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. 24589 (New)
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No. 24642 (New)
Senior Electronics Engineer
GEMINI OBSERVATORY
Tel:
URL1: www.gemini.edu

Attention: gemini-jobs@gemini.edu
At Gemini Observatory, it is our mission to teach humanity about the universe. Come join our international team operating two of the world’s cutting-edge telescopes, located in Hawaii & Chile.

We have an immediate opening in Hilo Hawaii, for an experienced Electronics Engineer to support electronic operations and future development. As well as supporting our operations you will be responsible for establishing and organizing a CCD/IR detector lab, as a technical centre. Major responsibilities will include: You will be responsible for the maintenance, troubleshooting and optimization of the controllers and optical and infrared light detector systems at both Gemini telescopes. Additionally, the successful candidate will provide support for and engage in instrument procurement of cryogenics, vacuum, detectors and motor control systems. On an intermittent basis the Senior Electronics Engineer will also provide managerial oversight, including but not limited to, acting as Telescope Technical Manager.

The successful candidate will have: Bachelor’s degree in Engineering/Electronics/related field; Advanced knowledge of astronomical instrumentation and optical and infrared detector systems; and six years relevant work experience.

Must be able to work at 14,000-foot elevation, possess a valid driver’s license, have a clean driving record, and be able to drive a 4WD vehicle. Must have or be able to obtain a valid passport for international travel.

We have an excellent benefits package including 24 paid vacation days and 12 paid holidays per year, paid relocation, life insurance, 401(a) and 403(b) retirement plans, tuition assistance, long term disability insurance, travel/accident insurance, flexible spending account, and medical and dental insurance.

How to Apply, please your resume along with the names of 3 references familiar with your work and salary history to gemini-jobs@gemini.edu

AA/EOE

No. 24643 (New)
Contract Professor
SEOUL NATIONAL UNIVERSITY
BK21 Frontier Physics Division, Dept. of Physics and Astronomy
Seoul National University, NS59
Seoul, -- 151-742
KOREA
Tel: +82-2-880-6623
FAX: +82-2-876-3973
URL1: http://astro1.snu.ac.kr/home/eng/Introduction/popup.html
Email Submission Address: bk21@phya.snu.ac.kr
Email Inquiries: bk21@phya.snu.ac.kr

Attention: Bon-Chul Koo, Prof.
Applications are invited for a contract professor position at the Astronomy Program, the Department of Physics & Astronomy of the Seoul National University in Seoul, Korea. Applicants from all fields of Astronomy are encouraged to apply. All applicants must have a Ph.D. in a related field with one year or more of postdoctoral experience, and meet all the requirements of the Seoul National University hiring policy. The appointment is initially for 2 years, but extendable for additional 2 years contingent upon the research productivity. Interested applications must send CV with current e-mail address and a full list of publications, two copies of the application form (available at the job announcement web page), statement of major research accomplishments and awards, statement of research objectives, two letters of recommendation, and other documents as described in the job announcement which provides more details on the position ( http://astro1.snu.ac.kr/home/eng/Introduction/popup.html ). The application deadline is May 31, 2008, and the expected date of appointment is September 1 (negotiable). The application materials must be submitted to BK21 Frontier Physics Research Division, Department of Physics and Astronomy, Seoul National University, NS59, Seoul 151-742, KOREA. The recommendation letters may be mailed directly to Director, BK21 Frontier Physics Research Division, Department of Physics and Astronomy, Seoul National University, NS59, Seoul 151-742, KOREA, or to e-mail: bk21@phya.snu.ac.kr, Fax: +82-2-876-3973.

Further questions should be directed to bk21@phya.snu.ac.kr

No. 24648 (New)
Senior Optical/Laser Engineer - Job Code ENG403PA
GEMINI OBSERVATORY
Tel:
URL1: www.gemini.edu

Attention: gemini-jobs@gemini.edu
At Gemini Observatory, it is our mission to teach humanity about the universe. Come join our international team operating two of the world’s cutting-edge telescopes, located in Hawaii & Chile.

We are seeking a talented Senior Optical/Laser Engineer to support the laser guide star facility, adaptive optics and instrumentation systems, and telescope operation at the Gemini Observatory in Hilo, Hawaii.

Responsibilities will include: - Optical systems team leader at Gemini North: supervision of a team of 4 engineers and technicians, interface with scientific staff. - lead and improve Laser Guide Star Facilities (LGSF) operation at Gemini North. The LGSF consists of a state-of-the art 12W solid-state 589nm laser propagated to the sky to form an artificial star. - participate in LGSF commissioning at Gemini South (50W). - Lead optics-related operational and development projects through internal and/or contracted efforts (for example active optics and image quality improvements); providing project engineering support; providing technical representation on the purchase of optical-related equipment; preparing documentation, schedules, and maintenance procedures; participating in design reviews (in particular in the suite of new exciting instruments, some including high-tech AO systems, like GPI).

The successful candidate will have: - BS in Optics/Laser/Engineering/Physics/related field - knowledge of optical design, laser and their operation, analysis software applications and a minimum of 3 years optical or laser engineering experience. - self-starter spirit with excellent leadership skills and the ability to work autonomously - Telescope or adaptive optics experience is preferred. - ability to work with various alignment tools, electronics systems, detectors, hardware, software and optical instruments.

To apply, please send you resume together with the names of 3 professional references and recent salary history to: gemini-jobs@gemini.edu AA/EOE.

No. 24649 (New)
Senior Electronics Engineer - Job Code ENG209PA
GEMINI OBSERVATORY
Tel:
URL1: www.gemini.edu

Attention: gemini-jobs@gemini.edu
At Gemini Observatory, it is our mission to teach humanity about the universe. Come join our international team operating two of the world’s cutting-edge telescopes, located in Hawaii & Chile.

How to Apply, please send your resume along with the names of 3 references familiar with your work and salary history to gemini-jobs@gemini.edu

AA/EOE

No. 24650 (New)
High-Level Software Engineers - Hilo, Hawaii & La Serena, Chile ENG713PS
GEMINI OBSERVATORY
Tel:
URL1: www.gemini.edu

Attention: gemini-jobs@gemini.edu
At Gemini Observatory, it is our mission to teach humanity about the universe. Come join our international team operating two of the world’s cutting-edge telescopes, located in Hawaii & Chile.

Gemini Observatory is seeking highly skilled and experienced software developers in Hilo, Hawaii and La Serena, Chile to become part of its High-Level Development Group (HLDG). The High-Level Group develops tools that astronomers use to plan and execute observations, process data, and control observatory hardware. The successful candidate will join a small but motivated international team focused on providing a user experience to match the world-class telescopes and instruments that Gemini provides to the research community.

We develop almost exclusively in Java, delivering web applications, Swing desktop applications, and distributed backend services. We employ RMI and Jini technologies, XML, XML-RPC, and web services among others. Our applications are built on the OSGi platform.

The job is development-oriented, but also includes maintenance and refactoring of an existing code base. We work as part of a multi-disciplinary engineering team, and communicate with scientists on a daily basis to understand their requirements and translate them to working solutions.

Qualifications: • A degree in Computer Science or equivalent experience (an advanced degree is preferred) • At least five years of software development experience, with demonstrated problem solving skills • Solid object-oriented design and development experience in Java • Knowledge of design patterns • Familiarity with developing in UNIX-like operating systems such as Linux or OS X • Proven track-record of providing technical leadership for large-scale applications in distributed environment Must be willing to work with a geographically distributed team. Excellent written and verbal skills in English are required, and Spanish language skills are a bonus. Must have, or be able to obtain, a valid passport and be willing to travel internationally, as required.

How to Apply, please send your resume along with the names of 3 references familiar with your work and salary history to gemini-jobs@gemini.edu

No. 24653 (New)
Editor
ASTRONOMY EDUCATION REVIEW
Tel:
Email Submission Address: timslaterwyo@gmail.com

Attention: Tim Slater, Chair AER Editor Search Committee
The American Astronomical Society is soliciting applications and nominations of candidates for the position of Editor of the Astronomy Education Review (AER). This person will replace the current Editor, Sidney Wolff, who is stepping down at the end of 2008. The AER is internationally known as the pre-eminent scholarly journal in astronomy education and research, and the new Editor will be responsible for enhancing the excellence of the Journal. The AAS Council has selected a Search Committee to fill this position, chaired by its Education Officer, Tim Slater.

The Search Committee has identified the following qualifications that must be satisfied by the successful applicant:

1. Recognized stature and achievement in astronomy and/or science education.

2. Experience with diplomatic management of peers, staff, or students.

3 A clear vision for the future of the AER.

4. Familiarity with budgets.

5. Experience as a referee.

6. Previous editorial experience would be useful but is not required.

The Editor is responsible for building and maintaining a cadre of referees and assigns most manuscripts submitted to the referees, assesses the referee's reports and recommends the papers for publication. The Editor is responsible for maintaining the efficient and timely flow of manuscripts. As part of this process, this person will also:

1. Actively recruit authors and referees.

2. Interface with the AAS Journals Manager.

3. Participate in the establishment and management of the Journal Budget.

4. Report to the Publications Board and the AAS Council on the status of the AER.

The Society expects to compensate the Editor at roughly $10,000 per year paid as a stipend and performance will be reviewed annually by the publications board. No additional infrastructure will be provided. Specific questions about the historical operations of the journal to date can be addressed to Sidney Wolff, swolff@noao.edu.

Candidates for this position should submit a cover letter, CV, bibliography, and names and contact information of three references to Tim Slater, Chair of the AER Editor Search Committee, at the above address. Email submission of PDF files is encouraged to timslaterwyo@gmail.com using AER Editor Search as subject line.

Nominations for the position may also be sent to the same address.

Selected candidates will be asked to provide evidence of institutional support for their assuming the above editorial duties.

The cover letter should address the candidate's qualifications, reason for interest in the position, for the operation, management, and future of the AER. In accordance with the Bylaws of the Society, the Search Committee will make its recommendations to the AAS Publications Board and AAS Council. The final selection is made by the Council. Application and nominations received by 15 June 2088 will be given full consideration. AAE/EOE.

The current website of the Astronomy Education Review is http://aer.noao.edu.

No. 24658 (New)
Astronomy/Astrophysics one year, full-time visiting position
BENNINGTON COLLEGE
One College Drive
Bennington, VT 05201
USA
Tel: 802-440-4460
FAX: 802-440-4461
Email Submission Address: jwatson@bennington.edu
Email Inquiries: jwatson@bennington.edu

Attention: Jo-Ann Watson, Program Coordinator
Bennington College, a small liberal arts college in southwestern Vermont, is seeking an astrophysicist or astronomer for a one-year, full-time visiting position beginning in the fall of 2008. Teaching responsibilities will include introductory physics and other classes in area of interest, ranging from intermediate level to more general interest.

