. For all fellowships, scientific excellence is the prime selection criterion.

We offer an attractive remuneration package including a competitive salary and allowances (tax-free), comprehensive social benefits, and provide financial support for relocating families.

The closing date for applications is 15 October 2010.

Please apply by completing the web application form available at http://jobs.eso.org.

No. 26607 (New)
Numerical and Experimental Studies of Radiative Accretion Shocks on Young Stellar Objects.
COMMISSARIAT À L'ENERGIE ATOMIQUE (CEA-SACLAY)
L'Orme des Merisiers
Service d'Astrophysique, Bat. 709
France
Tel: +33 1 69 08 92 58
FAX: +33 1 69 08 65 77
URL1: http://amrel.obspm.fr/~starshock/
URL2: http://irfu.cea.fr/Sap/
Email Submission Address: chieze@cea.fr
Email Inquiries: chieze@cea.fr

Attention: Jean-Pierre Chieze
The scientific objective of this post-doctoral position is the study of the structure and evolution of radiative shocks, and the dynamical and thermal instabilities they may suffer. The aim of this project, developed in the framework of the ANR STARSHOCK (2009-2013), is to understand the dynamics and the radiative properties of accretion columns linking the circumstellar disk to the surface of Young Stellar Objects. A proper calculation of the spectral signatures of this accretion process requires an accurate modeling of the accretion column, ultimately based on 3D radiative hydrodynamical studies, and of the photometric and spectroscopic features of the strong radiative accretion shock. The postdoc will be in charge of the numerical simulations of these phenomena, using several CEA radiation hydrodynamics codes adapted to the various aspects of the problem: ASTROLABE (1D moving grid, multiphysics code) and HERACLES (2D/3D finite volume, fixed grid code). These theoretical studies will be supported by laboratory experiments using large laser facilities, currently planned on PALS (Prague) and LIL (CEA/CESTA). The experiments will serve to study the small scale structure of radiative shocks and to test the numerical codes, in particular the coupling of the radiation transport with the hydrodynamics and the ability of the radiative transfer code to reproduce the experimental spectral profiles. Accordingly, the postdoc will model the shock structures which may be obtained in such experiments, and will provide simulations for designing the experimental setups.

The postdoc will be based at Service d’Astrophysique, part of the fundamental research division of CEA/Saclay, called IRFU. Large computing resource is available, from departmental cluster to 100 Tera-flops machines at the CEA and other national computing centres. Applications will be reviewed starting October 15th 2010, until the position is filled. Previous experience with large numerical simulations and/or parallel computing would be an advantage. Please send a Curriculum Vitae, list of publications, statement of research interests and experience, and arrange for three letters of reference to be sent to Jean-Pierre Chieze.

No. 26608 (New)
Theoretical Physics or Astrophysics
CALIFORNIA INSTITUTE OF TECHNOLOGY
1200 E. California Blvd.
Pasadena, CA 91125
United States
Tel:

Attention: Theoretical Physics or Astrophysics
A number of Prize Fellowships at the Postdoctoral Scholar level in Theoretical Physics or Astrophysics will be awarded on the basis of an international competition. They are to begin in Fall 2011. The Postdoctoral Scholar appointments are for a three-year duration, carry a competitive annual stipend and/or salary combination and offer an annual research expense fund.

This Fellowship program has been established to offer scientists, typically within a few years of receipt of the Ph.D., the best possible opportunity to develop their talents. Research will be encouraged in areas in which Caltech's faculty is currently active: Astrophysics Computational Physics Condensed Matter Physics Elementary Particle Physics Gravitational Physics Mathematical Physics Nuclear Physics Quantum Information Cosmology

Please apply online at http://www.pma.caltech.edu/GSR/positionsavail.html . Electronic copies of the curriculum vitae with email address and with citizenship indicated, publications list (indicate articles which appeared in refereed journals), and statement of research interests are required. Electronic Portable Document Format (PDF) submittals are preferred. The applicant is requested to ensure that at least three letters of recommendation are submitted via the web link provided in the electronic application. Deadline for the application is DECEMBER 1, 2010. Application materials may also be sent to THEORETICAL PHYSICS AND THEORETICAL ASTROPHYSICS FELLOWSHIPS, mail code 103-33, California Institute of Technology, Pasadena, CA 91125, to arrive by DECEMBER 1, 2010.

Fellowship candidates will automatically be considered for other available postdoctoral positions in their fields of interest. Email inquiries in regards to the application process may be sent to nell@its.caltech.edu.

Caltech is an Affirmative Action/Equal Opportunity Employer Women, Minorities, Veterans and Disabled Persons are encouraged to apply

No. 26609 (New)
Experimental Physics or Astrophysics
CALIFORNIA INSTITUTE OF TECHNOLOGY
1200 E. California Blvd.
Pasadena, CA 91125
United States
Tel:

Attention: Experimental Physics or Astrophysics
The Division of Physics, Mathematics and Astronomy offers a number of Prize Fellowships at the Postdoctoral Scholar level in Experimental Physics or Astrophysics. In the case of astrophysics, only candidates whose focus is primarily instrumental (not purely observational) will be considered. These Fellowships are to begin in Fall 2011 and are for a three year duration. They carry a competitive annual stipend and/or salary combination and offer an annual research expense fund.

This fellowship program has been established to offer scientists, typically within a few years after receipt of the Ph.D., the opportunity to pursue new and innovative experimental research. It is expected that this research will require the support and use of facilities of one of the established experimental groups at Caltech.

Currently, Caltech has groups working in: Astrophysical Detector Development Atomic Physics Condensed Matter Physics Gravitational Physics High Energy Astrophysics High Energy Physics Infrared & Sub-millimeter Astronomy Low Energy Particle Physics Microwave Background Observations Neurobiology Nuclear Physics Quantum Optics Radio Astronomy Solar Physics Surface Physics Ultraviolet Astrophysics

Please apply online at http://www.pma.caltech.edu/GSR/positionsavail.html . Electronic copies of the curriculum vitae with email address and with citizenship indicated, publications list (indicate articles which appeared in refereed journals), and statement of research interests are required. Electronic Portable Document Format (PDF) submittals are preferred. The applicant is requested to ensure that at least three letters of recommendation are submitted via the web link provided in the electronic application. Deadline for the application is DECEMBER 1, 2010. Application materials may also be sent to EXPERIMENTAL PHYSICS AND EXPERIMENTAL ASTROPHYSICS FELLOWSHIPS, mail code 103-33, California Institute of Technology, Pasadena, CA 91125, to arrive by DECEMBER 1, 2010.

Caltech is an Affirmative Action/Equal Opportunity Employer Women, Minorities, Veterans and Disabled Persons are encouraged to apply

No. 26610 (New)
Observational Optical or Infrared Astronomy
CALIFORNIA INSTITUTE OF TECHNOLOGY
1200 E. California Blvd.
Pasadena, CA 91125
United States
Tel:

Attention: Observational Optical or Infrared Astronomy
The Division of Physics, Mathematics and Astronomy offers one Prize Fellowship at the Postdoctoral Scholar level in Observational Optical or Infrared Astronomy. The Fellowship will begin in Fall 2011 and is for a three-year duration. It carries a competitive annual stipend and/or salary combination and offers an annual research expense fund. This fellowship program has been established to offer scientists, typically within two years of receipt of the Ph.D., the best possible opportunity to develop their talents. Fellowship recipients will have the opportunity to propose for time on all of Caltech’s astronomical facilities, including those at Palomar Observatory and at the W. M. Keck Observatory. Applications from individuals with experience in the design and construction of astronomical instrumentation as well as observations are encouraged.

Please apply online at http://www.pma.caltech.edu/GSR/positionsavail.html . Electronic copies of the curriculum vitae with email address and with citizenship indicated, publications list (indicate articles which appeared in refereed journals), and statement of research interests are required. Electronic Portable Document Format (PDF) submittals are preferred. The applicant is requested to ensure that at least three letters of recommendation are provided or sent directly to Caltech. Deadline for the application is DECEMBER 1, 2010. Application materials may also be sent to ASTRONOMY FELLOWSHIPS, mail code 103-33, California Institute of Technology, Pasadena, CA 91125, to arrive by DECEMBER 1, 2010.

Caltech is an Affirmative Action/Equal Opportunity Employer. Women, Minorities, Veterans and Disabled Persons are encouraged to apply.

No. 26612 (New)
Illinois-Paris Fellow: Next Generation Cosmic Probes
UNIVERSITY OF ILLINOIS AT URBANA-CHAMPAIGN
Tel:
Email Inquiries: thorman@illinois.edu

Attention: Benjamin Wandelt, Professor
Illinois-Paris Fellow: Next Generation Cosmic Probes

Outstanding candidates are invited to apply to work with Professor Ben Wandelt on design, simulation and the development of data analysis methods for the next generation of CMB and 21cm missions.

The successful candidate will enjoy inventing and implementing fast algorithms; exploring novel computational solutions; creating high performance statistical methods; and developing and studying the promise of massively interferometric design concepts for a next generation CMB polarization mission as well as radio-interferometric probes of cosmological 21-cm emission and absorption signals.

The study will be of combinations of design concepts and data analysis approaches and will focus on mission feasibility; ability to control or correct astrophysical, instrument, or data analysis systematics; and hence promise for science targets such as B-modes or non-Gaussianity.

The position will benefit from unparalleled access to high-performance computing resources and expertise at the University of Illinois and NCSA; a collaborative network of instrument design, theory, and cosmological data analysis experts at UW Madison, Brown, LBNL, Richmond, APC (Paris 7), and the opportunity for extensive collaboration with Wandelt's group at the Paris Institute for Astrophysics (IAP, Paris 6).

Please complete and submit your application at: https://my.physics.illinois.edu/join/ . It must include a cover letter, curriculum vitae, list of publications, brief description of research interests, and the names, addresses, and email addresses of three references. Review of applications will begin immediately and continue until the position is filled. Please contact Linda Thorman (thorman@illinois.edu or 217.333.1590) with any questions.

Illinois is an equal opportunity/affirmative action employer.

No. 26614 (New)
Einstein Fellowship Program
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
60 Garden Street
MS #4
Cambridge, MA 02138
USA
Tel: 617-496-7576
FAX: 617-496-7577
URL1: http://cxc.harvard.edu/fellows
Email Submission Address: aprestwich@cfa.harvard.edu
Email Inquiries: aprestwich@cfa.harvard.edu

Attention: Dr. Andrea Prestwich, Scientist
Einstein Fellowship Program

On behalf of the NASA Astrophysics Division, the Chandra X-Ray Center(CXC is pleased to announce the annual competition for the Einstein Postdoctoral Fellowship Program, in cooperation with host institutions throughout the United States. The primary objective of the Program is to provide opportunities for postdoctoral research on problems that are broadly related to the scientific goals of the NASA Physics of the Cosmos program as addressed by any of the missions of this program. These include high energy astrophsics relevant to the Chandra, Fermi, XMM-Newton, International X-Ray Observatory (formerly Constellation-X) missions, cosmological investigations relevant to the Planck and JDEM missions and gravitational astrophysics relevant to the LISA mission. This program is open to applicants of any nationality who earn doctoral degrees between January 1, 2008 and September 1, 2011 in astronomy, physics, or related disciplines. The Fellowships are tenable at any U.S. institution where Physics of the Cosmos related research can be carried out. The fellowship is initially for two years, with the expectation of a third year, contingent upon performance and available funding. Subject to the availability of NASA funding, up to 10 Einstein Fellows will be appointed this year, through grants to United States institutions. The Call for proposals, which includes detailed Program policies and application instructions, is available on the World Wide Web at http://cxc.harvard.edu/fellows/ . An application includes a cover form, a research proposal, letters of reference, a curriculum vitae, and other relevant materials as detailed in the instructions. Full instructions for submitting applications through the web are contained in the Call for Proposals. The application deadline is November 4, 2010 (5:00 pm EST)Einstein Fellow appointments are expected to begin on or about 1 September 2011. Women and members of minority groups are strongly encouraged to apply.

No. 26615 (New)
NSO Postdoctoral Research Associate (Solar Physics)
NATIONAL SOLAR OBSERVATORY
P.O. Box 26732
Tucson, Arizona 85726-6732
USA
Tel: (520) 318-8116
FAX: 520-318-8494
Email Submission Address: hrnoao@noao.edu

Attention: Human Resources Office, Postdoctoral Research Associate, Job #1030
The National Solar Observatory (NSO) invites applications for a postdoctoral research associate position starting October or November 2010. The successful candidate will be engaged in analysis of data from the Synoptic Optical Long-Term Investigation of Sun (SOLIS) facility. She/he will also work under the supervision of a SOLIS staff scientist on research relevant to the SOLIS project with particular emphasis on research based on data from the SOLIS Vector Spectromagnetograph (VSM). Research topics may include the understanding of the origin, evolution, and topology of magnetic fields in solar photosphere and chromosphere, the solar activity cycle, sudden energy releases in the solar atmosphere, and the connection between solar magnetic activity and the variability in total and spectral irradiance. Applicants with strong interest in other areas of solar physics relevant to the SOLIS project also will be considered. Additional details on the SOLIS project can be found at http://solis.nso.edu/ .

A PhD degree in astrophysics, physics, or a closely related field is required. Experience with UNIX, IDL, and SolarSoft, or similar operating systems and data-handling programs, is essential. Experience with data analysis from ground-based and space-borne (e.g., Hinode) instruments is desirable. The appointment will be for an initial period of one year with one additional annual extension contingent upon funding availability. The maximum expected term of this appointment is 2 years. The position will be based at the NSO/Tucson site in Arizona.

Applications received prior to September 30, 2010 are assured full consideration; however, the position will be open until filled. To apply, please submit an electronic CV and three professional letters of reference by September 30, 2010 to hrnoao@noao.edu (In the subject line, please reference Position Title and Job #1030), or mail to:

Human Resources Office NSO & NOAO (Postdoctoral Research Associate Job #1030) P.O. Box 26732 Tucson, AZ 85726-6732

NSO and NOAO are affirmative action and equal employment opportunity employers.

NSO and NOAO actively support efforts to broaden participation in all Observatory activities. Women and candidates from underrepresented minorities are particularly encouraged to apply.

No. 26616 (New)
Euclid Visible Instrument Scientist - Research Associate
MSSL/UNIVERSITY COLLEGE LONDON
Holmbury St Mary
Dorking, Surrey RH5 6NT
UK
Tel: 01483 204100
FAX: 01483 278312
URL1: http://www.ucl.ac.uk/hr/jobs/ (link to apply for position on UCL jobs page)
URL2: http://mssl.ucl.ac.uk (information about MSSL/UCL)
Email Submission Address: office@mssl.ucl.ac.uk
Email Inquiries: office@mssl.ucl.ac.uk

Attention: Julia Wehrle, Admin Assistant
Euclid Visible Instrument Scientist - Research Associate Mullard Space Science Laboratory/UCL

Grade 7 Hours Full Time Salary £28,983 - £35,646 per annum

Duties and Responsibilities

Applications are invited for the post of instrument scientist for the visible instrument (VIS) on Euclid, ESA’s candidate Dark Energy mission, in which the Mullard Space Science Laboratory/UCL has a significant involvement. The successful applicant will provide scientific expertise, carry out performance modelling and develop calibration strategies. The role will require close collaboration with the instrument team and wider science teams involved in the Euclid project, as well as the other members of the Astrophysics Group at MSSL/UCL. The applicant will also be encouraged to pursue a programme of research in the area of galactic formation and evolution.

The post is initially funded for 1 year, with the probability of further continuation should Euclid be approved.

Key Requirements

The post-holders will be expected to have a PhD in astronomy, space science or instrumentation and a working knowledge of one or more of the following: IDL, Java, Perl, C, Fortran 77/90/95, shell scripts, object-oriented concepts.

Further Details

To apply for this position (Job Ref 1150503) please go to the UCL Jobs Pages at http://www.ucl.ac.uk/hr/jobs/ Further information about MSSL can be found at http://www.mssl.ucl.ac.uk .

UCL Taking Action for Equality

Closing Date

30 Sep 2010

This appointment is subject to UCL Terms and Conditions of Service for Research and Support Staff. Please go to http://www.ucl.ac.uk/hr/salary_scales/Support_Research_tcs.php to view the terms and conditions.

No. 26617 (New)
Postdoctoral fellowship in theoretical and numerical stellar dynamics
WEIZMANN INSTITUTE OF SCIENCE
Dept of Particle Physics & Astrophysics
POB 26
Israel
Tel: +972-(0)8-9344483
FAX: +972-(0)8-9344172
URL1: http://www.weizmann.ac.il/weizsites/tal (Tal Alexander's homepage)
URL2: http://www.fgs.org.il/en/article.php?id=10 (Weizmann's postdoctoral fellowship program)
URL3: http://www.fgs.org.il/en/index.php (Weizmann's Feinberg Graduate School)
Email Submission Address: tal.alexander@weizmann.ac.il
Email Inquiries: tal.alexander@weizmann.ac.il

Attention: Prof Tal Alexander
A 2 year postdoctoral fellowship in theoretical and numerical astrophysics is available for working with Prof. Tal Alexander on fundamental dynamical processes near massive black holes in galactic nuclei, including, but not limited to processes related to sources of gravitational waves and/or those involving post-Newtonian dynamics. This position is supported by a large ERC grant, which also funded a recent acquisition of a fast large high performance computer cluster for simulations. The position's starting date is flexible, although an early start is preferable; an extension may be possible upon successful completion.

A strong background in stellar dynamics, stellar physics and computational physics is an advantage. Specific research projects are available. Time will be available for independent research. Research and teaching at the Weizmann institute are conducted in English. A significant fraction of the students and postdocs are from overseas.

Applications should arrive by January 15th 2011, and include a CV, a list of publications, a brief summary of current research, and 3 letters of recommendation (to be sent in directly). It may be sent by e-mail (preferred), fax, or regular mail. Email inquiries are welcome. There are no restrictions on citizenship. Candidates must hold a PhD in astronomy or physics by the date of appointment and be no more than 3 years after the award of the PhD.

No. 26618 (New)
Theoretical Cosmology International Chair Postdoc
INSTITUT D'ASTROPHYSIQUE DE PARIS
98 bis boulevard Arago
Paris, IDF 75014
France
Tel: +33 1 4432 8052
FAX: +331 44 32 8001
Email Submission Address: helliot@iap.fr
Email Inquiries: wandelt@iap.fr

Attention: Renata Helliot, Project Assistant
Theoretical Cosmology International Chair Postdoc- Paris Institute for Astrophysics (IAP)

Outstanding young scientists with a recent PhD are invited to apply to work with Prof. Ben Wandelt and his group at IAP, on topics of mutual interest in theoretical cosmology.

Selection will be principally based on past research accomplishments, the merits of the proposed research and the potential for productive collaboration.

The IAP is an internationally renowned center for theoretical, computational, and observational cosmology located in the heart of Paris. It is a major center for the analysis and scientific interpretation of cosmological data sets, including Planck. The successful candidate will have access to an outstanding research environment, unparalleled computing infrastructure and will be encouraged to pursue both independent and collaborative research projects.

Please apply by e-mail (subject: "Chair Postdoc") to Mme Renata Helliot (helliot"at"iap.fr) and arrange to have three letters of recommendation sent to the same address. The application should include a cover letter, curriculum vitae, a list of publications, and statements of past research accomplishments and proposed research (no more than 2 pages each). Review of applications will begin immediately and continue until the position is filled.

No. 26619 (New)
SALT Postdoctoral Fellowships
SOUTH AFRICAN ASTRONOMICAL OBSERVATORY
P O Box 9
Observatory
Cape Town, Western Cape 7935
South Africa
Tel: +27 21 447 0025
FAX: +27 21 447 3639
URL1: http://www.saao.ac.za (South African Astronomical Observatory)
URL2: http://www.salt.ac.za (Southern African Large Telescope)
Email Submission Address: linda@saao.ac.za
Email Inquiries: linda@saao.ac.za

Attention: Ms Linda Tobin, HR Manager
The South African Astronomical Observatory (SAAO, www.saao.ac.za) invites applications for positions as SALT Postdoctoral Fellows to support the commissioning and transition to full science operations of the Southern African Large Telescope (SALT; www.salt.ac.za). SALT is a 10-m optical telescope near Sutherland, some 380 km inland from the SAAO headquarters in Cape Town. The SAAO – South Africa’s national facility for optical/IR astronomy – operates SALT on behalf of 13 international partner institutions of the SALT Foundation. SALT Fellows will be part of the SALT Astronomy Operations team, currently consisting of 12 people.

Applicants should have recently completed a PhD, or expect to do so during 2010, in optical or IR observational astronomy. In addition applicants should have some experience in astronomical data reduction and ideally have experience in using or developing software for this purpose. SALT Fellows will be based at the SAAO headquarters in Cape Town and are expected to devote 50% of their time in supporting SALT and related SAAO activities, which could include interacting with research students, while the remaining time will be available for research. SALT support activities could include assisting in the commissioning of SALT and its instruments and software development. The latter may involve developing Java and web-based software tools for users and/or the Python/PyRAF-based data reduction pipeline software. Additionally, SALT Fellows will be expected to assist in updating information on the web for SALT users.

The position will initially be for a period of two years, with the possibility of an extension. The salary package will be commensurate with qualifications and experience. There are two positions to be filled as soon as possible.

Applicants should contact the SAAO HR Manager, Linda Tobin (linda@saao.ac.za) for further particulars and details on how to apply. Applications and three letters of reference (email is acceptable) must be received no later than 30 September 2010.

No. 26622 (New)
Post Doctoral Research
UNIVERSITY OF TEXAS AT ARLINGTON
502 Yates Street, 108 Science Hall
Box 19059
Arlington, TX 76019
USA
Tel: 817-272-0994
FAX: 817-372-3637
Email Submission Address: s.park@uta.edu
Email Inquiries: s.park@uta.edu

Attention: Sangwook Park, Assistant Professor
The Department of Physics of the University of Texas at Arlington has openings for postdoctoral research positions. The appointees will participate in our research programs on supernova remnants and pulsar wind nebulae utilizing data obtained with X-ray space telescopes on board Chandra, XMM-Newton, and Suzaku.

Our current research programs include three Chandra Large Projects for the detailed studies of supernova nucleosynthesis and dynamics in SNRs G299.2-2.9, 0049-73.6, and G292.0+1.8, and a Suzaku Key Project for the nucleosynthesis study of Kepler's SNR. The appointees will work primarily on these big projects, and will also be involoved in a number of SNR projects including a systematic study of the SNRs in the Large Magellanic Cloud.

A Ph.D. in Physics, Astronomy, or a related field is required. Expertise in X-ray data analysis and/or theoretical of supernova remnants/pulsar wind nebulae are preferred. The astronomy group of University of Texas at Arlington has major research efforts on supernova remnants utilizing observations with Chandra, XMM-Newton and Suzaku as well as theoretical studies of stellar activity and dark energy/dark matter. University of Texas at Arlington is a Carnegie I university with more than 28,000 students.

Its location in the heart of the Dallas-Fort Worth (DFW) metropolitan area provides excellent opportunities for collaboration with high-technology industries and neighboring universities, and the cultural benefits of the DFW Metroplex. The University of Texas at Arlington Department of Physics has 23 tenured and tenure track faculty members whose research activities include experimental and theoretical condensed matter physics, experimental high energy physics, theoretical/observational astrophysics, and space physics - see http://www.uta.edu/physics/ . The department also manages a state-of-the art planetarium - see http://www.uta.edu/planetarium/ .

The salary is commensurate with experience and competitive with other institutions. These appointments are initially for one year with the possibility of renewal contingent upon satisfactory progress and funding. These positions are immediately available. Interested candidates should send a cover letter, CV, list of publications, and a research statement (three pages or less) to Dr. Sangwook Park, to email address s.park@uta.edu or mail to University of Texas at Arlington, Department of Physics, Box 19059, Arlington, TX 76019. The applicant should also arrange for three letters of reference to be directly sent to the same address.

Review of the applications will begin immediately and will continue until the positions are filled. Further information can be obtained via email from Dr. Sangwook at s.park@uta.edu. The Universtiy of Texas at Arlington is an Equal Employment Opportunity and Affirmative Action Employer.

No. 26623 (New)
Postdoctoral Fellowship - McDonald Observatory (UT Austin)
MCDONALD OBSERVATORY (UT AUSTIN)
The University of Texas at Austin
1 University Station C1402
Austin, TX 78712-0259
USA
Tel: (512) 471-3300
FAX: (512) 471-1635
URL1: http://www.as.utexas.edu/astronomy/people/employment.html
URL2: http://www.as.utexas.edu/mcdonald/mcdonald.html
Email Submission Address: director@astro.as.utexas.edu
Email Inquiries: director@astro.as.utexas.edu

Attention: David L. Lambert, Director
Applications are invited for a position as a postdoctoral fellow at The W.J. McDonald Observatory, The University of Texas at Austin, to work with Dr. David L. Lambert on spectroscopic determinations of the chemical composition of stars and the interstellar medium.

Candidates are expected to hold a Ph.D., granted no earlier than December 2009, at the time of appointment.

Prior experience in abundance analysis is highly desirable. The position is offered for an initial period of one year, with an extension subject to performance. The position is available starting January 1, 2011.

Interested candidates should send a curriculum vitae, a list of publications and a statement of research interests to Dr. David L. Lambert at the above address, or via email (director@astro.as.utexas.edu). To send applications via express mail, please use the following address: Attn. Dr. David L. Lambert, The University of Texas at Austin, Department of Astronomy, 2511 Speedway, Robert Lee Moore (RLM) Hall - Rm. 15.208, Austin, TX 78712. Candidates should also arrange to have letters of recommendation sent to Dr. Lambert by three professional scientists familiar with the candidate's research. Applications will be considered after October 31, 2010.

No. 26624 (New)
ITC Fellow
HARVARD-SMITHSONIAN CENTER FOR ASTROPHYSICS
Tel:
URL1: http://www.cfa.harvard.edu/opportunities/fellowships/itc/
URL2: http://www.cfa.harvard.edu/itc/
Email Inquiries: itcpostdoc@cfa.harvard.edu

Attention: Gregory White, ITC Coordinator
Postdoctoral Research Positions Institute for Theory and Computation Harvard-Smithsonian Center for Astrophysics

Applications are invited for Postdoctoral Research Positions in the Institute for Theory and Computation (ITC) at the Harvard-Smithsonian Center for Astrophysics. One of the primary objectives of the ITC is to integrate conceptual theory with computational modeling. We are, therefore, interested in candidates working in any field related to theoretical and/or numerical astrophysics. Successful candidates will have access to our new computing facilities and will have the opportunity to interact and work with researchers in both the Harvard College Observatory (HCO) and the Smithsonian Astrophysical Observatory (SAO). Current senior members of the ITC include Harvard faculty Charles Alcock, Daniel Eisenstein, Doug Finkbeiner, Lars Hernquist, Avi Loeb, James Moran, Ramesh Narayan, Dimitar Sasselov, Irwin Shapiro, Alicia Soderberg, and Chris Stubbs, as well as SAO scientists Steven Cranmer, Angelica de Oliveira-Costa, Rosanne Di Stefano, Matt Holman, Eric Keto, and Ruth Murray-Clay. The nominal starting date is September 1, 2011, but earlier appointments are possible. The positions are for two years, renewable for a third year, contingent on performance and funding. Please submit applications electronically at http://www.cfa.harvard.edu/opportunities/fellowships/itc/ by 5:00pm EST, November 15, 2010. Further information about the ITC may be found at http://www.cfa.harvard.edu/itc/ ; please direct any questions on the application process to itcpostdoc@cfa.harvard.edu. Women and minorities are strongly encouraged to apply. AAE/EOE.

