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. 25693 (New)
ASSISTANT PROFFESOR IN DATA MINING COMPUTER SCIENCE DEPARTMENT - COLLEGE OF ENGINEERING
PONTIFICIA UNIVERSIDAD CATOLICA DE CHILE
Av. Vicuna Mackenna 4860
Macul
Santiago, Region Metropolitana 7820436
Chile
Tel: 56 2 3544440
URL1: http://dcc.puc.cl (Computer Sciende Dept.)
URL2: http://www.astro.puc.cl (Astronomy and Astrophysics Dept.)
URL3: http://www.ing.puc.cl/data-mining-position (Faculty Position Information)
Email Submission Address: vacantes-academicas@ing.puc.cl
Email Inquiries: marcos.sepulveda@ing.puc.cl

Attention: Dr. Marcos Sepúlveda, Head of Computer Science Department
The School of Engineering at Pontificia Universidad Católica de Chile offers a position in the Computer Science Department at the Assistant Professor level in the area of the Data Mining, or closely related disciplines, available immediately. The requirements are a Ph.D. degree (at the moment of assuming the position) and a demonstrated ability and commitment to excellence in independent research and teaching in the area of Mining Large Databases.

The successful candidate is expected to join a research group in machine intelligence and to participate in a new joint research center between the Faculty of Engineering and the Department of Astronomy and Astrophysics of the Faculty of Physics. This research center counts with state of the art computer clusters, able to match the increasing processing needs of current very large astronomical databases. This center has also a direct access to huge datasets coming from some of the most powerful telescopes in the world that are located in the north of Chile, and also from the upcoming Large Synoptic Survey Telescope (LSST).

While researchers in different related areas, such as machine learning, database, and astrophysics, are encouraged to apply, preference will be given to scientists working in areas related to data mining in large databases and analysis and interpretation of data from very large astronomical databases. Teaching duties are in computer science, at the undergraduate and graduate levels. Being able to teach in Spanish is desirable in the middle term, but is not a requirement to apply.

Applications later than August 31, 2009, should be considered until the position is filled.

No. 25706 (New)
OmegaCAM survey astronomer / project manager
OMEGACEN / KAPTEYN ASTRONOMICAL INSTITUTE
Tel:
URL1: http://www.astro.rug.nl/~omegacen (OmegaCEN webpages)
URL2: http://www.astro.rug.nl/~omegacam (OmegaCAM webpages)
URL3: http://www.astro-wise.org (Astro-WISE homepage)
Email Submission Address: valentyn@astro.rug.nl
Email Inquiries: valentyn@astro.rug.nl

Attention: Prof. E.A. Valentijn
Applications are invited for a Survey Astronomer to work at OmegaCEN. OmegaCEN is the wide field imaging expertise center at the Kapteyn Astronomical Institute of the University of Groningen. OmegaCEN and its international partners will commission the OmegaCAM 1 square degree wide field, optical, 16k X 16k camera for the VLT Survey Telescope (VST) in fall of 2009 at Paranal. The survey astronomer will manage and oversee the processing of the public Kilo-Degree Survey (KIDS), a collaboration with international partners (for example MPA, OAC) of at least 500 nights and also some other smaller OmegaCAM surveys. The astronomer will be involved in the science done with the observations, either weak lensing or galaxy evolution. OmegaCEN has designed and is operating the Astro-WISE information system for this task. The scientific focus of KIDS is on dark matter and energy constraints from weak lensing by galaxy halos and baryon oscillations on the large-scale galaxy distribution; evolution of galaxies and clusters and the search for very high-redshift QSOs.

The successful candidate will hold a PhD in astronomy and has proven expertise in processing and managing large imaging surveys including familiarity with associated technology such as reduction pipelines (in Python and C), databases and web services. Preference will be given to applicants with research expertise in the area of dark matter and/or galaxy evolution.

OmegaCEN is partner in Target, a regional knowledge cluster consisting of the University of Groningen Computing Center, Artificial Intelligence, OmegaCEN, the University Medical Center Groningen, ASTRON and various companies, with major contributions from IBM and Oracle. Target connects distributed information systems to 10 Petabyte scale storage systems and compute grids ranging from Linux clusters, IBM Blue Gene/P to the European network of EGEE GRID, EURO-VO and Astro-WISE. Target receives major funding and operates a 32M Euro programme for the coming 4 years. The appointment will be done in the framework of the Target programme.

The appointment will initially be for a period of up to 24 months, upon successful completion of a 2-month probationary period. Subject to project funding and employee performance, employment may be renewed for a longer term or made permanent.

Applicants should submit a curriculum vitae, list of publications, and brief description of research interests, and arrange for two letters of recommendation to be emailed to valentyn@astro.rug.nl.

Applications close : 1 August 2009

No. 25677 (New)
Canada Tier 1 Research Chair in Astronomy or Astrophysics
UNIVERSITY OF BRITISH COLUMBIA
6224 Agricultural Road
Vancouver, BC V6T 1Z1
Canada
Tel:
FAX: 604-822-5324
URL1: http://www.chairs.gc.ca/
URL2: http://www.physics.ubc.ca/Job_Appl_Info
Email Submission Address: jobs@physics.ubc.ca

Attention: Chair, CRC Astronomy Chair Search Committee
Canada Tier I Research Chair in Astronomy or Astrophysics UNIVERSITY OF BRITISH COLUMBIA

The Department of Physics & Astronomy at the University of British Columbia invites applications from exceptional candidates in all fields of Astronomy and Astrophysics for a Tier I Canada Research Chair (CRC) faculty position. The person hired will be a scientist with an outstanding international reputation in astronomy or astrophysics and will be expected to assume a leadership role in Canada’s various space or ground-based initiatives, as well as taking part in the research and teaching activities of UBC’s astronomy and astrophysics group. The position in the department will be a Professor with tenure and research support is expected from the Canadian Foundation for Innovation, Canadian aerospace industry, the Natural Sciences and Engineering Research Council of Canada, and the Canadian Space Agency. Information about the CRC program can be found at http://www.chairs.gc.ca/

UBC has an active program in astronomy and astrophysics with major participation in BLAST, MOST, Planck and Herschel, SKA, TMT and WMAP. UBC enjoys close proximity and collaboration with the National Research Council’s Herzberg Institute of Astrophysics in both Victoria and Penticton. The successful candidate will have access to computing facilities in the department and at Westgrid.

The University of British Columbia hires on the basis of merit and is committed to employment equity. We strongly encourage candidates with diverse backgrounds and experiences to apply, including women, people of colour, people of aboriginal origin, and people with disabilities. Canada Research Chairs are open to individuals of any nationality; offers will be made in accordance with Canada Immigration requirements associated with the Canada Research Chairs Program. The position is subject to review and final approval by the CRC Secretariat. Applicants are urged to submit online applications at http://www.physics.ubc.ca/Job_Appl_Info by August 31, 2009. A CV, publications list, a statement of research interests, and a summary of teaching interests and experience are required. Three letters of reference may be submitted (preferably) electronically to jobs@physics.ubc.ca, or sent by mail to: Chair, CRC Astronomy Chair Search Committee, Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road Vancouver, B.C. V6T 1Z1, Canada

No. 25685 (New)
Interferometry Specialist / Operations Staff Astronomer
EUROPEAN SOUTHERN OBSERVATORY (ESO)
Karl-Schwarzschild-Strasse 2
Garching, Bavaria 85748
Germany
Tel: +56-2-463-3164
FAX: +49-89-3200-6497
URL1: http://www.eso.org/public/ (General ESO Weg page)
URL2: https://jobs.eso.org/ (ESO Online Recruitment Portal)
URL3: https://jobs.eso.org/ESOCP370/documents/DOC0000228.PDF (Full job advertisement)
Email Submission Address: vacancy@eso.org
Email Inquiries: vacancy@eso.org

Attention: Marcia Saavedra, Ms
The European Southern Observatory is opening the position of Interferometry Specialist / Operations Staff Astronomer at Paranal (Chile).

Operations Staff Astronomers contribute to the challenge of operating the world leading astronomical facility. As Interferometry Specialist, the successful candidate will have the opportunity to provide expert knowledge on novel interferometric instrumentation, and may be given the overall responsibility for an instrument or system at the Very Large Telescope Interferometer (VLTI).

The successful candidate will:

- Contribute to the observing support in both visitor and service mode at Paranal, including short-term scheduling of observations, calibration of instruments and the assessment of the scientific quality of the astronomical data.

- Work with the team operating the VLT Interferometer (telescopes, optic train and delay lines, and VLTI instruments). The successful candidate will also be involved in the deployment of PRIMA, a phase-referenced instrument for imaging and micro-arcsec astrometry.

- Contribute in the VLTI operations-readiness of the second generation of interferometric instruments.

We are seeking an active research staff astronomer with experience in astronomical interferometry. A good command of English and a strong sense of team spirit are essential.

The position requires three letters of reference to be sent to vacancy@eso.org.

For more information and to apply online please visit https://jobs.eso.org/

No. 25686 (New)
Operations Staff Astronomer
EUROPEAN SOUTHERN OBSERVATORY (ESO)
Karl-Schwarzschild-Strasse 2
Garching, Bavaria 85748
Germany
Tel: +56-2-463-3164
FAX: +49-89-3200-6497
URL1: http://www.eso.org/public/ (General ESO Weg page)
URL2: https://jobs.eso.org/ (ESO Online Recruitment Portal)
URL3: https://jobs.eso.org/ESOCP370/documents/DOC0000227.PDF (Full text of advertisement)
Email Submission Address: vacancy@eso.org
Email Inquiries: vacancy@eso.org

Attention: Marcia Saavedra, Ms
The European Southern Observatory is opening the position of Operations Staff Astronomer at Paranal (Chile).

Operations Staff Astronomers contribute to the challenge of operating the world leading astronomical facility. The successful candidate will have the opportunity to provide expert knowledge on novel instrumentation, and may be given the overall responsibility for an instrument at the Very Large Telescope.

The successful candidate will:

- Contribute to the observing support in both visitor and service mode at the La Silla Paranal Observatory, with duty station on Paranal, including short-term scheduling of observations, calibration of instruments and the assessment of the scientific quality of the astronomical data.

- Work in collaboration with one or several of the teams operating the instruments currently on the mountain to improve their operations and scientific performances, and contribute to the VLT operations-readiness of the second generation of instruments.

The successful candidate (Ph.D. in Astronomy, Physics or equivalent) will be member of the ESO Science Faculty, with an appointment at the level of Assistant or Associate Astronomer. S/he will be expected and encouraged to actively conduct astronomical research. We are seeking an active research staff astronomer with substantial observing experience in any of the state-of-the-art observing techniques available at Paranal. A good command of English and a strong sense of team spirit are essential.

The position requires three letters of reference to be sent to vacancy@eso.org.

For further information and to apply online please visit https://jobs.eso.org/

No. 25689 (New)
Astronomy/Space Science
CHUNGNAM NATIONAL UNIVERSITY, DEPARTEMENT OF ASTRONOMY AND SPACE SCIENCE
220 Gung-Dong yusong-Gu
South Korea
Tel: + 82-42-821-5468
FAX: + 82-42-821-8891
Email Submission Address: euyiyu@cnu.ac.kr
Email Inquiries: euyiyu@cnu.ac.kr

Attention: Yu Yi, Department Chair
The Department of Astronomy and Space Science at Chungnam National University in Korea is seeking candidates for a tenure-track faculty of all levels (full time lecturer, assistant professor, associate professor, full professor, depending on experiences), starting preferably from September 1, 2009. Outstanding candidates in any field of astronomy and space science will be considered. This is a regular faculty position, but is open only to non-Korean nationalities.

The successful candidate will assume full teaching responsibilities for undergraduate and graduate courses in the Department of Astronomy and Space Science, and is expected to conduct vigorous research programs. Excellent English language communication skills are required. Applicants must demonstrate a strong record of research as well as strong interests for teaching and hold a Ph.D. in astronomy, or space science, or related field.

Interested applicants should send 1) curriculum vitae, 2) a list of publications, 3) a statement of research interests and plan to (by email), and should arrange three letters of recommendation to be sent to (by email): Prof. Yu Yi, Chair of Department of Astronomy & Space Science, Chungnam National University, Daejeon 305-764, Korea, euyiyu@cnu.ac.kr, by July 31, 2009.

No. 25623
Observational Astronomer
FLORIDA INSTITUTE OF TECHNOLOGY
Physics & Space Sciences Dept.
150 West University Blvd.
Melbourne, FL 32901
USA
Tel: 321-674-8098
FAX: 321-674-7482
URL1: http://cos.fit.edu/pss/
URL2: http://cos.fit.edu/pss/telescope.php
URL3: http://www.saraobservatory.org/
Email Submission Address: toswalt@fit.edu
Email Inquiries: toswalt@fit.edu

Attention: Dr. Terry D. Oswalt, Head
The Department of Physics and Space Sciences at the Florida Institute of Technology invites applications for a permanent faculty position that preferably will begin in August 2009. This position may be at any rank, assistant through full professor. Preference will be given to candidates with expertise in observational astronomy and an interest in serving as director of the Ortega Observatory on the FIT campus. The successful candidate will also have guaranteed access to the SARA facilities at Kitt Peak and Cerro Tololo. Candidates with experience in astronomical instrumentation, planetary, galactic and/or extragalactic research are particularly encouraged. Florida Tech is located on the eastern coast of central Florida, just south of the Kennedy Space Center. Information about the Department can be found at http://cos.fit.edu/pss/. To apply, please send a cover letter, CV, statement of research and teaching experience, and the names of at least three references to toswalt@fit.edu or via regular mail to Dr. Terry D. Oswalt, Head, Dept. of Physics and Space Sciences, Florida Institute of Technology, 150 W. University Blvd., Melbourne FL 32901, USA. Applications will be accepted until the position is filled. FIT is an equal opportunity employer.

