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March 2001JOB REGISTERAmerican Astronomical Society |
The National Academies
Cecil and Ida Green Building
2001 Wisconsin Ave., N.W.
Monday, Sept. 11 at 10 am (EASTERN)
Room 104
If you were unable to attend the briefing, a full text version of the giude will be available at COSEPUP's Webguide to Enhancing the Postdoctoral Experience for Scientists and Engineers at www.nationalacademies.org/postdocs beginning at 12 noon on September 11th. This Webguide contains resources and examples for all parties in the postdoctoral experience.
Our next event will be a day-long convocation at the National Academies on 2 March 2001 for postdocs, postdoc advisers, administrators, funding organizations, disciplinary societies, and distinguished researchers to discuss the postdoctoral experience. See the Webguide for more information on the convocation.
You may purchase copies of the report by contacting National Academy Press at 888-624-8373 or 202-334-3313 or online at www.nap.edu.
Questions on this project can be directed to Dr. Deborah Stine, Associate Director, COSEPUP and Project Director. She can be reached at 202-334-3239 or dstine@nas.edu. Questions regarding attending the public briefing should be directed to Rebecca Burka at 202-334-2455 or rburka@nas.edu.
Resumes are entered into a searchable database which is available to employers around the world. The identity of the job seeker and a complete resume will only be released to employers who contact AIP offices directly.
The site is located at: http://www.aip.org/resume_post
For more information contact:
Edwin Goldin
Manager, Career Services Division
American Institute of Physics
One Physics Ellipse
College, Park, MD 20740-3843
Tel: 301-209-3190
FAX: 301-209-0841
Email: cpp@aip.org
15 March - Deadline for the April Job Register
15 April - Deadline for the May Job Register
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The Job Register is published on the Web at: http://www.aas.org Click on Job Register.
The Job Register is published in postscript, PDF, and ASCII text and can be reached at: ftp.aas.org/jobs/jobreg or by performing the following:
prompt> ftp ftp.aas.org
username: anonymous
password: your e-mail address
ftp> cd /jobs/jobreg
ftp> get mar01.txt (for ASCII Text version)
ftp> get mar01.ps (for Postscript version)
ftp> binary (convert to binary mode)
ftp> get mar01.ps.Z (for compressed Postscript version)
ftp> quit
prompt>
Attention: Dale Alianiello
All qualified applicants receive consideration for employment without regard to race, creed, sex or national origin. AAE/EOE.
Attention: Dr. Robert W. Milkey, Executive Officer
The Applicant must have a doctoral degree in astronomy, or a closely related field, together with strong interest in practical and theoretical issues in astronomy education and a commitment to working on these issues. He/she must also have demonstrated organizational, interpersonal, and communications skills, and have direct experience in astronomy education at the graduate or undergraduate level. Experience with K through 12 education would be an added advantage. Ideally, the candidate should have an interest in, and knowledge of, national and state policy issues concerning science education, curricula and funding, as well as familiarity with the people involved in and the process of research on science education. Since the AAS is heavily reliant on Web and Internet communications, experience with this technology would also be advantageous.
The AAS encourages women and minority candidates to apply.
Applications should include information on educational background and relevant experience as well as an indication of salary expectations. These should be sent to Dr. Robert W. Milkey Executive Officer, at the above address.
We will start consideration of applications 1 February 2001. AAE/EOE.
Attention: Dr. Daniel Suson, Chairman, Physics Department
Attention: Leopoldo Infante, Director, Dept. Astronomy and Astrophysics
The Faculty of Physics at Pontificia Universidad Catolica de Chile offers a new position in Astronomy at the full, associate or assistant professor level, available as early as September 2001. The requirements are a Ph.D. and a demonstrated ability and commitment to excellence in independent research and teaching.
The successful candidate is expected to join the research and teaching activities of the Department and to strongly interact with students. Presently, the Department includes seven faculty and seven postdocs doing research in areas of observational and theoretical cosmology, extragalactic and stellar astrophysics. We are interested in developing the Department particularly in areas related to mm-radio astronomy and theory. However, applicants from all areas of astrophysics are strongly encouraged to apply. The successful applicant will have access to the 10% of all the telescope time in Chile, including VLT, Gemini, Megellan, and ALMA telescopes. Teaching duties are in astronomy and physics, at the undergraduate and graduate levels. Preference will be given to candidates able to teach in Spanish within a year. Further information can be obtained at http://www.astro.puc.cl or from L. Infante (linfante@astro.puc.cl).
Applicants should send a curriculum vitae and a description of research and teaching interests before 31 March 2001, preferably by e-mail. In addition, three letters of recommendation should be sent before the deadline directly to Prof. Leopoldo Infante, Director, at the above address (job@astro.puc.cl).
Attention: Professor Leopoldo Infante
The Department of Astronomy and Astrophysics of Pontificia Universidad Catolica, located in Santiago, Chile, invites applications for postdoctoral research positions in the areas of interest of its faculty members.