No. 26625 (New)
Postdoctoral position on stellar clusters dynamics in Grenoble
LABORATOIRE D'ASTROPHYSIQUE DE GRENOBLE
Observatoire de Grenoble
BP53
Grenoble Cedex 9, F- 38041
France
Tel:
URL1: http://www-laog.obs.ujf-grenoble.fr/ (Laboratoire d'Astrophysique de Grenoble)
Email Submission Address: emoraux@obs.ujf-grenoble.fr
Email Inquiries: emoraux@obs.ujf-grenoble.fr

Attention: Estelle Moraux
Applications are invited for a postdoctoral position at the Laboratoire d'Astrophysique de Grenoble in the framework of DESC (Dynamical Evolution of Stellar Clusters), a research project funded by the French National Research Agency (ANR).

The Laboratoire d'Astrophysique de Grenoble (LAOG) carries out observational and theoretical research in various field of astrophysics including the chemistry of interstellar medium, star and planet formation, and high energy phenomena. The LAOG is also involved in the technical development of major high angular resolution instruments for the VLT, VLTI and E-ELT.

The proposed research project will focus on numerical investigations of the early dynamical evolution of open clusters, with the aim to constrain the stellar cluster formation process(es). A special emphasis will be given to the comparison between simulations and observations, in the context of the preparation to the astrometric space mission Gaia. The successful candidate will be working in the star formation group in LAOG which has a vast experience in young cluster observations, including large scale photometric surveys and spectroscopic studies; and in collaboration with the Galaxy team in Strasbourg, which has strong expertise in gravitational dynamics and N-body numerical simulations.

Applicants must have a PhD and should have experience in N-body simulations or radiative transfer. Background in star formation theories or in stellar cluster observational studies will be an asset. The position is for two to three years, starting preferentially before the end of 2010.

Applications should include a CV, a list of publications and a statement of research interests and experience. The applicants should also arrange for two letters of recommendation to be sent independently. All materials should be directed to Estelle Moraux by October 15, 2010, either electronically or by mail at the given address.

No. 26627 (New)
Post-doctoral Position in Computational Astrophysics
UNIVERSITY OF ROCHESTER
Box 270171
Rochester, NY 14627
Tel: 585-275-4405
FAX: 585-273-2813
Email Submission Address: nhatler@pas.rochester.edu
Email Inquiries: nhatler@pas.rochester.edu

Attention: Nicole Hatler
Applications are invited for a post-doctoral/research assistant position in computational astrophysics in the theoretical research group at the University of Rochester. The group includes post-docs, graduate students and undergraduates as well current active collaborators at three other institutions. The prime scientific focus of the position will be the study of magnetically driven outflows from evolved and young stars. This program, run by Prof. Adam Frank and Prof. Eric Blackman, is part of a long-term study combining astrophysical observations, high performance computing and high energy density laboratory experiments. The successful candidate will use numerical tools to model both real astrophysical jets and dimensionally similar high energy density plasma jets created in pulsed power experiments. In addition to work on this project the successful candidate will also have a significant portion of their time to peruse their own scientific interests.

The computational group at the University of Rochester developed and uses a state of the art Adaptive Mesh Refinement code AstroBEAR ( http://www.pas.rochester.edu/~bearclaw/ ) and the successful applicant would be expected to contribute to both its development and application though the use of other codes is not precluded.

The computational astrophysics group is part of a vibrant multi-disciplinary, multi-institution research program in Rochester which includes infrared studies of star and planet formation, plasma laboratory astrophysics studies at Laboratory for Laser Energerics (housing one of the largest fusion laser facilities in the world), as well as X-ray studies of young stars and computational investigations of black holes at the Rochester Institute of Technology.

The position is for 2 years with a third year depending on performance. The successful applicant would have a share of time for his or her own projects.

Please send a CV, a statement of research interests and 3 letters of recommendation to Nikki Hatler at nhatler@pas.rochester.edu. Applications should be received by Dec 20 2010.

We prefer applications and letters of recommendation to be received electronically. If sending by post please use the following address

Computational Astrophysics Post-doc c/o Nikki Hatler Department of Physics and Astronomy University of Rochester, Rochester, NY 14627-0171

No. 26628 (New)
Hubble Fellow
SPACE TELESCOPE SCIENCE INSTITUTE
Tel:
URL1: http://www.stsci.edu/institute/org/spd/hubble-fellowship
Email Inquiries: hfinquiry@stsci.edu

Attention: 2011 Hubble Fellowship
The Space Telescope Science Institute announces the 21ST year of the Hubble Postdoctoral Fellowship Program and solicits applications for fellowships to begin in the fall of 2011.

The Hubble Fellowships support outstanding recent postdoctoral scientists to conduct independent research that is broadly related to the NASA Cosmic Origins scientific goals as addressed by any of the missions in this program: the Hubble Space Telescope, Spitzer Space Telescope, Stratospheric Observatory for Infrared Astronomy (SOFIA), the Herschel Space observatory, and the James Webb Space Telescope. The research may be theoretical, observational, or instrumental. This program is open to applicants of any nationality who have earned (or will have earned) their doctoral degrees on or after January 1, 2008, in astronomy, physics, or related disciplines. The fellowships are tenable at U.S. host institutions of the fellows' choice, subject to a maximum of one new fellow per host institution per year. The duration of the fellowship is up to three years: an initial one-year appointment and two annual renewals contingent on satisfactory performance and availability of NASA funds.

The Announcement of Opportunity, which includes detailed program policies as well as instructions both for the applicants and for their referees, is available at the web site:

http://www.stsci.edu/institute/org/spd/hubble-fellowship

Applicants and referees must follow the instructions for uploading their materials using the STScI Hubble Fellowships web interface as described in that Announcement. The deadline for applications is Thursday, November 4, 2010. Letters of reference are due by Thursday, November 11, 2010. Offers will be made before February 1, 2011, and new appointments are expected to begin on or about September 1, 2011.

Inquiries about the Hubble Fellowships may be directed to Dr. Ron Allen (hfinquiry@stsci.edu).

Women and members of minorities are strongly encouraged to apply; EOE/AA/M/F/D/V.

(Last update: 7/20/10)

No. 26629 (New)
Postdoctoral Position in X-Ray Astronomy
ARGELANDER INSTITUTE FOR ASTRONOMY AT BONN UNIVERSITY
Auf dem Huegel 71
Germany
Tel: +49-228-733642
FAX: +49-228-733543
URL1: http://dark-energy.net (Research Group)
URL2: http://www.astro.uni-bonn.de (Argelander Institute for Astronomy)
URL3: http://www.uni-bonn.de/news-1?set_language=en (Bonn University)
Email Submission Address: reiprich@astro.uni-bonn.de
Email Inquiries: reiprich@astro.uni-bonn.de

Attention: Thomas Reiprich, Professor
The Argelander Institute for Astronomy at Bonn University invites applications for a postdoctoral position.

The successful candidate is expected to work primarily with T. Reiprich on XMM-Newton, Chandra, Suzaku, and (the preparation for) eROSITA observations of galaxy groups and clusters. The research will likely focus on the physics and chemistry of the intracluster medium and/or on cosmology.

The appointment is for two years, extensions are possible depending on performance and availability of funds.

AIfA is one of the largest university astronomy departments in Germany and, together with the Max-Planck-Institute for Radioastronomy, constitutes a major astronomy center. AIfA is a Co-I institute of the eROSITA mission, to be launched in 2012. As Germany's former capital and with more than 2000 years of history, Bonn offers a culturally rich environment.

The successful applicant must have completed all Ph.D. requirements (in astrophysics, physics, or related field) before assuming the position. The position is available immediately; the actual starting date will be mutually agreed upon.

To apply, send a cover letter (indicating preferred starting date), CV, list of publications, and statement of research interests and experience (max three pages) to T. Reiprich. Please also arrange for three letters of recommendation to be sent. Email submission is preferred (PDF format, <10MB). Screening of applications will begin October 11, but applications will be accepted until the position is filled.

Bonn University is an equal opportunity employer and particularly welcomes applications from women, disabled persons, and members of underrepresented groups.

No. 26630 (New)
Swinburne Super Science Fellowship in Observational Galaxy Evolution
SWINBURNE UNIVERSITY OF TECHNOLOGY
Mail number H39
PO Box 218
Hawthorn, VIC 3122
Australia
Tel: +61 3 9214 4384
FAX: +61 3 9214 8797
URL1: http://astronomy.swin.edu.au/ (Centre for Astrophysics & Supercomputing)
URL2: http://www.swinburne.edu.au (Swinburne University)
URL3: http://www.swinburne.edu.au/corporate/hr/swin (Working ar Swinburne/HR information)
Email Submission Address: karl@astro.swin.edu.au
Email Inquiries: karl@astro.swin.edu.au

Attention: karl@astro.swin.edu.au, Professor
Applications are invited for an Australian Research Council funded Super Science Fellowship to be held in the Centre for Astrophysics and Supercomputing at the Swinburne University of Technology. The Super Science Fellowships are an Australian Government funded program targeted towards outstanding early-career researchers, whom must be within 3 years of their PhD award at the time of appointment, and is a fixed three year term full-time research position with a generous package of salary and research funding.

The Fellow will lead a research program collaborating with Swinburne astronomers including Karl Glazebrook, Michael Murphy & Emma Ryan-Weber to research the chemical evolution of the Universe from high to low redshift; taking advantage of new optical/IR data on galaxies and QSO absorbers from large telescopes and making predictions for the next generation of HI radio surveys from the Australian SKA Pathfinder. Independent research can also be pursued.

Essential criteria: A PhD in observational astrophysics and a background in extra-galactic studies coupled with strong research skills and a demonstrated publication track-record in peer-reviewed journals. Desirable criteria: experience with high-redshift galaxy or QSO surveys and optical and/or near-infrared imaging and spectroscopy, excellent oral and written communications skills.

The appointee will join an active research group in Australia's most rapidly growing astronomy department. Swinburne astronomers regularly obtain national observing time on the AAT, Gemini, HST, Magellan, ATCA and Parkes telescopes. They have institutional access to the W.M. Keck telescopes in Hawaii (15-20 nights per year). The Centre has a state-of-the-art supercomputer available in house as well as access to innovative 3D visualization facilities. Melbourne, consistently rated as one of the most liveable cities in the world, is a cosmopolitan place with a mild climate and many cultural and sporting events. Mountains, ocean and wine growing regions are easily accessible. The Centre itself is located in the diverse inner city suburb of Hawthorn with very good public transport connections.

Super Science Fellows receive an attractive package: the appointment is for fixed term for three years at a Lecturer equivalent position (Level B1). The salary is AUD 72,500 p.a. and the Fellow also receives a AUD 20,000 per year research expenses allowance. By ARC rules the applicant must usually be within three years of their PhD at the time of their appointment and must take up the appointment between July and December 2011.

Applications must include a CV, bibliography, statement of research interests and plans, and contact details of three referees and should be emailed to Prof Karl Glazebrook at the above address. Please quote position number 28395. Applications are due by 15th Dec 2010 and are required in PDF format. Please direct any enquiries about the position to Prof. Glazebrook and please instruct referees to email their references direct to Prof. Glazebrook by the deadline.

Swinburne is a 2010 Federally recognised "Employer of Choice for Women". Swinburne encourages applications from Indigenous people, people from culturally and linguistically diverse backgrounds, people with disabilities, women and men.

No. 26631 (New)
Swinburne Super Science Fellowship in Galaxy Simulation
SWINBURNE UNIVERSITY OF TECHNOLOGY
Mail number H39
PO Box 218
Hawthorn, VIC 3122
Australia
Tel: +61 3 9214 8624
FAX: +61 3 9214 8797
URL1: http://astronomy.swin.edu.au/ (Centre for Astrophysics & Supercomputing)
URL2: http://www.swinburne.edu.au (Swinburne University)
URL3: http://www.swinburne.edu.au/corporate/hr/swin (Working ar Swinburne/HR information)
Email Submission Address: cblake@astro.swin.edu.au
Email Inquiries: cblake@astro.swin.edu.au

Attention: cblake@astro.swin.edu.au, Senior Lecturer
Applications are invited for an Australian Research Council funded Super Science Fellowship to be held in the Centre for Astrophysics and Supercomputing at the Swinburne University of Technology. The Super Science Fellowships are an Australian Government funded program targeted towards outstanding early-career researchers, whom must be within 3 years of their PhD award at the time of appointment, and is a fixed three year term full-time research position with a generous package of salary and research funding.

The Fellow is expected to lead a research program collaborating with Swinburne astronomers including Chris Blake, Virginia Kilborn and Emma Ryan-Weber to simulate the evolution of cosmic gas from high to low redshift. The project aims to use existing observations to test the underlying physics governing the evolution of gas into galaxies, and make realistic predictions for the science achievable by the forthcoming Australian SKA pathfinder. Independent research can also be pursued.

Essential criteria: A PhD in astrophysics with research interests in numerical simulations or theory, coupled with strong research skills and a demonstrated publication track-record in peer-reviewed journals. Desirable criteria: a background in hydrodynamic modelling and high-performance computing, excellent oral and written communications skills.

The appointee will join an active research group in Australia's most rapidly growing astronomy department. The Centre has a state-of-the-art supercomputer available in house as well as access to innovative 3D visualization facilities. Melbourne, consistently rated as one of the most liveable cities in the world, is a cosmopolitan place with a mild climate and many cultural and sporting events. Mountains, ocean and wine growing regions are easily accessible. The Centre itself is located in the diverse inner city suburb of Hawthorn with very good public transport connections.

Applications must include a CV, bibliography, statement of research interests and plans, and contact details of three referees and should be emailed to Dr Chris Blake at the above address. Please quote position number 28394. Applications are due by 15th Dec 2010 and are required in PDF format. Please direct any enquiries about the position to Chris Blake and please instruct referees to email their references direct to Chris Blake by the deadline.

No. 26632 (New)
Postdoctoral Fellowships in Astronomy
CARNEGIE INSTITUTION OF WASHINGTON-DEPARTMENT OF TERRESTRIAL MAGNETISM
5241 Broad Branch Road, NW
Washington, DC 20015
USA
Tel: 202-478-8820
FAX: 202-478-8821
URL1: http://www.dtm.ciw.edu
Email Submission Address: fellowships@dtm.ciw.edu
Email Inquiries: fellowships@dtm.ciw.edu

Attention: Astronomy Fellowship Committee, Carnegie Institution of Washington
Applications are invited for a postdoctoral fellowship for independent research on the origin and evolution of stars, planets, and life. We are seeking theorists and observers working in the fields of star and planet formation, extrasolar planet detection and characterization, planetary astronomy, and the physical and chemical evolution of prebiotic compounds.

DTM has an active group of researchers in these and other areas. Vera Rubin’s work centers on extragalactic astronomy. Alan Boss and John Chambers head the theoretical effort to understand the formation of stellar and planetary systems, while Paul Butler is a leader in the spectroscopic search for extrasolar planets. Alycia Weinberger observes circumstellar disks, including nearby debris and protoplanetary disks. Scott Sheppard studies small, primordial bodies in our Solar System. Conel Alexander, Larry Nittler, and George Cody perform laboratory studies of pre-planetary materials (including circumstellar grains and interstellar organics) in meteorites and interplanetary dust. Planetary scientist Sean Solomon is involved in spacecraft missions at Mars and leads the MESSENGER mission to Mercury.

Our fellows have access to a wide range of facilities. Fellows are eligible to apply for time at Carnegie’s Las Campanas Observatory in Chile, including the twin 6.5-m Magellan telescopes. Theoretical calculations are performed on the Carnegie Clusters of Alpha, Xeon, and Harpertown processors. Spectroscopic techniques applied to pre-planetary materials include ion microprobe, solid-state NMR, GC-MS, and synchrotron X-ray and IR-spectrometry. DTM fellowships provide support for observing, travel, computing, and publication.

Applicants should have a Ph.D. in a relevant field and a promising record of research and publication. A C.V., list of publications, brief statement of research plans, and three letters of recommendation, sent directly to us by those familiar with your work, should be submitted to the above address by 1 December 2010. Fellowships may be renewed for up to three years. Women and minority candidates are especially encouraged to apply. AAE/EOE.

No. 26634 (New)
2011 KASI – Carnegie Joint Postdoctoral Fellowship
KOREA ASTRONOMY AND SPACE SCIENCE INSTITUTE & CARNEGIE INSTITUTION FOR SCIENCE
61-1, Hwaam-dong, Yuseong-gu
Daejeon, Chungnam 305-348
Republic of Korea
Tel: +82-42-865-3270
FAX: +82-42-865-3272
Email Submission Address: arl@kasi.re.kr
Email Inquiries: arl@kasi.re.kr

Attention: A-Ran Lyo, Researcher
Korea Astronomy and Space Science Institute (KASI) and The Observatories of the Carnegie Institution for Science (Carnegie Observatories) invite applications for a four (4) - year KASI-Carnegie Joint Postdoctoral Fellowship in astronomy, to begin in September 2011. The Fellow with a Korean Ph.D. degree is expected to work for the first two (2) years at the main office of the Carnegie Observatories in Pasadena and the following two (2) years at KASI in Korea. The Fellow with a Ph.D. degree obtained from countries other than Korea is expected to work for the first two (2) years at KASI and the following two (2) years at the main office of the Carnegie Observatories. However, the order of the work place assignment among KASI and Carnegie Observatories and the duration of each stay is negotiable.

We encourage applications from broad areas of astronomy and astrophysics, although preference will be given to researchers working in areas in which KASI and Carnegie have active research interests and particularly those relevant to the Giant Magellan Telescope (GMT). Both institutions are founding members of the GMT Corporation. The Fellow will have full access to all resources and facilities of both Institutions as outlined below. However, in the case of the twin 6.5-meter Magellan telescopes, the fellow shall have access only in collaboration with a Carnegie staff astronomer.

KASI resources and observing facilities include the 128 Core Xeon PC Cluster (RAM256GB), the 1.8-meter Bohyunsan optical telescope, the 1.0-meter Mt. Lemmon optical telescope, the 61-cm Sobaeksan optical telescope, the 14-meter Taeduk radio telescope, and the Korean Very Long Baseline Interferometer (KVN). Carnegie operates the Las Campanas Observatory in Chile, which in addition to the twin 6.5-meter Magellan telescopes includes the 2.5-meter Dupont telescope and the 1.0-meter Swope telescope.

Interested persons should submit the following documents to BOTH KASI and Carnegie Observatories: - a curriculum vitae - a statement of current research - a research plan based on the resources and facilities available at both institutions - three letters of reference sent directly by the letter writer

Applications should be submitted by 15th November 2010 via e-mail: arl@kasi.re.kr (for KASI) and k-cfellow@obs.carnegiescience.edu (for Carnegie Observatories). Selection of the successful candidate will be made by a joint KASI-Carnegie committee.

Enquiries may be addressed to: KASI – Dr. Lyo (e-mail: arl@kasi.re.kr) Carnegie Observatories – Dr. John Mulchaey (e-mail: k-cfellow@obs.carnegiescience.edu)

No. 26636 (New)
Postdoctoral Position in Cosmology
INSTITUTE OF THEORETICAL ASTROPHYSICS - UNIVERSITY OF OSLO
Tel:
URL1: http://uio.easycruit.com/vacancy/430138/64278?iso=gb
Email Inquiries: mota@astro.uio.no

Attention: http://uio.easycruit.com/vacancy/430138/64278?iso=gb
A postdoctoral fellowship in cosmology is open at the Institute of Theoretical Astrophysics of the University of Oslo. The fellowship is for 3 years. The position is available from 1st January 2011, but can be started later on.

Salary: NOK 448.200 – 510.000 depending on qualifications

Closing date for applications: 1 October 2010.

Applications must be submitted electronically: http://uio.easycruit.com/vacancy/430138/64278?iso=gb

The position is connected to the project ”Cosmological Probes of Modified Gravity”, funded by the Research Council of Norway. The successful applicant is expected to carry out research on cosmological structure formation within theories of gravity beyond General Relativity. The research will focus on both the linear and nonlinear regime of structure formation in the framework of scalar-tensor theories, vector-tensor theories and brane world models. It may involve testing these alternatives to dark energy using N-body simulations and/or lensing and/or the CMB and matter power spectra among others.

Applications must include:

• Research proposal • CV • List of publications • Short version of CV containing: 1) the institution where the master thesis was received and date of graduation, 2) the institution where the Ph.D. was received and date of the defense, 3) the institutions where the applicant has been employed after the Ph.D., 4) number of papers and 5) very brief description of field of research and how it is related to cosmological structure formation. (Please upload under section " other attachments"). • Two letters of reference to be sent by e-mail to d.f.mota@astro.uio.no.

No. 26638 (New)
Menzel Fellow Position 2011
HARVARD UNIVERSITY
60 Garden Street, Ms-67
Cambridge, MA 02138
USA
Tel: 617-495-7103
FAX: 617-496-7589
URL1: http://www.cfa.harvard.edu/opportunities/fellowships/menzel/
Email Submission Address: postdoc@cfa.harvard.edu
Email Inquiries: postdoc@cfa.harvard.edu

Attention: Christine Crowley, Fellowship Program Coordinator
Department of Astronomy and Harvard College Observatory Menzel Postdoctoral Fellow 2011

The Department of Astronomy and Harvard College Observatory (HCO), at the Center for Astrophysics (CfA), announce the availability of the 2011 Donald H. Menzel Postdoctoral Fellow position in astrophysics. Candidates with an exceptional record of research in any field of astrophysics, particularly theory, are encouraged to apply. Only applicants who received their Ph.D. on or after January 1, 2010 will be considered.

The CfA combines the resources and research facilities of the Harvard College Observatory and the Smithsonian Astrophysical Observatory under a single director. Nearly 350 Smithsonian and Harvard scientists work cooperatively in an environment that welcomes the ideas and contributions of young scientists. Facilities include the MMT (Fred Lawrence Whipple Observatory, Arizona), Magellan (Las Campanas Observatory, Chile), and other optical and infrared telescopes; radio telescopes, especially the Submillimeter Array on Mauna Kea, Hawaii; a large Beowulf cluster and network of workstations; a number of specialized laboratories; an outstanding library; and access to data from a wide range of space missions, especially the Chandra X-ray Observatory and the Spitzer Space Telescope.

No. 26640 (New)
Postdoctoral Fellowships
KAVLI INSTITUTE FOR PARTICLE ASTROPHYSICS AND COSMOLOGY
Tel:
URL1: http://www-group.slac.stanford.edu/kipac/competition/apply.html (Web interface for submission of applications)
URL2: http://www-group.slac.stanford.edu/kipac/ (For further information about KIPAC)
URL3: http://www-group.slac.stanford.edu/kipac/faculty.html (Informal inquires to any KIPAC faculty member)
Email Inquiries: postdoc-recruit@kipac.stanford.edu

Attention: http://www-group.slac.stanford.edu/kipac/competition/apply.html
The Kavli Institute for Particle Astrophysics and Cosmology (KIPAC) at Stanford University and the SLAC National Accelerator Center has a number of openings for Postdoctoral Research Fellows for the Fall of 2011. These appointments are for up to three years and are reviewed annually.

KIPAC is a joint institute formed by the Departments of Physics and Applied Physics at Stanford University, and by SLAC. Research interests at the Institute are broad but are focused at the interface between physics and astronomy, encompassing observational, theoretical, computational, and experimental topics.

We are seeking outstanding individuals with a commitment to carrying out a vigorous research program in any area encompassed by KIPAC's broad research goals in astrophysics and cosmology. Successful applicants will have the opportunity to collaborate with existing research groups at Stanford/SLAC, and to participate in a variety of ground and satellite-based projects. Research areas where applications are particularly encouraged include multiwavelength studies of galaxies and galaxy clusters; gravitational lensing; searches for dark matter; the Dark Energy Survey; the Large Synoptic Survey Telescope; cosmological parameter estimation; Cosmic Microwave Background polarization experiments, the Fermi Gamma-ray Space Telescope (FGST) and current and future TeV gamma-ray telescopes such as CTA. KIPAC also has an active research program in theoretical and computational astrophysics with an emphasis on compact objects and the formation and evolution of structure in the Universe, and welcomes applications in these areas.

Successful applicants should have, or be in the process of completing, a Ph.D. in Astronomy or Physics. They should posses a strong research background and provide evidence of outstanding potential. These positions are highly competitive and offer excellent salaries and benefits. Applicants will automatically be considered for other postdoctoral opportunities at KIPAC, including the Kavli Fellowships.

Applicants should provide a statement of research interests, a CV, and arrange for three letters of reference. All applications should be submitted through the web interface at http://www-group.slac.stanford.edu/kipac/competition/apply.html .

The deadline for receipt of documents is December 1, 2010, although late applications may be considered until the positions are filled.

Further information about KIPAC is available at http://www-group.slac.stanford.edu/kipac/ . Informal inquires regarding these positions may be addressed to postdoc-recruit@kipac.stanford.edu or to any KIPAC faculty member at http://www-group.slac.stanford.edu/kipac/faculty.html .

No. 26641 (New)
Kavli Fellowships at Stanford
KAVLI INSTITUTE FOR PARTICLE ASTROPHYSICS AND COSMOLOGY
Tel:
URL1: http://www-group.slac.stanford.edu/kipac/competition/apply.html (Web interface for submission of applications.)
URL2: http://www-group.slac.stanford.edu/kipac (For further information about KIPAC)
URL3: http://www-group.slac.stanford.edu/kipac/faculty.html (Informal inquires to any KIPAC faculty member)
Email Inquiries: postdoc-recruit@kipac.stanford.edu

Attention: http://www-group.slac.stanford.edu/kipac/competition/apply.html
The Kavli Institute for Particle Astrophysics and Cosmology (KIPAC) at Stanford University seeks young scientists of exceptional promise for Kavli Fellowships in astrophysics and cosmology. This fellowship program offers outstanding young scientists with experience in computation, instrumentation, observation, or theory, opportunities to develop innovative research programs in astrophysics and cosmology. Kavli Fellows will have great freedom, but may collaborate with existing KIPAC groups when appropriate. We expect to appoint one or more fellows this year. The positions offer excellent salary and benefits and a term of three years. The successful candidates will also receive a generous annual budget to support research expenses.

KIPAC is a joint venture between the Stanford Department of Physics and SLAC National Accelerator Laboratory. Research interests cover the interface between physics and astronomy, including a broad range of experimental, computational, observational, and theoretical topics.