No. 25613
Astrocamp Instructor - School Year Position
ASTROCAMP
PO Box 3399
Idyllwild, CA 92549
USA
Tel: 951-659-6062
FAX: 951-659-9843
URL1: www.astrocamp.org (Astrocamp website)
Email Submission Address: mdobson@guideddiscovereies.org
Email Inquiries: mdobson@guideddiscoveries.org

Attention: Michael Dobson, Program Director
Instructor – School Year Position

We are currently hiring instructors for the fall season, beginning August 24, 2009 and ending November 23, 2009 with opportunities to work future seasons as well. Astrocamp is a unique non-profit education center that specializes in astronomy and physical sciences. Located on a forested campus near the town of Idyllwild at an elevation of 5,600 feet amidst the beautiful San Jacinto Mountains of Southern California. Over 16,000 students from 8-14 years old attend Astrocamp each year. With excellent teaching facilities we bring science to life through hands-on, experiential classes and activities. Our labs and facilities include an olympic sized pool; extensive ropes course and rock wall, innovative classrooms, and two state of the art telescope viewing areas with CCD capabilities. Instructors have small group sizes and remain with the same group of students throughout their 3-5 day program. Astrocamp provides incredible experiences for kids and instructors alike. Check us out at www.astrocamp.org or visit www.guideddiscoveries.org.

To Apply: Send a resume, reference list, and cover letter to Michael Dobson at mdobson@guideddiscoveries.org or send to Michael Dobson, P.O. Box 3399, Idyllwild, CA 92549. Applications will be accepted until all positions are filled.

No. 25535
Branch Head of the Radio/IR/Optical Sensors Branch
NAVAL RESEARCH LABORATORY
Naval Research Lab, Code 7200
4555 Overlook Avenue SW
Washington, DC 20375
USA
Tel: 202-767-2351
URL1: http://rsd-www.nrl.navy.mil/7210/
Email Submission Address: richard.bevilacqua@nrl.navy.mil

Attention: Richard M. Bevilacqua, Superintendent
BRANCH HEAD FOR THE NRL RIOS BRANCH

The Remote Sensing Division at the Naval Research Laboratory in Washington, D.C. is seeking applicants for a research leadership position as Head of the Radio/IR/Optical Sensors (RIOS) Branch. This Branch conducts a broad spectrum of basic and applied research in the development and exploitation of sensor systems at wavelengths ranging from the radio through X-ray. Particular areas of expertise are in the use of interferometric techniques for imaging, in the development and exploitation of adaptive and active optical systems, and in basic research in astronomy and astrophysics.

The Branch Head is responsible for the formulation of the scientific goals of the Branch and works in collaboration with the Section Heads and other senior Branch members to conceive, plan, implement, and adjust short-term and long-range research goals of the program projects. The projects frequently entail collaboration with other parts of NRL, particularly the Space Science Division, and with external agencies and national and international research organizations. He/she is also encouraged to maintain an independent research program.

The Branch Head is responsible for assuring that the Branch research programs are adequately represented at national and international meetings, conferences and committees in order to further the exchange of ideas and advances in the field and to nurture fruitful collaborations. The Branch Head is also responsible for planning, directing and coordinating the effective administration of the Branch Programs, ensuring the modification and construction of new facilities as required, and assisting the recruitment of post-docs and young scientists.

Recent and/or ongoing Branch research projects include: The Long Wavelength Array (LWA; a major astrophysics research instrument for frequencies below 100 MHz), the soon to be launched Herschel Infrared Space Telescope, the Navy Prototype Optical Interferometer (NPOI; one of the largest optical interferometers in the world), Adaptive Optics (AO) and Carbon Fiber Reinforced Polymer (CFRP) telescope design and construction, as well as collaboration with and use of national and international ground-based and space-based telescopes and research facilities.

The Branch consists of ~30 mainly PhD level scientists and engineers split into the four Sections of Infrared-Submillimeter Astrophysics and Techniques, Radio Astrophysics and Sensing, Optical Remote Sensing, and Wavefront Sensing and Control, each with a Section Head reporting to the Branch Head. The Branch Head administers an annual budget of ~$12M with the assistance of a Branch Secretary and additional budgeting and administrative support from the Division level.

The successful candidate will preferably have a Ph.D. in physics or astronomy with experience in astrophysics research and, preferably, in research and personnel management. The position is U.S. Civil Service at an NP-IV level, which is equivalent to GS 14-15, with a salary range from $101,087 - $157,081 per annum, which includes the Washington area cost of living increment.

Interested parties should transmit via e-mail a cover letter describing their interest in the position and a CV to Dr. Richard Bevilacqua, Division Superintendent, [Richard.Bevilacqua@nrl.navy.mil; tel. (202) 767-2351]. Applications will be considered until the position is filled. More information on the Branch research programs is available at http://rsd-www.nrl.navy.mil/7210/ and associated links.

Navy is an Equal Opportunity Employer

No. 25668 (New)
Postdoctoral Position in High Energy Astrophysics
HARVARD-SMITHSONIAN CENTER FOR ASTROPHYSICS
Tel:
Email Inquiries: asiemiginowska@cfa.harvard.edu

Attention: Aneta Siemiginowska
Applications are invited for a postdoctoral position in the High Energy Astrophysics Division at the Harvard-Smithsonian Center for Astrophysics, to work with Dr. Aneta Siemiginowska on topics of interest which include one or more of the following: multi-wavelength observations of quasars, quasar jets, AGN/quasar feedback. X-ray studies will be the primary focus, with additional multi-wavelength imaging and spectral analysis. The appointee will have additional opportunities to pursue his/her research interests.

Candidates must possess a PhD in physics or astrophysics at time of appointment. Demonstrated experience in X-ray data analysis is desired, but not required. Applicants should be skilled at oral and written communication. This is a 2-year position which will be offered for an initial period of one year, with an extension to a second and possibly third year subject to performance; the expected start date is fall-2009, or earlier.

Interested candidates should send (preferably by email): (1) a curriculum vitae, (2) list of publications, (3) a brief statement of research interests, especially as it pertains to any of the aforementioned topics, or other related topics of relevance, and (4) arrange for letters of recommendation sent by three professional scientists familiar with the candidate's research. Closing date for receipt of applications: August 1, 2009.

SAO is an Equal Opportunity / Affirmative Action employer. Applications from women and minority candidates are strongly encouraged.

No. 25671 (New)
Post Doc position in protoplanetary disk : observation and modelisation
CEA SACLAY / SERVICE D'ASTROPHYSIQUE
Centre de l'Orme les Merisiers, Batiment 709
France
Tel: +33 1 69 08 61 30
FAX: +33 1 69 08 65 77
URL1: http://irfu.cea.fr/Sap/
Email Submission Address: charnoz@cea.fr
Email Inquiries: charnoz@cea.fr

Attention: Sebastien Charnoz
Applications are invited for a 1 year (+1 year possible extension) postdoctoral position at the Service d’Astrophysique at Saclay, France.

The holder of this position will work on VISIR data (mid-infrared spectro-imager operating at the VLT, see http://www.eso.org/sci/facilities/paranal/instruments/visir/ ) of protoplanetary disks in order to characterize their structure and dust component to bring new constrains on planet formation. The results from these data will be compared with numerical simulations performed by our team in Paris, and other collaborators based in Grenoble and Lyon (France). The successful applicant will take an active part in a research consortium ("DUSTYDISK") which is gathered on a 4 years project aimed at making significant and comprehensive progresses in understanding the protoplanetary disks. This consortium includes both observations specialists and numerical simulation experts. The holder will also participate in making simulations of disks radiative transfer coupled with dynamical simulations to assess the performances of future mid-IR instruments on ELTs in this field. In a second phase, he will also participate to the scientific prospective and the preparation of the JSWT/MIRI instrument in the field of circumstellar disks.

Applicants should have an interest in planetary formation, be familiar with data processing (IDL). They should have obtained their PHD in astronomy.

The working place will be in the "IRFU/SAp", the Astrophysics department of the french Commission for Atomic Energy (CEA Saclay) located 30km southeast of Paris. The institute gathers more than 100 researchers working in various astronomical fields (http://irfu.cea.fr/Sap/).

The net salary will be around 2000 euros/month (after tax deduction), depending on qualifications and experience. The medical care is included.

Applications will be accepted until the position is fulfilled.

The starting date of the position is flexible from October 2009 to the beginning of 2010 according to the applicant’s availability.

Applicants should take contact with Dr. Pantin (eric.pantin@cea.fr) or Dr Charnoz (charnoz@cea.fr) as soon as possible.

No. 25673 (New)
Post Doctoral Opportunities
LAWRENCE LIVERMORE NATIONAL LABORATORY
Tel:
URL1: https://jobs.llnl.gov

Attention: HR
Would you like to be part of an organization whose breakthroughs have a global impact? A position at Lawrence Livermore National Laboratory gives you the opportunity to support research and development in the national interest. Make history by being a vital part of our future.

Responsibilities: Lawrence Livermore National Laboratory (LLNL) is actively seeking qualified applicants for post-doctoral research staff positions in the areas of space science and astrophysics. LLNL has multiple immediate opportunities spanning a wide range of scientific and national security applications involving advanced space and ground-based sensor systems and networks. Specific projects range from observational cosmology, exo-planet imaging, x-ray astrophysics and optical transient detection to space situational awareness, persistent surveillance and hyper-spectra reconnaissance.

Requirements: The successful candidate should have a recent PhD in Physics, Engineering, Computer Science or a related discipline. In addition, applicants should have experience in one or more of the following areas: advanced instrumentation development, high performance computer modeling and simulation, large-scale data analysis and visualization, real-time signal and image processing.

LLNL offers a challenging environment and a competitive salary/benefits package. To view and apply for these positions, go to https://jobs.llnl.gov and search by job #008164. When applying and prompted please mention where you saw this ad. LLNL is operated by the Lawrence Livermore National Security, LLC, for the U.S. Department of Energy, National Nuclear Security Administration. We are proud to be an equal opportunity employer with a commitment to workforce diversity.

No. 25674 (New)
Postdoctoral Positions in Astrophysics
CENTRO DE RADIOASTRONOMIA Y ASTROFISICA, UNAM
Antigua Carretera a Patzcuaro 8701
Col. Ex-Hacienda de San Jose de la Huerta
Morelia, Michoacan 58090
Mexico
Tel: +52 443 322 27 95
FAX: +52 443 322 27 93
URL1: http://www.crya.unam.mx (Institution website)
URL2: http://www.crya.unam.mx/postdoc_unam (Webpage with additional information)
Email Submission Address: d.garcia@crya.unam.mx
Email Inquiries: d.garcia@crya.unam.mx

Attention: Diana Garcia, Director's Assistant
The Centro de Radioastronomia y Astrofisica (CRyA) of the Universidad Nacional Autonoma de Mexico (UNAM) invites researchers to submit applications for UNAM postdoctoral fellowships in astrophysics, to begin in March 2010. The appointment is for one year, renewable for a second year depending on performance. The CRyA is located in the beautiful city of Morelia, 300 km west of Mexico City, with direct flights to Houston, Los Angeles, and Chicago.

Fellows are expected to carry out original research in any area of astrophysics, collaborating with faculty and/or students. The main selection criteria will be outstanding research accomplishments and promise of future achievement. Fellows will have access to the San Pedro Martir National Astronomical Observatory, near Ensenada, Baja California. Astronomers at Mexican institutions have competitive access to the EVLA, the VLBA, and in the near future to ALMA, via a collaboration with the USA National Radio Astronomy Observatory; they can also compete for the Mexican share of observing time on the 10.4-m Gran Telescopio Canarias (GTC). The CRyA has computing facilities on site and has access to the UNAM supercomputer KanBalam (an HP CP 4000 rated at 7.1 TFlops with 3 Tbytes of memory and 160 Tbytes of storage). The CRyA provides funds for publishing, and limited support for observing and traveling.

At the starting date of their appointment, applicants should have a PhD in astronomy, physics, or related disciplines, earned within the last 3 years, and be less than 36 years old. Knowledge of English and/or Spanish is required. Salary and benefits are compatible with international standards.

Candidates must send a letter of interest, a research proposal, an abstract of her/his Ph.D. thesis, a complete curriculum vitae including the full list of publications, and two recommendation letters to Diana Garcia at the CRyA. All materials must be received at the CRyA by October 15th, at the latest. Unsigned material can be sent by e-mail; letters can be sent by e-mail (scanned) or by courier. Please do not use regular mail. Short-listed candidates will be requested to submit an official application form at a later date.

All interested applicants should contact Diana Garcia (d.garcia@crya.unam.mx) before the deadline for additional information; Ms. Garcia can offer assistance concerning the application procedure, in particular filling out the application form.

No. 25675 (New)
Post-doctoral Positions in Astrophysics
CENTRO DE RADIOASTRONOMIA Y ASTROFISICA, UNAM
Antigua Carretera a Patzcuaro 8701
Col. Ex-Hacienda de San Jose de la Huerta
Morelia, Michoacan 58190
Mexico
Tel: +52 443 322 27 95
FAX: +52 443 322 27 93
URL1: http://www.crya.unam.mx (Institution website)
URL2: http://www.crya.unam.mx/postdoc_unam (Webpage with additional information)
Email Submission Address: d.garcia@crya.unam.mx
Email Inquiries: d.garcia@crya.unam.mx

Attention: Diana Garcia, Director's Assistant
The Centro de Radioastronomia y Astrofisica (CRyA) of the Universidad Nacional Autonoma de Mexico (UNAM) invites researchers to submit applications for UNAM postdoctoral fellowships in astrophysics, to begin in March 2010. The appointment is for one year, renewable for a second year depending on performance. The CRyA is located in the beautiful city of Morelia, 300 km west of Mexico City, with direct flights to Houston, Los Angeles, and Chicago.