These include observational and theoretical cosmology, groupings of galaxies on all scales from pairs to superclusters, galaxy formation and evolution, Galactic structure, microlensing, stellar populations and evolution, neutron stars, and supernovae.
The best applicants, who must have received their PhD after 1 January 1999, will be sponsored in their applications for postdoctoral research grants from the national fund for science and technology, FONDECYT, and the ESO-Chile astronomy committee.
The grants provide salary and research funds to work at the Department of Astronomy and Astrophysics for up to three years, starting April or September 2002.
During this period, fellows may apply for the 10\% Chilean time share at all the telescopes located in the country, including the VLTs, Gemini, and Magellan, all progressively coming into operation, in addition to the other telescopes at La Silla, CTIO, and Las Campanas observatories.
Information about the Department is available at {http://www.astro.puc.cl}.
Applicants should send, before 31 March 2001, and preferably by e-mail, their CV, publication list, statement of research interests, and arrange for three letters of recommendation to be sent to Professor Leopoldo Infante, at the above address.
Attention: Rogier A. Windhorst, Professor of Astronomy
Funding is anticipated for a Postdoctoral Research Associate to be involved in the reduction, analysis, and publication of images from HST primary and parallel surveys. Applications are solicited from candidates with a PhD degree plus a strong record in extragalactic astronomy and observational cosmology. Candidates are expected to have substantial experience with CCD data reduction and analysis and LINUX or UNIX.
The successful applicant will be involved in Cycle 9--10 HST projects at ASU, such as the mid-UV morphology of nearby galaxies as template for accurate high-redshift galaxy classifications, or the STIS parallel search for the Hydrogen reionization edge, a faint uniform signal in the integrated background leftover from the epoch of reionization.
Opportunities to conduct astronomical research at ASU are excellent. ASU has access to the Steward Observatory facilities, including the new 6.5m MMT at Mt Hopkins, the 2.3m Steward, 1.5m Catalina, and 1.8m VATT telescopes, and starting in 2002 also the two 6.5m Magellan telescopes in Chile and 2x8.5m Large Binocular Telescope at Mt Graham.
Applicants must send their CV plus statement of research interests to Professor R. Windhorst at the above address. Deadline is 31 January 2001 (or the 15th or last day of each month thereafter until filled). Applicants should have at least three letters of reference sent by that date, as well as (p)reprints of their work. AAE/EOE.
Attention: Jean Jesensky, Human Resources Specialist
We have several opportunities for software developers to provide software engineering support for data obtained by NASAs Chandra mission. The Smithsonian Astrophysical Observatory operates the Chandra X-ray Center which supports calibration of the Chandra telescope and science instruments, generates the observing program, supports proposal preparation, and receives, processes, and distributes Chandra data. We're also responsible for the data archive and a portable software package that supports scientific data research.
Responsibilities: Interact with scientists to acquire and understand specifications, develop and test software, use software configuration tools for code management, and conform to project coding standards.
Requirements: Experience in C/C++ in a UNIX environment and established skills in Perl and shell programming and familiarity with software tools such as software debuggers and code checkers. Candidates for our Archive team must possess experience in SQL and relational databases.
View the complete vacancy announcement for this position at http://cfa-www.harvard.edu/cfa/hr/postings/20-41.htm.
We offer a competitive salary, excellent benefits, and a stimulating environment. Interested candidates should forward their resume to the above address.
Attention: Jean Jesensky, Human Resources Specialist
We have opportunities for entry- to mid-level Data Specialists in the Smithsonian Astrophysical Observatory's Chandra X-ray Observatory Science Center (CXC) in Cambridge, Massachusetts.
The Data Specialists will provide support of astrophysical research on data obtained by NASA's Chandra. Launched in 1999, Chandra is a large, orbiting x-ray telescope which searches the universe for x-rays from high energy sources such as black holes, quasars, and supernova remnants. The CXC supports ground and flight calibration of the Chandra telescope and science instruments, generates the observing program, supports proposal preparation, and receives, processes, and distributes the Chandra data.
Duties may include specifying, testing, writing, modifying, debugging, and/or documenting software for data analysis, proposal planning, mission planning, simulations and modeling; running software and analyzing data output; developing and analyzing algorithms; developing and maintaining databases; drafting and maintaining materials for web sites; and providing support to users via personal interaction and email.
To qualify, candidates should possess, at a minimum, a Bachelor's degree (or comparable experience), with a major in computer science or related field, or a major in astronomy, physics or a related field which included computer-related course work. Experience in computer operations and/or software development, ideally in a UNIX environment, is required. Knowledge of astronomy, physics, C/C++, data analysis, and/or HTML is a plus. A combination of experience and education will be considered.
For more detailed information about these positions, please view http://cfa-www.harvard.edu/cfa/hr/postings/20-22.htm and http://cfa-www.harvard.edu/cfa/hr/postings/21-24.htm.
We offer a competitive salary, a comprehensive benefits package, and a stimulating environment. Interested candidates should forward their resume or curriculum vitae to the above address.