Existing programs include studies of dark energy, cosmic dynamics and structure formation, probing inflation with Cosmic Microwave Background polarization experiments, searches for dark matter, and studies of black holes, galaxies, clusters of galaxies, stars (including the sun) and other astrophysical sources. KIPAC members are involved in projects such as the Fermi Gamma-Ray Space Telescope, the AGIS and CTA TeV Gamma-Ray Observatory, CDMS, the BICEP-2/ Keck Array, CHIP, Polar, Planck, and QUIET CMB experiments, DES, JDEM, LSST, NuSTAR, ASTRO-H and the International X-ray Observatory. There are excellent laboratory facilities for instrumental development and significant computational resources for theoretical astrophysical research and data analysis.

Successful applicants should have, or be in the process of completing, a Ph.D. in astronomy or physics. They should possess a strong research background and provide evidence of future potential. Applicants will automatically be considered for all available postdoctoral opportunities at KIPAC.

Applicants should provide a CV, research statement and arrange for three letters of reference. Please visit http://www-group.slac.stanford.edu/kipac/competition/apply.html to submit your application. The deadline for receipt of all documents is December 1, 2010, although late applications may be considered until the positions are filled.

Further information about KIPAC may be found at the website http://www-group.slac.stanford.edu/kipac . Informal inquires regarding these positions may be addressed to postdoc-recruit@kipac.stanford.edu or to any KIPAC faculty member, listed at http://www-group.slac.stanford.edu/kipac/faculty.html considered until the positions are filled.

No. 26642 (New)
Postdoctoral Research Scientist -- Nearby and Low-Mass Stars
AMERICAN MUSEUM OF NATURAL HISTORY
Central Park West at 79th street
New York, NY 10024
USA
Tel: 212-496-3312
FAX: 212-769-5007
URL1: http://research.amnh.org/astrophysics
Email Submission Address: lepine@amnh.org
Email Inquiries: lepine@amnh.org

Attention: Sebastien Lepine, Department of Astrophysics
Applications are invited for a Postdoctoral Research Scientist position in the Department of Astrophysics at the American Museum of Natural History, New York City, to begin in the Fall 2010 or later.

The successful candidate will be working with Dr. Sebastien Lepine and his collaborators on an all-sky survey of stars located within 100 parsecs of the Sun, as part of a comprehensive census of possible targets for exoplanet search programs. The candidate will also work on a multiplicity census of low-mass stars using Hubble Space Telescope archival data and the new SUPERBLINK proper motion catalog built by Dr. Lepine. Responsibilities will include conducting follow-up observations of various targets of interest, and performing reduction and analysis of both imaging and spectroscopic data.

Experience in stellar spectroscopy required. Experience in astrometric observations and/or adaptive optics imaging a plus.

This position is funded for a term of 2 years.

Interested applicants should send a curriculum vitae, bibliography, two letters of reference and a brief statement of research interests electronically to lepine@amnh.org. Review of applications will begin October 1st 2010, and will continue until the position is filled. For further information, please contact Dr. Sebastien Lepine (lepine@amnh.org).

No. 26643 (New)
AAAS Science and Techonology Policy Fellowships
AMERICAN ASSOCIATION FOR THE AVANCEMENT OF SCIENCE
Tel:
Email Inquiries: fellowships@aaas.org

Attention: Fellowships
APPLY YOUR SCIENCE TO SERVE SOCIETY

For more than 35 years, the AAAS Science & Technology Policy Fellowships have provided scientists and engineers with a unique opportunity to apply their knowledge and skills to national and international issues in the federal policy realm, while learning first-hand about establishing and implementing policy.

Fellows select assignments in Congressional offices or federal agencies. This is a year-long opportunity, beginning September 1 and ending August 31. Most federal agencies offer Fellows the ability to renew for a second year.

AAAS seeks candidates from a broad array of backgrounds and a diversity of geographic, disciplinary, gender, and ethnic perspectives. Fellows have ranged in age from late 20s to early 70s. They represent a spectrum of career stages, from recent PhD graduates to faculty on sabbatical to retired scientists and engineers. Fellows also come from a range of sectors, including academia, industry, non-profit organizations, and government labs.

AAAS partners with more than 30 scientific societies that also sponsor fellowships. They conduct separate application and selection processes and provide different stipend and benefits support. Individuals interested in the AAAS Science & Technology Policy Fellowships are encouraged to apply with all scientific societies for which they qualify.

The deadline is December 5th, 2010. AAAS accepts online applications only. Full details at http://www.fellowships.aaas.org .

No. 26647 (New)
James Webb Space Telescope Postdoctoral Fellowships
NASA'S GODDARD SPACE FLIGHT CENTER
Building SC-200
1299 Bethel Valley Road
Oak Ridge, TN 37830
USA
Tel: 865-574-3172
URL1: http://nasa.orau.org/postdoc/ (NASA Postdoctoral Program and on-line application)
URL2: http://jwst.nasa.gov/ (James Webb Space Telescope website)
URL3: http://www.springerlink.com/content/h2374012xk30qpw5/fulltext.pdf (JWST review paper)
Email Inquiries: jonathan.p.gardner@nasa.gov

Attention: Janeen Pointer, NASA Postdoctoral Program
The James Webb Space Telescope (JWST) Project at NASA’s Goddard Space Flight Center (GSFC) invites applications through the NASA Postdoctoral Program (NPP) to carry out postdoctoral research in astrophysics or astronomical instrumentation. The applicant will work directly with one of the JWST Project Scientists and will be resident within the Astrophysics Science Division at GSFC. The science objectives of JWST include the initial formation of galaxies in the early Universe, galaxy evolution including active galactic nuclei (AGN), star and planetary system formation, and the study of extra-Solar planets and Solar System objects. Astronomical research relevant to JWST’s science goals could include theoretical studies or be based on observations taken with current space-based or ground-based facilities. Examples of interest to the JWST Project Scientists include spectroscopy and HST imaging of lensed galaxies at high redshift; discovery and characterization of highly-obscured AGN; integral field unit or multi-object spectroscopy; Hadamard transform spectroscopy with the IRMOS instrument (Proc. SPIE, 7249, 25, 2009); studies of debris disks and exoplanets using coronagraphic or transiting techniques; and infrared instrumentation, including advanced detectors and optics. Additional information about JWST is available through the website http://jwst.nasa.gov , and from the review paper Gardner et al 2006, Space Sci. Rev. 123, 485 (astro-ph/0606175).

The next NPP Fellowship application deadline is November 1, 2010. Please contact Jonathan Gardner, jonathan.p.gardner@nasa.gov before the deadline for assistance in preparing the application. The NPP Fellowship appointment is initially for one year, and can be renewed for up to two more years based on acceptable performance and availability of funding. Appointments come with competitive stipends and a generous travel budget. Applicants will be judged on their academic accomplishments, letters of reference, the merit of their research proposal and its relevance to NASA programs. Applications should be submitted through the NPP website at: http://nasa.orau.org/postdoc/ .

No. 26649 (New)
Harlan J. Smith Postdoctoral Fellowship
MCDONALD OBSERVATORY (UT AUSTIN)
The University of Texas at Austin
1 University Station C1402
Austin, TX 78712-0259
USA
Tel: (512) 471-3300
FAX: (512) 471-1635
URL1: http://www.as.utexas.edu/astronomy/people/employment.html (McDonald Observatory Employment web site)
URL2: http://www.as.utexas.edu/mcdonald/mcdonald.html (McDonald Observatory web site)
Email Submission Address: director@astro.as.utexas.edu
Email Inquiries: director@astro.as.utexas.edu

Attention: David L. Lambert, Director
The University of Texas McDonald Observatory announces competition for the Harlan J. Smith Postdoctoral Fellowship. This Fellowship is restricted to new Ph.D. graduates without previous postdoctoral experience. The applicant’s research interest may be in any area of astronomy and astrophysics and may be either observational or theoretical. The observing facilities of McDonald Observatory available for research include the 9.2-m Hobby-Eberly Telescope, the 2.7-m Harlan J. Smith Telescope, the 2.1-m Otto Struve Telescope, and the 0.8-m wide-field imaging telescope. Access to the robotic ROTSE and MONET telescopes is also available. McDonald Observatory also supports a program in millimeter wavelength research with the Caltech Submillimeter Observatory on Mauna Kea. The Texas Advanced Computing Center includes the Ranger and Lonestar computers and the Visualization Laboratory. Information on research and facilities is available at: http://www.as.utexas.edu/ . The Fellowship has a three year term and includes funding of $8,000 per year for research expenses, including travel. Additional funds are available for publication expenses related to work completed during the Fellow’s tenure, and for relocation expenses. Initial appointment will be for one year beginning September 2011, with the expectation of renewal for a second and third year following satisfactory research performance. Candidates are expected to hold a Ph.D. upon arrival and to reside in Austin.

Applicants should send a resumé and a statement of proposed research to be conducted at UT Austin during the Fellowship to Dr. David L. Lambert at the above address, or via email (director@astro.as.utexas.edu). To send applications via express mail, please use the following address: Attn. Dr. David L. Lambert, The University of Texas at Austin, Department of Astronomy, 2511 Speedway, Robert Lee Moore (RLM) Hall - Rm. 15.208, Austin, TX 78712. Candidates should also arrange to have letters of recommendation sent to Dr. Lambert by three professional scientists familiar with the applicant's research by November 30, 2010. EOE/AAE.

No. 26650 (New)
Associate Specialists in Theoretical Astrophysics and Relativity
KAVLI INSTITUTE FOR THEORETICAL PHYSICS
Kavli Institute for Theoretical Physics
Kohn Hall
Santa Barbara, CA 93106-4030
United States
Tel:
URL1: http://www.kitp.ucsb.edu/for-scientists/programs-conferences (Institute Website)
Email Submission Address: pdapps@kitp.ucsb.edu
Email Inquiries: bildsten@kitp.ucsb.edu

Attention: David Gross, Director
Postdoctoral Positions in Theoretical Astrophysics Kavli Institute for Theoretical Physics Kohn Hall University of California, Santa Barbara Santa Barbara, CA 93106-4030 Inquiries to Lars Bildsten (bildsten@kitp.ucsb.edu) The Kavli Institute for Theoretical Physics (KITP) expects to appoint Researchers as Associate Specialists in theoretical astrophysics at the postdoctoral level, starting September 1, 2011. The Institute is especially interested in candidates who can contribute to the diversity and excellence of the academic community through research, teaching and service. The KITP's purpose is to contribute to the progress of theoretical physics, especially in areas overlapping the traditional subfields, in ways that are not easily realized in existing institutions. The scientific work is carried out by approximately 70 members, including the director, deputy director, 4 permanent members, 15 researchers at the postdoctoral level, and 50-55 visiting senior members. KITP permanent members and postdoctoral fellows are active in all areas of theoretical physics, including astrophysics. Most visiting members are participants in programs that last 2-5 months, there are at least ten programs per year. Current and future astrophysics programs include Galaxy Clusters: the Crossroads of Astrophysics and Cosmology (Winter 2011), Asteroseismology in the Space Age (Fall 2011), and Faint Galaxies and Faint Dwarfs: Clues to Small Scale Structure of Cold Dark Matter (Winter/Spring 2012).

KITP researchers at the postdoctoral level have opportunities for international collaborations with CITA and MPA-Garching. For current information on this and other programs, see http://www.kitp.ucsb.edu/for-scientists/programs-conferences . Applications for these positions should be made electronically via our web page at http://www.kitp.ucsb.edu/for-scientists/fellowships/postdocs . Inquiries regarding scientific and/or programmatic issues may be addressed to Professor Lars Bildsten (bildsten@kitp.ucsb.edu). In the event that you are unable to upload your documents, hard copies should be sent to Professor David Gross, Director, Kavli Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106-4030. The deadline for applications and all materials is December 1, 2010. Later applications will be considered only as long as openings exist.

The University of California, Santa Barbara is an Equal Opportunity/Affirmative Action Employer.

No. 26651 (New)
Postdoctoral Fellow In Observational/Theoretical Studies of Quasars
YORK UNIVERSITY
Tel:
URL1: http://www.physics.yorku.ca/ (York University Dept. of Physics and Astronomy)
URL2: http://www.academicjobsonline.org/ (AcademicJobsOnline.org)
URL3: http://www.cita.utoronto.ca/ (Canadian Institute for Theoretical Astrophysics)
Email Inquiries: yorkphall@gmail.com

Attention: AcademicJobsOnline.org
Applications are invited for a postdoctoral fellowship at York University in Toronto, Ontario, Canada, starting July 2011 or later. A PhD is required. The successful applicant will work with Prof. Patrick Hall and collaborators on studies of quasars at the interface between theory and observation. The preferred major research topic is the nature and dynamics of quasar outflows, particularly their connections to accretion disks. Other research topics of interest include studies of quasar broad-line regions and of intervening absorption lines.

Astronomers in Canada have free access to the CFHT-Legacy Survey and competitive access to the Gemini telescopes, the CFHT, the JCMT, NRAO radiotelescopes including ALMA, and the SHARCNET high-performance computing network.

Faculty in the Physics and Astronomy Department at York University have interests in active galactic nuclei, chemical evolution of galaxies, radio studies of pulsars and supernovae, and particle astrophysics. York University is located in suburban Toronto, 45 minutes from the University of Toronto Department of Astronomy and Astrophysics and the Canadian Institute for Theoretical Astrophysics (CITA).

The position is initially for one year and is renewable for up to two more, subject to satisfactory performance. Applicants particularly interested in theoretical studies will be considered for partial support from a CITA National Fellowship.

For full consideration, applicants must submit a statement of proposed near-future research interests, a bibliography, a CV and the names of three professional references to http://www.academicjobsonline.org by November 1, 2010. Submission by other means is strongly discouraged. The position will remain open until filled.

No. 26652 (New)
YCAA Postdoctoral Prize Fellowship in Astronomy & Astrophysics
YALE UNIVERSITY
260 Whitney Avenue
P.O. Box 208120
New Haven, CT 06520-8120
USA
Tel: 203-432-9950
FAX: 203-432-3824
URL1: http://www.yale.edu/physics (Yale University Department of Physics)
URL2: http://www.yale.edu/ycaa (Yale Center for Astronomy & Astrophysics)
URL3: http://www.astro.yale.edu (Yale University Department of Astronomy)
Email Submission Address: nikhil.padmanabhan@yale.edu
Email Inquiries: nikhil.padmanabhan@yale.edu

Attention: Nikhil Padmanabhan, Professor
Yale University Postdoctoral Prize Fellowship Yale Center for Astronomy and Astrophysics Submit Applications To: https://academicjobsonline.org/ajo/jobs/364 Attention: Professor Nikhil Padmanabhan P.O. Box 208120 New Haven, CT 06520-8120 USA Tel: 203-432-9950 Fax: 203-432-3824 URL1: http://www.yale.edu/physics (Yale University, Department of Physics) URL2: http://www.yale.edu/ycaa (Yale Center for Astronomy & Astrophysics) URL3: http://www.astro.yale.edu (Department of Astronomy)

Email Inquiries: nikhil.padmanabhan@yale.edu

The closing date for receipt of applications: 11/12/2010

The Yale Center for Astronomy and Astrophysics invites applications for the YCAA Postdoctoral Prize Fellowship in Astronomy and Astrophysics, to be awarded to a young scientist of exceptional ability who will have received her/his Ph.D. by June 2011 in observational, theoretical, or experimental astronomy or astrophysics/cosmology. The Fellowship is for three years (renewed annually subject to performance), and offers competitive salary ($60,000), benefits, and research funds.

Conveniently located between New York City and Boston, Yale offers a lively intellectual environment and access to world-class astronomical facilities, including the Keck, WIYN and SMARTS telescopes, and to Chilean telescopes through collaboration with the Univ. de Chile. Yale is an institutional member of the SDSS-3 collaboration, and the Fellow will have the opportunity to develop projects with these data. The Fellow will also have access to the High-Performance Computing facilities at Yale.

The YCAA Prize Postdoctoral Fellow will be free to carry out his/her own research program, although preference will be given to research interests that align with those of the Yale astrophysics faculty (see http://www.yale.edu/ycaa/membership.html ). Active research at Yale includes solar astrophysics, nuclear astrophysics, astrometry, star formation, stellar evolution, galactic structure, black holes, local group galaxies, high-energy astrophysics, multiwavelength surveys (QUEST, GOODS, COSMOS, MUSYC, SDSS), active galaxies and blazars, galaxy evolution, galaxy clusters, large-scale structure, gravitational lensing, dark matter, dark energy, and cosmology.

Applicants are encouraged to apply online at https://academicjobsonline.org/ajo/jobs/364 and must send their curriculum vitae, bibliography, and a brief description of their anticipated research program by November 12, 2010 (online submission is strongly preferred). Mail submissions may be sent to the address listed above. Candidates should also arrange for at least 3 letters of recommendation to be submitted to the above URL by November 12. Fellowship candidates will automatically be considered for any open postdoctoral positions at Yale in their fields of interest, unless they ask to be considered only for the YCAA Prize Postdoctoral Fellowship. Yale is an Affirmative Action/ Equal Opportunity Employer, and we particularly encourage applications from women and members of minority groups.

No. 26653 (New)
Plaskett Fellowship
NATIONAL RESEARCH COUNCIL CANADA - HERZBERG INSTITUTE OF ASTROPHYSICS (NRC-HIA)
5071 West Saanich Road
Victoria, B.C. V9E 2E7
Canada
Tel: 250-363-0050
FAX: 250-363-8766
URL1: http://www.nrc-cnrc.gc.ca/eng/ibp/hia/fellowship/plaskett/index.html
Email Submission Address: plaskett@nrc-cnrc.gc.ca
Email Inquiries: plaskett@nrc-cnrc.gc.ca

Attention: Competition 40-10-22, PLASKETT FELLOWSHIP, NATIONAL RESEARCH COUNCIL of CANADA (NRC)
The NRC-HIA invites applications for Plaskett Fellowships tenable at DAO. The awards are made to outstanding recent doctoral graduates in astrophysics or a closely related discipline to conduct independent research in a stimulating, collegial environment. The award is for a maximum of three years; the initial appointment of two years may be extended for one further year (subject to performance and availability of funds). In addition to highly competitive benefits and salary, Fellows receive support for observing and conference travel, page charges, and access to professionally managed computers and the Canadian Astronomy Data Centre, which is home to the Canadian Virtual Observatory and data archives from, e.g., CFHT, CGPS, HST, Gemini, JCMT.

Staff expertise is in observational astrophysics, but we welcome applications from theoreticians whose research requires close interaction with observers. Fellows are eligible to apply for Canadian time on ALMA, CFHT, Gemini & JCMT, to use the optical and radio telescopes operated by NRC-HIA in Victoria and Penticton, and/or to apply for time on other facilities with open proposal processes. NRC-HIA is a leading developer of instrumentation for ground and space-based telescopes (e.g., ALMA, CFHT, Gemini, JCMT, JWST, TMT), and Fellows are welcome to participate in development or commissioning of new instruments.

Applicants must have acquired their Ph.D. within the last five years or expect to obtain the degree before taking up the Fellowship in fall 2011. Applications should be made by 1 November 2010, via the process described at the URL provided.

NRC is an equal opportunity employer.

Vous pouvez obtenir ces renseignements en français au site web indiqué ci-haut.

No. 26654 (New)
Southern Cosmology Survey-University of KwaZulu-Natal Postdoctoral Fellowship
UNIVERSITY OF KWAZULU-NATAL
University Road
Westville
Durban, KwaZulu-Natal 4001
South Africa
Tel: +27-31-2602543
FAX: +27-31-2607806
URL1: http://www.acru.ukzn.ac.za/ (Astrophysics and Cosmology Research Unit)
URL2: http://www.physics.princeton.edu/act (Atacama Cosmology Telescope)
URL3: http://www.salt.ac.za/ (Southern African Large Telescope)
Email Submission Address: moodleyk41@ukzn.ac.za
Email Inquiries: moodleyk41@ukzn.ac.za

Attention: Kavilan Moodley, Dr
We invite applications for a postdoctoral research associate position in observational or theoretical cosmology at the Astrophysics and Cosmology Research Unit at the University of KwaZulu-Natal. This position forms part of a multi-institutional postdoctoral program coordinated through the NSF Partnership for International Research and Education (PIRE).

We seek exceptional candidates with proposed research programs based on SZE data from the Atacama Cosmology Telescope ( http://www.physics.princeton.edu/act ), optical data from SALT ( http://www.salt.ac.za ) and other ground-based telescopes with a scientific focus on fundamental cosmology, related theoretical or observational studies of galaxy formation and evolution of galaxy clusters, or combined science from the millimeter and optical data. Possible projects include experimental and theoretical work on the CMB, secondary CMB effects, clusters of galaxies, galaxy evolution, stellar populations at high redshift, and weak lensing. Further, there will be a very strong collaboration with our US and Chilean (Universidad Catolica) partners in the PIRE program. Extended visits to US partners (Princeton University, University of Pennsylvania, Rutgers University) will be supported and strongly encouraged. There will be significant funds for travel.

Appointments are for two years, renewable to three years based on satisfactory performance. Starting dates between January 1, 2011 and March 1, 2011 are preferred. Applicants should e-mail a curriculum vitae, bibliography and statement of research interests to Kavilan Moodley (moodleyk41@ukzn.ac.za), and arrange to have three letters of recommendation e-mailed to the above address, by October 15, 2010. For more information visit http://www.acru.ukzn.ac.za/ and for further inquiries please contact Kavilan Moodley.

No. 26656 (New)
Postdoctoral Research Fellows and Associates in the Star and Planet Formation department (Reference number 10-13)
MAX-PLANCK-INSTITUTE FOR ASTRONOMY
Koenigstuhl 17
Heidelberg, Baden-Wuerttemberg D - 69117
Heidelberg
Tel: +49 6221 528201
FAX: +49 6221 528339
URL1: www.mpia.de
Email Submission Address: janssen@mpia.de

Attention: Maria Janssen-Bennynck
The Max-Planck Institute for Astronomy (MPIA) in Heidelberg is seeking a number of ambitious, highly qualified post-doctoral researchers to work in any of the following areas: formation of planetary systems, search and characterization of brown dwarfs and extrasolar planets, observational and theoretical studies of the earliest phases of low- and high-mass star formation, and extragalactic (resolved) star formation. Two or more positions will be available.

The “Star and Planet Formation” department at MPIA is pursuing a wide range of astrophysical re-search along these lines, encompassing large observing programs, instrument development and theoretical modelling (see http://www.mpia.de for details). A number of exciting new research oppor-tunities are available to MPIA, including the PanSTARRS1 Survey, imaging and spectroscopy at the Large Binocular Telescope (LBT), and guaranteed time programs with the HERSCHEL mission. In addition, the successful candidates will have access to the 2.2 and 3.5 m telescopes on Calar Alto, to the Very Large Telescope, the Very Large Telescope Interferometer facility, and the APEX sub-millimeter telescope in Chile. MPIA astronomers also extensively use the 2.2 m MPG telescope on La Silla and the IRAM facilities.

Applicants should have a PhD in astronomy, astrophysics, or a closely related field. The appointment will be for an initial period of two years with a likely extension to three years and MPIA provides funds for publications, travel, etc. The available positions range from independent work within the broad research direction of the “Star and Planet Formation” department to more project-oriented positions.

Interested candidates should send application materials, including curriculum vitae, and a brief state-ment of research interests to the address below by December 1st, 2010. They should also arrange for three letters of reference to be sent directly to that address by the same date.

Max Planck Institute for Astronomy Attn. Maria Janssen-Bennynck (Ref. No. 10-13) Koenigstuhl 17 69117 Heidelberg, Germany

Email submission: janssen@mpia.de Tel: +49-6221-528-201 Fax: +49-6221-528-339

The Max Planck Society is an equal opportunity employer. Applications from women and historically under-represented groups are particularly welcome. The MPIA supports its employees in their search for suitable child care institutions.

No. 26657 (New)
Postdoctoral Positions
INSTITUTE OF ASTRONOMY AND ASTROPHYSICS, ACADEMIA SINICA
PO Box 23-141
Taipei, Taiwan 106
ROC
Tel: +886-2-23665300
FAX: +886-2-23677849
URL1: http://www.asiaa.sinica.edu.tw/jobopening/ (On-Line Submission Form)
URL2: http://www.asiaa.sinica.edu.tw/ (ASIAA)
URL3: http://www.sinica.edu.tw/ (Academia Sinica)
Email Inquiries: asiaa@asiaa.sinica.edu.tw

Attention: Dr. Paul Ho, Director
The Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) has several openings for postdoctoral positions. Candidates with a PhD in any area of theoretical, observational, or instrumental astronomy are invited to apply.

ASIAA is an institute of Academia Sinica, the national research organization of Taiwan. The Institute has approximately 182 staff members (including 34 Faculty, 6 visiting scholars, 32 Postdocs, 30 Engineers/Technicians, and 30 Graduate Students). Areas of research include: the Solar System, Star Formation, Stellar Evolution, Astrochemistry, Galactic Dynamics, Active Galaxies, Galaxy Evolution, Cosmology, and Instrumentation Developments. We are partners in the SMA project, and have joined the ALMA project through collaborations with Japan and North America. We participate in instrumentation development on the CFHT and Subaru Telescope. We have observing time on the CFHT and participate in the Hyper Suprime-Cam survey on the Subaru Telescope. The TAOS project is in operation on Lulin Mountain in Taiwan to conduct a survey for small objects beyond Neptune. The AMiBA is in full scientific operation on Mauna Loa for the study of the CMB anisotropy and clusters of galaxies through the Sunyaev-Zel'dovich effect. Theoretical and computational astrophysics is being pursued both in ASIAA/TIARA in Taipei and TIARA in Hsinchu in collaboration with National Tsing-Hua University. A new initiative at TIARA aims to develop numerical simulators to bridge ALMA observations and theories in fluid dynamics, chemistry, and radiative transfer. A newly formed VLBI group investigates super massive black holes with sub-millimeter and space VLBIs through international collaborations. More information on each topic can be found in our Home page.

We seek scientists who actively participate in the Institute's projects, in particular: (1) optical/IR or radio astronomers to pursue research topics related to Institute interests; (2) astronomers with radio interferometry experience to participate in ongoing tests/software-development and scientific observations with the SMA, AMiBA, ALMA, or VLBI; (3) solar system and planetary astronomers to participate in the study of small objects beyond Neptune through TAOS; (4) scientists and engineers to participate in instrumentation development for Optical/IR telescopes and radio telescopes; or (5) scientists with backgrounds in astrophysics or planetary sciences to pursue topics in theoretical astrophysics, computational fluid dynamics, or MHD. More information on target areas of postdoc recruitment can be found at http://www.asiaa.sinica.edu.tw/jobopening/

The postdoc appointments at ASIAA will initially be for two years, with possible extension for additional two years based on satisfactory performance.

Applicants should submit on-line at http://www.asiaa.sinica.edu.tw/jobopening/ (1) a curriculum vitae, (2) a brief summary of past research or instrumentation experience, and (3) a future research plan.

Applicants are also requested to arrange three letters of recommendation to be sent to: Email: asiaa@asiaa.sinica.edu.tw, or the above address. Applications submitted before or on 15 December 2010 will receive full consideration.