Bennington College encourages innovation in curricular development and invites creative approaches to course design. All courses may be designed around candidate’s particular interests and specialties. The College maintains an observatory housing a 16-inch reflecting telescope with recently upgraded control systems and software. Bennington’s calendar includes a seven-week internship term from January through February with no teaching obligations. Candidates should have Ph.D. or be near completion of degree or have significant pertinent professional experience.

Submit application materials, including CV and a brief statement of teaching interests and approaches to Jo-Ann Watson, Science/Math Program Coordinator, Bennington College, 1 College Drive, Bennington, VT, 05201 or e-mail jwatson@bennington.edu. Arrange for two letters of recommendation to be sent directly to the same address. Review of applications will begin May 15, 2008 and continue until the position is filled.

No. 24567
IT Specialist (Data Specialist)
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
60 Garden Street
Cambridge, MA 02138
USA
Tel:
URL1: http://cfa-www.harvard.edu/cfa/hr/postings/28-16.html
Email Submission Address: saoresumes@cfa.harvard.edu
Email Inquiries: saoresumes@cfa.harvard.edu

Attention: Recruiter #461, Job #28-16
IT Specialist (Data Specialist)

The Data Specialists will provide computer-related support to the Chandra X-ray Center's Calibration Group. This group analyzes both space-based and ground based data relating to Chandra instrument performance, provides quantitative calibration information and documentation and interfaces with external Chandra elements, including the scientific community. Primarily the Data Specialist will be involved in software development related to instrument performance for the Low Energy Transmission Grating instrument, developing and analyzing numerical algorithms, data reduction and analysis, documenting and organizing results, and participating in the daily operations of one of NASA's Great Observatories-the Chandra X-ray Observatory

Requirements: * BS/MS or comparable experience in Computer Science, Astronomy, Physics or related field * Knowledge of and experience with UNIX and/or Linux * Experience in computer operations and/or software development in a science environment * Knowledge of a programming language, such as FORTRAN, C, Perl , and HTML * Good communication and interpersonal skills and self-motivational qualities * Knowledge of, databases and data analysis software (e.g., IDL) to extract information * Willingness to support occasional off-hour/weekend responsibilities

For further information and requirements, view the complete Job Vacancy Announcement, at: http://cfa-www.harvard.edu/cfa/hr/postings/28-16.html

Qualified applicants should forward their resume to: Recruiter #461, Job Code #28-16, at the Smithsonian Astrophysical Observatory, 60 Garden St., MS-17, Cambridge, MA 02138, or via e-mail to: saoresumes@cfa.harvard.edu. Please note that this email address is for application materials only.

Applicants who have experience in a research environment are encouraged to augment their resumes by elaborating on their 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.

We are an Equal Opportunity Employer, committed to diversity in our workplace.

No. 24568
IT Specialist (Software Developer)
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
60 Garden Street
Cambridge, MA 02138
USA
Tel:
URL1: http://www.cfa.harvard.edu/hr/postings/28-02.html
Email Inquiries: saoresumes@cfa.harvard.edu

Attention: Recruiter #461, Job #28-02
IT Specialist (Software Developer) Trust Fund (Non-Federal), Temporary $44,897 to $76,989/yr with excellent benefits Salary commensurate with qualifications and experience.

Recent Graduates are Encouraged to Apply

The Virtual Observatory (VO) is an international collaboration aimed at ensuring interoperability of astronomical data from major data archives world-wide.

Work on the VO is at the forefront of data interoperability prototypes and takes advantage of the public availability of rich datasets in astronomy. The Smithsonian Astrophysical Observatory is a partner in the National Virtual Observatory (NVO), a collaboration of US institutions funded by NSF to develop VO infrastructure. SAO's work in the VO collaboration focuses on developing data models, which are at the basis of the VO infrastructure.

The successful candidate's primary focus will be on developing Java classes to instantiate VO data models (Space Time Coordinates and Spectrum). Responsibilities will include software design, development and testing, and user documentation. The incumbent also will install and test VO software developed by other groups, participate in setting up the Harvard-Smithsonian Center for Astrophysics VO node, and work with other SAO and Harvard groups involved in VO software development.

To view the complete vacancy announcement for this position and requirements for higher salary levels, go to http://www.cfa.harvard.edu/hr/postings/28-02.html

Interested candidates should submit resumes to Recruiter #461, referring to Job Posting #28-02, at the Smithsonian Astrophysical Observatory, 60 Garden Street, MS-17, Cambridge, MA 02138, or via email to saoresumes@cfa.harvard.edu. Please note that the email address is for the submission of application materials only. If you are relying on education to qualify, please furnish a copy of your college transcripts. The Smithsonian Astrophysical Observatory is an equal opportunity employer committed to diversity in our workplace.

No. 24579
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Tel:

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No. 24592
Director of SMA Hilo Operations Astrophysicist
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
60 Garden St
Cambridge, MA 02138
USA
Tel:
URL1: http://cfa-www.harvard.edu/hr/postings/
Email Submission Address: saoresumes@cfa.harvard.edu
Email Inquiries: saoresumes@cfa.harvard.edu

Attention: Smithsonian Astrophysical Observatory
Director of SMA Hilo Operations Astrophysicist, GS-1330-15, $95,390 - $124,010 SMA - Smithsonian Astrophysical Observatory

Applications are invited for an outstanding astrophysicist to join the Submillimeter Array (SMA) at its Observatory based in Hilo, HI. All US citizens and Non-Citizens as allowed by appropriations and statute may apply.

The Submillimeter Array (SMA) is a collaborative effort between the Smithsonian Astrophysical Observatory (SAO) and the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) of Taiwan. It is the world's first submillimeter interferometer, and is designed for observations in the major atmospheric windows from 180 GHz to 900 GHz. SAO and ASIAA are currently adding receivers to include the 320 - 420 GHz frequency range, which will enable dual-polarized operation near 350 GHz. Developments underway include a doubling of the array bandwidth for single-receiver operation; upgrades to 650 GHz receiver sensitivity; extension of current polarimetry capabilities; and the addition of a second set of 650 GHz receivers for dual-polarized operation across this band. Looking forward, the SMA group is extremely interested in improving the sensitivity of the SMA at all wavelengths and assessing scientific opportunities enabled by enhancements to the SMA, such as extending interferometric observations down to 200 microns.

The successful candidate will direct the operations of the SMA to ensure that planned scientific observations and engineering tests are carried out efficiently. In addition, the incumbent will provide administrative, technical, and scientific guidance to Hilo-based SMA staff. As an internationally-recognized authority in millimeter or submillimeter radio astronomy, the incumbent will also conduct his or her own program of research in submillimeter observational astronomy and support development of enhanced capabilities for the SMA.

This position requires extensive knowledge of millimeter and submillimeter wavelength astronomy, expertise in the area of aperture syntheses and spectroscopy, and extensive experience providing guidance, leadership, direction, and oversight to staff. Demonstrated leadership skills and the ability to function with others in a research environment are required. The candidate should have knowledge of state-of-the-art astronomical instrumentation and scholarly competence necessary to formulate, conduct, and present the results of programs of advanced research. For further information regarding this position, please visit: http://cfa-www.harvard.edu/hr/postings/

The Smithsonian Astrophysical Observatory is an EEO/Affirmative Action Employer, and encourages women and minorities to apply. Interested applicants should forward a curriculum vita and bibliography, statement of interest, and three professional letters of recommendation to the Smithsonian Astrophysical Observatory, MS-17 (28-19), 60 Garden Street, Cambridge MA 02138 or via e-mail to saoresumes@cfa.harvard.edu . Applications must be received by July 30, 2008.

No. 24608
Receiver Engineer
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
60 Garden St
Cambridge, MA 02138
USA
Tel:
URL1: http://cfa-www.harvard.edu/hr/postings/
Email Inquiries: saoresumes@cfa.harvard.edu

Attention: Smithsonian Astrophysical Observatory
Receiver Engineer

Physicist / Engineer, GS-14/15, $99,347 - $149,000 SMA - Smithsonian Astrophysical Observatory

Applications are invited for a highly qualified physicist or engineer to join the Submillimeter Array at the Smithsonian Astrophysical Observatory in Cambridge, MA.

The successful candidate will lead an effort to implement receiver control hardware and software algorithms to better enable remote operations of the array; will lead the production, testing, installation, and commissioning of receiver instrumentation for the SMA; will coordinate and further develop a test program to verify instrument performance and readiness; and will participate in ongoing and future receiver developments. The incumbent will be expected to help identify, define, and select specific areas of opportunity to guide ongoing development of the SMA. In addition, the incumbent will be expected to provide guidance and assistance to the research activities of work performed by students and technical personnel supporting the development of instrumentation and subsystems for the array, serve on a variety of internal committees, and prepare results of research and developments for publication in scientific and technical journals.

This position requires broad advanced knowledge of physics and astronomy as might be evidenced by a Ph.D. in physics, astronomy, or electrical engineering, plus substantial related or comparable professional experience. Knowledge of submillimeter receiver technology, superconducting mixers, heterodyne receiver systems, and spectroscopy is required. In addition, the incumbent must possess advanced skill in real time control software and have hands-on experience at developing and fielding sophisticated millimeter or submillimeter receiver systems for astronomical observation.

For further information regarding this position, please visit: http://cfa-www.harvard.edu/hr/postings/

The Smithsonian Astrophysical Observatory is an EEO/Affirmative Action Employer, and encourages women and minorities to apply. Exceptionally well qualified candidates may be paid a recruitment bonus. Interested applicants should forward a curriculum vita and bibliography, statement of interest, and three professional letters of recommendation to the Smithsonian Astrophysical Observatory, MS-17 (JP 28-20), 60 Garden Street, Cambridge MA 02138 or via e-mail to saoresumes@cfa.harvard.edu

No. 24614
ASSISTANT ENGINEER
CALTECH/PALOMAR OBSERVATORY
Tel:
URL1: http://www2.recruitingcenter.net/clients/CalTech/publicjobs/controller.cfm?jbaction=JobProfile&Job_Id=14074&esid=az (To apply for this position)

Attention: Caltech HR
ASSISTANT ENGINEER Caltech/Palomar Observatory Salary Grade: 42

Caltech is a small, coeducational university dedicated to exceptional instruction and research in engineering and science. The student body is composed of about 900 undergraduate and 1,000 graduate students who maintain a high standard of scholarship and intellectual achievement. With an outstanding faculty – including several Nobel Laureates – and such off-campus facilities as the Jet Propulsion Laboratory (JPL), Palomar Observatory, and the W. M. Keck Observatory, Caltech is one of the world’s major research centers.

Summary

This position is located at Palomar Mountain Observatory on Palomar Mountain approx. 150 miles south of Los Angeles in North San Diego County.