Candidates must send a letter of interest, a research proposal, an abstract of her/his Ph.D. thesis, a complete curriculum vitae including the full list of publications, and two recommendation letters to Diana Garcia at the CRyA. All materials must be received at the CRyA by October 9th, at the latest. Unsigned material can be sent by e-mail; letters can be sent by e-mail (scanned) or by courier. Please do not use regular mail. Short-listed candidates will be requested to submit an official application form at a later date.

No. 25676 (New)
Planetary Atmospheres Research Associate
UNIV. OF WISCONSIN-MADISON SPACE SCIENCE AND ENGINEERING CENTER
1225 West Dayton Street
Madison, WI 53706
USA
Tel: 608-263-6785
FAX: 608-262-5974
URL1: Research Associate (http://www.ssec.wisc.edu/employment/)
Email Submission Address: larry.sromovsky@ssec.wisc.edu

Attention: Dr. Lawrence A. Sromovsky, Senior Scientist
Notice of Research Associate Opening at the University of Wisconsin-Madison TITLE: Planetary Atmospheres Research Associate (Postdoctoral) DEPARTMENT: Space Science and Engineering Center, Univ. of Wisconsin-Madison (visit http://www.ssec.wisc.edu for more information about SSEC and employment opportunities). ADDRESS: 1225 West Dayton Street, Madison, WI, 53706 CONTACT: Dr. Lawrence (Larry) Sromovsky, Senior Scientist CONTACT PHONE: 608-263-6785 (Office) CONTACT EMAIL: larry.sromovsky@ssec.wisc.edu REQUIREMENTS: PhD in Astronomy, Atmospheric Sciences, Physics, or related field, awarded no more than 5 years prior to start date. Experience with atmospheric radiation transfer. Good English communication and writing skills. Experience with IDL and Fortran languages. Familiarity with outer-planet atmospheres. JOB DUTIES: The main duty is analysis of imaging and spectroscopic observations of the outer planets under the direction of Dr. Sromovsky. Extensive data sets to be analyzed are from the Keck II telescope and NASA Infrared Telescope Facility on Mauna Kea, the Hubble Space Telescope, and from the Galileo, Cassini, and New Horizons missions. The primary analysis targets are the cloud structures and parent gas mixing ratios on Jupiter, Uranus, and Neptune. Duties include learning how to operate existing radiation transfer codes and developing improvements to speed the process of fitting of cloud structure parameters to match observed radiances. Duties also include planning research, preparation of data for analysis, carrying out analysis tasks, preparing figures, and writing descriptions of results for publication as well as for presentation at professional meetings. BENEFITS: Based on 100% employment: 22 days of annual paid vacation, health insurance, and sick leave. SALARY RANGE: $50K-$55K, depending on experience. START DATE: 1 August 2009 (Negotiable) DURATION: 1 year, with extension to 2 years, depending on performance and funding. CLOSING DATE FOR RECEIPT OF APPLICATIONS: 31 July 2009. APPLICATION PROCEDURES: Send email to larry.sromovsky@ssec.wisc.edu. with Research Associate Position in the subject line and with an attached resume in pdf format. Also arrange for two letters of reference to be sent to the same email address, or to Dr. Sromovsky at the above department address.

No. 25678 (New)
Postdoctoral Position in Observational or Theoretical Cosmology (Ref. 09-04)
MAX PLANCK INSTITUTE FOR ASTRONOMY
Koenigstuhl 17
Germany
Tel: +49-6221-528-211
FAX: +49-6221-528-339
URL1: www.mpia.de (Institute homepage)
Email Submission Address: koltes@mpia.de
Email Inquiries: joe@mpia.de

Attention: Susanne Koltes-Al-Zoubi (Ref. 09-04)
The Max Planck Institute for Astronomy (MPIA) in Heidelberg, Germany, is seeking ambitious highly qualified candidates to fill one postdoctoral research position in Dr. Joseph Hennawi's extragalactic research group.

We are particularly interested in research on: quasar absorption lines, the Lyman alpha forest and the intergalactic medium, the epoch of Helium reionization, cosmological hydrodynamical simulations, strong and weak gravitational lensing, and studies of quasars and active galactic nuclei at high redshifts, especially in relation to large surveys. Both theorists and observers are encouraged to apply.

At present, the 'Galaxies and Cosmology' department at MPIA is pursuing a wide range of astrophysical research encompassing large observing programs, instrument development and theoretical modelling. MPIA researchers have privileged access to the twin 8.4 meter Large Binocular Telescope in Arizona, the 2.2 m MPG telescope on La Silla, the 2.2 and 3.5 m telescopes on Calar Alto, and access to all ESO facilities and the Very Large Telescope (+ Interferometer) in Chile. In addition to these facilities, MPIA astronomers regularly use (sub-)millimeter observatories such as IRAM and APEX. A number of exciting new research opportunities will soon become available to MPIA, including the PanSTARRS1 Survey, the SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS), guaranteed time programs with the HERSCHEL mission, and an improved computing cluster.

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 a total of three years; MPIA provides funds for publications, travel, etc.

Candidates should send a single pdf file containing their application materials, including curriculum vitae and a brief statement of research interests to the address above and arrange for three letters of reference to be sent directly to that address. Letters will not be acknowledged. Applications received by September 1st, 2009 will receive full consideration. Late applications will be considered until the position is filled. For further inquiries, please contact Joseph Hennawi (joe@mpia.de).

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

No. 25680 (New)
3D radiation transfer of accretion flows
OBSERVATOIRE DE PARIS
5 Place Jules Janssen
FRANCE
Tel: +33 1 45 07 74 16
FAX: +33 1 45 07 71 00
URL1: www.obspm.fr (Observatoire de Paris)
URL2: lerma.obspm.fr (LERMA)
Email Submission Address: chantal.stehle@obspm.fr
Email Inquiries: chantal.stehle@obspm.fr

Attention: STEHLE, Chantal, Dr
The ANR STARSHOCK (2009-2013) collaboration aims at understanding the 3D dynamics and radiative properties of accretion columns in Young Stellar Objects. Accretion on young stars, like the classical T-Tauri stars, is thought to occur at high velocities along magnetospheric columns, which connect the circumstellar disk to the stellar photosphere. This accretion generates a strong shock with associated spectral signatures that are used to derive the accretion rate. Radiative shock experiments carried out at large-scale experimental plasma facilities will provide new insights on the small scale structure of these shocks and will be used to benchmark hydrodynamics and radiation transport codes.

The postdoc will work on the development of a 3D radiative transfer tool that will provide quantitative spectroscopic diagnostics bridging MHD simulations of radiative shocks and experiments conducted at high-energy laser facilities. The code will incorporate a detailed description of the plasma, of the opacities, and assess departures from Local Thermodynamic Equilibrium. The radiative transport tool will be applied to interpret the laboratory experiments and predict spectral signatures of accretion shocks in Young Stellar Objects.

The postdoc will be based at LERMA-Meudon and will have to interact with project partners, most especially with I. Hubeny (University of Arizona) and T. Lanz (University of Maryland).

Experience in developing large codes for numerical simulations in physics/ astrophysics is required. Expertise with radiation transport strongly preferred.

The contract will run for a period of 3 years.

Applications will be reviewed starting Sept. 1, 2009, until the position is filled.

No. 25681 (New)
Postdoctoral Position in Extragalactic X-ray Survey Astronomy
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
60 Garden Street
Cambridge, MA 02138
USA
Tel: 617-495-7057
FAX: 617-495-7356
URL1: http://hea-www.harvard.edu/CHAMP/ (Chandra Multiwavelength Project page)
URL2: http://hea-www.harvard.edu/~pgreen/ (Paul Green's home page)
URL3: http://www.cfa.harvard.edu/ (Center for Astrophysics)
Email Submission Address: pgreen@cfa.harvard.edu
Email Inquiries: pgreen@cfa.harvard.edu

Attention: Paul Green, Astrophysicist
Applications are invited for a postdoctoral stipend position in our High Energy Astrophysics Division to work on extragalactic X-ray science primarily involving the Chandra Multi-wavelength Project (ChaMP). The ChaMP is a serendipitous extragalactic X-ray survey using Chandra archival data that covers about 30 square degrees to intermediate flux levels, complementing deep surveys that cover smaller areas to deep flux levels. The ChaMP detects thousands of active galaxies, and hundreds of clusters, many at high redshift.

The successful applicant will work with Dr. Paul Green and others on a variety of projects which may include co-adding of X-ray information for classes of galaxies, studies of local environment, modeling of galaxy/AGN source populations, and/or optical spectrosopic observing and/or analysis. The successful candidate will interact with the ChaMP team, use and develop the extensive existing database for the ChaMP, and publish scientific results. Candidates should have some experience in one or more of (1) observation and analysis of optical spectroscopy, (2) survey science and related statistics, modeling or simulation, or (3) data analysis at X-ray or other wavelengths. A strong scientific interest in working in this area is key.

This position will be for two years initially, with possible extension for up to 3 years. Interested candidates should provide electronically their curriculum vitae, bibliography, and names, addresses, telephone numbers, and email addresses of 3 professional references to the above address.

We are an equal employment opportunity employer committed to diversity in our workplace.

No. 25682 (New)
Postdoctoral Fellow(s) - Exo-Planets, Brown Dwarfs and Young Stars
UNIVERSITY OF TORONTO
50 St. George Street
Room 101
Toronto, Ontario M5S 3H4
Canada
Tel: 416-946-5243
FAX: 416-946-7287
URL1: www.astro.utoronto.ca
Email Submission Address: rayjay@astro.utoronto.ca
Email Inquiries: rayjay@astro.utoronto.ca

Attention: Ray Jayawardhana, Professor
Applications are invited for one or more postdoctoral research position(s) at the University of Toronto to start in January 2010 or later. The successful candidate(s) will work with Prof. Ray Jayawardhana and his collaborators on observational and analytical studies of extra-solar planets, brown dwarfs and young stars, and will be encouraged to pursue independent research on related topics. On-going projects include high-contrast imaging searches for companions around young stars, the SONYC (Substellar Objects in Nearby Young Clusters) ultra-deep survey, photometric and spectroscopic studies of exo-planets, and investigations of brown dwarf variability, using data from VLT, Subaru, Gemini, Keck, Spitzer, Las Campanas and other major observatories. The position is for two years, with extension to a third year possible, and comes with funds for research expenses. Applicants should send a curriculum vitae, a description of research interests and plans and a list of publications, and should arrange for three letters of recommendation to be sent directly to the above address. E-mail submission preferred. Applications received before 2009 August 15 will receive full consideration. Early expressions of interest and inquiries are welcome.

No. 25683 (New)
Postdoctoral Researcher
SETI INSTITUTE
515 N. Whisman Road
Mountain View, CA 94044
USA
Tel: 650961-6633
FAX: 6509617099
URL1: http://www.seti.org/Page.aspx?pid=1277
Email Submission Address: vschwerin@seti.org

Attention: Human Resources, Postdoctoral Researcher Position
The SETI Institute, in collaboration with the NASA Ames Astrochemistry Laboratory and Leiden University (Netherlands), is seeking candidates to fill a Postdoctoral position in Astrophysics, which entails improving spectroscopic models of polycyclic aromatic hydrocarbon infrared emissions. Consideration of applications will commence immediately. Candidates with a Ph.D. in astrophysics and experience in molecular physics, spectroscopic analysis, and theoretical development are invited to apply. Interested applicants should apply on line at: http://www.seti.org/Page.aspx?pid=1277

No. 25684 (New)
Postdoctoral Research Associate
PURDUE UNIVERSITY
Department of Physics
525 Northwestern Ave
West Lafayette, IN 47907
United States
Tel: 765-494-5193
FAX: 765-494-0706
Email Submission Address: peters11@purdue.edu
Email Inquiries: peters11@purdue.edu

Attention: Prof. John Peterson
Applications are invited for a postdoctoral fellowship at Purdue University with Professor John Peterson on the study of clusters of galaxies. Areas of collaboration include the physics of clusters of galaxies, dark matter/dark energy measurements with clusters, weak gravitational lensing, X-ray and optical observations of clusters, large cluster surveys, astrostatistics, and photon Monte Carlo simulations. Prof. Peterson has projects involving clusters surveys using X-ray and optical telescopes as well as a role in image simulations for the Large Synoptic Survey Telescope (LSST). The applicant will also be strongly encouraged to pursue their own scientific interests.

Opportunities to collaborate with other members of the astrophysics and particle physics groups also exist. Both observers and theorists are encouraged to apply. Strong data analysis and/or simulation experience is preferred. The postdoctoral fellowship is for one year, and can be renewed up to two more years contingent on performance and continued funding. Candidates must hold a Ph.D. or equivalent in physics or astronomy. The position's start date is negotiable.

To apply, please send a CV, a statement of proposed research, and three letters of recommendation sent to: Professor John Peterson, Department of Physics, 525 Northwestern Avenue, Purdue University, West Lafayette, Indiana 47907 or electronically to the address above. The position will remain open until filled, although applications received before September 15, 2009 will receive first consideration. Purdue University is an Equal Opportunity/Affirmative Action employer.

No. 25687 (New)
Research Associate UK ALMA Regional Support Centre
JODRELL BANK CENTRE FOR ASTROPHYSICS, UNIVERSITY OF MANCHESTER
Tel:
URL1: http://www.alma.ac.uk (UK ALMA Regional Centre)
URL2: http://www.jb.man.ac.uk (Jodrell Bank Centre for Astrophysics)
URL3: http://www.manchester.ac.uk (The University of Manchester)

Attention: http://www.manchester.ac.uk/aboutus/jobs/research/vacancy/index.htm?ref=157280
The European ALMA Regional Support Centre (ARC) node based in the Jodrell Bank Centre for Astrophysics (JBCA) on the University of Manchester campus is offering a postdoctoral research position commencing October 2009.

This is an exciting opportunity for a suitably qualified person to play a leading role in establishing the UK ARC, which will become a major focus for ALMA-related science in the UK over the coming years as ALMA comes online. In addition to providing the essential mm-wave expertise to enhance and extend the ARC's support activities (75%), the successful candidate will be expected to engage in their own independent research program (25%) which has relevance to ALMA science.