No. 26659 (New)
Postdoctoral Research Associate in Theoretical/Computational Star Formation
THE UNIVERSITY OF WESTERN ONTARIO
1151 Richmond Street
Department of Physics and Astronomy
London, Ontario N6A 3K7
Canada
Tel: 519-661-2111 ext 86438
FAX: 519-661-2033
URL1: http://www.physics.uwo.ca/people/jobs.html
Email Submission Address: jodi@uwo.ca
Email Inquiries: jodi@uwo.ca

Attention: Jodi Guthrie, Chair's Assistant
Applications are invited for a postdoctoral fellowship at The University of Western Ontario to study star and planet formation. This position is advertised in conjunction with the CITA National Fellowship program. The successful candidate will work with Prof. Shantanu Basu to perform numerical simulations and theoretical modeling of the formation and evolution of star-disk systems. Candidates with suitable experience in these areas will be given special consideration. Current and future projects in the group may include the study of non-ideal MHD effects in fragmentation, collapse, and disk evolution, the study of the formation of multiple systems, including possibly giant planets, and the analysis of observations in order to make useful comparisons with theoretical models.

The Astronomy Group at Western has recently expanded, with eleven faculty members focusing on AGN's, nearby galaxies, planetary science, star formation, and stellar astronomy. A postdoctoral fellow can expect to have lively interactions with faculty, several other pdfs, and a growing group of graduate students. Researchers at Western have access to the computational resources of SHARCNET, a multi-institution regional supercomputer consortium.

The position is for two years, with possible renewal for a third year subject to performance and availability of funds. Interested individuals should send a curriculum vita and a statement of research interests, and arrange for three letters of reference to be sent to Jodi Guthrie (jodi@uwo.ca) at the above address. Complete (preferably electronic) applications must be received by October 22, 2010.

The University of Western Ontario is committed to employment equity.

No. 26661 (New)
Research Fellowship in Solar/Stellar Flares
QUEENS UNIVERSITY BELFAST
Belfast, Northern Ireland BT7 1NN
UK
Tel:
URL1: http://www.qub.ac.uk/sites/QUBJobVacancies/ResearchJobs/
Email Inquiries: M.Mathioudakis@qub.ac.uk

Attention: The Director of Human Resources
Applications are invited for a 3-year Postdoctoral Research Fellowship position, funded by the Leverhulme Trust, in the physics of solar and stellar flares. The post is located within the Astrophysics Research Centre (ARC) of the School of Mathematics and Physics.

The successful candidate will work on a project within the Solar and Cool Star Physics Group in ARC involving high time resolution observations of both the solar atmosphere and those of other cool stars. This Group makes extensive use of a wide range of solar and astronomical satellites and ground-based telescopes, with current activities focused on the study of oscillatory and transitory phenomena in solar and stellar atmospheres. Recently, we have built and commissioned the Rapid Oscillations in the Solar Atmosphere (ROSA) imaging system that can observe the solar atmosphere in as many as 6 wavelengths simultaneously, and with a cadence of up to 200 Hz. ROSA is currently at the National Solar Observatory in New Mexico USA. The Group makes extensive use of image reconstruction techniques for the analysis of ground-based solar observations from ROSA and other instruments. In addition, the Group uses the ULTRACAM instrument for high cadence observations of cool star atmospheres.

Applicants must have a PhD in a relevant subject either awarded or submitted by the time of taking up the post. Experience is essential in either (i) the reduction and analysis of solar and/or cool star observations from satellite-borne or ground-based instruments, or (ii) the development of theoretical models of solar and/or cool star atmospheres. Also essential are experience with the IDL computing environment, and a reasonable number of high quality publications commensurate with stage of career.

Post reference 10/101468.

No. 26662 (New)
Research Fellow in Solar/Stellar Flares
QUEENS UNIVERSITY BELFAST
Belfast, Northern Ireland BT7 1NN
UK
Tel:
URL1: http://www.qub.ac.uk/sites/QUBJobVacancies/ResearchJobs/
Email Inquiries: M.Mathioudakis@qub.ac.uk

Attention: The Director of Human Resources
Applications are invited for a 3-year Postdoctoral Research Fellowship position, funded by the Leverhulme Trust, in the physics of solar and stellar flares. The post is located within the Astrophysics Research Centre (ARC) of the School of Mathematics and Physics.

Post reference 10/101468.

No. 26663 (New)
Three Post Doctoral Fellowships in Extragalactic Astronomy and Cosmology
INSTITUTE FOR ASTRONOMY, UNIVERSITY OF EDINBURGH
University of Edinburgh
Royal Observatory
Edinburgh, Midlothian EH9 3HJ
UK
Tel: +44 131 668 8374
FAX: +44 131 668 8416
Email Submission Address: nohd@roe.ac.uk
Email Inquiries: jap@roe.ac.uk

Attention: Ms Nathalie Dupin
Applications are invited for Post Doctoral Fellowships to work at the Institute for Astronomy (IfA), Royal Observatory Edinburgh, in the area of Extragalactic Astronomy and Cosmology. Our research strengths include testing cosmological models using large-scale structure and gravitational lensing; observations of high-redshift galaxies and active galaxies; modeling of the intergalactic medium; stellar populations in nearby galaxies. Appointments are possible in any of these areas, although we expect that at least one of the positions will be in the area of testing cosmological models.

We are looking for international-quality applicants to join the current research staff at the IfA (11 Academics; 22 postdocs; 26 postgraduates). The successful candidates will become members of the Pan-STARRS Science Consortium, and will have full access to data from that survey. There is also the possibility of involvement in our other major projects, such as GAMA; Herschel; SCUBA2; GAIA; JWST.

The posts are available immediately. Two of the appointments will be for 2 years in the first instance, funded through the IfA's STFC rolling grant, with the possibility of extension. We expect in addition to be able to offer a third position for a fixed term of approximately 18 months. The salary scale is GB£29853 - GB£35646 (or GB£38951 subject to performance).

Informal enquiries should be made to Professor John Peacock (jap@roe.ac.uk). Applications must be made online at https://www.jobs.ed.ac.uk/ quoting reference 3013243.

Letters of reference from 3 referees should be sent directly to Ms Nathalie Dupin (nohd@roe.ac.uk), to arrive by the closing date.

No. 26665 (New)
Carnegie-Princeton Postdoctoral Fellowship
CARNEGIE OBSERVATORIES
Tel:
Email Submission Address: www.obs.carnegiescience.edu/fellowships
Email Inquiries: c-pfellow@obs.carnegiescience.edu

Attention: John Mulchaey
The Observatories of the Carnegie Institution of Washington and the Department of Astrophysical Sciences of Princeton University invite applications for a four-year postdoctoral fellowship in astronomy, to begin in September, 2011. The Fellow is expected to work two years at the main offices of the Observatories in Pasadena and two years at Princeton, in an order to be negotiated by the applicant. The Carnegie-Princeton Fellow is expected to carry out original research in any area of astronomy or astrophysics, either independently or in collaboration with staff, faculty or students at the host institutions. The principal selection criteria will be outstanding research accomplishments and promise of future achievement, although preference will be given to researchers working in those areas in which Carnegie and Princeton have active research interests.

The Fellow will have access to all of the resources and facilities of both institutions. In particular, Carnegie operates the Las Campanas Observatory in Chile, which includes the twin 6.5-meter Magellan telescopes, the 2.5-meter Dupont and 1.0-meter Swope telescopes, and provides an excellent environment for observational astrophysics and cosmology. The Department of Astrophysical Sciences at Princeton is a major partner in the Apache Point Observatory, the Sloan Digital Sky Survey, the Wilkinson Microwave Anisotropy Probe, the Atacama Cosmology Telescope, and the Large Synoptic Survey Telescope, and is collaborating with the Japanese astronomical community on large surveys with the Subaru Telescope. Together with research groups in the Physics Department and the nearby Institute for Advanced Study, the department offers an unparalleled environment for research in theoretical astrophysics and cosmology. The fellowship provides support for observing, travel, computing and publications, and the observing facilities will be accessible for the entire duration of the fellowship.

Further information on the host institutions is available at http://www.obs.carnegiescience.edu/ and http://www.astro.princeton.edu .

Applicants should send a curriculum vitae, bibliography, and research plan to BOTH the Observatories and to Princeton via the web at http://www.obs.carnegiescience.edu/fellowships/ AND http://jobs.princeton.edu by November 15, 2010. The research plan should address how the applicant intends to use the resources and facilities available at both host institutions. Selection of the successful candidate will be made by a joint Carnegie-Princeton committee. All applicants will automatically be considered for all postdoctoral positions in the Astrophysical Sciences department at Princeton and for the Carnegie Fellowship at The Observatories; however, they should clearly state in the cover letter that they wish to be considered for the Carnegie-Princeton Fellowship.

Applicants must also arrange for three letters of reference to be submitted to BOTH Carnegie Observatories via e-mail (c-pfellow@obs.carnegiescience.edu) AND Princeton University via the online application. The Carnegie Institution of Washington is an Equal Opportunity Employer. Princeton University is an Equal Opportunity Employer and complies with applicable EEO and Affirmative Action regulations.

For questions or additional information, please send email to c-pfellow@obs.carnegiescience.edu and/or postapp11@astro.princeton.edu . For additional information on the fellowship program at Carnegie, please visit: http://www.obs.carnegiescience.edu/fellowships . For information about voluntary self-identification, please link to: http://www.princeton.edu/dof/about_us/dof_job_openings

No. 26666 (New)
Carnegie Postdoctoral Research Fellowship in Astronomy
CARNEGIE OBSERVATORIES
Tel:
Email Submission Address: www.obs.carnegiescience.edu/fellowships/
Email Inquiries: cfellow@obs.carnegiescience.edu

Attention: John Mulchaey
Carnegie Postdoctoral Research Fellowship in Astronomy THE CARNEGIE OBSERVATORIES 813 Santa Barbara St. Pasadena, CA 91101 Email Inquiries: cfellow@obs.carnegiescience.edu Submission URL: http://www.obs.carnegiescience.edu/fellowships

Attention: Dr. John Mulchaey, Chair, Fellowship Committee

We invite applications for The Carnegie Fellowship at the Carnegie Observatories in Pasadena, California, to begin September 2011.

The fellowship is intended to encourage long-term research in observational or theoretical astronomy and/or instrumentation. We are particularly interested in applicants who have received their Ph.D. degree within the past three years. Fellowships are awarded for one year and may be renewed for two additional years. The successful applicant must have completed the Ph.D. requirements before assuming the fellowship.

Carnegie observing facilities include the two 6.5-meter Magellan telescopes, the 2.5-meter du Pont telescope and the Swope 1.0-meter telescope all at Las Campanas, Chile. Fellows will have access to these facilities on the same basis as the scientific staff. The Carnegie Fellowship provides ample support for observing, travel, computing, and publications.

The application should include a curriculum vitae, bibliography, a brief essay describing the applicant's current research, and a research proposal based on the facilities available at the Observatories. These materials must be submitted via the web to http://www.obs.carnegiescience.edu/fellowships/ by November 15, 2010.

In addition, applicants should arrange for three letters of reference to be emailed to cfellow@obs.carnegiescience.edu by the deadline.

E-mail inquiries may be sent to Dr. John Mulchaey at cfellow@obs.carnegiescience.edu.

All applications for the Carnegie-Princeton fellowship will also be considered for this fellowship. It is not necessary to submit a separate application.

The Carnegie Institution of Washington is an Equal Opportunity Employer.

No. 26667 (New)
Postdoctoral Research Fellow in Theoretical Astrophysics
UNIVERSITY OF MICHIGAN
Tel:
URL1: http://www.astro.lsa.umich.edu/~mateuszr
Email Submission Address: mateuszr@umich.edu
Email Inquiries: mateuszr@umich.edu

Attention: Prof. Mateusz Ruszkowski
The Department of Astronomy at the University of Michigan in Ann Arbor is seeking to hire a postdoctoral research fellow to work with Prof. Mateusz Ruszkowski on topics broadly related to gas dynamics, magnetohydrodynamics and cosmic rays in the context of the physics of AGN feedback, galaxies, galaxy clusters, and structure formation. Candidates with interest in these topics are particularly encouraged to apply.

Candidates must hold a Ph.D. in Astrophysics or equivalent field. Background in computational astrophysics and computer science is highly desirable but not required. A successful candidate will have access to a new and dedicated 384-processor cluster owned by the department.

Salary will be commensurate with qualifications and experience. The position will initially be for one year and may be extended up to three years, depending on satisfactory performance and availability of funding.

Qualified applicants should send their resume, publication list and a statement of research interests, and arrange for three letters of reference to be sent to the above address. Review of applications will begin on December 1, 2010 and continue until the position is filled.

The University of Michigan is an Affirmative Action/Equal Opportunity Employer. Women and members of minority groups are encouraged to apply.

No. 26671 (New)
Research Associate in Theoretical and Observational Astrochemistry
UNIVERSITY COLLEGE LONDON
Tel:
URL1: http://www.ucl.ac.uk/hr/jobs/ (Application process)
URL2: http://www.star.ucl.ac.uk (Group Page)
Email Inquiries: sv@star.ucl.ac.uk

Attention: http://www.ucl.ac.uk/hr/jobs/
UCL, Physics and Astronomy Salary (inclusive of London allowance) £31,778 per annum

Duties and Responsibilities:

The postholder will work in the group of Dr Serena Viti in the Physics and Astronomy Department at UCL. The main aim of the post is to implement theoretical and experimental results on the formation and destruction of glycolaldehyde (a basic sugar) into astrochemical models of star forming regions. The post holder will also be involved in observational programmes aimed at detecting glycolaldehyde in a range of star forming regions. This post is part of a newly funded project to investigate glycolaldehyde formation, desorption and destruction using experimental, theoretical, astrochemical modelling and observational techniques. The post is funded by a grant from the Leverhulme Trust, and the work will be performed in collaboration with Dr Wendy Brown and Dr Ben Slater (Chemistry). The post will be for 2.5 years.

Start date 1st January 2011 or as soon as possible thereafter.

Key Requirements:

The successful candidate should have a PhD degree or equivalent in Astrophysics or a related discipline. Experience in astrochemical or radiative transfer modeling and some observational sub-mm astronomy is essential.

Further Details:

For informal inquiries, please contact Dr S. Viti - Email:

sv@star.ucl.ac.uk

Applications should be made online via this website:

http://www.ucl.ac.uk/hr/jobs/

Please select "Click Here for UCL Current Vacancies", then enter the job reference number 1153288 into "Ref No". Please register and complete the application procedure as directed, also providing a statement of research and a CV with list of publications. References from three referees should be directly emailed to Dr Viti (sv@star.ucl.ac.uk) by the deadline.

UCL Taking Action for Equality

No. 26674 (New)
UT Austin Prize Postdoctoral Fellowship
UNIVERSITY OF TEXAS AT AUSTIN
Department of Astronomy
One University Station, C1400
Austin, TX 78712
U.S.A.
Tel: (512) 471-3000
FAX: (512) 471-6016
Email Submission Address: s.stone@astro.as.utexas.edu

Attention: Shelley Stone, Administrative Associate
The University of Texas Department of Astronomy, along with McDonald Observatory, invites invitations for The U.T. Austin Prize Postdoctoral Fellowship. We will make one appointment to an outstanding researcher broadly interested in observational extragalactic astronomy who has received his or her PhD by November 2011.

The Fellowship will be taken at UT Austin, which is also the location of the new Texas Cosmology Center. The research facilities include the 9.2-m Hobby-Eberly Telescope, the 2.7-m Harlan J. Smith Telescope, the 2.1-m Otto Struve Telescope, and the 0.8-m wide-field imaging telescope. Access to the robotic ROTSE and MONET telescopes is also available, and McDonald Observatory supports a program in millimeter wavelength research with the Caltech Submillimeter Observatory on Mauna Kea. U.T. Austin is also a member of the Giant Magellan Telescope (GMT) consortium.

The candidate will be free to conduct an independent research program. The fellowship has a three year tenure, with an initial 1 year appointment that will be renewed with satisfactory performance. The salary and research budget are highly competitive.

Applicants should submit a CV, a statement of proposed research to be conducted at UT Austin during the Fellowship, and letters of recommendation from at least three scientists familiar with the applicant's research to Shelley Stone at s.stone@astro.as.utexas.edu by December 1, 2010.

No. 26675 (New)
Leo Goldberg Fellowship
NATIONAL OPTICAL ASTRONOMY OBSERVATORY
PO Box 26732
Tucson, AZ 85726-6732
USA
Tel: 520-318-8116
FAX: 520-318-8456
URL1: http://www.noao.edu/staffdir/staff-research.php (NOAO Staff and Research)
URL2: http://www.noao.edu/goldberg (Past Goldberg Fellows)
URL3: http://www.noao.edu/dir/lrplan/2010-noao-lrp.pdf (NOAO Long-Range Plan: FY 2010-2014)
Email Submission Address: hrnoao@noao.edu
Email Inquiries: najita@noao.edu

Attention: Leo Goldberg Fellowship - Job #980
LEO GOLDBERG FELLOWSHIP

The National Optical Astronomy Observatory (NOAO) will award the Leo Goldberg Fellowship in observational astronomy, astronomical instrumentation, or theoretical astrophysics, to recent Ph.D. recipients of outstanding promise. These Fellowships are intended to advance innovative and groundbreaking scientific research, to encourage long-term projects, and to engage talented individuals in the mission that NOAO undertakes on behalf of the community. The Fellow will have access to the wide range of resources at NOAO, including the telescopes of the International Gemini Observatory, Kitt Peak National Observatory and Cerro Tololo Inter-American Observatory. In addition to engaging in any research program of their own choosing, the Fellow is encouraged to participate in current NOAO activities (e.g., ongoing NOAO instrumentation, survey programs, or the scientific and/or technical aspects of the ground-based System of facilities). These include the Large Synoptic Survey Telescope (LSST), the Gemini Telescopes, and the Dark Energy Survey, projects in which NOAO is playing an important role on behalf of the community.

The Fellowship provides support for five years at a competitive salary, and it carries a benefit package and a generous research budget for travel and other expenses. During the first four years of the appointment, the candidate will reside at either NOAO/North in Tucson, Arizona, or NOAO/South in La Serena, Chile. Residence in Chile has an additional benefits package to further support and assist expatriates and their families. During the fifth year, the Fellow may reside at any US University or astronomical research institute willing to host the Fellow.

The unique 5-yr time span of the Goldberg Fellowship provides an opportunity to carry out ambitious, long-term projects, and we strongly encourage candidates to consider this aspect in their applications. Fellows will be selected based on (1) Their promise for an outstanding career in astronomy; (2) Their proposed use of Gemini, KPNO, CTIO, and other open access facilities; (3) The relationship of their research to and proposed interaction with NOAO programs to develop community facilities, and (4) The relationship of their research to programs conducted by the NOAO staff ( http://www.noao.edu/staffdir/staff-research.php ). For further information, please contact Dr. Joan Najita (najita@noao.edu). Information on past Goldberg Fellows is available at http://www.noao.edu/goldberg .

Applicants are required to submit: (1) A description of their proposed research, addressing in particular the timeline for the project within the five year duration of the Fellowship; (2) A choice of residence at NOAO/North or NOAO/South, including a discussion of possible interactions with on-going NOAO research programs and next-generation developmental programs (see http://www.noao.edu/dir/lrplan/2010-noao-lrp.pdf for details); (3) A vita, bibliography, and brief description of their current research; (4) Three letters of recommendation. Applications will be reviewed beginning November 8, 2010 and applicants are encouraged to submit all materials by this date to receive full consideration.

Women and candidates from underrepresented minorities are particularly encouraged to apply. We are an affirmative and equal opportunity employer.

Please submit your application electronically to: hrnoao@noao.edu (or) by mail to: NOAO Human Resources Office Attn: Leo Goldberg Fellowship Committee, Job #980, P. O. Box 26732 Tucson, AZ 85726-6732

No. 26676 (New)
4 Year Postdoctoral Position: mm-wave science and support
CONICYT
Bernarda Morín 551, 3er Floor
Providencia
Santiago, 0 0
Chile
Tel: 56 2 365 4441
FAX: 56 2 435 4353
URL1: www.conicyt.cl
URL2: www.conicyt.cl/astronomia
Email Inquiries: postdoc_alma@conicyt.cl

Attention: María Elena Díaz, 4 Year Postdoctoral Position: mm-wave science and support
The Chilean Comision Nacional de Investigación Científica y Tecnologica (National Commision for Scientific and Technological Research) CONICYT, invites applications for a 4 year postdoctoral fellowship position. The postdoc will form the nucleus of the Chilean ALMA ARC (ALMA Regional Center.

The requirements are a Ph.D. degree, a willingness to support ALMA and APEX users in Chile, and a demonstrated ability to excellence in research. The position is for a period of 4 years, extendable by one year depending on performance. While the position is open to all fields, previous experience with interferometry and mm-wave astronomy is expected, The postdoc is expected to spend 70% of his/her time onsupport duties and the remaining 30% on independent research associated to a Chilean University. He/she will support Chilean users on ALMA (proposal and observingpreparation, technical evaluation, data processing support) and APEX (proposal evaluation and observing support).The specific functions are similar to those of astronomers working in an ALMA ARC. More details can be obtained from www.conicyt.cl/astronomia/

The selected candidate will have access to the Chilean 10% share of all international observatory telescope time in Chile, including ALMA, APEX, ASTE, VLT, Gemini, and Magellan. Note that the postdoc period is expected to start around the ALMA Early Science call for proposals.

Salary is up to US$50,000 per year, depending on seniority. Benefits include an annual health insurance allowance and a US$5,000 annual budget for travel and operational expenses.Expenses for support-related travel will be paid by CONICYT.

Proposal materials - in english - should be sent as a single pdf file to postdoc-alma@conicyt.cl and must include a cover letter (max. 2 pages), CV, list of publications inthe last five years, and a description of the candidates proposed research(max. 2 pages). In addition, three letters of reference should be sent directly to the same email address. The deadline for proposal receipt is 15 October 16:00 hours.

No. 26677 (New)
Postdoctoral Position in Computational Astrophysics
UNIVERSITY OF NOTRE DAME
225 Nieuwland Science Hall
Notre Dame, IN 46556
USA
Tel: (574) 631-9639
FAX: (
Email Submission Address: dbalsara@nd.edu
Email Inquiries: dbalsara@nd.edu

Attention: D. S. Balsara, Prof.
The Computational Astrophysics group at the Univ. of Notre Dame invites applications for a postdoctoral position in computational astrophysics. The group is actively involved in a large number of extremely interesting computational projects in a wide variety of astrophysical fields. A general interest in the areas of star and planet formation, interstellar medium, turbulence, supernovae, accretion disc physics, compact objects, jets, outflows etc. is desirable, but strong applicants from any area will be considered. Applicants with an interest in star and/or planet formation or ISM turbulence are especially encouraged to apply. Prior experience in carrying out astrophysical simulations would be an asset because the projects do involve high performance computation. Knowledge of object-oriented programming either in F90 or C++ is also desirable. The group has access to large supercomputers at the university and national level. The projects are all science-oriented and the positions would give the successful applicant an excellent opportunity to work at the cutting edge of computational astrophysics. The intellectual environment at Notre Dame as well as the scientific projects are very stimulating and the remuneration is competitive.

Applicants should send a CV, list of publications and a statement of research interests to the above-mentioned address. Applicants should also arrange for three letters of recommendation to be sent to Prof. Balsara. Applications may be submitted electronically. We will start considering completed applications by Dec. 1, 2010 but applications received thereafter will also be considered.

No. 26679 (New)
AAO / Macquarie University Postdoctoral Research Fellow -- Formation and Evolution of Nearby Galaxies
AUSTRALIAN ASTRONOMICAL OBSERVATORY (AAO) / MACQUARIE UNIVERSITY
Tel:
URL1: http://www.aao.gov.au/local/www/jobs/
URL2: http://www.innovation.gov.au/careercentre
Email Submission Address: jobs@aao.gov.au
Email Inquiries: zucker@aao.gov.au or ahopkins@aao.gov.au

Attention: Dr Daniel Zucker and A. Prof. Andrew Hopkins
AAO / Macquarie University Postdoctoral Research Fellow

The Australian Astronomical Observatory (AAO) and Macquarie University wish to appoint a highly motivated Research Fellow in the general area of the Formation and Evolution of Nearby Galaxies. This research position, suitable for a recent PhD graduate, is a joint appointment between the Australian Astronomical Observatory and Macquarie University; the two institutions are located close to each other in Sydney, Australia, a lively, culturally-diverse city with a pleasant climate and a high standard of living. The successful candidate will interact with the staff of the AAO and the staff and students of the rapidly-growing Astronomy and Astrophysics group at Macquarie University. The position is initially for 2 years, with a possibility of further extension subject to performance and external funding.

The Research Fellow will conduct their own research program in the general area of the Formation and Evolution of Nearby Galaxies – that is, the galaxies in the Local Group and the Local Volume, including the Milky Way itself. This research will be carried out independently as well as in collaboration with Dr Daniel Zucker and the other members of the Astronomy group at the AAO and the Astronomy and Astrophysics CORE (Centre of Research Excellence) at Macquarie University. The Research Fellow will have 67% of their time available for research. They will be expected to assist in the operations of the AAO for the remaining 33% of their time. Such duties may include observing support at the AAT, and other roles required by the Astronomy group to ensure the continued smooth running of the Observatory.

The excellent facilities of the Australian Astronomical Observatory and other telescopes open to Australian astronomers (including Gemini and Magellan) are available for use in the research component of the role. The Observatory comprises the 3.9-metre Anglo-Australian Telescope (AAT) and the 1.2-metre UK Schmidt Telescope near Coonabarabran, NSW, and a laboratory in Epping, in the suburbs of Sydney. The AAO also hosts the Australian Gemini Office. There is a scientific staff of 14 highly active and productive astronomers at the AAO, most of whom are based in Epping, next to the headquarters of the Australia Telescope National Facility (ATNF), which operates Australia's radio telescopes.

Macquarie University, a dynamic research and teaching institution, is located on a park-like campus in close proximity to the headquarters of the AAO and ATNF. The Astronomy and Astrophysics group – within the Macquarie Department of Physics and Astronomy – has undergone a rapid expansion in the past 5 years, now comprising over 35 faculty, postdoctoral researchers and students (see www.astronomy.mq.edu.au), making it one of the largest and most active astronomy groups within Australia. In addition to the successful candidate for this position, four additional Australian Research Council-funded postdoctoral Super Science Fellows will be joining the group over the next 12-16 months.

Candidates must have a strong background in astronomy, astrophysics or a related branch of experimental physics. Expertise with or an interest in existing AAO instrumentation is desirable, as is an interest in the development, commissioning and subsequent scientific use of HERMES, the next AAT instrument, scheduled for 2012. HERMES is a high-resolution spectrograph fed by 400 fibres, for which the main science drivers are large stellar surveys to study the formation of the Galaxy and its closest companions.

The position is located on the Epping campus, and is a 2-year appointment, subject to the satisfactory completion of a 6-month probation period. The salary will be in the range of $66761 - $71153 p.a. (AAO level 4.1 to 4.3), depending on the experience of the candidate, plus employer superannuation contributions and annual leave loading. A fixed relocation allowance plus other relocation expenses (including airfare to Australia and return on completion of the appointment) may also be paid for applicants from outside the Sydney area.

To apply for this position you will need to obtain the employment information package which is available from our website http://www.aao.gov.au/local/www/jobs/ or by contacting the AAO personnel officer Rajni Prasad on +61 2 9372 4863. All applications should be sent electronically to jobs@aao.gov.au.