Works closely with the astronomers using the Hale Telescope to calibrate and operate the instrumentation employed in the research programs and with other observatory engineers to maintain these instruments at peak efficiency. Specifically, this work will entail assisting other engineers to maintain the observatory computers and associated software; testing and repairing instruments; monitoring and recording instrument performance; maintaining manuals and documentation.

Job Duties

• Assist and train astronomers in the operation of telescope instrumentation.

• Troubleshoot, repair and maintain telescope instrumentation and computers.

• Analyze, test, report and log instrumentation performance.

• Update instrumentation manuals and documentation.

• Assist in software maintenance of instrumentation computers.

• Occasionally will act as relief Night Assistant.

• Assist in operation of laser guide star adaptive optics system.

• Other Duties as assigned.

Minimum Requirements

• Requires Bachelor of Science degree in astronomy, physics, or engineering (or equivalent educational experience).

• Familiarity with UNIX and C programming languages is required.

• Must have three or more years experience working with precision optical instrumentation.

• The selected candidate must pass a post-offer physical examination to be hired for this position.

Additional Requirements

• Must be able to work at altitude of 5600 feet. Must be in good physical condition and be able to lift up to 50 pounds of equipment and/or tools.

• Must work holidays as assigned

• Must work evenings as assigned

Knowledge, Skills & Abilities

• Must have good troubleshooting abilities.

• Must have good understanding of optical instrumentation.

• Must be able to read and understand electronic and mechanical drawings.

• Familiarity with UNIX and C programming languages is required.

• Must interface well with supervisors, fellow employees and astronomers.

• Must be a self motivated person with the ability to work with minimum supervision and exercise good judgment as to safety of equipment and personnel.

How to Apply

Caltech offers a competitive salary, commensurate with qualifications and experience, as well as an excellent benefits package. To be considered for this position, please submit your resume at the following link: http://www2.recruitingcenter.net/clients/CalTech/publicjobs/controller.cfm?jbaction=JobProfile&Job_Id=14074&esid=az To view a complete list of Caltech open staff positions, please visit us at www.Caltech.edu.

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

No. 24629 (New)
Reader/Lecturer in Low Mass Stars and Exoplanets
QUEENS UNIVERSITY BELFAST
University Road
Belfast, Northern Ireland BT7 1NN
UK
Tel: +44 2890973044
URL1: http://www.qub.ac.uk/sites/QUBJobVacancies/AcademicJobs/ (Post application Details)
URL2: http://star.pst.qub.ac.uk (QUB Astrophysics Research Centre)
Email Inquiries: a.fitzsimmons@qub.ac.uk

Attention: The Director of Human Resources, Personnel Department
Reader/Lecturer in Exoplanets Ref. 08/100368 School of Mathematics and Physics

The School of Mathematics and Physics at Queen's University Belfast seeks to make an appointment in Astrophysics by July 1st 2008 or as soon as possible thereafter. The position will be at either the Reader or Lecturer level. The successful candidate will be expected to contribute to the teaching, research and administrative activities of the School.

The research interest of the successful candidate will be in the area of Low Mass Stars and Extra-solar Planets (exoplanets), and should complement and extend existing research within the Astrophysics Research Centre. The interests of the current members of the Centre may be found at http://star.pst.qub.ac.uk. In particular, we have a vigorous and highly productive research programme which uses the SuperWASP extra-solar planet detection facility.

Applicants must have a PhD (or equivalent) in Astrophysics or a related discipline, a record of high quality research publications commensurate with experience and the position applied for. They must be able to teach Mathematics and/or Physics at all levels through the medium of English. Demonstrably successful teaching experience in the Higher Education sector is desirable, as is a track record of successful grant applications. For a Readership, teaching experience in the Higher Education sector, a track record of successful grant applications and a record of successful Ph.D. supervision are all essential.

Applicants should clearly state if they wish to be considered for the Reader post, the Lecturer post, or both.

Informal enquiries may be directed to: Professor A.Fitzsimmons, e-mail a.fitzsimmons@qub.ac.uk, telephone +44 (0)28 9097 3124.

An application pack for the post, containing further details of the essential and desirable criteria, as well as instructions on how to submit an application, is available from our website:

http://www.qub.ac.uk/sites/QUBJobVacancies/AcademicJobs/

A PhD studentship has been allocated to work with the successful candidate. In addition, a generous start-up package will be available.

Salary: 27,466-35,837 pounds (AC2), 33,779-44,074 pounds (AC3), 42,791-54,206 pounds (AC4) per annum (including contribution points).

Closing date: 4.00 pm, Friday 6 June 2008.

No. 24640 (New)
Professor of Experimental Physics
MONASH UNIVERSITY
Clayton, Victoria 3800
Australia
Tel:
URL1: http://www.physics.monash.edu.au/ (School of Physics Website)
URL2: http://www.adm.monash.edu.au/human-resources/employment/senior/ (Selection Documentation)
Email Submission Address: bronwen.meredith@adm.monash.edu.au
Email Inquiries: michael.morgan@sci.monash.edu.au

Attention: Ms Bronwen Meredith
Monash University is seeking to appoint an outstanding research physicist or observational astronomer as a Professor of Experimental Physics and future Head of the School of Physics.

Monash Physics aims to position itself as one of the leading Schools of Physics in Australia. The Professor of Experimental Physics is pivotal to achieving this, and will lead the further development of experimental physics within the school.

Based at the Clayton campus, Monash Physics maintains teaching and research programs in astronomy, experimental physics and theoretical physics. It is a major contributor to the Cooperative Research Centre in Biomedical Imaging Development, the ARC Centre of Excellence for Coherent X-ray Science and the base for the Monash Centre for Synchrotron Science. The Australian Synchrotron, which began operation in 2007, is adjacent to the University.

The successful candidate will have: a research doctorate in a relevant discipline, an outstanding internationally recognised record of research in experimental physics; demonstrated success in establishing and leading successful research teams and innovative research programs; a proven capacity to attract competitive research funding; a record of successful supervision of postgraduate students; proven commitment to excellence in teaching and demonstrated skills in management and development of staff.

The appointment as a professor will be on a continuing basis. The school headship is typically rotated on three-year terms and the successful candidate may be required to serve as head within two years of appointment.

Remuneration: professorial salary (currently) $A128,856 per annum, plus generous superannuation. An allowance will be applicable for the role of head of school. Relocation travel, removal allowance and salary packaging are available.

Confidential enquiries regarding the position may be made with Associate Professor Michael Morgan, Head of School: telephone +61 3 9905 3645; facsimile +61 3 9905 3637; email: michael.morgan@sci.monash.edu.au

Applications, which must specifically address all of the selection criteria, should reach Ms Bronwen Meredith, Senior Academic Appointments, Monash University, Victoria 3800, Australia, or by email to bronwen.meredith@adm.monash.edu.au no later than Friday 13 June 2008.

Enquiries regarding the application process may be directed to Ms Meredith, by email or telephone +61 3 9905 6193.

No. 24644 (New)
Assistant prof of physics
THE UNIVERSITY OF PUERTO RICO AT HUMACAO
college Sta
Humacao, Puerto Rico oo791
USA
Tel: 787-850-9381
FAX: 787-850-9308
Email Submission Address: rjmullerporrata@gmail.com
Email Inquiries: rjmullerporrata@gmail.com

Attention: RJ Muller, Chairman, dept of Pysics and electronics
Department of Physics and Electronics The University of Puerto Rico at Humacao Assistant Professor Starting date August, 2008

The Department of Physics of the Univ. of Puerto Rico at Humacao invites applications for a tenure-track position at the Assistant Professor level. The candidate should be ready to pursue an independent research program and effectively teach undergraduate courses of an applied physics program plus the physics courses of an associate degree program in electronics. The areas of interest to the department at present are material science and astronomy/astrophysics. The successful candidate is expected to involve undergraduate students in his (her) research efforts and to communicate in Spanish within a reasonable short period of time (2 years). A PhD in Physics or Astronomy is required; postdoctoral and previous teaching experience will be strongly considered.

Applicants should submit curriculum vitae, a letter describing plans for research, 2 letters of reference and copies of recent publications to Chairman, Department of Physics, The Univ. of Puerto Rico at Humacao, CUH Station, Humacao, PR 00791

The Univ. of Puerto Rico at Humacao is a public, four year co-ed institution located on the east coast of Puerto Rico. It is an equal opportunity /affirmative action employer. Applications from under-represented minorities and women are encouraged.

This announcement is required by the By-Laws of the UPR, #6479, Cert#114, Series 1980-81 from the Council on Higher Education, today Board of Trustees of the UPR, as amended. Approved by the State Elections Commission CEE-C-08-025, submitted 12 Dec 07

No. 24654 (New)
Tenure-Track Faculty Position(s) in Astronomy
UNIVERSITY OF MASSACHUSETTS/AMHERST
Department of Astronomy, LGRT-B 619E
710 North Pleasant Street
Amherst, MA 01003-9305
USA
Tel: 413-545-2194
FAX: 413-545-4223
URL1: http://www.astro.umass.edu (Department Web Site)
Email Submission Address: terri@astro.umass.edu
Email Inquiries: nsk@astro.umass.edu or calzetti@astro.umass.edu

Attention: Astronomy Faculty Search, c/oTerri Grzybowski
TENURE-TRACK FACULTY POSITION(S) IN ASTRONOMY – UNIVERSITY OF MASSACHUSETTS/AMHERST

The Astronomy Department at the University of Massachusetts/Amherst is seeking to fill a tenure-track faculty position(s)at the Assistant or Associate levels with a preference for the areas of theoretical astrophysics and/or extragalactic observational astronomy. We seek individuals whose research will complement and expand the current scientific activities of the department that include studies of interstellar/intergalactic media, galactic structure and dynamics, extragalactic and galactic star formation, galaxy formation and evolution, and large-scale structure and cosmology. The Department will shortly complete the Large Millimeter Telescope (LMT), the world's largest single dish telescope for millimeter-wavelength astronomy in cooperation with Mexico, and a large local computational facility. We particularly encourage applicants that can lead future scientific investigations using either of these major new facilities. Rank and salary will be commensurate with qualifications. Applicants should have a PhD in Astronomy, Physics, or a related field, a strong record of achievement in astronomical research, and a commitment to excellence in undergraduate and graduate education. The start date can be as early as January 2009. Interested individuals should submit a curriculum vitae, a list of publications, and a research statement and also arrange for three letters of recommendation to be sent to the search committee. Review of applicants will begin on July 15, 2008 and continue until the positions are successfully filled. Email Inquires: Neal S. Katz (nsk@astro.umass.edu) or Daniela Calzetti (calzetti@astro.umass.edu).

The University of Massachusetts is an Affirmative Action/Equal Opportunity Employer. Women and members of minority groups are encouraged to apply. The Department is committed to increasing the diversity of the faculty and student body.