We are an equal employment opportunity employer committed to diversity in our workplace.
Attention: David Hughes and William Wall, Doctor
ASTROPHYSICS WITH THE LARGE MILLIMETER TELESCOPE (To see the complete version of this ad, see web page http://www.inaoep.mx/~astrofi/ad2000.txt)
The Instituto Nacional de Astrofisica Optica y Electronica (INAOE) is seeking candidates for three research positions (tenure-track level) in Astrophysics and several postdoc positions. Preference will be given to candidates with experience in millimetre-wave Observational Cosmology and/or millimeter-wavelength instrumentation and general mm-wave observing experience, including molecular cloud observations. However, candidates with expertize in other fields are also encouraged to apply.
INAOE is currently engaged in a joint collaboration with the University of Massachusetts to develop and build the Gran Telescopio Milimetrico - Large Millimeter Telescope (GTM/LMT) and its suite of instrumentation. The LMT is a single dish 50-meter telescope designed to perform at millimeter and submillimeter frequencies up to 350 GHz. Astronomers at INAOE will have significant access to the largest, most sensitive, most technologically advanced millimeter-wave telescope ever built. The LMT is currently under construction on Cerro La Negra, a high-altitude (4600m) ultra-dry site in the central Mexican state of Puebla.
Salaries are competitive by international standards. Please contact Dr. Miguel Chavez (mchavez@inaoep.mx) for details.
Applicants must send their full curriculum vitae, list of publications, and arrange for two reference letters to be sent to the following address Dr. David Hughes and Dr. William Wall at the above address.
Attention: Peter Timbie, Associate Professor of Physics
The University of Wisconsin has recently initiated a program in observational cosmology and invites applicants to join our experiments to measure the properties of the 2.7 K cosmic microwave background radiation. A major goal is to measure the polarization of the background radiation (see POLAR and COMPASS experiments at http://cmb.physics.wisc.edu). We are developing high-performance detectors of millimeter and sub-millimeter radiation as well as novel cryogenic techniques for future ground-based, balloon-borne, and space-based missions. Our work is in close collaboration with the UW X-ray detector program led by Dan McCammon. Participation in the development of a new public outreach program is encouraged. We have two positions; successful candidates must have a Ph.D. in physics or a related field. Experience in some of the following areas will be useful: cosmology, low-noise detectors, cryogenics, microwave circuits, and antennas. Interested candidates should send or email a letter of application, a vita, and names and addresses of three references to Professor Peter Timbie. Please address questions to timbie@wisp.physics.wisc.edu. The University of Wisconsin especially encourages women and minorities to apply. AAE/EOE.
Attention: Dan McCammon, Professor-physics
The X-ray Astronomy group at the University of Wisconsin, Madison, has openings for two postdoctoral researchers to assist with its program of developing microcalorimeter detectors for high resolution X-ray spectroscopy and applying them to sounding rocket and satellite investigations of the diffuse X-ray background and the "missing baryon" problem. We are looking people with strong laboratory skills, a predilection toward instrumentation, a willingness to develop an interest in high energy astrophysics, and the ability to lead independent investigations with the assistance of graduate and undergraduate students. Experience in X-ray astronomy, sounding rockets, silicon microfabrication, superconductivity, and/or sub-Kelvin cryogenics is a plus. The emphasis of this position could be in any or all of these areas, depending on the interests and experience of the applicant. Coupled applications are welcome. A more senior position could be available for a candidate with suitable experience and qualifications. Interested parties should send a letter of application with vita and names of three references to Prof. Dan McCammon, at the above address. Questions can be addressed to mccammon@wisp.physics.wisc.edu. The University of Wisconsin especially encourages women and minorities to apply. AAE/EOE.
Attention: Jean Jesensky, Human Resources Specialist
Applications are invited for an Astrophysicist to join the Chandra Multi-wavelength Project (ChaMP) extragalactic and galactic plane (ChaMPlane) survey collaborations in our High Energy Astrophysics Division. The ChaMP is a serendipitous X-ray survey using Chandra archival data that will cover about 30 degrees over 5 years to intermediate flux levels, complementing the deep surveys which cover small areas to very deep flux levels. The ChaMP will find thousands of active galaxies, and hundreds of clusters, many at high redshift. The ChaMPlane survey will cover about 10 degrees of the galactic plane over its five year duration and find a large sample of X-ray emitting stars and binaries.
The successful applicant will work with Dr. Belinda Wilkes and Dr. Paul Green (ChaMP) and Professor Josh Grindlay (ChaMPlane) primarily with the optical imaging analysis groups for both extragalactic (ChaMP) and galactic (ChaMPlane) fields to develop and implement data reduction and analysis of the large amount of optical imaging data already in-hand. He/she will also assist in writing proposals and observing at NOAO, SAO and other telescopes as needed. The tasks of the successful candidate will also include interaction with the X-ray analysis team to identify optical counterparts and to assist in development of a database for the ChaMP and ChaMPlane surveys.