Applicants should have a good research and observational expertise record in the field of mm and sub-mm astronomy, and preference will be given to exceptional candidates at the second post-doctoral level. The position is open to all nationalities and the appointment will be for up to 4 years.

No. 25688 (New)
Postdoctorate Position In Astronomy CONICYT-CNRS
CNRS -CONICYT
Bernarda Morin 551
Providencia
Santiago, Region metropolitana 8320000
Chile
Tel: 56 2 3654441
FAX: 56 2 3654446
URL1: www.conicyt.cl/astronomia
Email Submission Address: postdoc_cnrs@conicyt.cl
Email Inquiries: mnorambuena@conicyt.cl

Attention: Dra. Monica Rubio, Postdoctorate Position In Astronomy CONICYT-CNRS
Call for the Contest on Postdoctoral Position CONICYT- CNRS In Chilean Universities 2009

The National Commission of Scientific and Technological Investigation, CONICYT, makes a call for foreign investigators, which have obtained a doctorate degree in Astronomy in a French University, to participate in the contest of: “Postdoctoral Position CNRS-CONICY 2009”.

The objectives of this contest are: To fortify the cooperation in the scientific and technological investigation environment; to stimulate the productivity and scientific leadership of future investigators, which must hold a PhD in Astronomy or Astrophysics given by a French University; to contribute with the exchange program of investigators and entailment between scientific Chilean–French communities.

The candidate must have the sponsorship of a Chilean University.

Through this contest CONICYT will finance a Postdoctoral Position for two years.

This call will be published in the Web page of CONICYT and spread in France by the CNRS.

Applications should be sent, before October 5, 2009 by email to:

postdoc_cnrs@conicyt.cl

More information in the contest:

http://www.conicyt.cl/astronomia

No. 25690 (New)
Postdoctoral Postiion in Observational Radio Pulsar Astrophysics
MCGILL UNIVERSITY
Physics Department
3600 University Street
Montreal, QC H3A 2T8
Canada
Tel: 1-514-398-6412
FAX: 1-514-398-8434
URL1: http://www.physics.mcgill.ca/~pulsar/ (McGill Pulsar Group Homepage)
URL2: http://www.physics.mcgill.ca/ (McGill Physics Department Homepage)
URL3: http://www.mcgill.ca/ (McGill University Homepage)
Email Submission Address: vkaspi@physics.mcgill.ca
Email Inquiries: vkaspi@physics.mcgill.ca

Attention: V. Kaspi, Prof.
Applications are invited for a postdoctoral position in radio pulsar astrophysics, to be held in the McGill Pulsar Group.

The pulsar group currently consists of 12 members and studies neutron stars mainly at radio and X-ray energies. This position is primarily for, though not restricted to, observational radio pulsar work. The successful applicant will do computer simulations of radio pulsar surveys with the upcoming Australia Square Kilometer Array Pathfinder (ASKAP) telescope. The goal of this work is to determine optimal observing parameters for an ASKAP pulsar survey. For this work, the applicant will have access to our two group-dedicated Beowulf computer clusters. There will also be opportunities for involvement in other group-based projects, at the postdoc's discretion.

The ideal candidate will have a PhD in a closely related field, excellent computer skills, familiarity with Linux, and experience in radio astronomy. Experience with Beowulf clusters, with radio interferometry, or with radio or X-ray observations of radio pulsars or other types of neutron stars are also assets.

The position will be for initially 2 years with the possibility of extension for a third. The salary is at least $55,000 CDN per year, commensurate with experience, with additional budget for research expenses provided.

Please send a CV, one-page statements of research experience and research interests, along with the names and contact information for 3 references to the address provided. Email applications are acceptable but application materials should be merged into a single pdf file and sent to vkaspi@physics.mcgill.ca, with subject line "Radio Pulsar Postdoc Application".

The deadline for applications is August 31, 2009. The successful applicant's position can commence as early as September 2009, or on a mutually agreed upon date.

No. 25691 (New)
Post Doctoral
SPACE TELESCOPE SCIENCE INSTITUTE
3700 San Martin Drive
Baltimore, MD 21218
USA
Tel:
URL1: http://www.stsci.edu/institute/employment
Email Submission Address: careers@stsci.edu
Email Inquiries: careers@stsci.edu

Attention: Human Resources: #09-0036
Applications are invited for a Postdoctoral Research position at the Space Telescope Science Institute (STScI) starting as early as November 2009.

The initial appointment is for two years, with a possible extension for a third year, pending on funding and satisfactory performance. The successful applicant will work with Dr. Ilaria Pascucci, member of the Research Staff at the Institute, on the approved Herschel survey of "Gas in Protoplanetary Systems." This 400-hour Open Time Key Program will provide the first systematic survey of gas in circumstellar disks with ages covering the dominant epoch of planet formation. The two key goals of the survey are: 1) measure the gas disk lifetime and thus constrain the formation time and the main formation pathway of giant planets; and 2) test whether water vapor remains long in the planet formation era to affect the volatile abundance of terrestrial planets (For more information on the Herschel Key Program see website at http://www.laeff.inta.es/projects/herschel/ ). The work will involve the reduction and analysis of Herschel/PACS data and modeling of the disk properties.

The postdoctoral researcher will also participate in the data reduction and analysis of the Cycle 16 Hubble Space Telescope program "Imaging Survey of Protoplanetary Disks and Brown Dwarfs in the Chamaeleon I Star-Forming Region" in collaboration with Drs. Massimo Robberto, Daniel Apai and Ilaria Pascucci at STScI and Kevin Luhman at Penn State University. This 40-orbit program recently obtained very deep optical WFPC2 images of the circumstellar environment of low-mass stars and brown dwarfs and provide data complementary to those already obtained with Spitzer and planned with the Herschel Space Observatory. This large survey will allow detailed comparative studies of circumstellar disks as a function of stellar mass. The successful applicant is expected to take a leading role in the analysis and publication of the results. Independent research in related areas will be supported. Requirements A PhD in astronomy or astrophysics is required. Research experience in space-based optical and infrared observations, infrared spectroscopy, and star & planet formation is desirable.

The Space Telescope Science Institute manages the Hubble Space Telescope and the James Webb Space Telescope and hosts the Kepler Mission Data Center. The Institute provides a uniquely dynamic and diverse environment for professional development.

STScI, located on Johns Hopkins University Campus in Baltimore, Maryland, also offers an excellent benefit package, competitive salaries, and a stimulating work environment. STScI's pay is commensurate to the year of Ph.D.

Applicants are requested to complete an online application at www.stsci.edu/institute/employment . Find the position using the requisition number listed above, click "apply online" at the bottom of the job details page, create an account, and upload the following items as PDF files into the "Resume Upload" section: 1) curriculum vitae, 2) list of publications, 3) brief statement of research interests, accomplishments, relevant technical expertise and 4) contact information for three individuals that will be submitting reference letters. Please include requisition number 09-0036 in the file name for each uploaded attachment. The three letters of recommendation should be submitted separately to careers@stsci.edu with #09-0036 in subject line. Completed applications received by August 31, 2009 are assured of full consideration. Interviews may be arranged during the IAU General Assembly in Brazil.

Committed to the benefits of diversity, we strongly encourage qualified women and minority candidates to apply. STScI is an affirmative action/equal opportunity employer. EOE/AA/M/F/D/V.

No. 25692 (New)
Postdoctoral positions with the Cosmic Origins Spectrograph Science Team
CENTER FOR ASTROPHYSICS AND SPACE ASTRONOMY, UNIVERSITY OF COLORADO AT BOULDER
1255 38th St.
Boulder, CO 80303
Tel: 303-492-0376
FAX: 303-492-5941
URL1: http://cos.colorado.edu/ (Cosmic Origins Spectrograph)
Email Submission Address: cynthia.froning@colorado.edu
Email Inquiries: cynthia.froning@colorado.edu

Attention: Dr. Cynthia Froning
The University of Colorado at Boulder is the PI institution for the Hubble Space Telescope Cosmic Origins Spectrograph (COS). As part of its mission, the COS team has guaranteed time with HST to execute a science program focusing on the origin of large scale structure and the evolution of the intergalactic medium, the formation, evolution and ages of galaxies, the interstellar medium, and the origins of stellar and planetary systems. The COS team at the University of Colorado at Boulder intends to make it final round of Research Associate (post-doctoral level) hires to work closely with science team members (James Green, Cynthia Froning, Mike Shull, Ted Snow and John Stocke) at the University of Colorado at Boulder, and analyze and publish data acquired during our guaranteed time program. We are especially interested in persons working in the areas of the interstellar medium and absorption from diffuse structures in the IGM. Experience in the analysis and interpretation of spectroscopic data is highly desirable. The start date for these positions is negotiable, but could begin as early as January 1, 2010. The positions will be for 2 years, with a possible extension for a third year. A Ph.D. in astronomy, physics or related field is required.

To apply for a position, please send a CV and a letter stating your scientific interests. Specifically address how you would contribute to the scientific goals of the project. Please arrange for two letters of recommendation to be sent directly to same address as this application. Consideration of applications will begin on September 1, 2009 and will continue until the positions are filled.

The University of Colorado at Boulder is committed to diversity and equality in education and employment; and conducts background checks on all applicants being considered for employment.

No. 25694 (New)
Research Associates in Observational Astronomy
P. UNIVERSIDAD CATÓLICA DE CHILE
Av. Vic. Mackenna 4860
Macul
Santiago, RM 7820436
Chile
Tel: 56-2-354-4940
FAX: 56-2-354-4948
URL1: www.astro.puc.cl (Department of Astronomy and Astrophysics)
URL2: www.mpia.de (Max-Planck Institut für Astronomie)
Email Submission Address: director@astro.puc.cl
Email Inquiries: linfante@astro.puc.cl

Attention: Prof. Leopoldo Infante, Director Centre for Astro-Engineering
The Department of Astronomy and Astrophysics of Pontificia Universidad Católica de Chile (PUC) and the Max-Planck Institute for Astronomy in Heidelberg, Germany, (MPIA) invites applications for two Associate Research positions in observational astronomy. Selected applicants must spend 1/3 of their working time, approximately 60 nights per year, on La Silla Observatory to support observations at the 2.2m ESO/MPIA telescope, and for the other 2/3 working time, they are expected to carry out their own research, with residence in Santiago. The position starts as soon as November 2009 and lasts for 2 years, renewable for another 2 years. The Department of Astronomy and Astrophysics provides an international environment with about twenty active researchers and a similar number of graduate students. The available computational facilities include a 512 core supercomputer intended for numerical simulations/databases/data analysis. Chile has the greatest concentration of large telescopes in the southern hemisphere; while resident at Universidad Católica, the fellows will qualify as members of the Chilean community and therefore will be eligible to apply for observing time on all telescopes in Chile, including ESO's 4x8m VLT, 3.5m NTT, and 3.6m, Gemini-South 8m, Carnegie's 2.5m and Magellan 2x6.5m, CTIO’s 4m, ASTE and APEX.

Applicants should send a curriculum vitae, list of publications, a research plan, and arrange for three letters of recommendation to be sent by 31 July 2009. The research plan should address how the applicant intends to make use of the facilities available to Universidad Católica. There will be a training period at the MPIA in Heidelberg, Germany. Applications and letters of recommendation should be sent electronically.

No. 25696 (New)
Research position for Pan-STARRS1 project.
THE JOHNS HOPKINS UNIVERSITY
517 Bloomberg Center
3400 North Charles Street
Baltimore, MD 21218
USA
Tel: 410-516-7804
FAX: 410-516-5096
URL1: www.ps1sc.org
Email Submission Address: bmd@pha.jhu.edu

Attention: Barbara Dreyfus, Research Support Analyst
Subject to the availability of funds, the Center for Astrophysical Sciences at The Johns Hopkins University (JHU) expects to hire one or more junior researchers to work with our faculty on the analysis of data from the Pan-STARRS1 project. Depending on the experience of the applicant, the position could be filled at the rank of Postdoctoral Fellow, Assistant Research Scientist, or Associate Research Scientist.

The Pan-STARRS1 Science Consortium (www.ps1sc.org) is using the largest astronomical camera ever built to conduct a set of optical imaging surveys. These surveys represent an enormous increase in our ability to investigate the time domain, and also provide multicolor images of unmatched depth over such large angular scales. JHU, as a member of the Pan-STARRS1 Science Consortium, is playing an important scientific role in several key areas. We are especially seeking researchers to work in cosmology (including supernovae and large scale structure), data intensive science, Galactic structure, galaxy evolution (including active galactic nuclei), and planetary science (including small bodies in the solar system and extra-solar planets). The starting date for the appointment is flexible within the range August to December 2009.

Candidates should send a letter of application, CV, and statement of research interests to Barbara Dreyfus, 517 Bloomberg Center, Department of Physics & Astronomy, Johns Hopkins University, Baltimore, MD 21218. These materials may also be submitted electronically (bmd@pha.jhu.edu). Please arrange for three letters of reference to be sent either by mail or electronically to the same addresses. The deadline for receipt of application materials is August 1, 2009.

No. 25697 (New)
Assistant Research Scientist in Planet Formation
THE JOHNS HOPKINS UNIVERSITY
366 Bloomberg Center, Dept of Physics & Astronomy
3400 North Charles Street
Baltimore, MD 21218
USA
Tel:
URL1: http://www.laeff.inta.es/projects/herschel/index.php
Email Submission Address: pascucci@pha.jhu.edu
Email Inquiries: pascucci@pha.jhu.edu

Attention: Ilaria Pascucci, JHU Associate Research Scientist & STScI Astronomer
Applications are invited for an Assistant Research Scientist position in the field of planet formation at the Department of Physics and Astronomy of The Johns Hopkins University (JHU) starting as early as November 2009.