No. 24559
Faculty Position in High Energy Density Physics
UNIVERSITY OF ROCHESTER
University of Rochester
Rochester, NY 14627-0171
USA
Tel: (585) 275-4351
FAX: (585) 273-3237
URL1: www.pas.rochester.edu (Department Web Site)
Email Submission Address: shirl@pas.rochester.edu.

Attention: Ms. Shirley Brignall
The Department of Physics and Astronomy at the University of Rochester (www.pas.rochester.edu) is seeking to fill a new tenure track faculty position opening in Experimental High Energy Density (HED) Physics . Candidates whose interests are synergistic with the unique opportunities offered through the Laboratory for Laser Energetics (www.lle.rochester.edu) are particulary encouraged to imply. These areas of interest include, but are not limited to, HED physics, Inertial Confinement Fusion, Laboratory Astrophysics, and high intensity laser-plasma interactions. The Department maintains a strong program in plasma astrophysics and the Laboratory for Laser Energetics is a unique ICF facility that includes the OMEGA 60 beam and OMEGA EP, 4 beam Petawatt laser system.

Each candidate should submit a cover letter of application, a curriculum vitae including a list of publications, and a description of research and teaching plans. The candidate should arrange for at least four letters of recommendation to be sent to: Faculty Search Committee c/o Ms. Shirley Brignall Department of Physics and Astronomy University of Rochester Rochester, New York 14627-0171, USA Applications may also be submitted by email sent to shirl@pas.rochester.edu.

Applications will be considered on an ongoing basis. The University of Rochester has a strong commitment to diversity and actively encourages applications from candidates from groups underrepresented in higher education. The University of Rochester is an Equal Opportunity/Affirmative Action employer and encourages applicants from members of minority groups and women. All applications are considered without regard to race, sex, age, religion or national origin. Salary will be competitive.

No. 24585
Tenure-track position on Galactic Archeology/Near Field Cosmology
ASTROPHYSICAL INSTITUTE POTSDAM (AIP)
An der Sternwarte 16
Germany
Tel: +49 331 7499 381
FAX: +49 331 7499 267
URL1: www.aip.de
Email Submission Address: msteinmetz@aip.de

Attention: Prof. Matthias Steinmetz, Director
The Astrophysikalisches Institut Potsdam (AIP) invites applications for a tenure-track position starting in the fall of 2008. For exceptionally qualified candidates, a tenure appointment may be considered. The successful candidate should have a strong research record in the area of galactic archeology/near field cosmology and is expected to carry out a corresponding independent research programme. She/he is foreseen to head a research group at the AIP and to supervise the AIP involvement in large galactic surveys such as RAVE, SEGUE and GAIA.

The AIP is located in the beautiful Potsdam/Babelsberg area, at the southwestern border to Berlin. About 90 scientists work on a variety of astrophysical topics. The AIP is partner in the LBT project and is developing the high resolution spectrograph/polarimeter PEPSI. It has a strong record in the development of instrumentation for 3D-spectroscopy and is a main partner in the development of the VLT integral field spectrograph MUSE. It leads the international RAVE survey and participates in the SDSS.It is involved in the XMM survey science center and participates in the eRosita mission scheduled to launch in 2010. The AIP is currently establishing a remote station for the LOFAR radio telescope. The AIP coordinates the German AstroGrid and features excellent computer facilities and has access to supercomputers. Potsdam further hosts the Albert-Einstein Institute for Gravitational Physics, the Astronomy department of Potsdam University and several other research institutions.

Applications should be sent with the usual materials, including curriculum vitae and a statement of research interests and perspectives, to the address above by May 31st, 2008. Applicants should arrange for three letters of recommendation to be sent by the same date. Later applications will be considered until all posts are filled.

The AIP is an equal opportunity employer and particularly encourages applications from women.

No. 24607
NRAO Assistant Director - North American ALMA Science Center
NATIONAL RADIO ASTRONOMY OBSERVATORY
520 Edgemont Road
Charlottesville, VA 22903
USA
Tel: 434-296-0312
FAX: 434-296-0202
URL1: http://www.nrao.edu/administration/personnel_office/careers.shtml (Careers page)
Email Submission Address: resumes@nrao.edu

Attention: Human Resources - CV4079 AD NAASC
We seek an outstanding scientific leader to serve as Assistant Director of the North American ALMA Science Center (NAASC), located at the NRAO Headquarters in Charlottesville, Virginia, which will serve the North American users of the Atacama Large Millimeter/Submillimeter Array. ALMA is an international project in which NRAO is a major partner.

The person holding this position will have the overall responsibility for scientific leadership, development, and operation of the Center. The NAASC supports users from proposal submission through data archiving, distribution, and analysis. In addition, the NAASC will solicit community advice on operation and future development of ALMA; sponsor scientific conferences, training programs, schools, and special events that foster development of the user community; participate in the future development of ALMA; and supervise ALMA education and public outreach activities. We seek a person who will provide clear direction and strong leadership in these areas. The NAASC AD reports to the NRAO ALMA Project Director during construction and to the Observatory Deputy Director thereafter.

Candidates are required to have a Ph.D. or equivalent in astronomy, physics, or a related field. Excellent communication and organizational skills are required. Research experience in millimeter-wave interferometry is highly desirable, as is a background in supporting users of astronomical observatories or data/science centers. Prior experience in management and budget development and control is desirable.

NRAO offers competitive compensation, full benefits, and the opportunity to work with talented professional colleagues – some of the best in the field today. For consideration, please send a resume with a cover letter listing three references to: NRAO Human Resources, 520 Edgemont Road, Charlottesville, VA 22903 or send electronically to resumes@nrao.edu. Please reference CV4079-AD NAASC in the subject line. Applications received by April 30, 2008 will receive full consideration. The NRAO is an equal opportunity employer. Women and minorities are encouraged to apply.

No. 24611
Joint ALMA Observatory Project Manager
ATACAMA LARGE MILLIMETER ARRAY
El Golf 40
Piso 18
Chile
Tel: 0056 2 467 6120
FAX: 0056 2 467 6104
Email Submission Address: searchALMApm@alma.cl
Email Inquiries: tdegraau@alma.cl

Attention: T. de Graauw, Interim ALMA Director
The Joint ALMA Observatory(JAO) is seeking a Project Manager with outstanding management abilities for the international ALMA Project in Chile.

The Atacama Large Millimeter/submillimeter Array (ALMA) will be a (sub)millimeter wave interferometer consisting of at least 66 antennas located on the Chajnantor Altiplano in the Atacama Desert of northern Chile at 5000m altitude. Built and operated by a North-American (United States and Canada), European (13 ESO member states) and East Asian (Japan and Taiwan) partnership, in cooperation with the Republic of Chile, ALMA will be equipped with receivers covering at least six atmospheric windows between 30 and 950 GHz. The project, with a budget which exceeds a billion dollars, is being carried out jointly by the European Southern Observatory (ESO), the National Radio Astronomy Observatory (NRAO) managed by the Associated Universities Incorporated (AUI) on behalf of NSF, and the National Astronomy Observatory of Japan (NAOJ) on behalf of the National Institute of Natural Sciences (NINS).

The ALMA Board, consisting of members representing the partners, has created the Joint ALMA Observatory (JAO) in Chile. The JAO is responsible for the overall leadership and management of construction, commissioning and operations of ALMA. The Executives of the three partners have each created an ALMA Regional Center (ARC) to interface between ALMA and the astronomy community.

Under delegation by the Director, the Project Manager is responsible for the overall management and technical direction of the ALMA construction and integration being carried out by the JAO and the three regional (European, East Asian and North American) project managers. The ALMA Project Manager has, inter alias, the responsibility for maintaining the integrity of the project schedule and work breakdown structure, for maintaining the schedule, cost, schedule of values and assignment of deliverables. The Project Manager provides written and oral reports to the ALMA Board and summarizes the state of the project periodically to the ALMA Management Advisory Committee.

Basic requirements for the position include an advanced degree in the physical sciences or engineering, and an established track record of success in managing large technical projects. The project manager must also have the communication skills required to work within a complex international partnership. Experience in the management of international scientific projects is highly desirable.

The Project Manager reports to the ALMA Director and will be employed by either ESO or AUI/NRAO or NAOJ. Each of these offers attractive remuneration packages including a competitive salary, comprehensive benefits, and provides the financial support in relocating families. The duty station is Santiago, Chile with frequent visits to the observatory’s mid and high altitude sites. Also frequent international travel is required.

Qualified engineers or scientists are invited to apply for the ALMA Project Manager position by submitting their curriculum to the Director of the JAO and should also include their bibliography and the names of three references who may be contacted about the qualifications of the candidate. All materials submitted electronically to searchALMApm @alma.cl by May 31, 2008 will receive full consideration. More information can be obtained from T. de Graauw (tdegraau@alma.cl).

No. 24603
Assistant Scientist, Green Bank Focal Plane Array Development Program
NATIONAL RADIO ASTRONOMY OBSERVATORY
P O BOX 2
GREEN BANK, WV 24944
USA
Tel: (304) 456-2011
URL1: http://www.nrao.edu/administration/personnel_office/careers.shtml (Careers page)
Email Submission Address: gbresumes@nrao.edu

Attention: Shirley Curry - GB4212
The 100m Robert C. Byrd Green Bank Telescope (GBT) is the world’s premiere single-dish radio telescope operating at centimeter/long millimeter wavelengths. It is making significant advances in many areas, including the study of pulsars and compact objects, astrochemistry, star formation, the content of nearby galaxies, the universe at high redshift, and cosmology. The GBT currently operates at frequencies up to 50 GHz (wavelengths down to 7mm), and preliminary observations have been made at 3mm.

We have initiated a program to develop focal plane arrays with the long-term goal of equipping the GBT with array receivers at a many wavelengths. As the first stage of this development we have recently started construction of a seven-pixel K-band (18-26 GHz) heterodyne feed-horn array receiver. We invite applications for the position of Project Scientist for this program. The successful candidate will be responsible for finalizing the scientific requirements and specifications for the K-band array, providing scientific guidance to the project manager and project team, and leading the testing and commissioning of the receiver on the GBT. In the longer term, the Project Scientist will provide scientific vision and leadership for the focal plane array development program as a whole.

The position is located at the NRAO at Green Bank, WV, which combines an academic setting with a rural environment. The Project Scientist will join a staff of 10 PhD astronomers and more than two dozen other professionals engaged in research and development in the fields of engineering, computing, and education.

The appointment is at the level of Assistant Scientist for 3 years, with the possibility of renewal. The successful candidate will spend 75% of their time executing the duties described above, and will have 25% of their time available for independent research. Support for research and travel are provided, as well as vacation accrual, health insurance, and a moving allowance. The appointment is available immediately, with the precise start date to be decided by mutual agreement. The appointment may be made at the Associate Scientist or Scientist level under exceptional circumstances.