Candidates must posses a Masters or equivalent (Ph.D. is strongly preferred) in astronomy, physics, astrophysics, or a related field, or comparable experience. Candidates also should have experience in observation and analysis of optical CCD images, experience with surveys and catalogs, and a strong scientific interest in working in this area. Experience with data analysis at X-ray or other wavelengths is also desirable.
This position will be for two years initially, with possible extension subject to future funding levels.
For more detailed information, please view the complete vacancy announcement for this position at http://cfa-www.harvard.edu/cfa/hr/postings/21-21.htm.
Interested candidates should forward curriculum vitae, bibliography, and names, addresses, telephone numbers, and email addresses of three professional references to the above address.
ChaMP and ChaMPlane personnel will be available at the 197th AAS meeting in San Diego, CA to interview interested candidates.
We are an equal employment opportunity employer committed to diversity in our workplace. AAE/EOE.
Attention: Professor Cheng-Chung Chi, Chairman
The Graduate Institute of Astronomy at the National Tsing Hua University invites applications, in all astronomy and astrophysics research areas, for several faculty positions to start in the 2001-2002 academic year. Assistant, associate and full professorship will be considered according to qualification. Successful candidates are expected to teach at both undergraduate and graduate levels, and to develop independent research programs. Research and teaching experiences beyond Ph.D. are preferred. Applicants should arrange to have a resume, a list of publications, a few recent reprints, a description of research plan, and at least three reference letters sent to Prof. C.C. Chi, Chairman, at the above address. All application materials must be received by 31 March 2001 to receive full consideration. For detailed information on astronomy and astrophysics programs at National Tsing Hua University, please contact Prof. Dean-Yi Chou (chou@phys.nthu.edu.tw).
Attention: Linda Tobin, Personnel Officer
Astronomical Research Fellow - SAAO
Applications are invited for a postdoctoral research fellowship at the South African Astronomical Observatory (SAAO). The appointment will be for two years, with a likely extension to a third year. Preference will be given to candidates with an interest in infrared and/or optical instrumentation.
The SAAO is the National Facility for optical/infrared astronomy in South Africa. Its headquarters are in Cape Town where the successful applicant will be based. Observing facilities, situated 360 km away at Sutherland, comprise four common user telescopes and a recently commissioned 1.4-m Infrared Survey Facility (IRSF) run in collaboration with Nagoya University, Japan. Construction of the Southern African Large Telescope (SALT), a 10-m class instrument, should be completed by 2004.
While the successful applicant will spend most of their time on research, they will also be encouraged to contribute to the SAAO's instrumentation or software development programmes as well as supporting visiting astronomers. More details of the SAAO, SALT and the current research interests of their staff are available at www.saao.ac.za and www.salt.ac.za.
SAAO is committed to Equity.
Applicants must have a PhD in astrophysics or a related subject. They should submit a curriculum vitae, with a statement of research and instrumentation interests to: The Personnel Officer, Ms Linda Tobin, at the above address. Applicants should also arrange for three professional referees to supply letters of recommendation to the same address by the due date of 1 March 2001.
Attention: Linda Tobin, Personnel Officer
Astronomer/Instrument Scientist - SAAO
The South African Astronomical Observatory (SAAO) seeks an astronomer with a strong interest in infrared/optical instrumentation.
The SAAO is the National Facility for optical/infrared astronomy in South Africa. Its headquarters are in Cape Town where the successful applicant will be based. Observing facilities, situated 360 km away at Sutherland, comprise four common-user telescopes and a recently commissioned 1.4-m Infrared Survey Facility (IRSF) run in collaboration with Nagoya University, Japan. Construction of the Southern African Large Telescope (SALT), a 10-m class instrument, should be completed by 2004.
The preferred applicant will have experience in working with near-infrared and/or optical CCD arrays. A PhD in astrophysics or a related subject is essential as she/he will also be expected to spend about 50% of their time on research. More details of SAAO, SALT and the current research interests of their staff are available at www.saao.ac.za and www.salt.ac.za.
SAAO is committed to Equity.
Applicants should submit a curriculum vitae, with a statement of research and instrumentation interests to: The Personnel Officer, Ms Linda Tobin, at the above address. Applicants should also arrange for three professional referees to supply letters of recommendation to the same address by the due date of 1 March 2001.
Attention: Kent Honeycutt
The Astronomy Department at Indiana University, Bloomington, invites qualified senior astronomers to apply for the newly endowed Daniel Kirkwood Chair in Astronomy. We seek to fill this position with an individual who will positively impact our existing programs and facilities. There is a departmental research emphasis on stars and stellar systems, which is supported by our participation in the WIYN Observatory as well as access to several smaller telescopes. The department also has access to an extensive array of high-performance parallel computer systems. Degree programs from the B.S. to the Ph.D. are offered by the department, as well as a variety of introductory courses for nonmajors. We therefore value quality teaching as well as research. Descriptions of our instructional and research programs can be found at http//www.astro.indiana.edu/. Interested observational astronomers, theorists, or instrumentalists with a distinguished research record should direct inquiries or applications to Kent Honeycutt at the above address.