Applications must include all of the following:- * A curriculum vitae outlining career history, education and qualifications, awards and distinctions. * Full list of publications, separated into (a) accepted papers in refereed journals and (b) conference proceedings and other publications. Please do not include papers or preprints with your application. * A statement addressing the selection criteria. Each criterion must be addressed explicitly. * A one page outline of current research interests and a two page proposal for the research program to be carried out at the AAO / Macquarie University. * Contact details, including e-mail and phone, of three referees. It is the applicant’s responsibility to ensure that reference letters arrive by the closing date for applications.

The Australian Astronomical Observatory supports flexible working arrangements, including part-time positions where appropriate, and is an equal opportunity employer

No. 26680 (New)
Chamberlain Fellowship
LAWRENCE BERKELEY NATIONAL LABORATORY
Berkeley, CA 94720
Tel:
URL1: http://www.jobclub.com/banman/a.aspx?ZoneID=0&BannerID=488&AdvertiserID=33&CampaignID=1786&Task=Click&SiteID=1&RandomNumber=296584

Attention: Chamberlain-Fellow2010
Chamberlain Fellowship at Lawrence Berkeley National Laboratory

The Lawrence Berkeley National Laboratory's Physics Division invites outstanding recent Ph.D. recipients to apply for the Owen Chamberlain Fellowship in experimental particle physics and cosmology. Students who expect to receive their Ph.D. degree by the spring of 2011 are also invited to apply.

The Chamberlain Fellow is appointed for three years, with a two year extension possible. The Chamberlain Fellow is given time to review the Division's research program, and participate in any aspect of it, subject to funding limitations. He/she may also pursue new initiatives within experimental particle physics or cosmology subject to approval by the division director. In addition to salary, the Chamberlain Fellow receives a $5,000 annual research supplement.

For information on the LBNL Physics Division's research program, please consult http://www.lbl.gov/LBL-Programs/physics/

This Fellowship honors Berkeley Nobelist Owen Chamberlain, who (with Emilio Segre,Clyde Wiegand, and Thomas Ypsilantis) discovered the antiproton at the Berkeley Bevatron in 1955.

Apply online at http://www.jobclub.com/banman/a.aspx?ZoneID=0&BannerID=488&AdvertiserID=33&CampaignID=1786&Task=Click&SiteID=1&RandomNumber=296584 and follow the on-line instructions to complete the application process. As part of the online application process, please submit a single attachment that includes your resume or CV, statement of your research interests and publication list. Please be sure to reference where you found out about the position.

In addition you must arrange to have at least three letters of reference and copies of your resume or CV, statement of research Interests and publication list sent via email to: Chamberlain-Fellow2010@lbl.gov by November 1, 2010. Refer to Job Number 24803 in the subject line.

Berkeley Lab is an affirmative action/equal opportunity employer committed to the development of a diverse workforce.

No. 26682 (New)
Postdocotral Positions
PRINCETON UNIVERSITY
Tel:
URL1: https://jobs.princeton.edu (Web submission)
URL2: http://www.princeton.edu/astro/ (Department website)
Email Inquiries: postapp11@astro.princeton.edu

Attention: Web submissions only: https://jobs.princeton.edu
The Department of Astrophysical Sciences, Princeton University, anticipates offering a number of postdoctoral and more senior positions in theory, observation and instrumentation, including (but not limited to): the Lyman Spitzer, Jr. Postdoctoral Fellowship in Astrophysics, the Henry Norris Russell Postdoctoral Fellowship in Astrophysics, the Joint Postdoctoral Fellowship with Carnegie Observatories and Princeton University, positions in cosmology, supernova theory, protoplanetary disks, and a software scientist position to work on large-scale surveys. We encourage applications from those working in all areas of astronomy and related fields.

Princeton astronomers with whom the successful applicants may work with faculty and research staff including Neta Bahcall (large-scale structure, clusters of galaxies), David Bowen (UV astronomer) Adam Burrows (supernovae, planetary and stellar atmospheres), Renyue Cen (cosmological simulations), Christopher Chyba (solar system), Bruce Draine (interstellar medium), Jeremy Goodman (gamma-ray bursts, accretion disks), J. Richard Gott (cosmology, general relativity), James Gunn (galaxies, instrumentation), Ed Jenkins (UV astronomy, interstellar medium), Russell Kulsrud (plasma astrophysics), Jill Knapp (interstellar medium, radio astronomy), Robert Lupton (image processing, astronomical surveys), Rachel Mandelbaum (gravitational lensing), Jeremiah P. Ostriker (galaxies, cosmology), Roman Rafikov (planet formation and dynamics), David Spergel (cosmology, extrasolar planets), Anatoly Spitkovsky (neutron stars, high-energy astrophysics), James Stone (MHD, star formation), Michael Strauss (extragalactic astronomy, surveys) and Ed Turner (extrasolar planets, gravitational lensing), as well asabout 20 postdoctoral fellows and associate research scholars. There are also strong research groups in the Physics, Geosciences, and Mechanical and Aerospace Engineering Departments and at the nearby Institute for Advanced Study with interests in astrophysics.

For details on specific positions, see http://www.princeton.edu/astro/resources/job/jo/index.xml . Applicants should apply via the web at: http://jobs.princeton.edu . The application should include curriculum vitae, bibliography, a description of past research and future plans, and contact information for three references.

All applications received by November 15, 2010 will be fully considered, but applications will continue to be accepted until the positions are filled. Only web submissions will be considered. All applications will be considered for all postdoctoral positions available in the department, but you will be asked in the application form which positions you are interested in. Princeton University is an equal opportunity employer and complies with applicable EEO and affirmative action regulations.

No. 26685 (New)
Science Fellow
GEMINI OBSERVATORY
Tel:
FAX: 877-571-2008
URL1: http://www.gemini.edu
Email Submission Address: gemini-job@gemini.edu
Email Inquiries: gemini-jobs@gemini.edu

Attention: Human Resource
Gemini Science Fellow

Gemini has an opening for a Gemini Science Fellow at Gemini South in La Serena, Chile. Gemini Science Fellows acquire significant training and experience in large ground-based telescope operations—becoming proficient both in state-of-the-art astronomical instrumentation and research, and in the techniques of modern, queue-based observing methods, pioneered by Gemini Observatory.

Science Fellows at Gemini are actively involved in personal research projects. Forty percent (40%) of the Fellow’s time is available for independent astronomical research, supported by a personal research budget. In addition, a fraction of the time available on both Gemini telescopes is reserved for successful peer-reviewed staff proposals.

Gemini Science Fellows currently spend approximately 15 to 20 nights per semester executing observations on the telescope utilizing any of the three or more active instruments. The number of nights spent observing is subject to change and may decrease in the future. Fellows also support investigators in the community in preparing their observations; and employ queue planning tools to construct nightly observing plans from a large database of potential observations. Science Fellows have the opportunity to become intimately involved in instrumentation projects, data analysis tools, or other observatory development projects, depending on their interests.

The next few years will see the implementation of significant and exciting new capabilities at Gemini South, including a near-IR multi-object spectrograph and imager (Flamingos-2), a laser guide star multi-conjugate adaptive optics system and high resolution imager (GeMS) and later the Gemini Planet Imager. More information about present and future instrumentation at Gemini South can be found on the Gemini web pages.

Gemini offers an attractive and competitive salary and benefit package. The duration of Fellow positions is three years, with a possible two-year extension. The majority of the successful applicants’ time is spent at the base facility. The Gemini South base facility is located in La Serena, Chile, a popular beach town with a mild climate, modern amenities, and a substantial international astronomical community supporting four nearby observatories.

Requirements: Ph.D. in astronomy, physics or related discipline. Significant optical and/or infrared observational, data analysis and/or instrumentation experience is highly desirable. Experience and/or knowledge in one or more of the following areas is a plus: optical and near-infrared multi-object and IFU spectroscopy; near and mid infrared imaging; adaptive optics and high spatial resolution imaging.

Must be safety conscious; possess or be able to obtain a valid passport; willing and able to travel internationally; possess a valid driver's license with a good driving record; and be able to drive 4WD vehicles. Applicants must be able to work nights at the altitude of the Cerro Pachon summit, 2900 m.

The Gemini Observatory is a partnership of seven countries: the USA, UK, Canada, Australia, Argentina, Brazil and Chile, conducting forefront astronomical research with 8-m optical/infrared telescopes in Hawaii and Chile.

Send resume, cover letter relating your experience and education to the duties of the position, statement of research, and a statement of Observatory support interests. Arrange to have letters from three professional references sent to application address below. Please include the AAS Job Register number in your cover letter. Applications will be considered as they are received and all applications received by October 15, 2010 will receive full consideration. Starting dates are negotiable but are expected to be between February 2011 and October 2011.

Further information on Gemini can be found at: http://www.gemini.edu . Application materials should be submitted to gemini-jobs@gemini.edu or the mailing address listed above. AA/EOE

No. 26688 (New)
NORDITA Fellowships
NORDITA
Tel:
URL1: http://www.nordita.org/ (Nordita home page)
URL2: http://apps.nordita.org/ (application web form; required)
Email Inquiries: brandenb@nordita.org

Attention: larus@nordita.org
NORDITA FELLOWSHIPS 2011 - 2013

NORDITA, the Nordic Institute for Theoretical Physics in Stockholm, Sweden, invites applications for post-doctoral fellowships in theoretical physics. The deadline for applications is November 15, 2010. Appointments are for two years starting September 1, 2011 or some other date to be agreed upon.

NORDITA was founded in 1957 in Copenhagen, Denmark, but was relocated to the AlbaNova University Center in Stockholm in January 2007 where it is jointly hosted by Stockholm University and the Royal Institute of Technology (KTH). Research at NORDITA covers a wide range of modern theoretical physics including astrophysics and astrobiology, atomic physics, biological physics, condensed matter physics, gravitation and cosmology, high-energy physics, nuclear physics, and statistical physics. The research activity of the local academic staff is supplemented by NORDITA Scientific Programs, which bring together groups of leading experts to work on specific topics for extended periods. There is also ample opportunity for collaboration with faculty and research staff at local universities. Further information about NORDITA can be found at http://www.nordita.org

The fellowships are primarily intended for scientists who have a recent PhD and wish to carry out research in fields represented at NORDITA. Candidates working in other areas will be considered when it is scientifically justified.

The deadline for applications is November 15, 2010. Only online applications will be accepted. The application procedure is posted on http://apps.nordita.org

No. 26689 (New)
Post-doc Positions in Astrophysical Dynamos
NORDITA
Tel:
URL1: http://www.nordita.org/~brandenb/AstroDyn/ (project page)
URL2: http://apps.nordita.org/ (application web form; required)
Email Inquiries: anne@kth.se

Attention: brandenb@nordita.org
Post-doc Position in Astrophysical Dynamos at Nordita NORDITA - The Nordic Institute for Theoretical Physics

In connection with a 5-year project on Astrophysical Dynamos/, there is a vacancy for a 2-year post-doc position at the Nordic Institute for Theoretical Physics (Nordita) in Stockholm. The project is supported through an Advanced Grant of the European Research Council to improve our understanding of astrophysical dynamos. For details, see the project page http://www.nordita.org/~brandenb/AstroDyn/ on Astrophysical Dynamos.

The group consists of 4 PhD students, 4 post-docs, one assistant professor, one or two visiting professors, and Axel Brandenburg as PI. The research in the group focuses on improving our understanding of the solar dynamo.

Qualifications: Eligible for the post-doc positions are applicants with a PhD completed not earlier than five years before the application deadline.

Employment: The positions are supported by a post-doc stipend for a period of 2 years. The position will start on September 1, 2011, or some other date agreed upon.

Application: The applications should include a curriculum vitae together with a list of publications, 2 letters of recommendation, as well as a research plan. The application deadline is December 1, 2010, and applications must be filed though our web interface http://apps.nordita.org/ .

No. 26691 (New)
Grainger Postdoctoral Fellowship
UNIVERSITY OF WISCONSIN-MADISON
Astronomy Department
475 N. Charter Street
Madison, WI 53706
USA
Tel: 608 262 2965
FAX: 608 263 6386
URL1: http://www.astro.wisc.edu/ (Department of Astronomy, University of Wisconsin-Madison)
Email Submission Address: angela@astro.wisc.edu
Email Inquiries: sstanimi@astro.wisc.edu (Prof. Snezana Stanimirovic)

Attention: Grainger Search Committee (c/o Angela Normington)
The Department of Astronomy at the University of Wisconsin - Madison announces the newly-initiated Grainger Postdoctoral Fellowship. The Fellowship provides opportunities for outstanding independent postdoctoral research on problems that are broadly related to the scientific interests of the department. The current departmental areas of expertise include observational, experimental and theoretical research in: stellar astrophysics and star formation, the interstellar and intergalactic media, extragalactic astrophysics, cosmology, plasma astrophysics, high energy astrophysics, and astronomical instrumentation.

The successful applicant will join the vibrant astronomy community at the University of Wisconsin and is expected to reside in Madison, WI. The Department has a 26% share of the WIYN (Wisconsin-Indiana-Yale-NOAO) 3.5m and 0.9m telescopes on Kitt Peak and a 15% share of the 11m Southern African Large Telescope (SALT) in South Africa.

The duration of the fellowship is up to three years including an initial appointment of one year, and two annual renewals contingent on satisfactory performance. The annual stipend is approximately $60,000 plus benefits, with an additional allowance of $10,000 per year for travel and other research costs. The program is open to applicants of all nationalities who have earned a PhD in astronomy, astrophysics, or a closely related discipline by October 1 2011. The exact start date is negotiable.

Applications should include a curriculum vitae, bibliography, and statement of research interests and plans (limited to four pages, including figures and references). Applicants should arrange for 3 letters of recommendation to be sent to Grainger Search Committee (c/o Angela Normington), Department of Astronomy, University of Wisconsin, 475 N. Charter Street, Madison, WI 53706. Material can be sent electronically to graingerpostdoc@astro.wisc.edu .

Applications received by December 1, 2010 are guaranteed full consideration.

The University of Wisconsin-Madison is an affirmative action/equal opportunity employer. Women and minorities are encouraged to apply. Finalists cannot be guaranteed confidentiality.

No. 26692 (New)
Postdoctoral Fellowships and Research Fellowships in Cosmic Magnetic Fields
THE UNIVERSITY OF SYDNEY
K06 - 1-3 Ross Street
Sydney, NSW 2006
Australia
Tel: +61 2 8627 1218
URL1: http://sydney.edu.au/positions/ (Submit applications online; use reference number 2234/0710)
URL2: http://sydney.edu.au/science/physics/sifa/possum (POSSUM project)
URL3: http://sydney.edu.au/science/physics/~bmg/ (Prof Bryan Gaensler's WWW page)
Email Submission Address: fabrice.noel@sydney.edu.au
Email Inquiries: fabrice.noel@sydney.edu.au

Attention: Fabrice Noel, Principal Recruitment Consultant
The Sydney Institute for Astronomy (SIfA) within the School of Physics at The University of Sydney is seeking to appoint two researchers to work on scientific and technical problems related to the Polarization Sky Survey of the Universe's Magnetism ("POSSUM"), a wide-field radio polarization and Faraday rotation experiment to be undertaken on the Australian Square Kilometre Array Pathfinder (ASKAP).

The positions are full-time fixed-term for up to five years, and are funded as part of Professor Bryan Gaensler's Australian Laureate Fellowship.

This is an exciting opportunity to contribute to the success of the POSSUM project via the development of relevant simulations, software and data products, and to simultaneously lead a self-directed research program in areas relevant to the POSSUM survey. People with skills in any of the following areas are encouraged to apply:

* Radio polarimetry and Faraday rotation * Cosmological simulations of magnetic fields * Simulations of radio source populations * Polarization of radio galaxies and of active galactic nuclei * Calibration of wide-field aperture synthesis data * Ionospheric Faraday rotation and ionospheric calibration * Software pipelines and source finding * Astronomical data catalogs and large redshift surveys * Magnetic fields in the Milky Way, galaxies, clusters and the intergalactic medium

Successful candidates will be part of a strong and dynamic research group working on a variety of activities related to wide-field surveys in radio and optical astronomy. Appointees will also have the opportunity to co-supervise undergraduate and postgraduate students, and to apply for additional research funding through the competitive grant schemes of the Australian Research Council.

Prospective candidates are encouraged to contact Bryan Gaensler, bryan.gaensler@sydney.edu.au , for additional information before applying. All applications must be submitted via The University of Sydney careers website. Visit http://sydney.edu.au/positions and search for reference number 2234/0710 .

No. 26693 (New)
Postdoctoral posion in Plasma/High Energy Astrophysics or Astronomical Polarimetry
KAVLI INSTITUTE OF ASTRONOMY AND ASTROPHYSICS
Peking University
Hai Dian District
Beijing, Beijing 100871
China
Tel: (86) 10-62755605
FAX: (86) 10-62767900
URL1: http://kiaa.pku.edu.cn/~hryan/postdoc.html
Email Submission Address: hryan@pku.edu.cn
Email Inquiries: hryan@pku.edu.cn

Attention: Huirong Yan
Applications are invited for a postdoctoral position based in the Kavli Institute for Astronomy and Astrophysics (KIAA) at Peking University. The successful applicant will work on projects of mutual interests with Prof. Huirong Yan and her collaborators. Applicants with expertise on MHD simulations, plasma processes or polarimetry observations are particularly encouraged to apply.

The Institute is designed to be a forum for global scientific exchange and a training centre for international postdocs and students. KIAA organizes a variety of academic activities and programs to stimulate research and promote interdisciplinary interactions. The working language of KIAA is English and there is a broad mix of international faculty and postdocs. The successful candidate will be given a research budget and have the opportunities for international collaborations.

The appointment will be for two years with a possible extension to the third year upon successful performance. The possible starting date can be as soon as January 2011, though alternative dates can be considered as well.

Salary and compensation depends on qualifications and experience. Applicants should submit a curriculum vitae, list of publications, a 1-2 page statement of current and future research interests, and arrange for three letters of recommendation to be sent directly to hryan@pku.edu.cn. Applications received before Oct 31th will receive full consideration, but consideration of applications will proceed until the suitable candidate is found.

No. 26694 (New)
Super Science Fellow
AUSTRALIAN NATIONAL UNIVERSITY, RESEARCH SCHOOL OF ASTRONOMY AND ASTROPHYSICS
Mount Stromlo Observatory
Cotter Road, Weston
Canberra, ACT 2615
Australia
Tel: +61 2 61256861
FAX: +61 2 6125 9510
URL1: http://info.anu.edu.au/hr/Jobs/Current_Vacancies (Full application submission details)
URL2: http://info.anu.edu.au/hr/Jobs (Information on application procedures)
URL3: http://rsaa.anu.edu.au/ (Home page, Research School of Astronomy and Astrophysics)
Email Inquiries: Gary.DaCosta@anu.edu.au

Attention: Michelle McWilliam, HR Consultant
The Research School of Astronomy and Astrophysics of the Australian National University, located at Mt Stromlo Observatory, seeks to appoint TWO highly motivated Super Science Fellows to pursue vigorous full-time research programs related to the physical and chemical properties of ultra-faint dwarf galaxy satellites of the Milky Way. The Super Science Fellows will work with the leaders of the ultra-faint dwarf satellites Super Science team (Da Costa, Jerjen, Kobayashi, Norris) and will have access to national observing facilities in Australia (AAT) and overseas (Gemini, Magellan), and to first-rate computing facilities. The research Programs of the Fellows can be either observational or theoretical in context.

The Super Science Fellowships are funded for 3 years and each carries with it research support funds of AUD$20,000 per year. The positions are available from 1 July 2011 and are open to candidates with preferably a maximum of 3 years postdoctoral experience.

Applications must be submitted through the Australian National University jobs site at http://info.anu.edu.au/hr/Jobs (under current vacancies, academic positions, Reference No. A389-10TG). Candidates should include in their application a CV, list of publications, research program outline, and a description of relevant experience such as in astronomical imaging, photometry, and spectroscopy, or with appropriate modeling codes. Applicants should also include the names and email addresses of 3 referees who have agreed to send letters of reference supporting the application. Applications and letters of reference must be received by 1 December 2010.

Questions can be addressed to Professor Gary Da Costa, telephone +61 2 61258913 or email Gary.DaCosta@anu.edu.au

No. 26695 (New)
Johannes Kepler Postdoctoral Program in Astrophysics
UNIVERSITY OF VIENNA
Tuerkenschanzstr. 17
Vienna, A 1180
Austria
Tel: +43 1 4277 53814
FAX: +43 1 4277 9518
URL1: http://astro.univie.ac.at/ (Department home page)
Email Submission Address: manuel.guedel@univie.ac.at
Email Inquiries: manuel.guedel@univie.ac.at

Attention: Manuel Guedel, Professor
The University of Vienna announces the opening of its newly established Johannes Kepler Postdoctoral Program in Astrophysics. Johannes Kepler positions will be awarded to outstanding postdoctoral scientists demonstrating a high research profile in observational, numerical, or theoretical astrophysics in areas covered at the Department of Astronomy in Vienna. Kepler postdocs will carry out their independent research programs, but are strongly encouraged to engage in collaborations within the Department. A modest level of teaching is expected.

The present announcement is for a position dedicated preferentially to the area of galactic star formation and pre-main sequence stars, including research on protoplanetary disks and planet formation, but excellent candidates in other fields of the Department's research will also be considered. Johannes Kepler positions are awarded for four years. Funds are made available to support travel expenses and conference participation.

The Kepler postdoc will have access to all observatories of ESO and ESA; for numerical work, two in-house clusters and, for high-performance computing, the Vienna Scientific Cluster will be accessible. The institute provides a lively research environment including approx. 70 staff members, postdocs, and PhD students. There are many opportunities to interact within ongoing or planned instrument projects for example related to Plato, Spica, or ESO observatories.

Applications include a CV, a publication list, a summary of past research (max 2 pages) and an outline of the proposed research program for the duration of the employment (max. 4 pages). These documents must be submitted electronically as a PDF file to the above address or via http://jobcenter.univie.ac.at/en/applications/ .

Review starts 10 October 2010 but applications submitted thereafter will be fully considered until the post is filled. Applicants should arrange for three letters of reference sent by the referees directly to the same address. Future announcements will be made upon availability of positions. Female candidates are especially encouraged to apply.

The Johannes Kepler Postdoctoral Program in Astrophysics at the University of Vienna is managed by the board of professors at the Department of Astronomy. For inquiries, contact Prof. M. Guedel ( manuel.guedel@univie.ac.at).

No. 26698 (New)
Event Horizon Telescope Postdoctoral Position
MIT HAYSTACK OBSERVATORY
Off Route 40
Westford, MA 01886
USA
Tel: 781 981 5400
FAX: 781 981 0590
URL1: http://www.haystack.mit.edu/
Email Submission Address: job@haystack.mit.edu
Email Inquiries: sdoeleman@haystack.mit.edu

Attention: Alan Blackburn, Assistant to the Director
The MIT Haystack Observatory invites applications for a postdoctoral position within the Observatory's Event Horizon Telescope (EHT) program. The EHT is a network of (sub)mm wavelength facilities forming a Very Long Baseline Interferometry (VLBI) array with angular resolutions of 20 micro arcseconds. At wavelengths of 1.3mm, the EHT can probe emission at the innermost accretion regions surrounding several nearby super massive black holes. The EHT has already resolved Event Horizon scale structures in SgrA*, the 4 million solar mass black hole at the Galactic Center. Ongoing technical efforts within the program include extension to 0.8mm wavelength, enabling polarimetric observations, and work on instrumental developments to increase array sensitivity such as new high-speed VLBI recorders and phased array technology. Planned observations in 2011 will include contemporaneous xray, NIR and 1.3mm VLBI of SgrA* with a goal of resolving time variable activity near the Event Horizon. The postdoc will have opportunities to work with some of the highest angular resolution data ever obtained, contribute to efforts aimed at testing GR with new EHT observations, and develop new instrumentation.

Independent research is encouraged, as are interactions with astrophysics groups on the MIT campus and the Harvard-Smithsonian Center for Astrophysics in Cambridge. Applicants with experience in interferometry, software development and instrumentation (including FPGA/GPU experience) are encouraged to apply. Candidates with relevant experience and interest in modeling and simulating black holes on Event Horizon scales are also encouraged to apply.

Haystack Observatory is an MIT interdisciplinary research center situated on 1300 acres of forested land, 35 miles northwest of the MIT campus. The salary is competitive and appointments will initially be for two years, with possible extension to a third year.

Applications consisting of CV, research statement and the names of three references should be sent to (job@haystack.mit.edu).

No. 26699 (New)
Beatrice Watson Parrent Postdoctoral Fellowship - ID#10441
RESEARCH CORPORATION OF THE UNIVERSITY OF HAWAII
2530 Dole Street
Sakamaki Hall D-100
Honolulu, Hawaii 96822
United States
Tel: 808-956-3100
FAX: 808-956-5022
URL1: www.rcuh.com

Attention: Recruitment
Institute for Astronomy, University of Hawaii

CLOSING DATE: 12/30/10

The Institute for Astronomy (IfA) at the University of Hawaii (UH) invites applications for the Beatrice Watson Parrent Postdoctoral Fellowship. We seek researchers displaying significant promise in any field of astrophysics or solar physics, including observation, theory, and instrumentation. The term of the fellowship is for up to 3 years, starting around Fall 2011. The IfA has guaranteed access to the entire suite of observational facilities on the summits of Mauna Kea and Haleakala. The IfA is also the lead institution in the Pan-STARRS-1 wide-field optical telescope, which is carrying out a multi-year synoptic survey mission. More information is available at http://www.ifa.hawaii.edu .

The successful candidate will undertake a program of independent research and participate in the academic and scientific life of the IfA. Applicants should demonstrate outstanding promise as a researcher, as reflected by research and letters of recommendation, and should have completed a Ph.D. in astronomy, physics, or equivalent areas by the start date of employment. The Fellow will be provided an annual salary of approximately $62,500, a research budget of $15,000/year, and assistancewith relocation expenses to Hawaii. The Fellow will also be able to apply for UH telescope time and have access to the Pan-STARRS-1 survey data.

APPLICATION REQUIREMENTS: The preferred method of applying for a job is through our on-line application process. Please go to www.rcuh.com, click on “Employment” and navigate to “Job Announcements/Apply for a Job.” However, if you prefer, you may apply by submitting a curriculum vitae, including a list of publications; cover letter including Recruitment ID#, referral source, and narrative of your qualifications for position and current CV; statement of current and future research interests; and copy of degree(s)/transcripts/certificate(s) to confirm your credentials, by fax (808) 956-5022, mail, or hand-deliver to: Director of Human Resources, Research Corporation of the University of Hawaii, 2530 Dole Street, Sakamaki Hall D-100, Honolulu, HI 96822 before the closing date. Online applications and faxed documents must be submitted/received by the closing date (11:59 P.M. Hawaii Standard Time/RCUH receipt time). Mailed documents must be postmarked by the closing date. Hand-delivered documents must be received by our HR office by 4 P.M. Hawaii Standard Time/RCUH receipt time. If you have questions on the application process and/or need assistance, please call (808)956-3100. EEO/AA Employer.