Candidates should have, or expect to have by the agreed start date, a PhD in astronomy, physics, or a related field, and should have a plan of continuing independent research. Experience with radio astronomy instrumentation, and in particular focal plane arrays, is highly desirable. The ability to work well in a small team of scientists and engineers is essential. Applications should include a statement of planned research, a description of relevant experience, a curriculum vitae including a publication list, and the names of three scientists who have agreed to provide letters of reference. All material should be submitted as a single PDF file of the form “LastNameFirstInitial.AssistantScientist.pdf” via email to: gbresumes@nrao.edu. Letters of recommendation may be submitted separately via email. Please reference “FPA Assistant Scientist Position, Req: GB4212” in the subject line. Applications will be accepted until the position is filled. Initial review of applications will begin on April 15, 2008. Women and minorities are encouraged to apply.

No. 24625 (New)
Head of ESO Public Outreach Office
EUROPEAN ORGANISATION FOR ASTRONOMICAL RESEARCH IN THE SOUTHERN HEMISPHERE (ESO)
Karl-Schwarzschild-Str. 2
Garching near Munich, Bavaria 85748
Germany
Tel:
FAX: +49-89-3200-6497
URL1: http://www.eso.org/public/ (Public ESO Web page)
URL2: https://jobs.eso.org/ (Electronic Recruitment Portal)
URL3: https://jobs.eso.org/ESOCP370/documents/DOC0000106.PDF (Full text of vacancy notice)
Email Submission Address: vacancy@eso.org
Email Inquiries: vacancy@eso.org

Attention: Mrs Nathalie Kastelyn
ESO is opening the position of Head of the ESO Public Outreach Office. The Head of the ESO Public Outreach Office with duty station in Garching near Munich (Germany) selects, manages and performs outreach and communication tasks directed to its target groups which include the public, educators, the ESO user community, industrial partners, and decision makers within current and potential member states. The goal is to promote astronomy as a stimulating scientific activity and to propagate the widespread awareness that Europe is a major player in astronomy in general and specifically that ESO constructs and operates major ground-based observatories. There is close liaison with the ESA-funded Hubble European Information Centre at the Space Telescope – European Coordinating Facility.

The Public Outreach Office falls within the ESO Science Directorate and its Head reports to the Director for Science. S/he manages a group of about fifteen people in Garching and Santiago, manages the working of the office and decides the optimum deployment of the available resources. The Head determines the priorities to be accorded to the various tasks and is expected to be familiar with the mechanisms appropriate for reaching the different target groups with maximum efficiency and impact.

The current products of the Public Outreach Office include The Messenger, News and Photo releases, Video reports, various brochures and flyers and the ESO Annual Report to Council. The Office also mounts a number of exhibitions and displays and works closely with journalists and broadcasters to reach large and varied audiences.

The position requires a University degree in science, preferably in astronomy/astrophysics combined with public outreach training or equivalent. The candidate should have a proven record in scientific public outreach work and be well acquainted with astronomy. A familiarity with, and an aptitude to use effectively, modern communication techniques are expected. A very good knowledge of - and particularly an ability to write - English is required. Knowledge of another language, especially German or Spanish, would be an advantage.

No. 24554
Sr. Programmer Analyst
JOHNS HOPKINS UNIVERSITY
3400 N Charles
Wyman W600
Balitimore, MD 21218
Tel: 410 516- 8497
FAX: 410 516-4477
URL1: https://hrnt.jhu.edu/jhujobs/index.cfm?CFID=1701362&CFTOKEN=15799794 (Requisition #32480)
Email Submission Address: slingham@pha.jhu.edu

Attention: Joan Ostrowski, Sr. Employment Specialist
This position is related to the National Virtual Observatory ( NVO, http://www.us-vo.org/ ) project. The NVO’s primary mission is to federate digital astronomical datasets and make them seamlessly interoperable. The primary duties and responsibilities will be to design, develop and maintain scientific software and Web services for the NVO archives and applications in the Johns Hopkins University Center for Astrophysical Sciences; design and develop schema and SQL scripts for the relational database management system (DBMS) hosting archive data; design, develop and maintain enhancements to current NVO applications and Web Services; design and implement innovative and scalable approaches to parallel, distributed query execution; develop asynchronous workflow solutions for large query workloads; assist in the support & maintenance of databases; and participate in and contribute to NVO working group activities; work with JHU scientists. Duties will include supervision/guidance of junior programming staff, presentation of papers at conferences and publication of technical papers in journals, and assistance in writing proposals to funding agencies. Qualifications: Bachelor's degree and 5 years related experience. Candidates with lesser education and experience may be considered depending on the nature and quality of previous work experience. Knowledge of object oriented programming and design practices; knowledge of relational databases and SQL; two or more years of experience in C/C++/Java programming; experience with both UNIX/LINUX and Windows operating systems; C# knowledge a distinct advantage. Must have knowledge of XML Web services; must be well versed in software engineering methodology; must have good communication skills, and proven ability to write technical documentation.

No. 24615 (New)
Postdoctoral Research Fellow
CALIFORNIA INSTITUTE OF TECHNOLOGY
770 So. Wilson Ave.
MS 100-22
Pasadena, CA 91125
USA
Tel: 626-395-2418
URL1: http:// goals.ipac.caltech.edu/
Email Inquiries: meb@ipac.caltech.edu

Attention: Mary Ellen Barba, Supervisor of Staff Operations
Applicants are invited to apply for a postdoctoral research position to work with Drs. Lee Armus and Jason Surace on topics involving local luminous infrared and star-forming galaxies. The work will involve analysis of Spitzer and HST/NICMOS & ACS imaging of local Luminous Infrared Galaxies. These datasets are one facet of the Great Observatory All-sky LIRG Survey (GOALS), which is studying local infrared galaxies (the best analogs for galaxy/star formation at high redshift) in detail using multiple space-based datasets. These are based around a core of Spitzer Legacy programs - the applicant will become a member of the Legacy team, and will have the opportunity to pursue original research programs using the full GOALS dataset. Further information is given on the GOALS web site (http:// goals.ipac.caltech.edu/).

Research experience in extragalactic studies with an emphasis on interacting or starburst galaxies and UV/infrared emission is desired. Experience with the reduction and photometric measurement of space-based data (particularly NICMOS, IRS, ACS, or similar data) are also highly desired. The successful applicant will have access to the Caltech 200-inch and 60-inch Palomar telescopes. Candidates should have obtained, by the starting date, a Ph.D. in Astronomy, Physics, Astrophysics, or equivalent.

The appointment is for one year, renewable for an additional year, and will ideally begin on or before September 1, 2008. To apply, please send resume, publication list, and statement of research to the above address as soon as possible, and have three letters of reference forwarded to the same address. Caltech is an Affirmative Action/Equal Opportunity Employer. Women, Minorities, Veterans, and Disabled Persons are encouraged to apply.

No. 24619 (New)
Postdoctoral Fellow in CO/Gamma-Ray Studies
HARVARD-SMITHSONIAN CENTER FOR ASTROPHYSICS
60 Garden Street
Mail Stop 72
Cambridge, MA 02138
US
Tel: 617-495-7334
FAX: 617-495-7013
URL1: http://cfa-www.harvard.edu/mmw/
Email Submission Address: tdame@cfa.harvard.edu
Email Inquiries: tdame@cfa.harvard.edu

Attention: Thomas Dame
The millimeter-wave group at the Harvard-Smithsonian Center for Astrophysics is seeking a PhD in Astronomy or Physics to work on correlative studies of interstellar gas and diffuse gamma rays in the Milky Way. The successful candidate will work with Dr. Thomas Dame and Prof. Patrick Thaddeus and participate in completion of a CO survey of the entire northern sky with the CfA 1.2 meter telescope. This survey will be analyzed in conjunction with comparable 21 cm data and an all-sky diffuse gamma-ray survey to be obtained by the GLAST satellite. Related research initiatives using the 1.2 meter telescope or other instruments will also be encouraged.

The appointment is for two years, with possible extension for a third, and will provide a stipend of $54K plus health insurance. It will begin on October 1, 2008 or sixty days after the successful launch of GLAST, whichever is later. The current launch date is May 16, 2008. Applicants should mail or email a curriculum vitae with a list of publications, statement of research interests, and two or three letters of reference to: Dr. Thomas Dame, Mail Stop 72, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, tdame@cfa.harvard.edu. The Center for Astrophysics is an Affirmative Action/Equal Opportunity Employer - all qualified applicants will receive consideration without regard to race, creed, color, sex or national origin.

No. 24620 (New)
Post-Doc: Solar and Heliospheric Research -- Murchison Widefield Array (MWA)
MASSACHUSETTS INSTITUTE OF TECHNOLOGY (MIT)
Tel:
URL1: http://www.haystack.mit.edu
Email Submission Address: resume@haystack.mit.edu
Email Inquiries: doberoi@haystack.mit.edu

Attention: Alan Blackburn
A post-doctoral research appointment associated with the analysis of solar and heliospheric observations with the Murchison Widefield Array (MWA) is available at the MIT Haystack Observatory in Westford, Massachusetts. The MWA is an innovative digital low-frequency radio array currently under construction in a radio-quiet area in Western Australia. Information about the MWA and the Haystack Observatory is available at http://www.haystack.mit.edu.

The MWA science applications include imaging the Sun and solar radio bursts, and measuring the Faraday rotation and interplanetary scintillations of signals from distant background radio sources to determine the density, velocity and magnetic fields in solar wind structures. We seek a candidate primarily interested in the development of algorithms and software for the analysis of the MWA observations. Some experience in solar studies would be an added advantage. Candidates will have the opportunity to interact extensively with other science groups associated with the project, and to conduct independent scientific research. For inquiries or more information please contact Dr. Divya Oberoi (doberoi@haystack.mit.edu).

The salary for this position is competitive and the appointment can start immediately. The initial appointment will be for two years, with possible extension to a third year or a permanent staff position depending upon satisfactory performance and the availability of funding. Applications consisting of a CV, a brief statement of capabilities and research interests, and the names of three references should be sent to resume@haystack.mit.edu. To ensure full consideration, applications should be received by June 1, 2008, and will be accepted until the position is filled.

No. 24622 (New)
Postdoctoral Positions in Astrophysics: Gamma-Ray Bursts, Star Formation and Galaxy Evolution
UNIVERSITY OF ICELAND
Tel:
Email Submission Address: P.Jakobsson@herts.ac.uk
Email Inquiries: P.Jakobsson@herts.ac.uk

Attention: Pall Jakobsson
Applications are invited for 2 postdoctoral positions at the Science Institute, University of Iceland. Both appointments are for 2 years (possibly extended for a third year). The selected candidates are expected to start their work no later than December 2008. The candidates must hold a PhD degree in astronomy, obtained preferably not more than 4 years before the date of appointment.