This position will remain open until a candidate has been selected.
Women and minorities are encouraged to apply. AAE/EOE.
Attention: Robert Morse, Professor
One or more postdoctoral positions in experimental neutrino astrophysics are availabe at the Physics Department of the University of Wisconsin-Madison. The research will focus on analyzing data from the recently completed AMANDA neutrino detector at the South Pole (Antarctic Muon And Neutrino Detector Array). The research covers data-analysis, Monte-Carlo simulations, and operational support of the experiment at the South Pole. The scientific program includes the search for high-energy neutrinos from gamma-ray bursts, active galaxies, diffuse radiation of high energy neutrinos, and for dark matter. The successful candidate is expected to have a Ph.D. in physics. Experience with data analysis and programming methods used in particle physics is expected. The positions are initially for a period of one year with the expectation of 1-2 year extensions. The positions will be available in February 2001 and the search will continue until filled. Applicants should submit a resume, a summary of research interest, and arrange to have three letters of recommendation sent to Professor Robert Morse at the above address. AAE/EOE.
Attention: Drs. John Carr or Jackie Fischer,
The Infrared Group of the Naval Research Laboratory's Remote Sensing Division invites applications for NRL National Research Council Associateships in infrared astronomy. Candidates with interests in star formation, galaxy evolution, the interstellar medium, or infrared instrumentation are encouraged to apply. The group is currently using ground and space-based infrared spectroscopy and various modeling techniques to study infrared-bright galaxies, young stellar objects, and stellar chemical abundances. Other Laboratory astronomers carry out research programs in areas of radio through gamma-ray astronomy. Associateships are awarded to persons who have held their doctorate for less than five years at the time the award is offered. Awards are for two years. Applicants should submit an original research proposal for approval to the NRL-NRC advisor and for subsequent evaluation by an external review panel chosen by the NRC. The deadline for submission to the NRC is 15 April 2001. US citizenship or permanent residence is required. Application materials can be obtained online at: http://www4.nationalacademies.org/osep/rap.nsf or by writing to the Associateship Programs Office, at the above address. For detailed information contact Dr. Jackie Fischer (202-767-3058, fischer@irfp8.nrl.navy.mil) or Dr. John Carr (202-767-0670, carr@mriga.nrl.navy.mil) EOE/AAE.
Attention: Lynne A. Hillenbrand
Applications are solicited for appointment as a Postdoctoral Scholar in the Astronomy Department at Caltech with Lynne Hillenbrand. The main areas of interest are optical and near-infrared investigations of young stellar populations (working with Palomar and Keck data), and the evolution of primordial planet-building and secondary ``debris'' disks on Myr to Gyr timescales (SIRTF Legacy planning). In addition to making progress on these existing projects, the successful candidate will be encouraged to pursue independent but related research goals.
The application package should include a vita, list of publications, brief summary of research interests and experience, and the names of and contact information for at least three individuals familiar with the applicant's record. Receipt of the above materials by 5 March will ensure highest priority consideration, though later applications will be accepted. Salary will be commensurate with experience and competitive with other similar postdoctoral positions. The applicant should be ready to begin the appointment in the September/October time frame, negotiable.
Caltech's astronomical facilities include the Palomar Observatory, W.M. Keck Observatory, Owens Valley Radio Observatory, and Caltech Sub-millimeter Observatory. See [http://www.astro.caltech.edu] for additional information. Women, minorities, veterans, and disabled persons are encouraged to apply. AAE/EOE.
Attention: Human Resources
The Next Generation Space Telescope (NGST) is the centerpiece of the NASA Office of Space Science theme, the Astronomical Search for Origins, and the highest priority astronomy project for the next decade, according to the National Academy of Science. NGST will need to have the sensitivity to see the first light in the Universe to determine how galaxies formed in the web of dark matter that existed when the Universe was in its infancy (z ~10-20). To achieve this challenging goal, we must pursue an aggressive technology program and advance infrared detectors to performance levels beyond what is now possible.
As part of this program, NASA has selected the Independent Detector Testing Laboratory (IDTL), jointly operated by STScI and JHU, and located on the JHU campus, to be the laboratory for verifying comparative performance between prototype NGST detectors developed by Rockwell and Raytheon. The IDTL is charged with the mission of obtaining the best possible measurements of infrared detector performance in an ultra-low background (<0.01 e¯/s/pixel) environment which is similar to the on-orbit environment to be experienced by NGST. To address this challenge, we have assembled a team of experts from around the world to design and execute these measurements. Our formal partners in this project include Rockwell, Raytheon, NOAO, Gemini, and ESO.
Applications are invited for a postdoctoral research position at the Space Telescope Science Institute to work with Dr. Donald Figer. The successful applicant will assist in characterizing infrared array detectors for the NGST; design and conduct experiments on 1-5 micron infrared array detectors manufactured by Rockwell and Raytheon and assist NGST scientists and engineers in performing design studies in support of the NGST mission.