The initial appointment is for two years, with a possible extension for a third year, dependent upon funding and satisfactory performance. The successful applicant will work with Dr. Ilaria Pascucci (JHU), Joan Najita (NOAO), and W. Dent (ALMA JAO) on the project entitled “Water Transport and Dispersal of Gas in Protoplanetary Disks” which is supported by the National Science Foundation. The research program has two main goals: 1) Map out the distribution and evolution of water vapor in protoplanetary disks to test how and when terrestrial planets can acquire water; and 2) identify atomic gas lines that can best trace the transition from gas-rich to gas-poor disks and thus constrain the time available to form giant planets. The work will involve the reduction and analysis of high-resolution ground-based infrared spectra and modeling of the disk properties. The ground-based data will complement already available Spitzer/IRS spectra and scheduled Herschel/PACS far-infrared data from the Herschel Key Program “Gas in Protoplanetary Systems” ( http://www.laeff.inta.es/projects/herschel/index.php ).

The successful applicant is expected to take a leading role in the analysis and publication of the results. Research experience in infrared spectroscopy, disk modeling, star and planet formation is an advantage.

Applications should include a curriculum vitae, brief statement of research interests and relevant work experience, list of publications, and three letters of reference to be sent to the email above. Completed applications received by August 31, 2009 are assured of full consideration.

The JHU Department of Physics and Astronomy offers a dynamic environment that fosters creativity and provides excellent opportunities for professional growth. Research topics span from cosmology to solar system studies. JHU astrophysicists work on theory, observations as well as new-instrument development. Intellectual life is greatly enhanced by the close ties that exist with the Space Telescope Science Institute, located across the street from the Bloomberg Center for Physics and Astronomy.

The Johns Hopkins University is an affirmative action/equal opportunity employer, and welcomes applications from women and members of underrepresented groups.

No. 25698 (New)
Postdoctoral position in Galactic astrophysics
RADBOUD UNIVERSITY NIJMEGEN
P.O. Box 9010
Nijmegen, - 6500 GL
The Netherlands
Tel: +31-24-3652801
FAX: +31-24-3652804
URL1: www.iphas.org
Email Submission Address: secr@astro.ru.nl
Email Inquiries: p.groot@astro.ru.nl

Attention: Paul Groot, Head of Department
The Department of Astrophysics at the Radboud University Nijmegen invites applications for a three-year postdoctoral position in the field of Galactic astrophysics. The position will entail research on the European Galactic Plane Surveys (EGAPS = IPHAS + UVEX + VPHAS+), which are currently mapping the full Plane down to 21st magnitude in U,g,r,i,Halpha and He I 5875 at |b|<5 degrees. The postdoctoral researcher will work on the construction of a high resolution 3D dust extinction map of our Galaxy. The research will also include the global photometric calibration of the northern EGAPS surveys, in close collaboration with the IoA, Cambridge.

The Department of Astrophysics is part of the Institute of Mathematics, Astrophysics and Particle Physics (IMAPP) of the Faculty of Science at the Radboud University. The Radboud University Nijmegen participates in the Netherlands' Research School for Astronomy (NOVA).

Further information concerning this position can be obtained from prof.dr. P. Groot (p.groot@astro.ru.nl; tel +31-24-3652801). This postdoctoral position is funded by NWO, the Netherlands Organisation for Scientific Research.

Interested applicants should hold a PhD in (astro)physics. Candidates should submit a curriculum vitae, publication list, and a description of past research and future interests. Consideration of applications will begin September 7, 2009 and will continue until the position is filled. The application should include three names of researchers willing to write letters of reference. The salary is according to the Collective Salary Agreement of the Dutch Universities and starts at level 10.5 (2977 Euro/month gross), but depends on age and experience.

No. 25699 (New)
Postdoctoral position for Australian Square Kilometre Array Pathfinder science, University of British Columbia
UNIVERSITY OF BRITISH COLUMBIA
Tel:
Email Submission Address: stairs@astro.ubc.ca
Email Inquiries: stairs@astro.ubc.ca

Attention: Ingrid Stairs
Applications are invited for a postdoctoral position in the Department of Physics and Astronomy at the University of British Columbia in beautiful Vancouver, Canada. This project is funded by the Natural Sciences and Engineering Research Council of Canada as part of the Canadian Square Kilometre Array (SKA) program. The successful candidate will work in the pulsar research group of Associate Professor Ingrid Stairs on the development of pulsar search techniques for the upcoming Australian SKA Pathfinder (ASKAP) telescope, in particular addressing the problem of migrating search observations to an interferometer. The research work will involve investigation of hardware solutions to the problem of acquiring and storing fast-sampled data from the ASKAP correlator, development of a pipeline providing imaged time-series suitable for pulsar searches, and verification of these techniques as well as tied-array-beam pulsar modes on the Boolardy Engineering Test Array (BETA), which is the initial component of ASKAP to be installed in the next few years. The position will involve significant interaction with Canadian ASKAP collaborators, in particular at McGill University, and the Australian ASKAP team. The postdoc will also have time available for personal research that bears relation to science with the ASKAP and SKA projects.

The position will be available as early as Sept. 2009, or another date that is mutually agreeable. The initial appointment will be for two years, with a third year possible depending on performance. Applicants must have obtained a Ph.D. in Astronomy or Physics not more than 3 years prior to the start date. Experience in pulsar and/or radio interferometric observations will be a strong asset.

Only electronic applications will be accepted. Applicants should send a C.V. and statement of research interests, and arrange for three letters of reference to be sent by August 31, 2009 to Prof. Stairs at stairs@astro.ubc.ca .

The University of British Columbia hires on the basis of merit and is committed to employment equity. Information on the Department of Physics and Astronomy may be found on the web at www.physics.ubc.ca and www.astro.ubc.ca.

No. 25700 (New)
Astronomy
KOREA ASTRONOMY AND SPACE SCIENCE INSTITUTE & CARNEGIE INSTITUTION OF WASHINGTON
61-1, Hwaam-dong, Yuseong-gu
Daejeon, Chungnam 304-348
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, Dr
2009 KASI – Carnegie Joint Postdoctoral Fellowship

Korea Astronomy and Space Science Institute (KASI) and The Observatories of the Carnegie Institution of Washington (Carnegie Observatories) invite applications for a four (4) - year KASI-Carnegie Joint Postdoctoral Fellowship in astronomy, to begin in November 2009. The Fellow with a Korean Ph.D. degree is expected to work for the first two (2) years at th?e 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. 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 the resources and facilities of both Institutions.

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 include the twin 6.5-m Magellan telescopes, the 2.5-meter Dupont and the 1.0-meter Swope telescope.

Interested persons should submit the following documents: - a curriculum vitae; and - a statement of current research; and - a research plan based on the resources and facilities available at both institutions; and - arrange for three letters of reference to BOTH KASI and Carnegie Observatories.

Applications should be submitted by 30th August 2009 via e-mail: arl@kasi.re.kr (for KASI) and cfellow@ociw.edu (for Carnegie Observatories). Selection of the successful candidate will be made by a joint KASI-Carnegie committee.

The successful candidate will be provided with the remuneration (starting from around 46,000,000 Won (˜35,000 USD) per annum; the currency conversion rate between US Dollar and Korean Won employed here is 1.00 USD equates 1,300 Korean Won) and other benefits equivalent to those for the permanent staff working in KASI during his or/her stay at KASI, considering his or/her educational background and research experiences. While the equivalent sum of remuneration (around 54,000 USD per annum) to the one for the post-doctorate working in Carnegie Observatories will be paid during his (her) stay at Carnegie Observatories.

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

No. 25701 (New)
Postdoctoral Appointee
ARGONNE NATIONAL LABORATORY
9700 S. Cass Ave
Lemont, IL 60439
USA
Tel:

Attention: Giselle Sandi-Tapia, Program Coordinator - Postdoctortal
The High Energy Physics Division at Argonne National Laboratory has an immediate opening for a Postdoctoral Appointee to work on the Dark Energy Survey (DES). DES will study the characteristics of dark matter and dark energy with measurements of more than 100,000 galaxy clusters, weak lensing for 300 million galaxies, and over 3000 type Ia supernovae to a redshift z ~ 1. See the DES website (www.darkenergysurvey.org) for more information. Argonne scientists are involved with supernovae light curve simulations, CCD testing and analysis, and photometric calibration efforts. The photometric calibrations include preliminary tests in 2010 with a 4-CCD camera on a 1-meter telescope. The selected candidate will be expected to contribute to the CCD tests, photometric calibration efforts, and early DES science analyses with first light in 2011. Preference will be given to candidates with prior astrophysics experience, but it is not required. If the selected candidate comes from an on-going astrophysics experiment, they will be encouraged to continue with analysis of that data. Substantial knowledge of modern software environments and data analysis experience is desirable.

Interested candidates should send a detailed CV, along with a list of publications, and the names and addresses of three references through the Argonne web site at http://www.anl.gov/jobs under job search for postdoctoral/job openings, for requisition number 314740 HEP. A U.S. Department of Energy laboratory managed by UChicago Argonne, LLC.

Argonne is an equal opportunity employer, and we value diversity in our workforce.

No. 25702 (New)
Postdoctoral position in observational studies of galaxy clusters
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
Tel: 617 495 7043
Email Submission Address: pnulsen@cfa.harvard.edu
Email Inquiries: pnulsen@cfa.harvard.edu

Attention: Paul Nulsen
Applications are invited for a postdoctoral position in the High Energy Astrophysics Division to work on observational studies of galaxy clusters. The appointee will work in collaboration with Drs. Brian McNamara and Paul Nulsen on problems related to energetic outflows from the nuclei of galaxies. Applicants must have a PhD in astrophysics or a related discipline. Applicants with research experience in radio, X-ray, optical, and infrared observations of galaxy clusters will receive preference, but all observationally oriented applicants are encouraged to apply. The appointee must be willing to make extended visits to the the University of Waterloo and Perimeter Institute for Theoretical Physics in Ontario, where McNamara is primarily located.

The position is available immediately, but the starting date is negotiable. Funding is available for two years and may be extended if additional funds become available. Applicants should send electronic copies of a resume, a one-page summary of their research, and arrange for three letters of recommendation to be sent to the email address supplied by Sept. 1, 2009.

We are an equal employment opportunity employer committed to diversity in our workplace.

No. 25703 (New)
Postdoctoral Position in Star Formation
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
60 Garden St
Mail Stop 70
Cambridge, MA 01730
USA
Tel: 617-496-7766
FAX: 617-495-7356
URL1: http://www.cfa.harvard.edu/ (CfA home page)
URL2: http://hea-www.harvard.edu/~swolk/ (Scott Wolk's home page)
URL3: http://cxc.harvard.edu/ANCHORS/ (X-ray data in regions of star formation)
Email Submission Address: swolk@cfa.harvard.edu

Attention: Scott Wolk, Staff Astrophysicist
Applications are invited for the position of postdoctoral fellow at the Smithsonian Astrophysical Observatory (SAO) for a recent recipient of a Ph. D. degree, with expertise and interests in observational and analytical studies of star formation. The applicant should have experience with observations of star-forming regions in the X-ray and/or infrared and/or in continuum emission at centimeter, millimeter, or submillimeter wavelengths; should have a record of publications or achievements which have advanced our knowledge of star formation; and should be interested in pursuing a program of observations and analysis, with emphasis on physical conditions and processes in star-forming regions. Candidates also should have demonstrated strong scientific interest in working in this field. The successful applicant will participate in the analysis and interpretation of XMM data acquired in the region of the Orion A cloud, with supporting data from the Spitzer Space telescope, and archival Chandra data from ANCHORS. The successful applicant may also obtain, reduce, and analyze supporting ground-based observations using facilities such as the SMA and the MMT. The position is for two years, with extension to a third year possible, contingent on performance and funding. Interested candidates should submit a curriculum vita, a bibliography and a statement of research interests and plans, and should arrange for three letters of recommendation to be sent as soon as possible for full consideration.

All materials should be sent to Dr. S. Wolk at the above address or by e-mail before 1 September 2009. The SAO is an AAE/EEO employer committed to diversity in our workplace.

No. 25704 (New)
Post-doctoral Fellow in Astrophotonics - Photonic Applications for Astronomical Instrumentation
MACQUARIE UNIVERSITY/ANGLO-AUSTRALIAN OBSERVATORY
Tel:
URL1: http://www.aao.gov.au/
URL2: http://web.science.mq.edu.au/groups/mqphotonics/
URL3: http://www.physics.mq.edu.au/astronomy/
Email Submission Address: jsl@science.mq.edu.au
Email Inquiries: jsl@science.mq.edu.au

Attention: Dr. Jon Lawrence
This research position, suitable for a recent PhD graduate, is a joint appointment between the Anglo-Australian Observatory and Macquarie University. The successful candidate will closely interact with the staff in the instrument science group at the Anglo-Australian Observatory and the staff and students in the Photonics, and Astronomy and Astrophysics groups at Macquarie University – the two institutions are located close to each other in Sydney. The position is initially for 2 years, with a possibility of further extension subject to performance and external funding.

Astrophotonics is a rapidly emerging area that aims to apply frontier physical, optical, and photonic technologies to improve the power and efficiency of modern astronomical instruments. The Research Fellow appointed to this position will be expected to work on the development of integrated photonic spectrographs for astronomical telescopes, and other related astrophotonics projects.

The position requires: PhD (or near completion) in physics/astronomy/engineering or related field; background/experience in astronomy, astronomical instrumentation, optics, photonics, physics or related scientific disciplines; demonstrated record of research productivity.

Salary range: AUD$66,145 to $74,654 per annum (Academic Level A6-B1) plus employer superannuation contribution and leave loading.