The positions are supported by a generous Grant of Excellence from the Icelandic Research Fund. The candidates will join the research group of Pall Jakobsson, Gunnlaugur Bjornsson, Einar H. Gudmundsson and 2 recently started PhD students. A strong background in gamma-ray burst (GRB) research and their link to star formation, galaxy evolution and cosmology, is an advantage. We intend to hire (1) an observational expert willing to participate in GRB target-of-opportunity observations, using facilities such as the Very Large Telescope and the Nordic Optical Telescope; (2) an expert in theoretical and/or computational astrophysics taking advantage of large computer cluster facilities for parallel computing.

Our group collaborates closely with Jens Hjorth and Johan Fynbo and colleagues at the Dark Cosmology Centre in Copenhagen, and Nial Tanvir and colleagues at the University of Leicester. Travel funds are available for strengthening this collaboration and for conference attendance.

Applications should arrive by email before 1 August 2008, and include a statement of research interests (max 2 pages), a CV and a list of publications. The applicants should also arrange for 3 letters of recommendation to be sent separately. Email inquiries are welcome.

No. 24624 (New)
postdoctoral positions in theoretical astrophysics, observational astronomy, space science, and space geodesy
KOREA ASTRONOMY AND SPACE SCIENCE INSTITUTE (KASI)
61-1 Hwaam-dong, Yuseong-gu,
Daejeon, . 305-348
South Korea
Tel: +82 42 865 3324
FAX: +82 42 865 2006
URL1: http://www.kasi.re.kr (official website of KASI)
Email Submission Address: icapadmin@kasi.re.kr
Email Inquiries: icapadmin@kasi.re.kr

Attention: Ms. Kyoung-Suk Lee, Postdoctoral Positions
Korea Astronomy and Space Science Institute (KASI) invites applications for several postdoctoral positions in theoretical astrophysics, observational astronomy, space science, and space geodesy. The successful applicants are expected to carry out original research independently or in collaboration with KASI faculty.

The appointment is initially for one year and can be renewed based on satisfactory performance. The positions are available immediately. The starting annual salary is approximately US$30,000. Also, conference and observing travel will be supported. Other benefits such as health insurance and a dormitory space will be provided supplementarily.

Interested applicants should submit a resume, a list of publications, and a research plan, and arrange for two letters of recommendation, signed by the recommender, to be sent to the above address by June 30th, 2008. The successful applicants should join us by December 1st, 2008.

No. 24626 (New)
Postdoctoral Position in Stellar Astrophysics
MONASH UNIVERSITY
School of Mathemtical Sciences
Building 28
Monash University, Victoria 3800
Australia
Tel: +61 3 9905 4428
FAX: +61 3 9905 4403
URL1: http://www.maths.monash.edu.au/~johnl/ (SINS webpage)
URL2: http://www.cspa.monash.edu.au (CSPA Webpage)
URL3: http://www.maths.monash.edu.au (School of Mathematical Sciences webpage)
Email Submission Address: john.lattanzio@sci.monash.edu.au
Email Inquiries: john.lattanzio@sci.monash.edu.au

Attention: John Lattanzio, Professor
Postdoctoral Fellow

Stellar Interiors and Nucleosynthesis Group Centre for Stellar and Planetary Astrophysics Monash University Melbourne Australia

A position exists for a Postdoctoral Fellow within the SINS group at Monash University's Centre for Stellar and Planetary Astrophysics. We are seeking someone with expertise in modeling advanced stages of stellar evolution, with applications to Super-AGB stars, nucleosynthesis and electron-capture supernovae. The successful applicant will work directly with a team working on SAGB stars, consisting of John Lattanzio, Pilar Gil Pons and Lionel Siess.

The position is available now and is for 2 years initially, with the possibility of extension to a third year. Salary will be in the range $61,820 - $66,360 (Australian Dollars). A generous superannuation payment is included. The Fellow will be part of the SINS group, a very active and growing group consisting of Prof John Lattanzio, Dr Maria Lugaro, Dr Ross Church and Dr Richard Stancliffe, as well as postgraduate students and other members of CSPA.

The CSPA is housed at the main campus of Monash University in the suburbs of Melbourne. Monash is Australia's largest University and one of the prestigious "Group of Eight" most active research institutions in the country.

Melbourne is the capital of the state of Victoria, and the second largest city in Australia (population nearly 4 million). It is regularly rated as one the world's most livable cities, coming second in the 2008 list. It is an extremely multi-cultural city with excellent cultural life, restaurants, beaches and vineyards very nearby.

Applications, including three letters of reference, should arrive by 1 June at the following address:

Prof. John Lattanzio CSPA School of Mathematical Sciences Building 28 Monash University 3800 Australia

Further information is available from John Lattanzio: john.lattanzio@sci.monash.edu.au http://www.maths.monash.edu.au/~johnl/ CSPA: http://www.cspa.monash.edu.au SINS: http://www.maths.monash.edu.au/~johnl/sins/ Monash Univ: http://www.monash.edu.au Melbourne: http://www.thatsmelbourne.com.au/ http://www.visitvictoria.com/ http://www.melbourne.com.au/ http://www.visitmelbourne.com/

No. 24627 (New)
Postdoctoral Research Scholar
CALIFORNIA INSTITUTE OF TECHNOLOGY
770 So. Wilson Ave.
MS 100-22
Pasadena, CA 91125
USA
Tel: 626-395-1802
Email Inquiries: meb@ipac.caltech.edu

Attention: Mary Ellen Barba, Supervisor of Staff Operations
Exo-Planet Postdoctoral Scholar Position at the Michelson Science Center

The Michelson Science Center (MSC) Michelson Distinguished Postdoctoral Program invites applications for a research position in the area of extrasolar planet detection and characterization. The research involves working on problems of planet transit detection and ensuing astrophysical analysis using data from a variety of ground and space-based instruments.

Dr. David Ciardi will serve as postdoctoral advisor to the selected candidate. The successful candidate will work with existing high precision photometric data and will lead transit surveys being pursued by the transit group at the MSC. The successful candidate will be encouraged to pursue their own scientific program related to high precision photometry, stellar variability studies and the detection and characterization of exo-planets. The appointee will work within the exo-planet transit survey group at the MSC, and will be guided by the MSC advisor to ensure that the research work will result in publications in the open literature.

Applicants should have a Ph.D. in physics, astronomy, or a closely related field; at least two years of post-graduate experience is highly desired. The appointment is contingent upon evidence of completion of Ph.D. A history of academic endeavor with regards to transit detection as evidenced by published journal articles is highly desired. Excellent written, verbal, and personal skills are essential to this position. Postdoctoral scholar positions are awarded initially for a two-year period, and may be renewed for a third year.

Interested individuals should send a CV, bibliography, statement of research interests, and a list three people who may be contacted for letters of reference. Please send to Mary Ellen Barba at the above address by 2 June 2008.

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

No. 24630 (New)
Two Postdoc Positions in Near-Infrared Instrumentation
UNIVERSITY OF COLOGNE
1. Physikalisches Institut
Zuelpicher Strasse 77
Germany
Tel:
URL1: http://www.ph1.uni-koeln.de/workgroups/eckart/ (working group of Prof. Dr. A. Eckart)
URL2: http://www.mpia.de/LINC/ (LINC-NIRVANA project pages)
URL3: http://www.mpe.mpg.de/ir/gravity/ (GRAVITY project pages)
Email Inquiries: eckart@ph1.uni-koeln.de

Attention: Andreas Eckart, Prof. Dr.
Applications are invited for two postdoctoral positions in near-infrared instrumentation at the 1st Physics Institute of the University of Cologne, Germany. The successful applicants will work in the group of Prof. Dr. Andreas Eckart and Dr. Christian Straubmeier and will co-lead small local teams of scientists, engineers and graduate students. The work will focus either on the development of subsystems of the LINC-NIRVANA interferometer for the LBT, or the GRAVITY interferometer for the VLTI. Both projects are run by distributed European instrument consortia and the University of Cologne is developing and contributing crucial hardware components to these systems. The successful applicants would also be encouraged to pursue their own astrophysical research. Knowledge of the German language is desirable but not required.

Over the last 10 years, the 1st Physics Institute of the University of Cologne has become a major astronomical research institute among German universities. The research emphasis is on infrared to radio wavelengths and interferometry. Present fields of astrophysical research in observations, numerical simulations, and theory include the black hole at the center of the Milky Way, active galactic nuclei, star and planet formation, stellar evolution, as well as the evolution and interaction of galaxies. The institute is strongly involved in several international instrumentation projects e.g. for VLTI, LBT, Keck, SOFIA, Herschel, APEX, and is member of the International Max Planck Research School for Radio and Infrared Astronomy and the Bonn-Cologne Graduate School of Physics and Astronomy.

The positions are for 3 years with the possibility of extension afterwards. Earliest starting date is 1 July 2008. The salary scale will be Eur 36,500 to Eur 53,000 pa, depending on experience and qualification. Applicants should have a PhD or equivalent in Astrophysics, Physics, or a similar discipline, and should have at least two years of experience in the development of astrophysical instrumentation. Electronic applications including a CV, publication list, and research statement should be sent to the attention of Prof. Dr. Andreas Eckart (eckart[at]ph1.uni-koeln.de). Any attachments must be in PDF format. Other formats will not be accepted. Alternatively postal applications should be sent to Prof. Dr. Andreas Eckart, 1. Physikalisches Institut, University of Cologne, 50937 Cologne, Germany. The deadline for applications is 15 June 2008.

Applicants should also ask two referees to send letters of recommendation to this postal address or to eckart[at]ph1.uni-koeln.de by the same date. Enquiries may be sent to eckart[at]ph1.uni-koeln.de.

The University of Cologne is an equal opportunity employer.

No. 24632 (New)
Postdoctoral Research Position in Space/Astrophysical Plasma Theory
UNIVERSITY OF NEW HAMPSHIRE
Tel:
Email Inquiries: benjamin.chandran@unh.edu

Attention: www.unhjobs.com/applicants/Central?quickFind=182035
The Space Science Center of the University of New Hampshire invites applications for a Postdoctoral Research Associate in the field of space and astrophysical plasma theory. The successful applicant will carry out research in one or more of the following areas: plasma turbulence, wave-particle interactions in plasmas, and physical modeling of the solar-wind, solar corona, and solar flares. Applicants should have a strong background in theoretical or computational plasma physics and/or magnetohydrodynamics. The position is renewable for up to three years. Applicants should post a cover letter, CV, and statement of research interests to the UNH online employment site at www.unhjobs.com/applicants/Central?quickFind=182035 , and should arrange for at least two letters of recommendation to be sent to Professor Ben Chandran at benjamin.chandran@unh.edu. Inquiries regarding this position may be addressed to Prof. Chandran at the same email address. UNH is an AA/EEO Employer. UNH is committed to excellence through the diversity of its faculty and staff and encourages women and minorities to apply.