Candidates must hold a PhD in astronomy, physics, electrical engineering or related field by date of appointment. Substantial experimental experience and some knowledge of electronic design, optical design, cryogenic technology, and computer programming is required. However, candidates with experience in any of these areas would be considered. Experience with infrared detectors is a plus. The initial appointment is for one year, renewable for up to three years depending on performance and continued funding. There are no restrictions on citizenship.
STScI, located on Johns Hopkins University Campus in Baltimore, Maryland, offers an excellent benefit package, competitive salaries, and a stimulating work environment. The minimum salary is $41,900; however, STScI’s pay is commensurate to the year of Ph.D.
Applicants should send a cover letter with position applying for, curriculum vitae, list of publications, and a brief statement of research interests, accomplishments, and relevant technical expertise to the address below. They should also arrange for three letters of recommendation to be sent directly to the same address. Completed applications received by 16 March 2001 are assured of full consideration. EOE/AA/M/F/D/V.
Attention: Dr. David Guenther
The Department Astronomy and Physics at Saint Mary's University is seeking a scientist with recognized expertise in numerical astrophysics to serve as the first Director of an Institute for computational astrophysics. The individual, who accepts the challenge of creating a vibrant and scientifically productive enterprise, will manage daily operations, hire post-doctoral fellows, assist in filling subsequent positions, and work to secure additional funds for advanced computing machinery and infrastructure. The recommended teaching load will be no more than one course per term. This is a Tier I Canadian Research Chair position, with funding of $200,000CDN/year (seven years, unlimited renewals) for salary, benefits, and research expenses guaranteed under the Canadian Research Chairs Program. Canadian citizenship is not required. Applicants should send a detailed resume along with the names and e-mail addresses of three references to Dr. David Guenther, at the above address.
Attention: Philippe André, Dr.
As part of a European Commission Research Training Network on ``The Formation and Evolution of Young Stellar Clusters'', a postdoctoral position is available for two years in the Star Formation Group of CEA Saclay, France.
The Astrophysics Department at CEA Saclay is a major space astrophysics laboratory, located about 20 km south-west of Paris, close to several other astronomy centers. In particular, the department led the development of the ISOCAM mid-infrared camera aboard ISO, and is involved in the EPIC X-ray camera of XMM, as well as in the two bolometer-array cameras of the future Far InfraRed and Submillimeter Telescope (FIRST).
In recent years, our group has focused on (sub)millimeter studies of the earliest stages of star formation including protostars and pre-collapse cloud cores, and on high-energy/magnetic processes affecting young stars and their environment. We are also involved in hydrodynamical simulations of cloud fragmentation and collapse. We seek candidates wishing to work on one of these topics.
We invite applications from people with observational or theoretical experience in young stellar objects, molecular clouds, or related fields. Applicants should have a Ph.D. and should be 35 or under at the time of appointment, be a national of a European Community member or associated state other than France, or have lived in the EC for at least five years before appointment, and not have lived in France for more than 12 of the 24 months prior to appointment. The starting date is flexible before the end of 2001. The net salary, after deductions, will be around 14000 FF (2150 Euros)/month.
Please send a CV, a list of publications and a statement of research interests, and arrange for three letters of recommendation before 15 March 2001. Later applications may also be considered. Informal inquiries are welcome.
Attention: Stuart Vogel, Professor
The Laboratory for Millimeter-wave Astronomy (LMA) is seeking a programmer/scientist to participate in ongoing projects. The successful candidate will work with a team including two other programmer/scientists on one or more of the following: 1) radiometric phase correction for interferometers; 2) pipeline reduction for interferometric data; 3) real-time monitoring of data from interferometric arrays; 4) kinematic analysis of data cubes; 5) development of a spectrometer package for SOFIA; and 6) a SIRTF Legacy project on the formation of stellar systems. Persons with interests in any of these areas are encouraged to apply. We are looking for candidates with experience in object-oriented programming languages, such as Java or C++. Experience working within the AIPS++ environment is a plus. The position is initially for two years, with renewal possible beyond that period. Applications received by 30 March 2001 will receive full consideration.
Research interests within the LMA include star formation, interstellar medium, galactic structure, extragalactic studies, solar and planetary astronomy, and mm/submm instrumentation. The University of Maryland is a partner in BIMA (Berkeley-Illinois-Maryland Association), which operates the BIMA millimeter interferometer, an array of ten antennas operating at frequencies from 28 to 280 GHz at resolutions as high as 0.2 arcseconds. AAE/EOE.