Please also arrange to have three letters of reference sent confidentially to the same address by the closing date.

INQUIRIES: Dr. Rolf-Peter Kudritzki, Director, 808-956-8566, kud@ifa.hawaii.edu, or Dr. Michael Liu, 808-956-6666, mliu@ifa.hawaii.edu.

No. 26703 (New)
Cosmic Microwave Background Group Postdoctoral Fellow
HARVARD UNIVERSITY
60 Garden Street, MS-42
Cambridge, MA 02138
USA
Tel: 617-495-7331
FAX: 617-495-7345
Email Submission Address: sblock@cfa.harvard.edu

Attention: Sarah Block, Technical Secretary
Postdoctoral fellow in the Harvard Cosmic Microwave Background Group: our group seeks highly qualified applicants for one or more postdoctoral positions with the Keck Array and other ongoing CMB polarization projects. The selected postdoc will work closely with students and other members of the Keck Array team in support of deployments in the immediately coming season(s) and analysis of project data. Applicants must have received a Ph.D. in physics or astronomy or proof that all requirements have been met for their Ph.D. A background which includes experience in integration, testing, and field-deployment of complex microwave instrumentation is particularly sought. Demonstrated proficiency in analysis and simulation of complex data sets while working within a team setting is also desirable. The selected postdoc may also have opportunity to contribute to other CMB projects in our group, including the BICEP2 and POLAR-1 telescopes. These projects are supported by the National Science Foundation.

Appointments are for 1 year, with renewal for a second and third year likely, contingent upon satisfactory progress and funding. The starting date will be between 10/1/10 and 11/1/10, depending on the applicant's availability. Harvard University is an Equal Opportunity/Affirmative Action Employer where all qualified applicants receive consideration for employment without regard to race, creed, color, sex or national origin.

No. 26705 (New)
Assistant Professor/Post Doc Fellow - Physics/
UNIVERSITY OF MICHIGAN
Tel:
URL1: http://www.rackham.umich.edu/sof
Email Submission Address: society.of.fellows@umich.edu

Attention: Linda Elise Turner
The Michigan Society of Fellows invites applications from qualified candidates for three-year fellowships at the University of Michigan.

Candidates should be near the beginning of their professional careers. Those selected for fellowships must have received the Ph.D. degree between June 1, 2008, and September 1, 2011. Fellows are appointed as Assistant Professors or Research Scientists in appropriate departments and as Postdoctoral Scholars in the Michigan Society of Fellows. They are expected to be in residence in Ann Arbor during the academic years of the fellowship, to teach for the equivalent of one academic year, to participate in the informal intellectual life of the Society, and to devote time to their independent research or artistic projects. This is not an artist-in-residence program but rather an opportunity to develop one’s work in conversation with fellows from a range of disciplines during the three years of the fellowship. Applications from degree candidates and recipients of the Ph.D. or comparable artistic or professional degree from the University of Michigan will not be considered.

Applications will be reviewed by Society members and University faculty. Final selections will be made in late January by Senior Fellows of the Society. Eight Fellows will be selected for three-year terms to begin September 1, 2011. The annual stipend will be $51,500.

The online application is available at: http://www.rackham.umich.edu/sof

No. 26709 (New)
Covington Fellowship
NATIONAL RESEARCH COUNCIL OF CANADA - HERZBERG INSTITUTE OF ASTROPHYSICS (NRC-HIA)
717 White Lake Road
Penticton, BC V2A 6J9
Canada
Tel: 250-497-2316
FAX: 250-497-2317
URL1: http://www.nrc-cnrc.gc.ca/eng/ibp/hia/fellowship/covington/index.html
Email Submission Address: covington@nrc-cnrc.gc.ca
Email Inquiries: covington@nrc-cnrc.gc.ca

Attention: Competition 40-10-24, COVINGTON FELLOWSHIP, National Research Council of Canada (NRC)
The NRC-HIA invites applications for the Covington Fellowship, tenable at the DRAO in Penticton, BC. The fellowship is awarded to an outstanding recent doctoral graduate in radio astrophysics to enable independent research in the stimulating and collegial environment of NRC-HIA.

The award is for a maximum of three years; the initial appointment of two years may be extended for one further year (subject to performance and availability of funds). Fellows will receive support for research-related travel and journal page charges, and have access to professionally managed computer systems. The Fellowship also offers a highly competitive benefits and salary package.

NRC-HIA DRAO staff are currently engaged in a number of large radio surveys, such as the Canadian Galactic Plane Survey and the Planck Deep Field Survey using the telescopes at DRAO, the GALFACTS survey at Arecibo, and the CORNISH survey at the Very Large Array (VLA), but are also major users of radio telescopes around the world, including the VLA, VLBA, GBT, MERLIN, EVN, ATCA, LBA, Parkes and Arecibo. DRAO also carries out world-leading research and development of instrumentation and systems for radio telescopes, specifically the Expanded Very Large Array (EVLA), the Australia Square Kilometre Array Pathfinder (ASKAP), and the Square Kilometre Array (SKA). Fellows are welcome to participate in any of these projects.

Applicants must have acquired their PhD within the last five years or expect to obtain the degree before starting the Fellowship in Fall 2011. Application should be made by 1 November 2010, via the process described at the URL provided. For further information about the facilities and research programmes at DRAO, please contact sean.dougherty@nrc-cnrc.gc.ca.

NRC is an equal opportunity employer.

Vous pouvez obtenir ces renseignements en français au http://www.nrc-cnrc.gc.ca/fra/idp/iha/bourse/covington/index.html

No. 26544
ESA Postdoctoral Fellowships in Space Science
EUROPEAN SPACE AGENCY
Keplerlaan 1
Noordwijk, ZH 2200 AG
Netherlands
Tel:
FAX: 31 71 565 5452
URL1: http://www.rssd.esa.int/fellowship
Email Submission Address: temp.htr@esa.int
Email Inquiries: fellowship@rssd.esa.int

Attention: Fellowship Programme, Human Resources Division
The European Space Agency awards several postdoctoral fellowships each year. The aim of these fellowships is to provide young scientists, holding a PhD or the equivalent degree, with the means of performing space science research in fields related to the ESA Science Programme. Areas of research include planetary science, astronomy and astrophysics, solar and solar-terrestrial science, plasma physics and fundamental physics. The fellowships have a duration of two years and are tenable at the European Space Research and Technology Centre (ESTEC) in Noordwijk, Netherlands, or at the European Space Astronomy Centre (ESAC) in Villafranca del Castillo, near Madrid, Spain.

Applications are now solicited for fellowships in space science to begin in the fall of 2011. Preference will be given to applications submitted by candidates within five years of receiving their PhD. Candidates not holding a PhD yet are encouraged to apply, but they must provide evidence of receiving their degree before starting the fellowship.

The deadline for applications is 1 October 2010.

More information on the ESA Research Fellowship programme in Space Science, on the conditions and eligibility, as well as the application form can be found on the world-wide web at this address: http://www.rssd.esa.int/fellowship

Questions on the scientific aspects of the ESA Fellowship Programme in Space Science not answered in the above pages can be sent by e-mail to the fellowship coordinator, Dr. Guido De Marchi, at the address fellowship@rssd.esa.int

No. 26545
Herschel postdoctoral position in extragalactic astronomy
LABORATOIRE D'ASTROPHYSIQUE DE MARSEILLE, FRANCE
38 rue F. Joliot-Curie
Marseille, France F13376
France
Tel:
Email Submission Address: Alessandro.Boselli@oamp.fr
Email Inquiries: Alessandro.Boselli@oamp.fr

Attention: Alessandro Boselli, Dr.
Applications are invited for a Postdoctoral Research Fellow position within the team "Physique des Galaxies" at Laboratoire d'Astrophysique de Marseille to work on Herschel Guaranteed and Open Time Key Projects devoted to extragalactic astronomy. The successful applicant will be involved with the reduction and analysis of photometric data obtained with the PACS and SPIRE instruments. She/He will be able to work on the following Herschel Guaranteed and Open Time Key Projects: the Herschel Reference Survey (HRS;Boselli et al. 2010, PASP, 122, 261) and the Herschel Virgo Cluster Survey (HeViCS;Davies et al. 2010, A&A Herschel Special Issue) with possible implications on several other Herschel key projects (HerMES, ATLAS, H-GOODS, VNGS, DGS).

Research experience in extragalactic studies with an emphasis on star-forming galaxies and infrared emission is desired. Experience with the reduction and photometric measurement of space-based data will be appreciated. Candidates should have obtained, by the starting date, a Ph.D. in Astronomy, Physics, Astrophysics, or equivalent.

The appointment is for two years. To apply, please send a resume, publication list, and statement of research to Alessandro.Boselli@oamp.fr and have three letters of reference forwarded to the same address. The deadline for applications is September, 30th 2010.

No. 26571
Postdoctoral Fellow - Smithsonian Astrophysical Observatory - Astronomy/Astrophysics
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
60 Garden Street
Mail Stop 15
Cambridge, MA 02138
USA
Tel:
URL1: http://www.cfa.harvard.edu
Email Submission Address: adupree@cfa.harvard.edu
Email Inquiries: adupree@cfa.harvard.edu

Attention: Dr. Andrea K. Dupree, Senior Astrophysicist
This postdoctoral fellow appointment centers around AO imaging of Kepler target fields containing possible exoplanets, and the photometric and spectroscopic study of cool stars to aid in the interpretation of Kepler photometry. Observations are made principally at the MMT Observatory located on Mt. Hopkins, Arizona.

NASA's Kepler mission was launched in March 2009, and is performing superbly. This position includes follow-up imaging observations of potential targets of interest. Travel to and observations at the MMT are necessary. Construction and application of appropriate reduction procedures form a critical part of this research. Observational experience in infrared imaging is necessary and experience with spectroscopy is desirable. A recent PhD degree in astronomy, astrophysics, or related fields is necessary. Good communication and presentation skills are needed. Opportunities for spectroscopic studies and analysis of clusters in the Kepler field of view are also possible during the appointment.

This position is funded for two years, with a third year extension possible. Candidates should send a letter of interest, CV, list of publications, and description of all experience in astronomical imaging, photometry, and spectroscopy, in addition to experience with astronomical software and computer languages. Please include the names and email addresses of 3 references who can be contacted with knowledge of your experience. Applications will be reviewed beginning August 15, 2010.

The position is based at the Harvard-Smithsonian Center for Astrophysics in Cambridge MA, a large, vibrant, active research center covering practically all fields of astronomy and astrophysics.

No. 26580
Illinois-Paris Fellow in Computational/Theoretical Cosmology and Large Scale Structure
UNIVERSITY OF ILLINOIS AT URBANA-CHAMPAIGN
Tel:
Email Inquiries: thorman@illinois.edu

Attention: Benjamin Wandelt, Professor
Illinois-Paris Fellow in Computational/Theoretical Cosmology and Large Scale Structure.

Starting as early as Fall 2010, there is an opportunity for a recent PhD in computational cosmology to work with Professor Ben Wandelt on developing new observables to probe the primordial perturbations and dark energy phenomenology using large scale structure surveys. The successful candidate will be an expert in setting up initial conditions for, running, and analyzing large scale structure simulations, as well as working with and writing codes for high-performance computing facilities such as NCSA. Skills in perturbation theory; semi-analytic modeling of structure formation; data analysis; and modern statistical methods are highly desirable for this position. The successful candidate would benefit from the world-class computational infrastructure and intellectual environment at the University of Illinois and close collaboration with Wandelt's group at the Paris Institute for Astrophysics (IAP) in France. Applications will be considered immediately and until the position is filled.

Applicants should go online to: https://my.physics.illinois.edu/join/ to complete and submit their application which must include a cover letter, curriculum vitae, list of publications, brief description of research interests, the name, address, and email address of three references, at your earliest convenience. Please contact Linda Thorman (thorman@illinois.edu or 217.333.1590) if you have any questions.

Illinois is an equal opportunity/affirmative action employer.

No. 26587
SMA Postdoctoral Fellowship
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
Tel:
URL1: http://www.cfa.harvard.edu/opportunities/fellowships/sma/ (SMA Postdoctoral Fellowship Overview and Application)
URL2: http://www.cfa.harvard.edu/sma/ (Submillimeter Array)
Email Inquiries: smapostdoc@cfa.harvard.edu

Attention: http://www.cfa.harvard.edu/opportunities/fellowships/sma
The Submillimeter Array (SMA), a collaborative project of the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics (Taiwan), consists of eight movable 6 meter diameter antennas that together combine to make uniquely detailed images in the submillimeter part of the spectrum, through atmospheric windows that open up on the high, dry summit of Mauna Kea, Hawaii. With collecting area comparable to the largest single dish submillimeter telescopes and baselines to 500 meters, the SMA is used for subarcsecond resolution studies of a wide range of astrophysical phenomena, including Solar System bodies, protoplanetary disks, star forming regions, evolved stars, supermassive black holes, and galaxies both nearby and at cosmological distances.

Applications are invited for SMA Postdoctoral Fellowships starting in fall 2011. These positions are aimed chiefly at research in submillimeter astronomy, and successful candidates will participate either in observations with the SMA or in their interpretation. Applicants must have a recent Ph.D. in astronomy or a related field. Practical experience in millimeter or submillimeter wavelength astronomy, radio interferometry, instrumentation, or experience in any applicable branch of astrophysical theory is desirable. Applicants may choose to be based either at the Harvard-Smithsonian Center for Astrophysics in Cambridge, MA or at the SMA facility on the campus of the University of Hawaii, Hilo, HI. Information and instructions for submitting applications can be found at http://www.cfa.harvard.edu/opportunities/fellowships/sma/ . Please direct questions to smapostdoc@cfa.harvard.edu .

Online applications are due November 30, 2010.

The Smithsonian Astrophysical Observatory is an Equal Opportunity/Affirmative Action Employer where all qualified applicants receive equal consideration for employment without regard to race, creed, color, sex or national origin.

No. 26595
Exoplanet Characterization
MAX PLANCK INSTITUTE FOR ASTRONOMY
Koenigstuhl 17
Germany
Tel: +1-617-495-7158
FAX: +1-617-496-0121
URL1: http://cfa-www.harvard.edu/~lkaltenegger (research Kaltenegger)
URL2: www.mpia.de (MPIA homepage)
URL3: http://www.mpg.de/english/careerOpportunities/jobOffers/extern/ (MPG job offers)
Email Submission Address: lkaltene@cfa.harvard.edu
Email Inquiries: lkaltene@cfa.harvard.edu

Attention: Lisa Kaltenegger
The Max-Planck Institute for Astronomy (MPIA) Heidelberg is seeking a number of highly motivated, qualified and curious postdoctoral researchers in the field of exoplanet characterization in the new cross-disciplinary group of Lisa Kaltenegger on one of the following areas: atmospheric chemistry of extrasolar planets, planetary interiors and outgassing, Super-Earth observations with ground- and space-based telescopes and theoretical studies of habitability and biomarkers. 2 or more positions will be available starting Oct 2010. Working language of the group is English.

Applicants should have a PhD in astronomy, planetary science, or a related field. The appointments will be for up to a total of 3 years. Opportunities for research visits at Harvard University/CfA are part of these appointments.

Candidates should send a pdf file containing their application materials, including CV, publication list and a brief statement of research interests to lkaleteneATcfa.harvard.edu by Sept. 15 2010. 3 letters of reference should be sent separately to the same e-mail address. Applications after Sept 15 will be considered until positions are filled. Positions are available staring October 2010 but may be delayed for up to 9 months for exceptional candidates.

The “Extrasolar Planet Characterization” group at MPIA is a cross-disciplinary endeavor, pursuing a wide range of astrophysical and planetary science research, encompassing observing programs, instrument development and theoretical modeling. Collaboration with other research groups at MPIA, e.g. Star and Planet Formation, imaging and spectroscopy at LBT/VLT, instrument development teams for ELT/JWST as well as planetary science research departments at the University of Heidelberg is encouraged.

No. 26596
Research Fellow in Galactic Center Group
UNIVERSITY OF CALIFORNIA LOS ANGELES
430 Portola Plaza
Box 951547
Los Angeles, CA 90095-1547
USA
Tel: 310-206-0420
FAX: 310-206-2096
URL1: www.astro.ucla.edu/~ghezgroup/gc (UCLA Galactic Center Research)
Email Submission Address: ghez@astro.ucla.edu
Email Inquiries: ghez@astro.ucla.edu

Attention: Andrea Ghez, Professor
Applications are invited for a Research Fellow position in UCLA's Galactic Center Group( http://www.astro.ucla.edu/~ghezgroup/gc ) to Fall 2010 or later.

The successful candidate will work with Prof. Andrea Ghez and her collaborators on high angular resolution imaging and spectroscopic observations with the Keck telescopes of the Galactic center to study how the supermassive black hole interacts with its environs and what role it plays in the formation and evolution of our Galaxy. The primary responsibilities will be to assist designing an experiment to detect the effects of relativity and dark matter on the orbits of short-period stars focusing both on work with current adaptive optics (AO) systems and trade-studies with future AO systems.

This position will be filled either at the postdoctoral level or a research scientist level depending on the experience of the candidates. Applicants must have (or will shortly satisfy the requirements for) a PhD degree in astronomy, astrophysics, or related disciplines. Experience with adaptive optics data, precision astrometry, and/or orbital modeling will be considered a plus.

Interested applicants should send a curriculum vitae, bibliography, three letters of reference and a brief statement of research interest to ghez@astro.ucla.edu. Deadline for receipt of application is 1 October 2010. For further information, please contact Prof. Andrea Ghez (ghez@astro.ucla.edu).

No. 26511
Postdoctoral Scholar in Anomalous Microwave Emission
CALIFORNIA INSTITUTE OF TECHNOLOGY
1200 E. California Blvd.
MS 220-6
Pasadena, CA 91125
USA
Tel:
Email Inquiries: paladini@ipac.caltech.edu

Attention: Dr. Roberta Paladini
Applications are invited for a Postdoctoral Scholar position at the Spitzer Science Center/California Institute of Technology to study the anomalous microwave emission with Dr. Roberta Paladini (SSC/IPAC).

Anomalous microwave emission (AME) is the least known among Galactic foregrounds for CMB experiments, and there exists an increasing amount of evidence that, in our Galaxy, this additional component of the interstellar medium (ISM) is ubiquitous. According to currently favored theories, such an excess of emission is due to rapidly rotating very small dust grains (spinning dust).

The postdoctoral scholar will investigate the dust properties of Galactic objects for which signatures of anomalous emission have been detected by CMB experiments (COSMOSOMAS, VSA, CBI, etc.). He/she will use, for this analysis, mainly Spitzer (IRAC/MIPS/IRS) and IRAS data, complemented by a wide range of ancillary data (HI, CO, radio, etc.). The candidate will carry out both data reduction and interpretation of the data using state-of-the-art dust models, and will have the possibility of interacting with Caltech theoretical groups working on spinning dust. Among his/her duties, he/she will write proposals for radio/IR ground-based/space (VLA, ATCA, MOPRA, Herschel, etc.) observing facilities.

Applicants who have research interests in anomalous microwave emission, foregrounds for CMB experiments, the ISM, as well as experience with Spitzer data are particularly encouraged to apply.

Experience with interferometric data will be considered a plus. The appointment is initially for one year, with the possibility of renewal for an additional year. The start date is no later than January 2011, although Fall 2010 will be strongly favored.

Interested applicants should send a curriculum vitae, bibliography, three letters of reference and a brief statement of research interests to the above address. Deadline for receipt of applications is 1 October 2010. For further information, please contact Dr. R. Paladini (paladini@ipac.caltech.edu). Caltech is an Affirmative Action/Equal Opportunity Employer. Women, Minorities, Veterans, and Disabled Persons are encouraged to apply.

No. 26117
Postdoctoral Fellowships in Astrophysics
NAVAL RESEARCH LAB
4555 Overlook Ave., SW
Washington, DC 20375
Tel: 202-767-0668
FAX: 202-404-8894
URL1: http://www.nrl.navy.mil/
Email Submission Address: Namir.Kassim@nrl.navy.mil
Email Inquiries: Namir.Kassim@nrl.navy.mil

Attention: Namir Kassim, Research Physicist
The Remote Sensing Division of the Naval Research Laboratory (NRL) ( http://www.nrl.navy.mil/ ) is seeking postdoctoral applications from those with an interest in radio astronomy. The successful candidate will be expected to carry out innovative research programs in

1. Any area of astrophysics where existing or planned low-frequency radio observations (e.g., with [E]VLA, VLBA, Arecibo, GMRT, GBT, LWA, LOFAR) may contribute, such as high-redshift radio galaxies, clusters of galaxies, supernova remnants and pulsars, studies of propagation effects, searches for extrasolar planets, or the solar system (e.g., Jupiter or the Sun);

2. Radio astronomy digital signal processing or radio frequency interference (RFI) mitigation techniques; or

3. Imaging and calibration algorithm development for the emerging suite of telescopes, including the Long Wavelength Array (LWA) and the EVLA.

NRL radio astronomers carry out a wide range of observational programs at the VLA, VLBA, and the GBT, with a primary focus on the 74 and 330 MHz VLA and 330 MHz VLBA systems. The NRL-NRAO 74 MHz VLA system, with its 35 km baselines, is the highest angular resolution, highest sensitivity, low-frequency radio interferometer in operation today. Observational programs, such as the VLA Low-frequency Sky Survey ( http://lwa.nrl.navy.mil/VLSS/ ) and 74 and 330 MHz Galactic center ( http://rsd-www.nrl.navy.mil/7213/lazio/GC/ ) observing programs are pursued both for their science and also to address challenges for future low-frequency interferometers. NRL is also part of the Southwest Consortium (SWC), a University-based consortium led by the University of New Mexico (UNM), that is developing the Long Wavelength Array (LWA) ( http://lwa.unm.edu/ ). The LWA will explore the relatively neglected frequency regime below 80 MHz, by capitalizing on breakthrough ionospheric calibration techniques that inally permit development of very low frequency arrays larger than ~ 5 km. The ~ 400-km diameter LWA will realize improvements in both angular resolution and sensitivity by at least 2--3 orders of magnitude. The LWA frequency range favors studies of non-thermal and coherent (both known and unknown) emission sources, unique absorption processes, and provides an intrinsic link to shock physics, high-energy phenomena, and the high-red-shift Universe.

Successful candidates are normally resident at NRL in Washington, DC, but the option exists for residency in New Mexico, proximate to the University of New Mexico's Long Wavelength Array program. Postdoctoral applications should be pursued through the National Research Council (NRC). NRL-NRC Associateships are awarded to persons who have held their doctorate for less than five years at the time the award is offered. Awards are for one year. Applicants will need to submit an original research proposal to be approved by the NRL-NRC advisor for subsequent evaluation by an external review panel chosen by the NRC. US citizenship or legal US permanent residency is required. Application materials can be obtained at http://www.nas.edu/rap . Deadlines for applications include February 1, May 1, and August 1. For further information contact Dr. Namir Kassim at the above address. EOE/AAE

No. 24972
NASA Postdoctoral Fellowships
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION (NASA)
Tel:
URL1: http://nasa.orau.org/postdoc/
Email Inquiries: nasapostdoc@orau.org

Attention:
The NASA Postdoctoral Program (NPP) offers unique research opportunities to highly talented national and international scientists and engineers to engage in ongoing NASA research in space science, earth science, aeronautics, space operations, exploration systems, and astrobiology.

Awards:

· Approximately 50 Fellowships awarded annually

· One-year appointments, renewable up to three years

· Annual stipends start at $50,000, with supplements for specific degree fields and high cost-of-living areas

· Annual travel budget of $8,000

· Financial assistance for relocation

· Financial supplement for health insurance purchased through the program

· Apply at http://nasa.orau.org/postdoc

Application Deadlines:

Three each year - March 1, July 1, and November 1

Eligibility:

· U.S. Citizen

· Foreign Nationals with a J-1 visa status as a research scholar, Lawful Permanent Resident (LPR) status, or Employment Authorization Document (EAD) with pending LPR status

· Recent and senior-level Ph.D. recipients

Locations of Fellowship Positions:

· Ames Research Center, Moffett Field, CA

· Dryden Flight Research Center, Edwards, CA

· Glenn Research Center, Cleveland, OH

· Goddard Space Flight Center, Greenbelt, MD

· Goddard Institute for Space Studies, New York, NY

· Jet Propulsion Laboratory, Pasadena, CA

· Johnson Space Center, Houston, TX

· Kennedy Space Center, Kennedy Space Center, FL

· Langley Research Center, Hampton, VA

· Marshall Space Flight Center, Huntsville, AL

· Stennis Space Center, Stennis Space Center, MS

· NASA Headquarters, Washington, DC

· Various locations associated with the NASA Astrobiology Institute

To obtain more information and to apply for this exciting opportunity, please visit the NPP Web site at http://nasa.orau.org/postdoc.

No. 26600 (New)
Several PhD fellowships in Astronomy and Astrophysics
INTERNATIONAL MAX PLANCK RESERACH SCHOOL FOR ASTRONOMY & COSMIC PHYSICS, HEIDELBERG
Koenigstuhl 17
Germany
Tel: +49-(0)6221-528-387
FAX: +49-(0)6221-528-339
URL1: http://www.mpia.de/imprs-hd
Email Submission Address: imprs-hd@mpia.de
Email Inquiries: imprs-hd@mpia.de

Attention: IMPRS Heidelberg
The "International Max Planck Research School for Astronomy and Cosmic Physics at the University of Heidelberg" (IMPRS-HD) invites applications for its PhD program.

The school aims to offer outstanding research and training opportunities with excellent instrumental, observational, and theoretical research facilities at the Max Planck Institute for Astronomy, the Max Planck Institute for Nuclear Physics, the Astronomisches Rechen-Institut,the Landessternwarte Koenigstuhl, the Institute of Theoretical Astrophysics, and the Heidelberg Institute for Theoretical Studies.

The main research topics carried out at these institutions are planet and star formation; exoplanets and substellar objects; astrometry; formation, evolution and dynamics of; active galactic nuclei and massive black holes; gravitational lensing; cosmology and structure formation; high energy astrophysics; search for non-baryonic dark matter; and state-of-the-art instrumentation for astronomy and astroparticle physics.

IMPRS-HD is an independent part of the Heidelberg Graduate School for Fundamental Physics.

The fellowships are available for up to 3 years on a scale of 1100 Euro monthly average net income.

Interested students are invited to apply by December 5, 2010 for the academic year starting in September 2011. An earlier start of the thesis research is welcome.

Applicants must have a Master's degree or Diploma (or equivalent) in Physics/Astronomy including a corresponding thesis and a very good physics background.