Submit Resumes to: http://www.mq.edu.au/jobs/

For further details contact:

Dr. Jon Lawrence (jsl@science.mq.edu.au) Macquarie University/Anglo-Australian Observatory Sydney, NSW Australia

No. 25705 (New)
postdoctoral position in high energy astrophysics
PURDUE UNIVERSITY
525 Northwestern Ave
West Lafayette, Indiana 47907
United States
Tel: 765.494.5171
FAX: 765.496.2298
Email Submission Address: finley@purdue.edu
Email Inquiries: finley@purdue.edu

Attention: John P. Finley, Professor
Applications are invited for a postdoctoral position in high energy astrophysics in the Department of Physics at Purdue University. The successful applicant will work with the VERITAS group to pursue VERITAS-related science. VERITAS is an array of ground based gamma-ray telescopes currently operating in southern Arizona. The group is mainly interested in pulsars, pulsar wind nebulae/supernova remnants, microquasars, and active galactic nuclei. The successful applicant will also be strongly encouraged to pursue his/her own scientific interests and to collaborate with other members of the high energy astrophysics group.

The postdoctoral fellowship is for one year, with the possibility of renewal for additional two years contingent on performance and continued funding. Candidates must hold a Ph.D. or equivalent in physics or astronomy. The starting date is negotiable. To apply, please send a vita, bibliography, statement of research, and have three letters of recommendation sent to: Professor John P. Finley, Department of Physics, Purdue University, 525 Northwestern Avenue, West Lafayette, IN 47907-2036. The position will remain open until filled, although completed applications will be evaluated as soon as they are received. Purdue University is an equal opportunity/equal access/affirmative action employer fully committed to achieving a diverse workforce.

No. 25618
Research Associate in Neutron Star Astrophysics
WEST VIRGINIA UNIVERSITY
Tel:
URL1: http://astro.wvu.edu (WVU Astrophysics Group Website)
URL2: http://physics.wvu.edu (WVU Physics Department Website)
URL3: http://www.wvu.edu (West Virginia University)
Email Submission Address: astro@mail.wvu.edu
Email Inquiries: astro@mail.wvu.edu

Attention: Duncan Lorimer
Applications are invited for a postdoctoral researcher at West Virginia University (WVU). The successful applicant would join the WVU Center for Astrophysics, a rapidly growing research program currently consisting of four faculty members, one research assistant professor, two postdoctoral fellows, and ten graduate and undergraduate students. Applicants with expertise in observational and/or theoretical astronomy are encouraged to apply. A PhD in Astronomy, Physics or a related discipline is required. The applicant will work with Drs. Lorimer and McLaughlin, and other group members, on projects involving the theory and observations of pulsars and ideally will also have independent research projects in areas that will broaden the impact of the astrophysics group.

The applicant will have access to the group's dedicated Beowulf cluster. WVU is a vibrant and growing public university (22,000 undergraduates and 6,000 graduate students). Situated in Morgantown, WV, the University's proximity to both the Green Bank Telescope and other East Coast institutions makes it ideal for astronomy research. The WVU physics department consists of 17 faculty, 10 research faculty and postdocs and 60 graduate students. This position is made possible by a $1.4M award to the group to expand its astrophysics research program. Funding is available for conference travel and observing trips. The appointment is for two years, with a further year possible upon mutual agreement. Applicants should send a CV, publication list, statement of research interests (up to 2 pages) and contact information for three references to the email submission address. WVU is an Affirmative Action/Equal Opportunity employer.

No. 25624
Research Associate in Cosmology and Extragalactic Astrophysics
IMPERIAL COLLEGE LONDON
Dept of Physics, Blackett Laboratory
Prince Consort Road
UK
Tel: +44 (0)20 7594 7531
FAX: +44 (0)20 7594 7541
URL1: http://www.imperial.ac.uk/employment ((Link to online application - this method is preferred))
Email Submission Address: astro@imperial.ac.uk
Email Inquiries: astro@imperial.ac.uk

Attention: Dilly Osbahr, Group Administrator for Astrophysics
Salary £26,580 - £38,730 per annum

Fixed term: 2 years in the first instance, commencing 1 October 2009

Applications are invited for a two-year Research Associate position in the Astrophysics Group, to start on 1 October 2009. The post will be in the broad area of cosmology and extragalactic astrophysics to participate in the Group's activity in Cosmic Microwave Background science and specifically as part of the Planck Surveyor Satellite team, working closely with Professor Andrew Jaffe.

This work will include reduction and analysis of data from the Planck satellite and the presentation of the scientific results obtained. Specific scientific topics of interest include the global topology of the Universe and the determination of cosmological parameters and power spectra from CMB data. The postholder will be expected to contribute to the Department’s teaching activities up to approximately half a day per week during the academic year, as appropriate.

A PhD or equivalent level of professional qualifications and experience in Astrophysics or a related discipline, and a strong research background in cosmology and/or extragalactic astrophysics is essential. Experience in cosmological anisotropy and topoplogy, and the data reduction or analysis of Cosmic Microwave Background or other astrophysical data would be desirable.

Informal inquiries can be directed to Professor Andrew Jaffe at a.jaffe@imperial.ac.uk or +44(0)20 7594 7526.

Our preferred method of application is online via our website http://www.imperial.ac.uk/employment (please select “Job Search” then enter the job title or vacancy reference number NS2009070GA into “Keywords”). Please complete and upload an application form as directed, also providing a CV and list of publications.

Alternatively, if you are unable to apply online, please contact Dilly Osbahr on +44(0)20 7594 7531 or email astro@imperial.ac.uk to request an application form.

Closing date: 3 August 2009

Committed to equality and valuing diversity. We are an Athena Silver SWAN Award winner and a Stonewall Diversity Champion.

No. 25650
Postdoctoral Research Scholar
UNIVERSITY OF IOWA
University of Iowa
214 Van Allen Hall
Iowa City, IA 52242
USA
Tel: 319-335-1690
FAX: 319-335-1753
Email Submission Address: christine-stevens@uiowa.edu

Attention: Christine Stevens
The University of Iowa is searching for a postdoctoral research scholar to work in high energy astrophysics in collaboration with Prof. Philip Kaaret. The work may include data analysis from X-ray observatories and the VERITAS TeV telescope array and development of instrumentation for the detection of X-rays and gamma-rays. Candidates must hold a Ph.D. in physics or astronomy. Experience in data analysis and/or instrumentation hardware is preferred. US citizenship or green-card status are preferred. Applicants should submit a curriculum vitae, a list of publications, and a statement of research interests to christine-stevens@uiowa.edu or Christine Stevens, Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242. Electronic submissions in pdf format only are acceptable. Applicants should also make arrangements for three letters of recommendation to be sent directly. Letters of recommendation can be sent via e-mail. Review of applications will begin on September 1st, 2009, and continue until the position is filled. The University of Iowa is an EEO/AA employer. Women and members of minority groups are strongly encouraged to apply.

No. 25651
Postdoctoral Fellowship In Astrophysics
PRINCETON UNIVERSITY
Tel:
URL1: http://mri.pppl.gov (Princeton Magnetorotational Experiment)
Email Submission Address: postapp09@astro.princeton.edu
Email Inquiries: jeremy@astro.princeton.edu

Attention: Princeton Magnetorotational Experiment Postdoc
The Department of Astrophysical Sciences, Princeton University, invites applications for a Postdoctoral Fellowship in Astrophysics. Half of the Fellow's effort will be numerical simulations and theoretical analyses in support of the Princeton Magnetorotational Experiment (http://mri.pppl.gov) in collaboration with Professor Jeremy Goodman and Principal Research Physicist Hantao Ji. The other half will be research at the Fellow's discretion but within computational astrophysics or plasma physics, as the position is supported in part by the NSF Center for Magnetic Self-Organization. Professor James Stone, in addition to Goodman and Ji, will partipate in possible computational astrophysics projects. The start date can be as early as September 2009.

Appointments are for one year, renewable annually based on satisfactory performance, for a total of up to three years, funds permitting. Applicants should send a curriculum vitae, bibliography and statement of research interests, and arrange to have three letters of recommendation sent to the above electronic address. Applications will be reviewed beginning by July 1, 2009.

Princeton University is an equal opportunity employer and complies with applicable EEO and affirmative action regulations. For information about applying to Princeton and voluntarily self-identifying, please link to http://www.princeton.edu/dof/about_us/dof_job_openings/

No. 25656
Herschel/HIFI Instrument Control Center calibration / data analysis scientist
CESR/CNRS-UPS
9 Avenue du Colonel Roche
BP 43446
Toulouse Cedex 04, France 31029
France
Tel: (33) 561 556 689
FAX: (33) 561 556 701
Email Submission Address: caux@cesr.fr

Attention: Emmanuel Caux, Dr.
Post Doctoral Research Position offer for a

Herschel/HIFI Instrument Control Center calibration / data analysis scientist

CESR (Centre d’Etude Spatiale des Rayonnements) develops innovative instrumentation for astrophysical research on board international scientific satellites (e.g. from ESA or NASA). Scientific research, through the use of these instruments, constitutes an important facet of the CESR program.

CESR has participated to the building of the Heterodyne Instrument for the Far Infrared (HIFI) that will be flown on the Herschel Space Observatory of the European Space Agency (ESA). CESR provided the High Resolution Spectrometer (HRS), a flexible autocorrelator spectrometer with an ultimate spectral resolution of 125 kHz.

Main tasks :

- Participate in the preparation and data analysis focused on HIFI calibration, particularly for the HRS. - Participation in ground segment and spaced based activities supporting HIFI calibration. - Participation in HIFI Guaranteed Time Key Programs (CESR is involved in the following HIFI Guaranteed Time Key Programs : HS3F, HEXOS, WADI, PRISMAS).

Qualifications :

- PhD in (observational) astrophysics or Physics - Proven expertise in submillimeter/FIR observations and data analysis - Good knowledge in molecular spectroscopy - Knowledge of submillimeter/FIR instrumentation, preferably in heterodyne instrumentation - Good communication skills - Knowledge of the Python/Jython scripting language and or will be an asset

Employment conditions :

The position will be located at CESR, Toulouse, France. It requires frequent staying periods at the PI Institute of HIFI, also holding the Instrument Control Centre (ICC) responsible for the day-to-day operation and calibration of the HIFI instrument, which is located at SRON in Groningen (NL). During the Performance and Verification Phase (PVP, Launch to Launch + 6 months), the Post-Doc will have to stay at SRON for about 4/5 of his time.

The full-time position will be a French CDD (Contrat à Durée Déterminée) for one year renewable up to 3 years. The salary scale will depend on education and working experience, and will be in accordance with French CNRS salary grid. The starting date is as soon as possible.

For more information about the position please contact Dr. E. Caux (caux@cesr.fr), telephone +33-(0)561556689. Information about CESR can be found at http://www.cesr.fr.

Letters of applications:

Applications, including a full CV, statement of research interest, publication list and letters of reference (which can be sent separately) should be sent to E. Caux, CESR, BP 43446, 31028 Toulouse Cedex 04, France and by email to caux@cesr.fr.

No. 25658
Postdoctoral Position: Galaxy formation in the early Universe
PENN STATE UNIVERSITY
Dept. of Astronomy & Astrophysics
525 Davey Lab
University Park, PA 16802
USA
Tel: 814 863 7350
FAX: 814 863 2842
URL1: http://www.astro.psu.edu
Email Submission Address: yuexing@astro.psu.edu
Email Inquiries: yuexing@astro.psu.edu

Attention: Yuexing Li, Assistant Professor of Astronomy
Position /Title: Galaxy formation in the early Universe Institution: Pennsylvania State University

Submit Resumes To: Prof. Yuexing Li Department of Astronomy & Astrophysics The Pennsylvania State University 525 Davey Lab University Park, PA 16802

Email Submission Address: yuexing@astro.psu.edu Email Inquiries: yuexing@astro.psu.edu

The closing date for application: 09/30/2009

Job Description:

Applications are invited for a postdoctoral research position in galaxy formation. The successful candidate would work with Professor Yuexing Li and participate in any aspects of the program: the formation and evolution of galaxies and quasars in the early Universe with cosmological simulations; multi-wavelength properties of these objects with radiative transfer calculations; and cosmic reionization history. These projects involve both theoretical modelings and comparisons with observations.

The ideal candidate should have experience with numerical simulations or radiative transfer processes. A Ph.D. in astrophysics or related areas is required.

The position is available September 1, 2009 (negotiable). The review of applications will begin on July 1, 2009, and the search will continue until the position is filled. The appointment is for two years, renewable for a total of three years contingent upon continued funding.Please send a curriculum vitae with publication list, a statement of research interests, and three letters of recommendation to Prof. Yuexing Li at yuexing@astro.psu.edu.

Penn State is committed to affirmative action, equal opportunity and the diversity of its workforce.

No. 25660
Postdoctoral Researcher Position in Millimeter Astronomy
IRAM - INSTITUT DE RADIOASTRONOMIE MILLIMETRIQUE
300 rue de la Piscine
Domaine Universitaire
Saint Martin d'Heres, Saint Martin d'Heres 38406
France
Tel: +33-(0)4 76 82 49 06
FAX: +33-(0)4 76 51 59 38
URL1: http://www.iram.fr/IRAMFR/jobOffers.htm (IRAM job vacancies)
Email Submission Address: cox@iram.fr ; indigo@iram.fr
Email Inquiries: neri@iram.fr

Attention: Dr. Pierre COX, Director
Applications are invited for an astronomer position at IRAM, Grenoble.

To pave the road for future upgrades of the Plateau de Bure interferometer (PdBI) and to prepare for the arrival of ALMA, IRAM is committing substantial resources to disseminate and facilitate knowledge transfer in (sub)millimeter wave interferometry and provide research training opportunities to young scientists. The current position offers the opportunity for astronomers to work with world-class research facilities, pursue their career in a very dynamic and competitive field of research, and to foster collaborations in an international environment of top scientific research.

The successful candidate is expected to invest 50% of her/his time to further own astronomical research objectives in collaboration with astronomers within and outside IRAM, and 50% to participate in the scientific operation of the PdBI, provide technical expertise in the analysis and interpretation of data to visiting astronomers, and take part in software activities related to the development of the IRAM node of the European ALMA regional center.