Attention: Dr. Adair P. Lane
The Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) project is seeking an experimentalist to operate the first permanent submillimeter-wave telescope at the United States National Science Foundation Amundsen-Scott South Pole Station. Beginning in mid-2001, the incumbent will participate in data reduction and analysis and in preparation for the winterover year while stationed at the Harvard- Smithsonian Center for Astrophysics in Cambridge, MA. Late in 2001, he or she will spend 1-3 months at the South Pole during Austral summer to operate the instrument, assist with system upgrades, and conduct research. After another 9-month period in Cambridge, the incumbent will spend the year 2003 as the AST/RO scientist in residence at South Pole (as part of a crew of ~50), bearing sole responsibility for winterover operations of this state-of-the-art submm-wave telescope. The position will be renewable for a year following the winterover year, with residence in Cambridge.
AST/RO is currently outfitted with heterodyne receivers at 230, 460-492, and 810 GHz; a new high-frequency 4-channel array receiver was installed in November 2000, providing significantly expanded capabilities. AST/RO is the first submillimeter telescope to exploit the uniquely transparent sky over the Antarctic plateau in winter and is open to the astronomical community on a proposal basis. This position provides a unique opportunity for both personal and collaborative research projects which can be conducted nowhere else. More information about the AST/RO project can be found at our Web site at http://cfa-www.harvard.edu/~adair/AST_RO.
A Ph.D. or equivalent technical experience is required. A good general understanding of astronomical instrumentation and familiarity with computer operations and software, cryogenics, and electronics are desirable. Ability to work independently is critical. AST/RO is operated under the aegis of CARA, the Center for Astrophysical Research in Antarctica. Applications, including a statement of research interests and relevant experience, curriculum vitae, and three letters of reference, should be sent to Dr. Adair P. Lane at the above address before 31 March 2001. Women and minorities are encouraged to apply. AAE/EOE.
Attention: Steven R. Majewski
Applications are invited for a full time research support position for applicants at the BA/BS degree level. There is some flexibility in starting date, but a starting date as soon as June 2001 is preferred. The appointment would be for one year, with possibility of renewal for continuing years subject to favorable reviews and funding availability. The position will involve analysis of data relating to research on stellar populations in the Milky Way, and centered on the Grid Giant Star Survey, which is being conducted on behalf of NASA's Space Interferometry Mission (SIM; http://sim.jpl.nasa.gov/) specifically for the SIM Astrometric Grid. Other duties may include telescope observing in the southern and/or northern hemispheres. Applicants should have at least a BA/BS degree in Physics or Astronomy as well as basic computer skills, including programming ability (C, C++ or Fortran) and familiarity with the UNIX environment and IRAF. Previous experience with CCD reductions, either imaging or spectroscopy, and some familiarity with html would be especially useful.
Applicants should submit a vita, a statement of research experience, and their bibliography. They should also arrange to have three letters of recommendation sent. The University of Virginia is an Affirmative Action/Equal Opportunity Employer. Full consideration will be given to completed applications received no later than 4 May 2001, or until the position is filled. AAE/EOE.
Attention: Victoria Kaspi, Professor
Applications are invited for a postdoctoral position in observational radio pulsar astronomy. The ideal candidate will have a working knowledge of radio pulsar data and/or time series analysis, though excellent candidates with other related backgrounds will be considered.
McGill University is among Canada's premiere universities. Presently astrophysics topics studied at McGill, in addition to radio and X-ray observations of neutron stars, are ground-based gamma-ray astronomy (the STACEE collaboration), and a strong theory program in early universe physics and cosmology. McGill is English-language and is in the heart of downtown Montreal, a cosmopolitan city with a distinctly European flavor. Near McGill is University of Montreal, which also has an active astronomy program.
This position is for two years, possibly renewable to a third. Travel to observatories and conferences will be supported. Applicants must have a PhD by the start date in Sept 2001 and should mail a CV, statement of research interests, and arrange for at least three letters of recommendation to be sent. Applications received before 28 February 2001 will receive priority.
Applications should be sent to Prof. V. Kaspi, at the above address.
Attention: Leo O. Takalo
The Nordic Optical Telescope Scientific Association (NOTSA) invites applications for the post of Director of the 2.56-m Nordic Optical Telescope (NOT). The NOTSA, the members of which are Denmark, Finland, Iceland, Norway and Sweden, has constructed and operates the NOT on La Palma, Canary Islands, Spain. The Director is the Chief Executive Officer of NOTSA, responsible for the overall scientific, technical and financial planning and management of NOTSA. The Director will be appointed by the NOT Council for an initial period of three years with possibility for renewal. The Director is expected to set up his/her office in one of the member countries. The salary level will be equivalent to that of a full University Professor in the country of residence.
The starting date for the position is 1 May 2002. The applicant should have an excellent research record in observational astronomy as well as a proven record of managerial experience in running an astronomical institute and/or observatory. Fluency in Spanish is helpful, but not required. Applications (5 copies) should include a detailed curriculum vitae and bibliography, including a summary of past research and managerial experience and such further documentation the applicant wishes to be considered. Furthermore, an outline should be included, detailing how the applicant intends to maintain and improve the performance of the telescope and instrumentation. Applications should be addressed to The NOT Council and sent to Dr L. Takalo at the above address. The closing date for the applications is 1 April 2001.