Further details on IMPRS-HD and the application procedure can be found on our web-site at: http://www.mpia.de/imprs-hd/

No. 26645 (New)
PhD in Astrophysics/Astronomy
INTERNATIONAL MAX-PLANCK RESEARCH SCHOOL ON ASTROPHYSICS MUNICH
Giessenbachstrasse 1
P.O. Box 1213
Garching/Munich, N7A 85741
Germany
Tel: +49(0)89 30000 3650
FAX: +49(0)89 30000 3655
URL1: www.imprs-astro.mpg.de
Email Submission Address: office@imprs-astro.mpg.de
Email Inquiries: office@imprs-astro.mpg.de

Attention: Christa Ingram
The International Max-Planck Research School on Astrophysics is a joint graduate school of

* The Max-Planck Institute for extraterrestrial Physics (MPE) * The Observatory of the Ludwig-Maximilians University (USM) * The Max-Planck Institute for Astrophysics (MPA) * The European Southern Observatory (ESO)

Together, these institutes form one of the largest centers for astrophysical research in the world, covering every subject from planets, stars and galaxies to cosmology. Access to the world's largest telescopes and a stimulating scientific environment provide students with ideal conditions for their PhD research.

With the deadline of December 1st, 2010 we are soliciting applications for our PhD program. Applicants should have a Bachelor or Masters Degree or Diploma in Physics or Astronomy (or equivalent), including a corresponding thesis. All successful applicants will be awarded a PhD fellowship. We support students with all administrative matters such as VISA, housing etc.

More details on the IMPRS program and the admission requirements can be found on the IMPRS website http://www.imprs-astro.mpg.de/admission.html . All application material may be submitted by e-mail to: office@imprs-astro.mpg.de .

Closing date for applications is 01 December 2010 for the program starting on 01 September 2011.

No. 26655 (New)
PhD student exoplanet characterisation
MAX-PLANCK-INSTITUTE FOR ASTRONOMY
Koenigstuhl 17
Heidelberg, Baden-Wuerttemberg D - 69117
Heidelberg
Tel: +49 6221 528 0
FAX: +49 6221 528246
URL1: www.mpia.de
Email Submission Address: lkaltene@cfa.harvard.edu
Email Inquiries: lkaltene@cfa.harvard.edu

Attention: Lisa Kaltenegger, Dr.
The Max-Planck Institute for Astronomy (MPIA) Heidelberg is seeking a curious PhD student in the field of exoplanet characterization in the new cross-disciplinary group of Lisa Kaltenegger on one of the following areas: atmospheric chemistry of extrasolar planets, planetary interiors and outgassing, Super-Earth observations with ground- and space-based telescopes and theoretical studies of habi-tability and biomarkers. 1 or more positions will be available starting Oct 2010. Working language of the group is English.

Applicants should study astronomy, planetary science, or a related field. The appointments will be for up to a total of 3 years. Opportunities for research visits at Harvard University/CfA are part of these appointments.

Candidates should send a pdf file containing their application materials, including CV, publication list if available and a brief statement of research interests to lkalteneATcfa.harvard.edu by Oct. 15 2010. 3 letters of reference should be sent separately to the same e-mail address. Applications after Oct 15 will be considered until positions are filled. Positions are available staring October 2010 but may be delayed for up to 10 months for exceptional candidates.

No. 26687 (New)
PhD Program in Astrochemistry in The Netherlands
NETHERLANDS ORGANISATION FOR SCIENTIFIC RESEARCH (NWO)
Tel:
URL1: http://www.nwo.nl/astrochemistry (Dutch Astrochemistry Network home page)
URL2: http://www.nwo.nl/astrochemistry/vacancies (Information about the PhD program and online applications)
Email Inquiries: astrochemistry@nwo.nl

Attention: The Dutch Astrochemistry Network
The Dutch astrochemistry Network is a new initiative of the Netherlands Organisation for Scientific Research (NWO) to fund a coherent and integrated research program in the (astro)physics and chemistry, starting September 1, 2010. This highly interdisciplinary network combines the astronomical and chemical expertise in the Netherlands with the goal of understanding the origin and evolution of molecules in space and their role in the Universe. The Network has defined a highly integrated and coherent science program of astrochemical and astrophysical experiments, quantum chemical calculations, and laboratory spectroscopy of astronomically relevant species in combination with an active program on modeling and observations of astronomical sources. This science is organized in four thematic areas: gas phase chemistry, solid state chemistry, interstellar polycyclic aromatic hydrocarbon molecules, and astrobiology. The Dutch Astrochemistry Network invites applications for some ten PhD positions spread over these four thematic areas. Positions are available in astrochemistry, molecular physics, quantum chemistry, laboratory spectroscopy, but students will be encouraged to become involved in the activities related to the other science disciplines. Detailed descriptions of the different PhD projects can be found at the Network website. The researchers in the network have an international background. English is the common language. Applications are accepted only through our online application site. Applicants are requested to upload a curriculum vitae, a list of all university courses taken and transcripts of grades obtained, brief statements of research interests and experience, and the contact information for at least two referees. Successful candidates must have a MSc degree (or equivalent) by the starting date. The positions are open to candidates from all countries.

No. 26565
PhD Scholarships in Observational, Computational & Theoretical Astrophysics
SWINBURNE UNIVERSITY OF TECHNOLOGY
Centre for Astrophysics & Supercomputing
Mail H39, PO Box 218
Hawthorn, Victoria 3122
Australia
Tel: +61 3 9214 5818
FAX: +61 3 9214 8797
URL1: http://astronomy.swin.edu.au/study/postgradstudy.html (Information for PhD applicants)
URL2: http://astronomy.swin.edu.au/study/phdprojects.html (Description of PhD projects)
URL3: http://astronomy.swinburne.edu.au (Centre for Astrophysics & Supercomputing)
Email Submission Address: mmurphy@swin.edu.au
Email Inquiries: mmurphy@swin.edu.au

Attention: Dr. Michael Murphy, Graduate Admissions Coordinator
The Centre for Astrophysics & Supercomputing (CAS) at Swinburne University of Technology (Melbourne, Australia) invites applications for its PhD program and scholarships from high-calibre students of any nationality.

With 16 research faculty and 35 postdoctoral researchers and students from 20 different countries, CAS offers a vibrant, research-focused and friendly atmosphere where PhD students help conduct - and learn how to lead - cutting-edge research in all major areas of astronomy.

CAS has a collaborative agreement with Caltech guaranteeing up to 20 nights per year on the 10-m Keck Telescopes (Hawaii). CAS also hosts The Green Machine, one of Australia's most powerful supercomputers (~2000 nodes, ~10Tflops).

A range of PhD scholarships are available with tax-free stipends starting at AUS$25500 p.a. and tuition fees waived. PhD students are allocated a research budget to cover travel (e.g. conferences, telescope observing etc.) and computing (e.g. laptop).

Swinburne's Hawthorn campus is situated in a lively, urban setting just minutes by public transport from Melbourne's city centre. Melbourne, Australia's second-most populous city (4 million), is renowned for its restaurants, cafe-filled laneways, bars, boutiques, theatres, galleries, festivals, city parks, sports venues and teams.

For details about postgraduate study at CAS, including eligibility requirements, available supervisors, PhD topics and how to apply, see the above web links.

The formal application deadline is October 28, 2010. However, an Expression of Interest must be submitted first, then approved applicants must discuss PhD projects with possible supervisors well before the deadline. All application materials should reach CAS by October 21, 2010.

No. 26606 (New)
Electronics Engineer(TSD)
W. M. KECK OBSERVATORY
65-1120 Mamalahoa Hwy.
Kamuela, HI 96743
USA
Tel:
FAX: 808-885-4464
URL1: http://www.keckobservatory.org
Email Submission Address: employment@keck.hawaii.edu
Email Inquiries: employment@keck.hawaii.edu

Attention: TSD Electronics Engineer
The W. M. Keck Observatory is seeking an Electronics Engineer to develop new observatory capabilities and for upgrades to existing observatory infrastructure. Ideal candidate should be a motivated self-starter who can manage multiple projects and priorities within a fast paced environment.

Qualifications include a Bachelor of Science degree in Electrical Engineering, Project Management experience, and knowledge of electronics and electrical engineering standards.

The position is opened until filled. Employment is conditional on successful completion of drug tests and background check. Email resume, professional references, and salary history to employment@keck.hawaii.edu. Additional information about this position can be found on our web site at www.keckobservatory.org. EEO/M/F/D/V

No. 26672 (New)
Sr. Electrical Engineer
UNIVERSITY OF FLORIDA
Tel: 352 392 2052 ext 267
URL1: https://jobs.ufl.edu/applicants/jsp/shared/Welcome_css.jsp (Ref # 0805679)
Email Submission Address: sid@ufl.edu
Email Inquiries: sid@ufl.edu

Attention: Search committee
Senior Electronics Engineer

Location: Gainesville, FL Deadline for Application: Open until filled

The Astronomy Instrumentation Service Center at the University of Florida Department of Astronomy is seeking a Senior Electronics Engineer to assume responsibilities in design, specification, procurement, integration, testing and routine operations/maintenance activities of electronics associated with detectors, control and data acquisition systems for optical/infrared astronomical instruments for ground and space-based observatories. Key duties and responsibilities include:

Executing electronics projects associated with procurement, characterization and optimization of detector devices.

Performing regular operations and maintenance tasks on instruments that are used in the observatory.

Support and contribute to new proposals in the field of advanced electronics, detection electronics and data acquisition systems.

Qualifications: Bachelors Degree in Electronics Engineering or related discipline is required. Masters degree or higher is preferred. At least 2 years experience required working on electronics projects associated with optical/infrared astronomical detector devices in a multi-disciplinary team environment. Testing, characterization and optimization of focal plane electronics for optical instruments and IR instruments leading to successful deployment. Excellent demonstrated hands on skills in analog, digital and mixed circuit design.

Salary is commensurate with qualifications and experience.

To apply, visit https://jobs.ufl.edu/applicants/jsp/shared/Welcome_css.jsp* . Reference number for this vacancy is 0805679.

To ensure full consideration please apply by 10/15/2010, when the Search Committee will begin reviewing applications. Applications will be accepted until the position is filled. If an accommodation due to a disability is needed to apply for this position, please call (352) 392-2HRS or the Florida Relay System at (800) 955-8771 (TDD).

No. 26707 (New)
Ground Support Engineer
USRA - UNIVERSITIES SPACE RESEARCH ASSOCIATION
Tel:
URL1: http://www.sofia.usra.edu
Email Submission Address: gmengr@sofia.usra.edu
Email Inquiries: gmengr@sofia.usra.edu

Attention: Hiring Manager
THIS POSITION IS BASED AT DRYDEN AIRCRAFT OPERATIONS CENTER IN PALMDALE CA.

Universities Space Research Association (USRA) is inviting applications as a part of the Stratospheric Observatory for Infrared Astronomy (SOFIA) program.

SOFIA is a premier observatory for infrared and sub-millimeter astronomy. A 747-SP aircraft will carry a 2.5-meter telescope designed to make sensitive infrared measurements on a variety of astronomical objects. It will fly at an altitude up to 45,000 feet. Regular observing is expected to begin in 2010. SOFIA is a joint project between NASA and German Aerospace Center, DLR. USRA will operate the SOFIA Science Center at NASA’s Ames Research Center for NASA. The aircraft observatory will be based at NASA’s Dryden Flight Research Center at Edwards Air Force Base.

The Ground Support Engineer will support project scientists and engineers by providing overall support for SOFIA science and mission operations both at the SOFIA Science Center (SSC) and the SOFIA Operations Center (SOC). During development of the observatory the Ground Support Engineer will be responsible for development of the processes and procedures ,including documentation, under Mission Operations Development and then implementations of these under Mission Operations Execution to include Pre/Post and Day of-Flight execution; Science Instrument (SI) and Principal Investigator (PI) rack(s) installation on aircraft; SI and PI support on aircraft; Telescope Assembly (TA) and Layout of Personnel and Accommodation (LOPA) configuration for flight series; Mission Operations Maintenance such as Primary Mirror cleaning between flight series, Mirror Coating Facility (MCF) maintenance; Mirror Coating such as Primary Mirror handling support including Primary Mirror Assembly (PMA) Cart and crane operations; and Mission Operations Labs including setup and maintenance of the Optics Lab and Pre-Flight Integration Facility (PIF) and support setup of MCF at Dryden Aircraft Operations Facility (DAOF).

QUALIFICATIONS AND EXPERIENCE REQUIRED FOR THIS POSITION: • A Bachelor’s degree in engineering or a related technical field is preferred. (equivalent experience or certificate(s) demonstrating that the applicant possesses the appropriate technical qualifications may be considered). • 3+ years of lab experience in a scientific and/or research environment is required, where tasks similar to those described below were executed. • Possess the ability to work with a diverse group of scientists, engineers, technicians, and administrators. • Possess demonstrated experience in performing technical tasks in the operation, installation, testing, and maintenance of electronic and mechanical lab equipment including oscilloscopes, digital multi-meters, frequency analyzers, power supplies, data acquisition equipment, vacuum pumps and leak detectors. • Possess the engineering skills to perform engineering analysis of cryogenic systems such as gas flow rates and pressure drops. • Possess the ability to read and understand technical manuals, engineering and manufacturing drawings, including schematics, wiring diagrams and optical designs and layouts, and possess basic machining and electrical wiring skills. • Possess the ability to use an engineering design software package. • Possess the ability to acquire and maintain a working knowledge of existing and newly introduced mechanical and electrical/electronic equipment and instruments. • Possess demonstrated experience in learning to safely operate newly developed capital equipment by understanding and following the instructions of developing team members and possess the communications and organization skills to develop clear technical instructions that permit safe operations for maintenance tasks. • Possess the ability to communicate with remote support personnel, either by telephone or electronic mail, describing accurately and clearly, the symptoms of equipment failures and malfunctions, as well as the sequential corrective actions taken, through trouble logs and databases. • Possess the ability to independently devise, setup, conduct, and analyze tests on instruments to investigate performance characteristics. • Possess knowledge and skills in maintaining, calibrating, operating, and to some degree modifying, astronomical instruments, in particular instruments including cryogenic systems, optics, and detector arrays. Compensation for this position is competitive and based on candidates’ experience and expertise. E-Mail your Resume or CV to: gmengr@sofia.usra.edu with salary requirements, in Word or PDF with your last name and job number (example ‘Smith S1007’) as the document title. Please specify in your cover letter names and contact information of three references and if you will require an employer sponsored Visa.

USRA is an Equal Opportunity Employer. Applicants selected will be subject to a government security check. USRA performs detailed background investigations on all candidates as a condition of hire. USRA Participates in the E-Verify Employment Verification Process

No. 26708 (New)
Science and Mission Operations Laboratory Supervisor
USRA - UNIVERSITIES SPACE RESEARCH ASSOCIATION
Tel:
URL1: http://www.sofia.usra.edu
Email Submission Address: smolabsupv@sofia.usra.edu
Email Inquiries: smolabsupv@sofia.usra.edu

Attention: smolabsupv@sofia.usra.edu
THIS POSITION IS BASED AT DRYDEN AIRCRAFT OPERATIONS CENTER IN PALMDALE CA.

Universities Space Research Association (USRA) is inviting applications as a part of the Stratospheric Observatory for Infrared Astronomy (SOFIA) program.

SOFIA is a premier observatory for infrared and sub-millimeter astronomy. A 747-SP aircraft will carry a 2.5-meter telescope designed to make sensitive infrared measurements on a variety of astronomical objects. It will fly at an altitude up to 45,000 feet. SOFIA is a joint project between NASA and German Aerospace Center, DLR. USRA will operate the SOFIA Science Center at NASA’s Ames Research Center for NASA. The aircraft observatory will be based at NASA’s Dryden Flight Research Center at Edwards Air Force Base.

USRA is seeking a Science and Mission Operations Laboratory Supervisor to primarily support the Mission Operations staff and the Science Instrument Teams in the development and operation of Mission Labs of the SOFIA Operations Center (SOC) at the Dryden Aircraft Operations Facility (DAOF) in Palmdale, California. The main purpose of these labs is for testing and maintenance of science instruments and other mission equipment prior to and following flight activities. The Lab Supervisor will be involved in these activities, which include cryogen maintenance of the instruments, assistance with instrument measurements and data collection, and minor engineering tasks. During development, the Lab Supervisor will define and update laboratory requirements, monitor construction, and specify and setup equipment. The Lab Supervisor will also be responsible for development of processes and procedures (including documentation) for Mission Labs including all technical operating and safety training manuals based on intended use and all applicable NASA, USRA, and site specific regulations. The Lab Supervisor will be responsible for development and implementation of a Maintenance Plan for all Mission laboratory equipment and facilities. During normal operations, the Lab Supervisor will provide operations and safety training for all lab users, including Mission Operations staff as well as visiting Science Investigators. The Lab Supervisor will be the primary point of contract for lab operations and also provide basic lab support to staff and visitors.

Qualifications and experience required for this position: • A Bachelor’s degree in engineering or a related technical field is preferred, but equivalent experience or certificate(s) demonstrating that the applicant possesses the appropriate technical qualifications may be acceptable. • Four to Ten years of lab experience in a scientific and/or research environment is required, where tasks similar to those described below were executed. • Possess the ability to work with a diverse group of scientists, engineers, technicians, and administrators. • Possess demonstrated experience in performing technical tasks in the operation, installation, testing, and maintenance of electronic and mechanical lab equipment including oscilloscopes, digital multi-meters, frequency analyzers, power supplies, data acquisition equipment, vacuum pumps and leak detectors. • Possess the engineering skills to perform engineering analysis of cryogenic systems such as gas flow rates and pressure drops. • Possess the ability to read and understand technical manuals, engineering and manufacturing drawings, including schematics, wiring diagrams and optical designs and layouts, and possess basic machining and electrical wiring skills. • Possess the ability to use an engineering design software package. • Possess the ability to acquire and maintain a working knowledge of existing and newly introduced mechanical and electrical/electronic equipment and instruments. • Possess demonstrated experience in learning to safely operate newly developed capital equipment by understanding and following the instructions of developing team members and possess the communications and organization skills to develop clear technical instructions that permit safe operations for maintenance tasks. • Possess the ability to communicate with remote support personnel, either by telephone or electronic mail, describing accurately and clearly, the symptoms of equipment failures and malfunctions, as well as the sequential corrective actions taken, through trouble logs and databases. • Possess the ability to independently devise, setup, conduct, and analyze tests on instruments to investigate performance characteristics. • Possess knowledge and skills in maintaining, calibrating, operating, and to some degree modifying, astronomical instruments, in particular instruments including cryogenic systems, optics, and detector arrays.

Compensation for this position is competitive and based on candidates’ experience and expertise.

E-Mail your Resume or CV to: smolabsupv@sofia.usra.edu with salary requirements, in Word or PDF with your last name and job number (example ‘Smith S1008’ ) as the document title. Please specify in your cover letter names and contact information of three references and if you will require an employer sponsored Visa. USRA is an Equal Opportunity Employer. Applicants selected will be subject to a government security check. USRA performs detailed background investigations on all candidates as a condition of hire. USRA Participates in the E-Verify Employment Verification Process

Visit http://www.sofia.usra.edu/Employment/employment.html to see all SOFIA open positions

No. 26635 (New)
Staff Astronomer
INSTITUTO RADIOASTRONOMIA MILIMETRICA (IRAM)
300 rue de la Piscine
Saint-Martin d'Heres, Grenoble 38406
France
Tel: 0033476824900
FAX: 0033476515938
URL1: www.iram.es
Email Submission Address: cox@iram.fr
Email Inquiries: neri@iram.fr

Attention: Pierre Cox, Director
Staff Astronomer at IRAM/Granada, Granada 9.8.2010

Applications are invited for a staff astronomer at IRAM Granada/Spain.

The Institut de Radio Astronomie Millimétrique (IRAM) operates a 30-meter single-dish telescope near Granada in the Spanish Sierra Nevada and an interferometer of six 15-meter antennas located at Plateau de Bure in the French Alps near Grenoble. IRAM is an international research organisation for millimeter/submillimeter astronomy supported by the CNRS (France), the Max-Planck Gesellschaft (Germany), and the IGN (Spain).

We are seeking a staff astronomer with at least five years of experience after the PhD. The astronomer must possess a broad background in observational millimeter astronomy and millimeter techniques, and a good knowledge of the European astronomical millimeter community, enabling him/her to organize the scheduling of observing projects at the 30m telescope. The astronomer must possess excellent communication, interpersonal, and organizational skills, and a good mastery of English. Knowledge of the MySQL data base language and of PHP/python is an asset.

The successful candidate shall devote 50% of his/her time to

+ the scheduling of the 30m telescope. Besides setting up the detailed telescope schedule, this work includes writing bi-yearly calls-for-proposals, handling of the proposal submission process, as well as preparing and participating at the bi-yearly meetings of the program committee. This task further includes keeping statistical information of the telescope schedules. The successful candidate will also serve as the contact person for the RadioNet TransNationalAccess program with respect to the IRAM 30m telescope. The successful candidate will be introduced into this work over an adequate period of time, and is then expected to take over full responsibility. He/she will receive support from the scientific secretariat.

+ the testing and commissioning of new instrumentation at the 30m telescope under the coordination of the Station Manager.

Another 50% of the time shall be dedicated to astronomical research, ideally in collaboration with the Granada group of astronomers. The group currently includes four PhD students working on Photon Dominated Regions in the Milky Way and in nearby galaxies, the chemistry in galactic nuclei, and gas scaling laws in local galaxies. These projects are based on observations with both IRAM observatories and Herschel.

The appointment is initially for two years with the possibility of extension. To apply, please send curriculum vitae, bibliography, and statement of research interests, and arrange for three letters of reference. Selection of candidates will start beginning of October and will continue until the position is filled. The successful candidate could start as early as 1.1.2011. Applications are to be submitted by email to the IRAM Director Pierre Cox (cox@iram.fr) or by mail to Institut de Radio Astronomie Millimétrique (IRAM), 300 rue de la Piscine, F - 38406 St-Martin-d'Hères, France. Questions should be directed to the IRAM Head of Astronomy Roberto Neri (neri@iram.fr) (phone: +33-(0)476824982) or the station manager of IRAM/Granada and the 30m telescope, Carsten Kramer (kramer@iram.es) (phone: +34-(0)958-805461).

No. 26678 (New)
HEAD OF INSTRUMENTATION
AUSTRALIAN ASTRONOMICAL OBSERVATORY (AAO)
Tel:
URL1: www.aao.gov.au/local/www/jobs
URL2: www.innovation.gov.au/careercentre
Email Submission Address: jobs@aao.gov.au
Email Inquiries: director@aao.gov.au

Attention: Professor Matthew Colless, AAO Director
The Australian Astronomical Observatory (AAO) wishes to appoint a new Head of Instrumentation (HoI). The HoI is leads the AAO’s world-renowned Instrumentation group and is responsible for managing the AAO’s development and construction of astronomical instruments for the AAO’s facilities and other telescopes around the world. The role comprises scientific leadership of the group of 25 people, oversight of the AAO’s instrumentation program, management of the various instrumentation projects carried out by the group, interaction with the AAO’s Instrument Science group (which carries out R&D on new instrumentation technologies), and strategic planning for the Observatory and its facilities. The HoI reports to the AAO Director.

Applications are now sought for the position of Head of Instrumentation at the AAO. The position will be an ongoing appointment, subject to the satisfactory completion of a 6-month probationary period.

A fixed relocation allowance plus other relocation expenses (including airfare to Australia) will also be paid.

See http://www.aao.gov.au/local/www/jobs for an employment information package. All applications should be lodged electronically via jobs@aao.gov.au and should include the following supporting documents:

• Curriculum vitae, including career history, education and qualifications, instrumentation track record, and awards, grants and distinctions. • Full list of publications, separated into accepted papers in refereed journals, conference proceedings, and other publications. • Contact details (including email and phone) for at least three referees; it is the applicant's responsibility to arrange for references to be sent to AAO before the deadline.

No. 26697 (New)
Deputy Chief – Astronomy & Space Science
CSIRO - COMMONWEALTH SCIENTIFIC & INDUSTRIAL RESEARCH ORGANISATION
Tel:
URL1: https://recruitment.csiro.au/asp/job_details.asp?RefNo=2010%2F555 (Find Out More! Lodge your application on CSIRO's website.)
URL2: http://www.csiro.au/org/CASS.html (CSIRO Astronomy & Space Science)

Attention: Phil Diamond, Chief of CSIRO Astronomy and Space Science
CSIRO Astronomy and Space Science, (a new division) operates the Australia Telescope National Facility, the Canberra Deep Space Communication Complex and is building the Australian SKA Pathfinder. We offer the key leadership role of Deputy Chief reporting to the Chief to an outstanding individual. The appointee will be responsible for a range of activities and capabilities across radio science and engineering, radio astronomy operations, project management and support functions - including finance, human resources, communications and health, safety and environment. As a trusted advisor to the Chief and a member of the Executive Team the Deputy will play a key role in the development of a strategic vision for CSIRO’s astronomy and space science portfolio with specific emphasis on positioning Australia to host the Square Kilometre Array.

*Location: Sydney or Perth Australia *Salary: An attractive package is negotiable *Reference Number: 2010/555

The position is available for an initial term of three years, which may be extended by mutual agreement.

To be considered you need a minimum of 5 years leadership experience in a research or technology-based organisation, excellent organisational skills, the ability to think strategically, and you can anticipate and manage problems in a complex and dynamic environment.

No. 26541
NOAO Associate Director for KPNO
NATIONAL OPTICAL ASTRONOMY OBSERVATORY
PO Box 26732
Tucson, AZ 85726-6732
USA
Tel: 520-318-8116
FAX: 520-318-8456
URL1: www.noao.edu/news (NOAO Long Range Plan: 2010-2014)
URL2: www.noao.edu (NOAO web site)
URL3: www.noao.edu/kpno (KPNO web site)
Email Submission Address: hrnoao@noao.edu

Attention: Human Resources Office, Attn: NOAO Associate Director to KPNO
National Optical Astronomical Observatory (NOAO) seeks an astronomer with demonstrated leadership in scientific research, astronomical technology development, and program management to become the NOAO Associate Director for Kitt Peak National Observatory (KPNO). The Associate Director is expected to be an active advocate for the deployment of new science capabilities and operations modes on Kitt Peak in response to the needs of the US O/IR System and its users at large. As a member of the NOAO senior management team, the Associate Director is also involved in strategic planning for NOAO development and reports directly to the NOAO Director.

The Associate Director for KPNO is based in Tucson and has overall responsibility for day-to-day NOAO scientific and technical operations on Kitt Peak for both NOAO facilities and tenant facilities (as defined by their individual service agreements). Some KPNO administrative and operational activities are based at NOAO headquarters in Tucson. With other members of the NOAO senior management team, the Associate Director helps develop the NOAO annual and long-range (5-year) program plans that establish the strategic direction of NOAO. Presentations about KPNO status and development are given regularly by the Associate Director to national-level oversight committees.

A more detailed job description is available ( http://www.noao.edu/cas/hr/jobs/jobs_list.html ). Click on Position Title NOAO Assoc. Director for KPNO

KPNO is located near Tucson, Arizona on land leased by the National Science Foundation (NSF) from the Tohono O’odham Nation. It hosts a number of national and university research facilities, including the NOAO Mayall 4-m and WIYN 3.5-m telescopes. For detailed information about NOAO and KPNO, see the NOAO Long Range Plan: 2010 – 2014 (www.noao.edu/news) as well as the NOAO and KPNO Web site (www.noao.edu and www.noao.edu/kpno).