We are seeking candidates with a PhD in astronomy, preferably with a demonstrated observational experience or a strong interest in (sub)millimeter wave interferometry or related fields. Good English communication skills and a strong sense of team spirit are essential attributes.

Candidates should send their CV, bibliography and statement of research interests, and arrange for letters of reference, no later than August 15, 2009. The appointment is for two years with the possibility of extension, and could start as early as possible.

No. 25563
Postdoctoral Position for Low Frequency Cosmology (LUNAR Fellow)
NAVAL RESEARCH LABORATORY
4555 Overlook Ave., SW
Washington, DC 20375
Tel: 202-404-6329
FAX: 202-404-8894
Email Submission Address: Joseph.Lazio@nrl.navy.mil
Email Inquiries: Joseph.Lazio@nrl.navy.mil

Attention: Joseph Lazio, Astronomer
The Remote Sensing Division of the Naval Research Laboratory (NRL) is seeking postdoctoral applications from those with an interest in using the 21-cm line as a cosmological and astrophysical probe of the Dark Ages and Epoch of Reionization. The successful candidate will be expected to carry out an innovative research program of scientific research, algorithmic development, or hardware development aimed at enabling current and future telescopes to use the highly redshifted 21-cm line.

The NRL Remote Sensing Division is a member of the Lunar University Network for Astrophysics Research (LUNAR) team, under the recently established NASA Lunar Science Institute (NLSI). One of the key foci of the LUNAR project is to advance the development of a future, low radio frequency lunar telescope designed to exploit the highly redshifted 21-cm line for cosmological and astrophysical studies of the Dark Ages and Epoch of Reionization. Studies to be conducted under this program could include, but are not limited to, • Science observations using existing data or by acquiring new data from a current low radio frequency telescope such as the VLA, GMRT, LOFAR, or the Long Wavelength Demonstrator Array; • Algorithm development, such as obtaining high dynamic range images, using existing low radio frequency data from a current telescope such as the VLA or GMRT; or • Antenna development, specifically including conducting tests of candidate antenna designs for a future low radio frequency lunar telescope.

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 tow years, with a third year extension for satisfactory accomplishments in the first two years. 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. Each year, deadlines for submission to the NRC are February 1, May 1, and August 1. The current award stipend is $69,764 per year. US citizenship or permanent residency is required. Applications may be submitted at http://www.nationalacademies.org/rap/ . For further information contact Dr. Joseph Lazio at the above address; see also the NRL SNe/SNR/LFRA site. EOE/AAE.

No. 25577
Postdoctoral Position for Pulsar Timing Array Gravitational Wave Studies
NAVAL RESEARCH LABORATORY
4555 Overlook Ave., SW
Washington, DC 20375
Tel: 202-404-6329
FAX: 202-404-8894
Email Submission Address: Joseph.Lazio@nrl.navy.mil
Email Inquiries: Joseph.Lazio@nrl.nayv.mil

Attention: Joseph Lazio, Astronomer
The Remote Sensing Division of the Naval Research Laboratory (NRL) is seeking postdoctoral applications from those with an interest in detecting and studying gravitational waves via a pulsar timing array. The successful candidate will be expected to carry out an innovative research program aimed at improving the capabilities of current and future radio telescopes to detect and study gravitational waves or improving our knowledge of the source population for low frequency gravitational waves. Previous experience with pulsar observations is not a prerequisite. The NRL Remote Sensing Division participates in the North American Nanohertz Observatory of Gravitational Waves (NANOGrav), the focus of which is to assemble and use an array of millisecond pulsars to detect and study low frequency gravitational waves. Research topics to be conducted under this program could include, but are not limited to, • Studies of radio-wave propagation effects to understand and correct for these effects in pulsar timing programs; • Conducting timing observations of the known pulsar population to improve current limits on and detect gravitational waves; • Participating in on-going pulsar surveys designed at finding more millisecond pulsars; • Algorithm development, such as improved methods for RFI detection and excision or improved pulsar timing precision; or • VLBI surveys and observations to improve our knowledge of the supermassive black hole binaries thought to be the sources of low frequency gravitational waves. 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 two years, with a third year extension for satisfactory accomplishments in the first two years. 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. Each year, deadlines for submission to the NRC are February 1, May 1, and August 1. The current award stipend is $69,764 per year. US citizenship or permanent residency is required. Applications may be submitted at http://www.nationalacademies.org/rap/). For further information contact Dr. Joseph Lazio at the above address; see also the NRL SNe/SNR/LFRA site. EOE/AAE.

No. 25584
RESEARCH ASSOCIATE
NRC HERZBERG INSTITUTE OF ASTROPHYSICS (NRC-HIA), DOMINION ASTROPHYSICAL OBSERVATORY (DAO)
Tel:
URL1: English: http://careers-carrieres.nrc-cnrc.gc.ca/main_e.html
URL2: French: http://careers-carrieres.nrc-cnrc.gc.ca/main_f.html
Email Inquiries: Gerald.Schieven@nrc-cnrc.gc.ca

Attention:
The National Research Council of Canada’s Herzberg Institute of Astrophysics (NRC-HIA) has an opening for a Research Associate working with the Millimetre Astronomy Group (MAG) for the James Clerk Maxwell Telescope (JCMT). The position is to be based at the Joint Astronomy Centre in Hilo, HI, USA.

The Research Associateship 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). The successful candidate will carry out a program of high-caliber astronomical research, which includes use of the SCUBA-2 sub-millimetre camera at the Joint Astronomy Centre.

In addition to highly competitive benefits and salary, Research Associates 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.

The Research Associateship is offered to an outstanding recent doctoral graduate in astronomy/astrophysics. Applicants must have acquired their PhD within the last five years or expect to obtain the degree before starting the Associateship in 2009. Application should be made by 17 August 2009, via the process described in the poster for competition 40-08-22-1 at the above noted URL address.

Please note that you must submit a statement of proposed research, which includes the use of the SCUBA-2 sub-mm camera, along with your cv, cover letter, publication list, and at least two letters of reference. For further information about the facilities and research programmes at DAO, please contact Gerald.Schieven@nrc-cnrc.gc.ca. A starting date of late 2009 is envisaged.

NRC is an equal opportunity employer.

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

No. 25588
Postdoctoral Research Associate in cosmology/astrophysics
UNIVERSITY OF ILLINOIS
Physics Department
1110 W. Green St.
Urbana, Illinois 61801
USA
Tel: 217-333-8174
FAX: 217-333-4990
Email Submission Address: jjt@illinois.edu
Email Inquiries: jjt@illinois.edu

Attention: Jon Thaler, Professor of Physics and Astronomy
The High Energy Physics Group of the University of Illinois at Urbana-Champaign invites applicants for a Postdoctoral Research Associate position to work on the Dark Energy Survey (DES) project. DES is upgrading the Blanco 4-m telescope at CTIO in Chile. It will undertake a sky survey in order to study the properties of the dark matter and dark energy. First light is scheduled for early 2011. These websites have more information about the project: https://www.darkenergysurvey.org/the-project http://cosmology.uiuc.edu/DES/

Our group is in charge of the mountaintop software and some of the electronics. We are looking for a post-doc candidate who has experience with data acquisition software (hardware experience is secondary). The work will involve the specification and implementation of the data transport and control of the Dark Energy Camera (DECam).

A Ph.D. is required for this position. Applicants should have programmed in C or C++. Experience with scripting, data transport in a UNIX environment, and user interfaces is desirable, but not required.

We do not require that candidates have prior astrophysics experience. However, our group is actively involved in the supernova analysis, and also plans to work on large-scale structure. We expect that the successful candidate will join one of DES's science working groups.

The position is available September 1, 2009 (negotiable). The review of applications will begin on June 1, and the search will continue until the position is filled. We expect this to be a two-year position with the possibility of renewal for an additional one-two years. Renewal will be dependent on funding availability.

Applicants should submit a CV, a list of publications, a brief statement of research interests and arrange for at least three letters of recommendations to be sent via e-mail to Donna Guzy at dguzy@illinois.edu .

For more information, please contact: Jon Thaler jjt@illinois.edu 217-333-8174

The University of Illinois is an affirmative action, equal opportunity employer and encourages applications from women and minorities.

No. 25145
Postdoctoral Fellowships in Astrophysics
NAVAL RESEARCH LABORATORY
4555 Overlook Ave., SW
Washington, DC 20375
USA
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 two years. 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. 25561 (New)
PhD Scholarships - Astronomy & Astrophysics
MACQUARIE UNIVERSITY/ANGLO-AUSTRALIAN OBSERVATORY
167 Vimiera Road
Eastwood, NSW 2122
Australia
Tel: 61 2 93724863
FAX: 61 2 93724860
URL1: http://www.astronomy.mq.edu.au
URL2: http://www.astronomy.mq.edu.au/jobs/
Email Submission Address: jobs@aao.gov.au
Email Inquiries: qap@ics.mq.edu.au

Attention: Suzanne Tritton, Personnel Officer
The rapidly expanding Astronomy Group at Macquarie University now invites applications for seven PhD scholarships on a variety of research topics, including planetary nebulae, massive black holes, binary stars, galactic archaeology, dwarf galaxies, astronomical instrumentation/photonics and astronomy/science education.

Successful applicants will be supervised within the Astronomy and Astrophysics Concentration of Research Excellence (CORE) and the Photonics CORE at Macquarie, whose faculty includes Orsola De Marco, Jon Lawrence, Quentin Parker, Mark Wardle, and Daniel Zucker. (see http://www.astronomy.mq.edu.au/ )

Macquarie University is a dynamic research and teaching institution located on a park-like campus in Sydney, Australia, a lively, culturally-diverse city with a warm climate and a very high standard of living. Macquarie University astronomy also benefits from its very close proximity to the headquarters of the Anglo-Australian Observatory (AAO) and the Australia Telescope National Facility (ATNF); several Macquarie faculty members hold joint AAO appointments, and Macquarie PhD students have access to the expertise and research resources of the AAO/ATNF and opportunities for co-supervision by AAO astronomers.

Eligible applicants will be high calibre students of any nationality who should have the equivalent of an Australian 1st class honours degree in a relevant field. Scholarships provide tuition and a tax-exempt stipend.

For details on potential research projects and scholarship terms and links to the application process see: http://www.astronomy.mq.edu.au/jobs/

The deadline for receipt of applications, supporting materials and letters of reference is Friday, May 29th 2009.

No. 25628
Extragalactic Astronomy
DIAS SCHOOL OF COSMIC PHYSICS
31 FitzWilliam Place
Ireland
Tel: +353-1-7005866
FAX: +353-1-7005384
Email Submission Address: ejameurs@gmail.com
Email Inquiries: ejameurs@gmail.com

Attention: Prof. E.J.A. Meurs
PhD position in extragalactic astronomy.

Applications are invited for a PhD Scholarship in the DIAS School of Cosmic Physics to work with Prof. E.J.A. Meurs in the area of extragalactic astronomy. PhD projects are observational/interpretative in character, may involve model simulations; areas of interest include Gamma Ray Bursts, young galaxies, high-energy sources in nearby galaxies, and active galactic nuclei.

Applicants should have a degree in Astronomy and/or Physics. Remuneration is according to standard DIAS scales, plus a provision towards fees (the successful candidate has to register with one of the universities). Prospective starting date is September or October 2009.

Applicants should include a CV and the names and contact details of two academic referees. Submissions are requested by 31 July 2009. For further information contact Prof. E.J.A. Meurs, ejameurs@gmail.com, to whom also applications are to be submitted.

No. 25666
Radio Astronomy Instrumentation and Operations for OVRO
CALIFORNIA INSTITUTE OF TECHNOLOGY
PO Box 968
Big Pine, CA 93513
USA
Tel: (760) 938-2075
URL1: http://www.mmarray.org
URL2: http://www.ovro.caltech.edu
Email Inquiries: jmc@astro.caltech.edu, dbock@ovro.caltech.edu

Attention: Mary Daniel, Administrative Assistant
The California Institute of Technology invites applications for a staff position at the Owens Valley Radio Observatory (OVRO). We specifically seek applicants who will contribute to the continued development of the Combined Array for Research in Millimeter-wave Astronomy (CARMA) interferometer. We encourage candidates who can design new instruments for CARMA and/or improve the mechanical performance of the array. The candidate will need to work with scientists throughout the CARMA partnership in monitoring array operations.

The successful applicant will have technical/engineering experience with one or more of the following qualifications: (1) experience in the design, fabrication and operation of instruments in the frequency range from 30 to 300 GHz; (2)experience in both mechanical and electronics design; (3) a good understanding of interferometry techniques, and the ability to collect and analyze the complex data produced by millimeter-wave interferometers; and (4) the ability to work as part of a small team on some projects as well as ability to lead a team. A PhD in Engineering, Physics, Astronomy, or related discipline is preferred.

CARMA is a heterogeneous interferometer consisting of 10.4 m, 6.1 m and 3.5 m antennas that operates in the 1cm, 3mm, and 1mm atmospheric windows. The primary science areas carried out with CARMA are cosmology studies from the Sunyaev-Zel'dovich effect toward galaxy clusters, the evolution of molecular gas and dust in galaxies, the formation of stars and circumstellar disks, and the composition of planetary atmospheres and comets. The technical developments under way at CARMA span from state-of-the-art SIS and MMIC receivers to a new generation of multi-GHz digitizers and correlators.

For full consideration, apply online at http://www2.recruitingcenter.net/clients/CalTech/publicjobs/controller.cfm for position # CIT15317 by July 1, 2009, but later applications will be considered. Further information regarding this position can be obtained from John Carpenter (jmc@astro.caltech.edu) or Douglas Bock (dbock@ovro.caltech.edu).

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

No. 25707 (New)
Associate Director for Science Operations
GEMINI OBSERVATORY
Tel:
URL1: www.gemini.edu

Attention: gemini-jobs@gemini.edu
The GEMINI OBSERVATORY is seeking a senior astronomer for the position of ASSOCIATE DIRECTOR FOR SCIENCE OPERATIONS. The successful applicant will provide scientific direction and oversight of the Observatory’s science systems and will work closely with the Heads of Science Operations for Gemini South and Gemini North to ensure consistency of science operations across the two sites. Requires working as part of the high-level management team of the Observatory to maintain an effective, streamlined and standardized observing process at both Gemini Telescopes.