No. 24633 (New)
Postdoctoral Associate in Supernova Astrophysics
UNIVERSITY OF TEXAS AT AUSTIN
1 University Station, C1400
Austin, TX 78712
USA
Tel: 512-471-6407
FAX: 512-471-6016
URL1: http://www.as.utexas.edu/~wheel/ (Personal web page)
URL2: http://www.as.utexas.edu/ (Texas astronomy web page)
Email Submission Address: wheel@astro.as.utexas.edu
Email Inquiries: wheel@astro.as.utexas.edu

Attention: J. Craig Wheeler, Professor
A postdoctoral associate is sought to join the supernova research group at the University of Texas at Austin. Candidates will be considered with expertise in either observation or theory. Observational facilities include the Hobby-Eberly Telescope and the ROTSE robotic telescope. Expertise in spectroscopy is important. Expertise in spectropolarimetry is desirable, but not required. Facilities for theory include Ranger, the largest publically accessible supercomputer in the nation. Experience in magnetohydrodynamics is of particular interest.

The position is available beginning September 1, 2008, for two years with the possibility of extension to a third. Certification of Ph.D. is required.

Please submit your curriculum vitae with relevant work and research experience, a list of publications and a list of three references by e-mail to wheel@astro.as.utexas.edu.

The University of Texas is an Equal Opportunity/Affirmative Action employer with a strong institutional commitment to excellence through diversity. AAE/EOE

No. 24634 (New)
Postdoctoral Researcher: molecular clouds and star formation
UNIVERSITY OF EXETER
School of Physics
Stocker Road
Exeter, Devon EX4 4QL
United Kingdom
Tel: +44 1392 725512
FAX: +44 1392 264111
URL1: http://www.astro.ex.ac.uk/ (Exeter Astrophysics Home Page)
Email Submission Address: brunt@astro.ex.ac.uk
Email Inquiries: brunt@astro.ex.ac.uk

Attention: Chris Brunt, Lecturer
The University of Exeter intends to appoint a post-doctoral researcher in the field of molecular clouds and star formation, to work with Chris Brunt in the astrophysics group. Applicants with a background in mm/submm astronomy and/or star formation are particularly encouraged to apply; strong applicants from other areas will be considered.

The successful applicant will have an appropriate first degree and a PhD (or equivalent). Salary will be in the range £23,002 to £25,888 depending on qualifications and experience. This is a fixed term appointment for 3 years, to begin as early as 1st July 2008.

An application form is available on request, and applicants should send this, along with a description of their current research and future plans, a brief curriculum vitae, and a list of refereed publications to Dr C Brunt, School of Physics, University of Exeter, Exeter, EX4 4QL, UK, quoting reference number N1589.

The closing date is 31st May 2008. Please also ensure that 3 letters of reference reach Exeter by this date. Informal enquiries can be made by emailing brunt@astro.ex.ac.uk.

No. 24635 (New)
Postdoctoral Researcher in star formation
UNIVERSITY OF EXETER
School of Physics
Stocker Road
Exeter, Devon EX4 4QL
United Kingdom
Tel: +44 1392 264158
FAX: +44 1392 264111
URL1: http://www.astro.ex.ac.uk/ (Exeter Astrophysics Home Page)
Email Submission Address: th@astro.ex.ac.uk
Email Inquiries: th@astro.ex.ac.uk

Attention: Tim Harries, Senior Lecturer
The University of Exeter intends to appoint a post-doctoral researcher in the field of star formation, to work with Tim Harries in the astrophysics group. The successful applicant will conduct research into the circumstellar environment of pre-main sequence (PMS) stars, using a combination of observation and numerical modelling. Applicants with a background in optical and near-IR observations of PMS stars, or radiative-transfer/hydrodynamical modelling are particularly welcome. The research will involve the use of the UK's forefront observational facilities, and numerical simulations will be conducted on our new 1 million euro supercomputer.

The successful applicant will have an appropriate first degree and a PhD (or equivalent). Salary will be in the range £23,002 to £25,888 depending on qualifications and experience. The appointment will be for 3 years, with a start date as early as 1 July 2008.

An application form is available on request, and applicants should send this, along with a description of their current research and future plans, a brief curriculum vitae, and a list of refereed publications to Dr T Harries, School of Physics, University of Exeter, Exeter, EX4 4QL, UK, quoting reference number N1588.

The closing date is 31 May 2008. Please also ensure that 3 letters of reference reach Exeter by this date. Informal enquiries can be made by emailing th@astro.ex.ac.uk.

No. 24636 (New)
Early-type galaxies, groups, clusters of galaxies, radio galaxies
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
60 Garden St.
MS-4
Cambridge, MA 02138
USA
Tel: 617-496-7709
FAX: 617-495-7356
URL1: http://hea-www.harvard.edu (SAO High Energy Astrophysics Division homepage)
Email Submission Address: rkraft@cfa.harvard.edu
Email Inquiries: rkraft@cfa.harvard.edu

Attention: Dr. Ralph P. Kraft, Scientist
The High Energy Astrophysics Division in the Center for Astrophysics invites applications for two postdoctoral positions in the study of early-type galaxies, groups, clusters, and radio galaxies. In addition to studies of individual objects, the candidate also may be involved in surveys of all types of galaxies and AGN. The position involves the analysis and interpretation of data principally from Chandra and XMM. Data from other wavebands, including observations from Spitzer and the VLA, will be employed as needed. In addition to data analysis, the candidate will be expected to develop original investigations suitable for proposing for new observations with space-based observatories, especially Chandra and XMM.

Candidates must possess a Ph.D. or equivalent in astronomy, physics, or a closely related field, and must have experience in observational research related to galaxies, groups, and clusters and in the analysis of data, especially from X-ray missions. To carry out the required research tasks successfully, candidates must have familiarity with modern computer techniques, demonstrated ability to communicate and work with other scientists, and the ability to prepare material for publication and presentation at meetings. Familiarity with Spitzer and VLA data analysis will be an asset.

The initial appointment will be for one year, beginning about September 2008, and will be renewable for a second (and possibly a third year). Successful candidates will have access to facilities at SAO. Interested applicants should send a CV, statement of research interests, and the names of three references to the above address; applications received by 30JUN08 will given full consideration. For further information please contact Dr. W. Forman (617-495-7210; wrf@cfa.harvard.edu) Dr. C. Jones (617 495 7137; cjones@cfa.harvard.edu), or Dr. R. Kraft (617 496 7709; rkraft@cfa.harvard.edu) AAE/EOE.

No. 24637 (New)
Postdoctoral Position in High Energy Astrophysics
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 has an opening for a postdoctoral research scholar to work in high-energy astrophysics in collaboration with Prof. Philip Kaaret beginning in the Summer or Fall of 2008. The successful applicant will work on the development of X-ray detectors for imaging and polarimetry and on the analysis of data from on-going programs to study X-ray binaries and ultraluminous X-ray sources. Candidates must hold a Ph.D. in physics or astronomy. Experience in the development of detectors for ionizing radiation and astrophysics data analysis are desired. US citizenship or green-card status are a plus. The appointment will be for one year initially, and will likely be renewed for additional years dependent on performance and continued funding. Applicants should submit a curriculum vitae, a list of publications, and a statement of research interests. 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 June 1st, 2008, and continue until the position is filled. Women and members of minority groups are strongly encouraged to apply.

No. 24638 (New)
Research Fellow in Low Mass Stars and Exoplanets
QUEENS UNIVERSITY BELFAST
University Road
Belfast, Northern Ireland BT7 1NN
UK
Tel: +44 2890973044
URL1: http://www.qub.ac.uk/sites/QUBJobVacancies/ResearchJobs/ (Post and application details)
URL2: http://star.pst.qub.ac.uk (QUB Astrophysics Research Centre)
Email Inquiries: a.fitzsimmons@qub.ac.uk

Attention: The Director of Human Resources, Personnel Department
Research Fellow in Low Mass Stars and Exoplanets Ref. 08/100377 School of Mathematics and Physics, Queen's University Belfast

Applications are invited for a 3-year Post Doctoral Research Fellowship position in low mass stars and exoplanets, funded in part by the Science & Technology Facilities Council (STFC). The post is located within the Astrophysics Research Centre (ARC) of the School of Mathematics and Physics. ARC is one of the founders of the WASP Project and operates and maintains the SuperWASP facility on La Palma. The Exoplanet Group within ARC is well supported by STFC and is expanding. By mid-2008 the group is expected to consist of 3 academic staff, 3 research staff and a number of PhD students.

Applicants must have a PhD in a relevant subject either awarded or submitted by the time of taking up the post. Experience of observational techniques used in astrophysics, including spectroscopy and photometry plus associated data reduction techniques, are essential. However these do not have to be at optical wavelengths. Also essential is a reasonable number of high quality publications commensurate with stage of career.

Informal enquiries can be directed to Prof. Alan Fitzsimmons (email: a.fitzsimmons@qub.ac.uk).

An application pack for the post, containing further details of the essential and desirable criteria, as well as instructions on how to submit an application, is available from our website:

http://www.qub.ac.uk/sites/QUBJobVacancies/ResearchJobs/

Salary: 27,466-35,837 pounds per annum (including contribution points).

Closing date: 4.00 pm, Friday 6 June 2008

No. 24652 (New)
Postdoctoral fellow– Nordic ALMA regional centre node
ONSALA SPACE OBSERVATORY
Tel:
URL1: http://www.chalmers.se/en/ (Chalmers university webpage)
URL2: http://www.chalmers.se/rss/EN/ (Dept of Radio and Space Science)
URL3: http://www.eso.org/sci/facilities/alma/arc/ (European ARC organisation)
Email Inquiries: John.Conway@chalmers.se

Attention: John Conway
Onsala Space Observatory (OSO), the Swedish national facility for radio astronomy hosted by Chalmers University of Technology, has an immediate opening for a postdoctoral fellow in connection with its newly established European ALMA regional centre (ARC) node.

Background: The ALMA (sub)millimetre array in Northern Chile, presently under construction, will provide a leap in performance relative to existing millimetre-wave arrays. Onsala Space observatory and Chalmers University have a strong involvement in both the science of ALMA and its technical development. A permanent staff of approximately eight astronomers plus PhD students conduct a wide range of research from star formation to cosmology. Staff specialise in observing at radio through submillimetre wavelengths, but also make use of IR, optical and other observations. Additionally, theoretical work is conducted in astrochemistry, radiative transfer and N-body simulations. On the technical side for ALMA Onsala is/has been heavily involved in the areas of receiver development, water vapour radiometry design and the design of the antenna pad distribution. Onsala also manages the 23% Swedish share in the 12m diameter APEX (Atacama Pathfinder Experiment) submillimetre wavelength telescope at the ALMA site.