The ideal candidate will:

• hold a PhD in astronomy, astrophysics, or a related field; • be involved in frontier scientific research; • have a demonstrated ability to lead mixed teams of scientists, engineers, technicians, and administrative support personnel; • have 10 years or more of experience with observatory (or similar scientific facility) operations; • have 3 – 5 years of program management, with significant responsibility for budget planning and personnel management.

NOAO is the national center for ground-based nighttime astronomy in the United States and is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. NOAO operates world-class research facilities in Arizona and the Republic of Chile, and provides a gateway via peer review to other US research facilities in the US O/IR System, including Gemini and, currently, Keck and Magellan. Operational support is provided to more than 30 tenant observatories on three mountaintops. NOAO is involved in the development of major new facilities, optical/infrared instrumentation, and data management systems. The Large Synoptic Survey Telescope (LSST) telescope and site facility development is being led by NOAO. Deeper NOAO involvement with Giant Magellan Telescope (GMT) or Thirty Meter Telescope (TMT) is a key strategic goal.

NOAO offers an excellent benefits package, competitive salary commensurate with experience, and an extremely attractive work environment.

Applicants should submit a curriculum vitae, a publication list, a statement of recent research experience, a statement of relevant management and service experience, a description of future plans, and the names of three references. Send materials electronically to hrnoao@noao.edu (preferred) or to the address below.

NOAO will begin reviewing applications on October 1, 2010. NOAO will continue to accept applications until the position is filled.

Make reference to the NOAO Associate Director for KPNO-Job #1026 when submitting application relevant materials.

NOAO is an affirmative action and equal employment opportunity employer. Preference granted to qualified Native Americans living on or near the Tohono O'odham reservation.

NOAO and NSO foster a diverse research environment. Women and candidates from under-represented minorities are particularly encouraged to apply.

Human Resources Office National Optical Astronomy Observatory Attn: NOAO Assoc. Director for KPNO-Job 1026 PO Box 26732 Tucson, Arizona 85726-6732 Email: hrnoao@noao.edu FAX: 520-318-8456

No. 26620 (New)
PosiObservational and theoretical, galactic and extragalactic astrophysics, observational and theoretical cosmology, fundamental physics with astronomical
MAX PLANCK INSTITUTE FOR RADIO ASTRONOMY
Auf dem Hügel 69
Germany
Tel: +49 228 525 217
FAX: +49 228 525 229
Email Submission Address: angelaki@mpifr-bonn.mpg.de
Email Inquiries: imprs@mpifr-bonn.mpg.de

Attention: Emmanouil Angelakis, Dr.
Text of Job Announcement: PhD Positions in Astronomy Call for Applications Deadline: November 15th, 2010

International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne

A Marie-Curie Early Stage Training Site of the European Union

General

The International Max Planck Research School (IMPRS) for Astronomy and Astrophysics, is funded by the German Max Planck Society and is operated by the Max-Planck-Institut für Radioastronomie (MPIfR) in collaboration with the Argelander-Institut für Astronomie (AIfA) of the University of Bonn and the I. Physikalisches Institut at the University of Cologne. It offers three-year financed PhD courses. The official language is English. Currently it hosts roughly 40 students from 17 countries around the world.

Fields of Research

The IMPRS for Astronomy and Astrophysics offers a broad spectrum of topics in observational and theoretical, galactic and extragalactic astrophysics, observational and theoretical cosmology, fundamental physics with astronomical tools and instrumentation. Some examples:

AGN Astrophysics – Structure and Kinematics of AGN Jets – Extragalactic Relativistic Flows – Multi-band Blazar Astrophysics – Multi-frequency AGN Polarimetry – VLBI Studies of AGNs – Infrared Interferometry of Disks and Jets of Young Stars – Protoplanetary Disks – Radiative Transfer Modeling – Galactic Masers – Infra-Red Interferometry of AGN – Gravitational Lensing – Galactic and Extragalactic Magnetic Fields – High Precision Astrometry – Stellar Astrophysics and Stellar Evolution – Supermassive Binary Black Holes in AGN – Stellar Population Studies – Astro-chemistry – Galactic Dynamics – Binary Pulsars – Neutron Stars – Experimental tests of gravity – Transient Radio Sky – Faraday Galaxy Tomography – Radio Pulsars – Gravitational Wave Detection with Pulsar Timing – Stellar Custer Dynamics – Dark Matter – Galactic Center Studies.

Despite the expertise in radio astronomy of the MPIfR the IMPRS for Astronomy and Astrophysics provides the opportunity for scientific activity in all fields of contemporary science, all modern techniques, methods and energy bands.

Training The IMPRS for Astronomy and Astrophysics offers a competitive PhD program on the basis of a tightly structured curriculum, including:

• Advanced lectures on fundamental astrophysical fields • Soft skill seminars (e.g. presentation skills, time management, scientific reading) • Weekly students seminars • Annual, “students-only” workshop where they develop team activities aside from their main research interests • Colloquia at the three hosting institutions given by experts from all over the globe • University courses • Thesis committees monitor the progress of each student and provide scientific feedback to the PhD course

Furthermore, the students are strongly encouraged and funded to travel to international schools, conferences and the best observing facilities around the world. They are exposed to the most advanced techniques and methods using state-of-the-art earth-bound or space observatories, such as the unique 100-m radio telescope in Effelsberg and the most advanced instruments in millimeter and sub-millimeter astronomy as well as high-energy band observatories.

The call for applications is open until November 15, 2010. Encouraged to apply are students with a M.Sc. degree or diploma (preferably including a thesis) in Physics or closely related subjects. Solid astrophysical background is highly favored.

More details on the IMPRS program and the admission requirements and process can be found at the IMPRS website:

http://www.mpifr.de/imprs

IMPRS Max-Planck-Institut für Radioastronomie Auf dem Hügel 69 D-53121 Bonn, Germany Tel. +49 228 525 456 imprs@mpifr-bonn.mpg.de IMPRS Speaker: Prof. Dr. J. Anton Zensus IMPRS Coordinator: Dr. E. Angelakis IMPRS Assistant: Mrs S. Pott

No. 26621 (New)
IT Specialist (Data Management/Internet)
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
Tel:
URL1: http://www.cfa.harvard.edu/hr/postings/10-42.html (Apply online only.)

Attention: http://www.cfa.harvard.edu/hr/postings/10-42.html
IT Specialist (Data Management/Internet) Smithsonian Astrophysical Observatory

The Smithsonian Astrophysical Observatory in Cambridge, MA has an immediate opening for an enthusiastic individual to provide technical support to the scientific staff in acquiring, reducing, analyzing, and archiving spectroscopic and imaging data obtained at our telescope facilities. This work utilizes Linux systems and cluster computing. The incumbent is proficient in scripting languages such as python and IDL, and in using graphical and imaging applications for astronomy such as ds9 and IRAF. Experience with managing web access to large datasets is desirable. Duties require the organization of and solution of complex problems through the application of scientific, mathematical, and data handling techniques, including finding solutions requiring complex algorithms.

Requirements: • Knowledge of various interactive systems which incumbent uses to develop protocols for management and processing of large spectroscopic and imaging datasets obtained from telescopes.

• Knowledge of GUI based pipeline control systems to calibrate and reduce datasets from a near infrared spectrograph and imaging camera.

• Knowledge of data reduction techniques for spectroscopic and imaging data in astronomy as might be acquired from the formal study of astronomy or physics.

• Knowledge of the uses of spectroscopy and imaging in astronomy.

• Basic knowledge of astronomical spectra including the extraction of redshifts and line strengths.

We offer a competitive salary plus excellent benefits. To view the complete vacancy announcement and application requirements, visit our website at http://www.cfa.harvard.edu/hr/postings/10-42.html

No. 26664 (New)
Optical/Radio Interferometric Astrophysicist
NAVAL RESEARCH LABORATORY
Tel:

Attention: https://chart.donhr.navy.mil
OPTICAL/RADIO INTERFEROMETRIC ASTROPHYSICIST AT NRL The Radio/IR/Optical Sensors (RIOS) Branch of the Remote Sensing Division of the Naval Research Laboratory in Washington, D.C. is seeking applicants for a research position in optical and radio interferometry.

This position requires expertise in carrying out significant publishable research in both optical and radio interferometry, in planning and executing both optical and radio interferometry observations, and in evaluating the implications of that research for astrometric investigations, as well as knowledge of stellar and extragalactic astrophysics. Responsibilities include carrying out research and development in advanced interferometric technologies for use in remote sensing and Naval systems and interferometric imaging, devising methods to improve the accuracy of the results, and developing new data reduction methods. Results are expected to be presented in the form of scientific publications, formal technical reports, and oral presentations.

Ongoing interferometric research projects in the RIOS Branch include the Navy Prototype Optical Interferometer (NPOI, one of the largest optical interferometers in the world) and the Long Wavelength Array (LWA, a major astrophysics research instrument for frequencies below 100 MHz). Announcement opens 1 September 2010 and closes 30 September 2010. If interested, visit https://chart.donhr.navy.mil click on search for jobs, and enter vacancy announcement number NE0-1330-03NRL0991-DE. Qualifications information and instructions on how to apply are included in the vacancy announcement.

The Naval Research Laboratory is an Equal Opportunity Employer.

No. 26669 (New)
Senior Staff Member in High Energy Astrophysics
MAX-PLANCK-INSITUTE FOR EXTRATERRESTRIAL PHYSICS
Giessenbachstrasse
Germany
Tel:
URL1: http://www.mpe.mpg.de/main.html (MPI for Extraterrestrial Physics)
URL2: http://www.mpe.mpg.de/heg/www/index.html (MPE High Energy Group)
Email Submission Address: knandra@mpe.mpg.de
Email Inquiries: knandra@mpe.mpg.de

Attention: Kirpal Nandra, Prof.
Applications are invited for a Senior Staff Position in the High-Energy Group of the Max-Planck Institute for Extraterrestrial Physics in Garching. Applicants must have a Ph.D in astronomy, astrophysics or a closely-related field, together with extensive postdoctoral experience, and a record of exceptional research achievements and refereed publications in astrophysics.

The successful candidate will be expected to carry out and supervise an internationally recognised program of research in high-energy astrophysics. The post will also involve major personnel and/or project management duties. Candidates will be expected to have significant managerial experience, or to demonstrate strong leadership potential. A high degree of teamwork is also required. Preference will be given to candidates with research interests and experience in X-ray astronomy, particularly in X-ray studies of active galactic nuclei and/or clusters of galaxies.

The appointment will follow the framework of public service employees in Germany and be at the W2 level.

Applicants should submit a curriculum vitae, including the names and contact details of three referees, a list of publications, a description of research interests, and a research plan via email to jobs@mpe.mpg.de by 31 October 2010. Applications will nonetheless be accepted until the position is filled.

For details about MPE or the High-Energy-Group see http://www.mpe.mpg.de or http://www.mpe.mpg.de/heg/www/index.html . Informal enquiries can be directed to Kirpal Nandra knandra@mpe.mpg.de.

The Max-Planck Society is an equal opportunity employer and women and minorities are encouraged to apply.

No. 26684 (New)
Science Operations Positions(Non-Research)
GEMINI OBSERVATORY
Tel:
FAX: 877-571-2008
URL1: http://www.gemini.edu
Email Submission Address: gemini-jobs@gemini.edu
Email Inquiries: gemini-jobs@gemini.edu

Attention: Human Resource Department
Science Operations Positions(Non-Research)

Gemini Observatory has two immediate openings for Science Operations Specialists. One position will be at Gemini South, La Serena, Chile, one will be at Gemini North, Hilo, Hawaii. These positions are within the scientific staff and are 100% operations support. A Science Operations Specialist covers a range of essential operational duties that include operating the telescope, instruments and computer systems on behalf of the scientists and engineers during daytime and nighttime operations; and providing essential operational, technical and archival support for data handling at the Observatory.

Nighttime responsibilities include operating the telescope and/or instruments to perform scientific observations; assisting visiting and staff observers; working with engineers and science teams during instrument commissioning; and troubleshooting telescope and instrument systems. The typical schedule is a combination of day and nighttime work. Current staff in this group spends an average of 5 nights per month on the summit; this number is subject to change and varies by person within the group based on their responsibilities. Daytime responsibilities at sea level include scientific data quality assessment, instrument calibrations, software testing, preparing the telescope and instruments for nighttime operations, troubleshooting faults with the engineering team, analyzing data, and reporting status at daily coordination meetings. The specific duties of the successful applicants will depend on their skills and interests, and the needs of the Observatory.

The applicant must be safety conscious and willing to participate in safety training; may be required to assume responsibility for safety of personnel and equipment while on nighttime duty at the summit. Must possess good communication skills, knowledge of software and hardware systems, and be familiar with Unix/Linux. Must have a good understanding of observational astronomy. Previous experience in operation of ground-based telescopes and instruments, knowledge of astronomical instruments and optical and infrared observing techniques, and/or astronomical data processing is strongly preferred. A good working knowledge of PyRAF/IRAF, as well as experience with high-level scripting in Unix/Linux command shell and Python/Perl is preferred. Bachelor in science, engineering, astronomy, or computer science required. Master’s in astronomy or physics desirable. Requires valid driver’s license, clean driving record and ability to drive 4WD vehicles. Applicants must be capable of working in a remote location at an elevation of 2900 meters (8,900 ft) for Gemini South and 4200 meters (14,000 ft) for Gemini North. International travel is expected. Gemini offers an attractive and competitive salary and benefit package.

Gemini South base facility is located in La Serena, Chile, a popular seaside town with a population of about 140,000 people, a temperate climate, and a substantial international astronomical community. There are currently three observatories operating out of the AURA compound in La Serena, and two other observatories in the area. The Gemini South telescope is on the brink of an exciting new era of science operations: a laser-fed multi-conjugate adaptive optics system, the first of its kind, will begin commissioning in 2011 and three new instruments are expected to become available to our international community during the next two to three years.

The Gemini North base facility is located in Hilo, Hawaii, a town with a very diverse population of about 43,000 people, a tropical climate, and a large international astronomical community supporting the observatories on Mauna Kea. At Gemini North the near-IR spectrograph GNIRS is in the process of being re-commissioned and is expected to attract a high user demand starting already in 2011.

The Gemini Observatory mission is exploring the universe and sharing its wonders. Come join our international team operating two of the world’s leading ground-based 8m telescopes, located in Hawaii & Chile.

Send current resume with cover letter relating your experience, education and background to the needs of the position, along with the names and contact information of three individuals familiar with your work/credentials/qualifications from whom a reference may be obtained

For further information about the positions please contact either Dr. Bernadette Rodgers, Gemini-South Head of Science Operations (brodgers@gemini.edu) or Dr. Inger Jorgensen, Gemini-North Head of Science Operations (ijorgensen@gemini.edu). Further information on Gemini can be found at: http://www.gemini.edu . AA/EOE

No. 26686 (New)
Gemini Scientist
GEMINI OBSERVATORY
Tel:
FAX: 877-571-2008
URL1: http://www.gemini.edu
Email Submission Address: gemini-jobs@gemini.edu
Email Inquiries: gemini-jobs@gemini.edu

Attention: Human Resource Department
Gemini Scientist

Gemini has an opening for a Scientist at Gemini North, Hilo, Hawaii. Scientists at Gemini acquire significant training and experience in large ground-based telescope operations—becoming proficient both in state-of-the-art astronomical instrumentation and research, and in the techniques of modern, queue-based observing methods, pioneered by Gemini Observatory.

Scientists at Gemini are actively involved in personal research projects and have twenty percent (20%) of their time available for independent astronomical research, supported by a personal research budget. In addition, a fraction of the time available on both Gemini telescopes is reserved for successful peer-reviewed staff proposals.

Scientists can expect to spend approximately 15 to 20 nights per semester executing observations on the telescope utilizing any of the three or more active instruments. Scientists also support investigators in the community in preparing their observations; and employ queue planning tools to construct nightly observing plans from a large database of potential observations. Scientists have the opportunity to become intimately involved in instrumentation projects, data analysis tools, or other observatory development projects, depending on their interests.

At Gemini North, the near-IR spectrograph GNIRS is in the process of being re-commissioned and is expected to enter science operations in early 2011. Due to the expected high user demand for GNIRS, applications are especially encouraged from individuals with prior experience in using and supporting near-IR instrumentation with and without adaptive optics.

Gemini offers an attractive and competitive salary and benefit package. The current scientist position is a fixed term position, with an initial appointment of two years, and a possible 1-year extension. The majority of the successful applicant’s time is spent at the base facility. The Gemini North base facility is located in Hilo, Hawaii, a town with a very diverse population of about 43,000 people, a tropical climate, and a substantial international astronomical community supporting the observatories on Mauna Kea.

Requirements: Ph.D. in astronomy, physics or related discipline. Significant optical and/or infrared observational, data analysis and/or instrumentation experience is highly desirable. Experience and/or knowledge in one or more of the following areas is a plus: near and mid infrared imaging and spectroscopy; optical and near infrared multi-object and IFU spectroscopy; adaptive optics and high spatial resolution imaging.

Further information on Gemini can be found at: http://www.gemini.edu . Application materials should be submitted to gemini-jobs@gemini.edu or the mailing address listed above. AA/EOE

No. 26700 (New)
Kepler Support Scientist
BAY AREA ENVIRONMENTAL RESEARCH INSTITUTE AT NASA AMES RESEARCH CENTER
M/S 244-30
Moffett Field, CA 94035
USA
Tel:
URL1: http://kepler.arc.nasa.gov (Kepler Mission - NASA Ames)
URL2: http://www.nasa.gov/kepler (Kepler Mission - NASA Headquarters)
URL3: http://keplergo.arc.nasa.gov (Kepler Guest Observer Website)
Email Submission Address: Martin.D.Still@nasa.gov
Email Inquiries: Martin.D.Still@nasa.gov

Attention: Dr. Martin D. Still, Director, Kepler Guest Observer Office
The Kepler Operations Center at NASA-Ames is seeking a team-oriented research scientist to assist with the interpretation, exploitation and processing of the Kepler data through a joint appointment in the Kepler Science Office and Guest Observer Office. This work involves scientific interaction and collaboration with the Kepler Science Team, Guest Observers, the Asteroseismology Consortium, and public archive users. The successful applicant will make significant and effective contributions to the scientific output of the Kepler mission. Duties will include algorithm development to improve the quality and efficacy of the data for detecting small planets and conducting other astrophysical investigations; interaction with the data to assess, analyze, and interpret the scientific results; and processing, documentation, and distribution of the data to the community. The successful applicant will also develop and implement innovative ideas for engaging the broader scientific community and the public in the exploitation of the Kepler data.

Kepler is NASA's Discovery mission to find Earth-sized planets in the habitable zone of sun-like stars. The spacecraft is currently in an Earth-trailing orbit and collecting its second year of science data. It provides high-precision light curves for up to 170,000 simultaneous Galactic and extra-Galactic sources over a 100 square degree field in the Cygnus-Lyra direction with nearly uninterrupted cadences of 1- and 30-minutes over a nominal mission lifetime of 3.5 years. With its unique combination of high photometric sensitivity, high duty cycle, and long lifetime, Kepler provides a paradigm-changing opportunity to find Earth analogs and measure their frequency distribution, as well as to precipitate major advances in asteroseismology, stellar evolution, stellar activity, and accretion theory.

The successful applicant will join a strong team working to support and enable science by the Kepler Science Team, the international Kepler Guest Observer community, and the public. The specific role of Kepler Support Scientists is to develop deep expertise in several aspects of the mission - instrument performance and characterization, science pipeline development, or data analysis and archiving - and contribute to the exciting endeavor of discovering habitable exoplanets and maximizing the broader scientific return of the mission by involving and enabling the community. Support scientists are expected to spend 20% of their time leading scientific investigations of their own choosing and to regularly publish their results in refereed journals.

The strong applicant will possess many of the following attributes: experience exploiting space-based and/or photometric instrumentation; expertise developing and optimizing data reduction and analysis algorithms; ability to creatively solve a wide variety of complex problems; well-developed team, diplomacy, and communication skills; computer literacy at a level that allows MATLAB script development; strong scientific background in extra-solar planetary research or a related field of astrophysics; recognition within the scientific community as a skilled and accessible mission expert; demonstrated interest in promoting scientific collaborations within the community; and desire to work in a fast-paced environment with high expectations and hard deadlines.

Education/Requirements: A Ph.D. or equivalent career experience in astrophysics, physics, engineering, computer science, or a related field is required.

The Kepler Science Office and Guest Observer Office are embedded within the Kepler Operations Center at NASA-Ames Research Center, situated in the San Francisco Bay Area. This position will be funded through a cooperative agreement between NASA and the Bay Area Environmental Research Institute (see http://www.baeri.org ).

Please send a cover letter, a resume or CV, and a list of references to Dr. Martin D. Still at the address above. In your cover letter describe which of the above attributes are revealed by your experiences and interests, and indicate your preferred starting date. The deadline for applications is November 1, 2010, but applications will be accepted until the position is filled.

No. 26704 (New)
IT Specialist (Systems Administration)
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
60 Garden Street
MS-17
Cambridge, MA 02138
USA
Tel:
URL1: http://chandra.cfa.harvard.edu
URL2: http://www.cfa.harvard.edu/hr/postings/10-53.html
Email Submission Address: saoresumes@cfa.harvard.edu
Email Inquiries: saoresumes@cfa.harvard.edu

Attention: Recruiter #461, Job Posting #10-53
IT Specialist (Systems Administration) Trust Fund (Non-Federal)

Interested in space science and technology? Join our team at the Chandra X-Ray center (CXC) and perform all aspects of IT systems management on a network of unix workstations and servers. Major areas of responsibility are (1) general Unix systems administration; (2) hardware and software installation; (3) user support; (4) studies to determine future needs, both long and short term; and (5) network security. Learn more of the Chandra mission from our website http://chandra.cfa.harvard.edu U.S. citizenship or U.S. permanent resident status is required.

To view the complete vacancy announcement and qualification requirements, please view our website at http://www.cfa.harvard.edu/hr/postings/10-53.html . Interested candidates should submit resumes to Recruiter #461, Job Posting #10-53 at the Smithsonian Astrophysical Observatory, 60 Garden Street, MS-17, Cambridge, MA 02138, or via email to: saoresumes@cfa.harvard.edu. Please note that the email address is for the submission of application materials only.

Applicants who have experience in a research environment are encouraged to augment their resume by elaborating on their hardware, software and research experience by 1) briefly relating research projects and their objectives, and 2) describing how specific hardware/software was applied to the scientific research being conducted.

The Smithsonian Astrophysical Observatory is an equal opportunity employer committed to diversity in our workplace.

No. 26712 (New)
Program Director
NATIONAL SCIENCE FOUNDATION
4201 Wilson Boulevard
Room 395
Arlington, VA 22230
USA
Tel: 703-292-4350
URL1: http://www.nsf.gov/about/career_opps
URL2: http://jobview.usajobs.gov/GetJob.aspx?OPMControl=2003462
Email Submission Address: rotator@nsf.gov
Email Inquiries: rotator@nsf.gov

Attention: E20100093-Rotator
The National Science Foundation is seeking qualified candidates for the position of Program Director within the Division of Astronomical Sciences, Directorate for Mathematical and Physical Sciences.

The candidates selected for this position will have responsibility for coordination and management of elements of the AST individual investigator grants programs, including the themes within Astronomy and Astrophysics Research Grants, the instrumentation programs, and/or the Astronomy and Astrophysics Postdoctoral Fellowships Program.

The successful candidates will be involved in activities that include planning, budget development, the merit review and proposal recommendation process, the preparation of written material about the research supported by the Division, and interactions with other NSF programs, Federal agencies and organizations. Program directors are expected to bring their scientific expertise to the activities of the Division, and to serve as a liaison between the astronomical community and NSF, disseminating information about NSF and Division activities and opportunities. Candidates are expected to work with the astronomical research and education community to broaden the diversity of participants in NSF programs. Expertise in all areas and techniques of astronomy and astrophysics will be considered.

The positions will be filled on a temporary basis beginning immediately; two positions are available. Applicants must have a Ph.D. or equivalent experience in astronomy, astrophysics, physics, or a closely related field, plus six or more years of successful research, research administration, and/or managerial experience beyond the Ph.D.

Announcement E20100093-Rotator (Program Director) with position requirements and application procedures is located on the NSF Home Page at http://www.nsf.gov/about/career_opps and the USAJOBS Link: http://jobview.usajobs.gov/GetJob.aspx?OPMControl=2003462 . Telephone inquiries may be referred to Lindsey Boswell at 703-292-4350 or rotator@nsf.gov. For technical information, contact Dr. James S. Ulvestad, AST Division Director, 703-292-8820, julvesta@nsf.gov. (Hearing impaired individuals may call TDD 703-292-8044.)

Applicants are asked to respond to the following Quality Ranking Factors -

1. Knowledge and understanding of scientific principles and theories applicable to astronomy, astrophysics, and physics which have resulted in recognized status in the community of astronomical scientists.

2. Ability to communicate effectively and work productively with the scientific community, peers, and co-workers at all levels to advocate program policies and plans and to fulfill NSF’s mission. 3. Ability to organize, implement and manage a proposal-driven grant program, allocating resources to meet a spectrum of goals, including insuring integrity and consistency in the grant award/declination management process.

NSF IS AN EQUAL OPPORTUNITY EMPLOYER

No. 26581
Staff Position in High Energy Astrophysics
MAX-PLANCK-INSTITUTE FOR EXTRATERRESTRIAL PHYSICS
Giessenbachstrasse
Germany
Tel:
URL1: http://www.mpe.mpg.de (MPI for Extraterrestrial Physics)
URL2: http://www.mpe.mpg.de/heg/www/index.html (High Energy Group)
Email Submission Address: jobs@mpe.mpg.de
Email Inquiries: knandra@mpe.mpg.de

Attention: Paul Nandra, Prof.
Applications are invited for one or more staff positions in the High-Energy-Group of the Max- Planck Institute for Extraterrestrial Physics in Garching. Applicants must have a Ph.D in astronomy, astrophysics or a closely-related field, as well as signifi-cant postdoctoral experience, and have an internationally-recognised record of re-search achievements and refereed publications in astrophysics.

Successful candidates will be expected to carry out a program of research in high-energy astrophysics, and will benefit from access to a wide variety of telescopes and instrumentation, including the forthcoming eROSITA all-sky X-ray X-ray survey, due for launch in 2012. Preference will be given to candidates, whose skills and experi-ence are relevant to the exploitation of the core science of eROSITA, i.e. X-ray sur-veys for active galactic nuclei and clusters of galaxies, including multiwavelength fol-lowup work. All applications will be considered, however, and candidates with experi-ence in X-ray instrumentation and/or X-ray optics are also particularly encouraged to apply.

Appointments will be initially for 5 years, the position follows the framework of public service employees in Germany (TVöD). Salary will commensurate with level of experience.

Applicants should submit a curriculum vitae, including the names and contact details of three referees, a list of publications, and a brief description of research interests, via email to jobs@mpe.mpg.de by 30 September 2010. Applications will nonetheless be accepted until the position is filled.

For details about MPE or High-Energy-Group see http://www.mpe.mpg.de or http://www.mpe.mpg.de/heg/www/index.html . Informal enquiries can be directed to Kirpal Nandra knandra@mpe.mpg.de.