The position provides overarching scientific management of new science operations systems under development at Gemini. This includes the new Data Flow System and Products Project that involve data flow management, data reduction tools and the Gemini Science Archive. This position also manages Gemini’s Adaptive Optics Science Team which has members as both sites. Through his/her leadership role in the science staff and the operations development program, this key member of the senior management team of the Observatory will participate in defining Gemini’s evolving strategic vision.

Ph.D. astronomers actively pursuing research with experience in science and data systems management who are invigorated by and are willing to take on a new challenge are invited to apply. The desired starting date for the position is April 2010. The appointment is at the senior scientist level and is based in La Serena Chile. Under exceptional circumstances, a candidate wishing to be based in Hilo, Hawaii may be considered. This position requires extensive travel and extended stays in Hilo, Hawaii. The successful candidate will have time available for astronomical research focusing on areas in which Gemini can make a major impact.

The selected candidate will be an employee of AURA, which provides an excellent compensation and benefits package. Send current resume and research statement along with cover letter relating your experience and education to the needs of the position. Please include the names and contact information of three individuals familiar with your work and credentials from whom a reference may be obtained.

The consideration and evaluation of candidate materials will begin September 1, 2009 and will continue until the search has concluded.

EOE/AA

No. 25695 (New)
Scientific Cluster Administrator and Programmer
CANADIAN INSTITUTE FOR THEORETICAL ASTROPHYSICS (CITA)
60 St. George St
University of Toronto
Toronto, ON M5S 3H8
Canada
Tel: 416-978-5610
FAX: 416-978-3921
Email Submission Address: banhdon@cita.utoronto.ca
Email Inquiries: office@cita.utoronto.ca

Attention: Don Banh, Computing Facility Manager
In co-ordination with the Computing Facilities Manager and members of the computing committee, the incumbent will provide system administration and programming support to enable scientific research on CITA's high-performance, 1,600 core linux cluster and to operate and maintain other departmental systems. Major duties include maintaining, upgrading and modifying the cluster hardware, OS, compilers and software applications (including massively-parallel scientific codes) for optimal performance. The incumbent will provide programming support by advising and assisting researchers with numerical algorithms, compiler issues, serial and parallel programming techniques, debugging, porting, and optimizing scientific codes on parallel supercomputing platforms; and organizing and leading seminars and workshops on cluster usage and parallel programming for researchers and students. Additional duties will include assisting with system administration of departmental servers, workstations, network switches, firewalls, website etc.

B.Sc. in computer science, physics, engineering or an equivalent combination of education and experience is required as well as at least two years' related systems administration and programming experience. Ability to interface with parallel astrophysical programming needs, including massively parallel system configuration and programming is preferred. Experience in Redhat/Fedora/CentOS Linux operating system is preferred. Experience with RAID storage solution and cluster specific network configuration is preferred. Experience in programming languages of C, Fortan, Bash, Python is preferred. Experience with GPU programming in Nvidia CUDA/ATI OpenCL/Intel Larrabee is an asset but not required. Certification in RHCE, CCNA, CCNP is an asset but not required.

Salary range is $58,090 to $74,225 plus benefits.

Send resume, cover letter and contact details of three references from whom letters of reference may be obtained. Deadline to apply: July 31, 2009.

No. 25713 (New)
Astronomy Laboratory Supervisor
UNIVERSITY OF TEXAS AT ARLINGTON
Department of Physics
Box 19059
Arlington, TX 76019
Tel: 817-272-9041
FAX: 817-272-3637
Email Submission Address: jackymack@uta.edu
Email Inquiries: jackymack@uta.edu

Attention: Margie Jackymack, Administrative Assistant II
Supervise astronomy labs. Manage operation and administration of lab, oversee equipment maintenance, and preparation of laboratory setups. Develop and implement new experiments and instructional lab planetarium activities. Support instructional programs associated with the astronomy laboratories. Maintain major instrumentation and equipment. Support lab section teaching activities and instruct/prepare teaching assistants, as required. Train and supervise student laboratory assistants. Collaborate with Planetarium Director in public outreach and functions of the planetarium. Maintain involvement in professional activities, including visits to McDonald Observatory, workshops and related activities. Particiaption in activities related to the Planetarium. Required qualifications are a bachelor's degree, astronomy laboratory experience, and computer programming competency. Preferred qualification are a degree in Physics, Astronomy or related disciplines, Planetatium experience, public speaking experience, and astronomy laboratory experience with teaching component.

Please go to the website: http://utdirect.utexas.edu/pnjobs/pnjobs.WBX, and apply for the position Astronomy Laboratory Supervisor, posting number 09-06-29-01-4439.

No. 25621
IT Specialist (Data Specialist)
SMITHSONIAN ASTROPHYSICAL ABSERVATORY
60 Garden Street
MS-17
Cambridge, MA 02138
USA
Tel:
URL1: http://cfa-www.harvard.edu/hr/postings/29-29.html
Email Submission Address: saoresumes@cfa.harvard.edu
Email Inquiries: saoresumes@cfa.harvard.edu

Attention: Recruiter #461, Job Posting #29-29
IT Specialist (Data Specialist) Trust Fund (Non-Federal)

Interested in space science and technology? Since its launch on July 23, 1999, the Chandra X-ray Observatory has been NASA’s flagship mission for X-ray astronomy, taking its place in NASA’s fleet of ìGreat Observatoriesî. Join our team in the Chandra X-ray Center’s Director’s Office and perform a variety of computer-related duties in support of the Chandra mission and research related to Chandra data. Work involves interacting with and supporting Chandra observers and proposers as they prepare their proposals, plan observations, and obtain and analyze their data. Support is provided via email, web-pages and personal interactions. It also includes supporting and attending meetings, conferences and workshops, for example the AAS and the Chandra Peer Review.

To view the complete vacancy announcement and qualification requirements, please view our website at: http://cfa-www.harvard.edu/hr/postings/29-29.html

Interested candidates should submit resumes to Recruiter #461, Job Posting #29-29, 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 outlining their education, software, and research experience by 1) briefly relating research projects and their objectives, and 2) describing how specific 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. 25646
Staff or Postdoc position in ALMA Science
UNIVERSITY OF BONN
Auf dem Huegel 71
Bonn, D 53121
Germany
Tel: +49 228 733658
FAX: +49 228 731775
URL1: http://www.astro.uni-bonn.de/english/index.php (Argelander Institute for Astronomy)
URL2: http://www.astro.uni-bonn.de/ARC/ (Bonn-Cologne-Bochum ARC Node)
URL3: http://www.eso.org/sci/facilities/alma/arc/ (European ARC)
Email Submission Address: chstein@astro.uni-bonn.de
Email Inquiries: bertoldi@astro.uni-bonn.de

Attention: Christina Stein-Schmitz, Institute Secretary
Applications are invited for a position on ALMA-related science at the Argelander Institute for Astronomy. At the Bonn ARC node the successful candidate will join a growing submillimeter-interferometry research group, which has scientific interests ranging from galaxy evolution to star formation and evolved stars. The staff members of the ARC node are involved in a number of ongoing programs using observational facilities such as APEX, NANTEN2, Herschel, IRAM, SMA and eMerlin - including a number of key and legacy programs at these facilities. The successful candidate shall follow a strong research program that is related to the scientific mission of ALMA.

The applicant should have experience in (sub)millimeter or radio wavelength observations. He/she is expected to participate in the technical and scientific preparation for ALMA at the ARC node, e.g., by helping to define and pursue early science programs. He/she will have the opportunity for extended visits to the Joint ALMA Office in Chile to participate in ALMA commissioning.

Depending on the experience and qualifications of the applicant the position may be at the postdoc or staff scientist level.

Applicants should send (preferably as a single pdf) a CV, publication list, description of research interests, and arrange for the submission of three letters of recommendation to the above address. Applications will be accepted until the position is filled. Women and minorities are particularly encouraged to apply.

No. 25667
Data Process Developer
GEMINI OBSERVATORY
Tel:
URL1: www.gemini.edu

Attention: gemini-jobs@gemini.edu
DATA PROCESS DEVELOPER

Gemini Observatory has an immediate opening for a Data Process Developer to join our international team operating two of the world’s premier ground-based telescopes in Hawaii and Chile. We are looking for a talented individual to join our multidisciplinary team at Gemini North in Hilo, Hawaii. The Data Process Developer is a part of an international team of six people based in Hawaii and Chile.

The Data Process Developer will develop and test Gemini data reduction software for Gemini’s suite of cutting-edge instruments. He or she will contribute to the design, development, and deployment of the data processing node of the Dataflow Project. The current focus of the Dataflow Project is the creation of a reliable and powerful quality assurance and science quality data processing pipeline. The Data Process Developer will also help maintain the current IRAF, PyRAF, and Python data reduction software. Additional responsibilities will include providing support to users of the Gemini data reduction software as well as preparing public and internal releases of the software. The Gemini data reduction software is a critical component of the daily operations, and it is a tool that a large fraction of the Gemini user community relies on to prepare their data for science analysis.

Bachelor’s degree in Astronomy, Physics, Computer Science or related field is required; a master’s degree is preferred. Must be familiar with astronomical data and have experience working with UNIX/Linux, Programming experience in Python or C/C++ is essential. Must have experience programming for IRAF or PyRAF. Knowledge of astronomical data reduction techniques is preferred.

Gemini North head quarters are 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. Send resume, cover letter and contact details of three references from whom letters of reference may be obtained. Please specify the AAS Job Register number on your application. AA/EOE.

No. 25669
Test Scientist - ALMA
NATIONAL RADIO ASTRONOMY OBSERVATORY (NRAO)
Tel:
URL1: https://careers.nrao.edu (Test Scientist-ALMA)

Attention: Human Resources
The Atacama Large Millimeter/sub millimeter Array (ALMA) is an international collaboration to construct and operate a large sub millimeter - millimeter wavelength interferometer array of radio telescopes in the Atacama Desert of northern Chile. The ALMA observatory will consist of an array of 12m and 7m diameter antennas located on the Chajnantor Altiplano at 5000m altitude. ALMA will be equipped initially with dual-polarization receivers covering up to ten atmospheric windows: from 31 to 950 GHz. For more details see http://www.alma.cl/ .

ALMA construction and operations are led on behalf of North America by the National Radio Astronomy Observatory (NRAO), which is managed by Associated Universities, Inc. (AUI) and on behalf of Europe by ESO. Japan is also a major participant in the international ALMA collaboration and will provide major enhancements to the North American and European program. Japan’s effort is led by the National Astronomical Observatory of Japan (NAOJ) in cooperation with Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) in Taiwan.

ALMA is opening positions for Test Scientists to participate in system tests during the Assembly, Integration and Verification processes. The successful candidates will be part of the team responsible for ensuring that appropriate testing has been accomplished to verify that the system requirements have been met. These positions will develop qualification tests, analyze test results and approve reports. They support routine tests on antennas, such as holographic measurement and optical pointing, by performing data analysis, developing automated control and reduction scripts, and training operators, engineers and technicians. They also develop and execute tests to characterize integrated interferometric system behavior, including radiometric pointing, antenna and beam characterization, surface shape change with elevation, path delay, phase stability, bandpass stability changes, etc.

During array commissioning, Test Scientists will work with the engineering staff to develop tests and provide the analysis needed to help resolve problems with system performance. They will also work with the commissioning team to define tests needed to validate the system. Test Scientists are expected and encouraged to conduct active astronomical research programs.

These positions require an advanced degree in engineering, physics or astronomy at the Doctoral level; at least three years observational experience with radio astronomy, observing techniques, and data reduction; experience in techniques used in radio astronomy observations; experience in software development for astronomical applications (C++, Python); experience with and understanding of microwave and digital systems; experience with and understanding of aperture synthesis arrays; experience in techniques used in radio astronomy observations; experience working in a team environment. In addition, skills in C++, Python; a working knowledge of or willingness to learn Spanish; and a high level of communication and negotiation in English is preferred; willingness to travel to the ALMA sites near San Pedro de Atacama and abroad.Due to frequent travel requirements and work at high altitudes, a successful high altitude medical check is a necessary condition of employment for this position.

The positions are based in Santiago de Chile and will require frequent traveling to the ALMA Operational Support Facility near San Pedro Atacama.

Applicants can apply online at https://careers.nrao.edu and should include a description of relevant experience, curriculum vitae, and a cover letter. NRAO requires three letters of reference, which should be sent directly to tbrache@alma.cl. Applicants applying through ESO may do so online at https://jobs.eso.org or by sending the application to the ESO Personnel Office, Karl- Schwarzschild-Str. 2, Garching, D-85748 Germany. ESO requires three letters of reference which may be sent to vacany@eso.org. Review of applicants will begin on 14 July 2009; however, applications will be accepted until the position is filled.

For further information, please consult the NRAO web page at http://www.nrao.edu or the ESO Home Page at http://www.eso.org/ NRAO and ESO are Equal Opportunity Employers. M/F/D/V.

No. 25672
Data Process Developer
GEMINI OBSERVATORY
Tel:
URL1: www.gemini.edu

Attention: gemini-jobs@gemini.edu
Gemini Observatory has an immediate opening for a Data Process Developer to join our international team operating two of the world’s premier ground-based telescopes in Hawaii and Chile. We are looking for a talented individual to join our multidisciplinary team at Gemini North in Hilo, Hawaii. The Data Process Developer is a part of an international team of six people based in Hawaii and Chile.

Gemini offers an attractive and competitive salary and benefit package. Gemini North head quarters are 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. Send resume, cover letter and contact details of three references from whom letters of reference may be obtained. The position will remain open until filled. Please specify the AAS Job Register number on your application. AA/EOE.

American Astronomical Society

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