To support the use of ALMA for a wide range of astronomers ALMA regional centers (ARCs) are being established in Europe, North America and East Asia. The European ARC has a distributed structure with most core user operations (proposal handling, scheduling, archiving, standard pipeline data reduction etc) being concentrated at ESO headquarters in Garching (Germany) while face-to-face user support, most off-line data reduction, development of specialist data reduction and local community outreach will be functions covered by ARC 'nodes' covering countries or sub-regions within Europe. A Nordic ARC node is being established at Onsala (Sweden) to provide ALMA support functions to astronomers in the Nordic region (Sweden, Denmark, Finland, Norway and Iceland) and in the Baltic countries. The ARC node at Onsala will as a minimum consist of a part time director, two new permanent staff positions and postdoctoral positions. These positions will be filled in 2008 in order to prepare for supporting and exploiting ALMA science-verification and first-science operations in 2009 and 2010.

Job Description: The postdoctoral position is largely funded by the pan-Nordic funding agency, Nordforsk and will run for two years. The successful candidate is expected to run her/his own astronomical research programme in an area where ALMA will make a large impact, and will preferably make significant use of APEX observations in preparing for ALMA. Additional support duties (covering up to 50% of the time) will involve helping the ARC node become ready for ALMA operations. This will involve testing and becoming familiar with ALMA observing and reduction tools, providing face-to-face help to initial Nordic ALMA users and helping in outreach for ALMA in the Nordic region, including helping organise and run workshops. Establishing research collaborations with potential ALMA users, especially within the Nordic region will also be encouraged.

The position will have a gross salary of approximately 30,000 Swedish Kronor per month (approximately $5000/month or €3150/month). The position is available immediately and we hope to fill it before December 2008 at the latest.

Requirements: The successful candidate should have a PhD in astronomy, with a strong research record. Previous experience in millimetre or radio astronomy and /or in interferometric imaging would be strong advantages. Further Information and application: For further details of the position and for application details contact John Conway, (John.Conway@chalmers.se) The deadline for applications is 1st July 2008. The application should consist of a curriculum vitae/resume and a research plan. The applicant should also arrange for two letters of reference to be sent.

No. 24577
Postdoctoral Position in Astrophysics
NICHOLAS COPERNICUS ASTRONOMICAL CENTER
ul. Bartycka 18
Poland
Tel: 48-22-3296121
FAX: 48-22-8410046
Email Submission Address: pam@camk.edu.pl
Email Inquiries: pam@camk.edu.pl

Attention: Pawel Moskalik
Applications are invited for a postdoctoral position in the Nicholas Copernicus Astronomical Center (NCAC), the leading astronomical institution in Poland. The current research at NCAC focuses on stellar photometry and spectroscopy, evolution of stars and binary systems, helio- and asteroseismology, observations and theory of planetary nebulae and circumstellar matter, search for extrasolar planets, high-energy astrophysics (pulsars, gamma-ray bursts, black holes, X-ray binaries, AGNs), accretion disks, large-scale structure of the Universe, cosmology, dynamics of stellar systems and hydrodynamical simulations in astrophysics. The successful candidate is expected to work in one of these fields.

Both theorists and observers are encouraged to apply. Preference will be given to applicants with PhD in astronomy or physics, received no earlier than in 2006. Successful candidates are expected to start their appointment no later than January 1st, 2009. The position is awarded for a 3 year period. The salary will be commensurate with those of polish researchers. For more information contact Pawel Moskalik (e-mail: pam@camk.edu.pl, tel: 48-22-3296121).

Applicants should send a copy of the PhD diploma, a CV, a resume with statement of research interests and plans, a publication list and should arrange for two letters of reference to be sent to: Copernicus Astronomical Center, Bartycka 18, 00-716 Warszawa, POLAND. Application deadline: May 26th, 2008.

No. 24578
Postdoctoral position in Astrophysics at UNAM
INSTITUTO DE ASTRONOMIA, UNIVERSIDAD NACIONAL AUTONOMA DE MEXICO
Apdo. Postal 70-264
Cd. Universitaria
MEXICO, DF 04510
MEXICO
Tel: 52-55-56-22-39-06
FAX: 52-55-56-16-06-53
URL1: www.astroscu.unam.mx (Institution website)
URL2: www.astroscu.unam.mx/~wlee/posdoc.html (Webpage with additional information)
Email Submission Address: juanita@astroscu.unam.mx
Email Inquiries: juanita@astroscu.unam.mx

Attention: Juana Orta
The Universidad Nacional Autonoma de Mexico (UNAM) invites researchers to submit applications for postdoctoral fellowships in astrophysics, to begin in September 2008. The appointment is for one year with a possible extension for a second. Fellows will work either in the Institute of Astronomy in Mexico City or in the city of Ensenada (Baja California).

Fellows are expected to carry out original research in any area of astrophysics, collaborating with staff, faculty or students at the host institution. The main selection criteria will be outstanding research accomplishments and promise of future achievement.

Fellows will have access to all of the resources and facilities of the National Astronomical Observatory. In particular, the Institute operates the San Pedro Martir Observatory near Ensenada, which includes a 2.1-meter, a 1.5-meter and an 84-cm telescope, equipped with modern instrumentation for optical and near- and mid-infrared imaging and spectroscopy. The Institute is also a partner in the GTC (Gran Telescopio Canarias) Consortium due to operate fully in 2008. Additionally, the computing center at UNAM operates KanBalam, the fastest supercomputer in Latin America (rated at 7.1TFlops with 3TB RAM and 160TB storage space). The fellowship provides some support for observing, traveling and publishing. These facilities will be accessible for the entire duration of the fellowship.

By the submission deadline, applicants should have a PhD in Astronomy or in Astronomical Instrumentation. University policy requires that by the starting date applicants be less than 35 years old, and have earned their PhD degrees at most 3 years earlier. Knowledge of the English and/or Spanish language is required. Salary and benefits are compatible with international standards.

Applicants should send a curriculum vitae, bibliography, and research plan, and arrange for three letters of recommendation to be sent to Juana Orta at the Institute of Astronomy by May 15, 2007. Preference for an appointment in Mexico City or Ensenada should be stated in the cover letter. All interested applicants should contact Juana Orta (juanita@astroscu.unam.mx) before that date for additional information, as well as check the page maintained at http://www.astroscu.unam.mx/~wlee/posdoc.html for additional information.

No. 24580
Postdoctoral Scholar
CALIFORNIA INSTITUTE OF TECHNOLOGY
770 So. Wilson Ave.
MS 100-22
Pasadena, CA 91125
USA
Tel:
Email Submission Address: apple@ipac.caltech.edu
Email Inquiries: apple@ipac.caltech.edu

Attention: Dr. Phil Appleton
Applications are invited for a postdoctoral scholar position in extragalactic IR astronomy at Caltech. The successful applicant will work jointly with Dr. Phil Appleton at the NASA Herschel Science Center, and Dr. Patrick Ogle of the Spitzer Science Center on IRS spectroscopy of molecular hydrogen in extragalactic environments. Recent observations by Spitzer’s Infrared Spectrograph (IRS) have discovered very strong molecular hydrogen lines in the Mid-IR which are believed to originate in large-scale shocks or accretion driven flows onto galactic nuclei. In some cases, the line emission represents a significant fraction of the bolometric luminosity from the galaxies. The mechanism for the formation of such powerful emission in the H2-lines is not yet understood.

The Postdoc will be expected to participate in several studies aimed at understanding powerful H2 emission, including a complete analysis of new data on Stephan’s Quintet, and from several radio-galaxies in which H2 is detected. In addition, we expect that the project will involve analyzing a survey of 30 compact groups of galaxies, using Spitzer data to be obtained in the coming 12 months. The work will involve coordinated observations with ground-based facilities in the IR, optical and radio/submm as well as comparisons with shock-models. Experience with observational astronomy, especially in the IR or radio/submm spectroscopy and molecular astrophysics will be highly desirable.

Candidates should have obtained, by the starting date, a Ph.D. in astronomy, physics or equivalent, in an area relevant to these projects. The appointment is for two years (with the possibility of a renewal for an additional year) and could start as early as August 2008.

To apply, please send a resume, publication list, and statement of research to Dr. Appleton (apple@ipac.caltech.edu) by 6/30/2008. Also, please arrange to have three letters of reference forwarded to the same address.

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

No. 24586
Postdoctoral Position at Copernicus Astronomical Center
NICHOLAS COPERNICUS ASTRONOMICAL CENTER
ul. Bartycka 18
Poland
Tel: 48-22-3296117
FAX: 48-22-8410046
Email Inquiries: pam@camk.edu.pl

Attention: Anna Wyrebek
Applications are invited for a postdoctoral position in the Nicholas Copernicus Astronomical Center (NCAC), the leading astronomical institution in Poland. The current research at NCAC focuses on stellar photometry and spectroscopy, evolution of stars and binary systems, helio- and asteroseismology, observations and theory of planetary nebulae and circumstellar matter, search for extrasolar planets, high-energy astrophysics (pulsars, gamma-ray bursts, black holes, X-ray binaries, AGNs), accretion disks, large-scale structure of the Universe, cosmology, dynamics of stellar systems and hydrodynamical simulations in astrophysics. The successful candidate is expected to work in one of these fields.

No. 24591
Joint Yale-Universidad de Chile Postdoctoral Position in Star Formation
YALE UNIVERSITY
P.O. Box 208101
260 Whitney Ave.
New Haven, CT 06520-8101
USA
Tel: 203-432-3000
FAX: 203-432-5048
URL1: http://www.astro.yale.edu
URL2: http://www.das.uchile.cl/
Email Submission Address: susan.delong@yale.edu
Email Inquiries: hector.arce@yale.edu or guido@das.uchile.cl

Attention: Susan DeLong, Sr. Administrative Asst.
The Department of Astronomy at Yale University and the Department of Astronomy at the Universidad de Chile invite applications for a joint Yale-U. de Chile post-doctoral research position in observational star formation. The successful applicant will conduct independent research and will collaborate with Professors Guido Garay, Diego Mardones and Leonardo Bronfman (Universidad de Chile) and with Prof. Hector Arce (Yale University) on studies of star forming regions using millimeter, sub- millimeter and infrared data as well as radiative transfer codes.

The post-doctoral fellow is expected to spend at least 3/4 of the year at the Department of Astronomy in the Universidad de Chile (in Santiago), thus he or she will be able to have PI status for the 10% observing time reserved for Chilean astronomers on all astronomical facilities in Chile. The successful applicant may choose to spend the rest of the time at Yale University or to stay in Chile. The post- doctoral fellow will also have direct access to Yale resources including the WIYN telescope, the SMARTS telescopes, and the Palomar- QUEST large-area survey.

Postdoctoral positions are awarded for a two-year per

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