Attention: Jean Jesensky, Human Resources Specialist
Applications are invited for an Astrophysicist to participate in research projects involving the analysis of Chandra and XMM observations of galaxies. The successful candidate will be part of a team exploring the properties of the X-ray emission of galaxies, and how they may vary with morphological type and evolutionary state. Areas of investigation include the properties and evolution of the hot ISM, populations of X-ray sources, and low-level nuclear activity.
To qualify, candidates must possess, at a minimum, a Master's or equivalent degree in astronomy, physics, astrophysics, or a closely related field, or comparable experience. A Ph.D. is preferred. Candidates may have either an observational or a theoretical background, but must have demonstrated abilities in data analysis techniques and experience with X-ray data analysis.
For more detailed information, please view http://cfa- www.harvard.edu/cfa/hr/21-27.htm. Technical inquiries about the position may be made to Dr. G. Fabbiano at gfabbiano@cfa.harvard.edu.
The initial appointment is for up to two years, with the possibility of extension.
We offer a competitive salary, a comprehensive benefits package, and a stimulating environment. Interested candidates should forward curriculum vitae, bibliography, a brief description of research interests, and the names, addresses, email addresses, and telephone numbers of three professional references to the above address.
We are an equal employment opportunity employer committed to diversity in our workplace. AAE/EOE.
Attention: Jean Barrette, Chair
The Department of Physics at McGill University in Montreal is expanding its research in astrophysics. Applications are invited for a tenure-track faculty position at the rank of Assistant Professor, beginning as early as September 2001.
We seek candidates with a proven record of excellence in research and who will strengthen or add to our existing research interests. Faculty members are currently active in radio, X-ray, and gamma-ray astronomy, with an emphasis on high-energy phenomena. However, candidates for this position can be from any field in astrophysics. Candidates are expected to have a capacity for excellence in teaching.
Applicants should submit a detailed curriculum vitae and a statement of teaching interests as well as a research plan. They should also arrange for three letters of reference to be sent directly to Professor Jean Barrette, Chair at the above address.
The deadline for the receipt of applications and letters of recommendation is 15 April 2001. In accordance with Canadian Immigration requirements, priority will be given to Canadian citizens and permanent residents of Canada. McGill University is committed to equity in employment.
Attention: Human Resources
El Camino Community College is seeking outstanding candidates to apply for a Planetarium Director or Manager. Application package must be received by 4:30 p.m. on Friday, 30 March 2001, in the Office of Human Resources. Under the general direction of the Dean of Natural Sciences, the Director/Manager will be responsible for developing and presenting educational, entertaining programs on Astronomy both in the planetarium and observatory for the college community, school age students and general public. If qualified, the Planetarium Director may teach Astronomy courses as needed.
Minimum qualifications for Director - Master's degree and one year of formal leadership training, internship, or leadership experience reasonably related to the administrative assignment.
Minimum qualifications for Teaching - Master's degree in Astronomy or Astrophyics OR Bachelor's degree in Astronomy or Astrophyics and a Master's degree in Physics, Engineering Mathematics or Geophysics.
Minimum qualifications for Manager - Bachelor's degree in Science or Engineering and a minimum of twelve college units in Astronomy.
The position is a full-time, twelve month position. Opportunities to organize a science lecture series for the public, to submit articles to local and national science publications. El Camino College is committed to diversity and equality in education and employment. AAE/EOE.
Attention: Dr. David Huenemoerder
The MIT Center for Space Research has an opening for a Research Scientist/Physicists in the Chandra X-Ray Observatory Center (CXC) group to support the data analysis of diffraction grating spectra. Specific task include the specification and improvement of Chandra data processing software, verification of software, development of improved or advanced analysis techniques, development of software prototypes, preparation of calibration reference data, editing or authoring technical reference documents, verifying production data quality and participating in CXC service role, up to 40% of the effort will be allocated to independent scientific investigations.
The MIT group works closely with CXC calibration scientist and the HETG Instrument Principal Investigator team at MIT, with the MIT ACIS team and in collaboration with CXC scientists and programmers at the Harvard-Smithsonian Center for Astrophysics.
The candidate must have a strong background in observational astronomy, preferably in X-ray spectroscopy, and proven ability to conduct independent research. Substantial experience with data analysis techniques for imaging and/or spectroscopy is required: the primary task is to support the processing and analysis of the Chandra diffraction grating instruments, HETG and LETG.
The position requires a Ph.D. in Astronomy, Physics, or closely related field. Qualified applicant should send their resumes and three letters of reference to Dr. David Huenemoerder at the above address. AAE/EOE.
Attention: Henry H. Plotkin, Associate Director
Position is that of Research Scientist in the Goddard Earth Sciences and Technology Center (GEST), and will be located at the NASA Goddard Space Flight Center (GSFC), Greenbelt, MD. GEST is a Cooperative Agreement between the University of Maryland, Baltimore County (UMBC) and GSFC to collaborate in research programs in the Earth, Information, and Instrumentation sciences. GEST is a Consortium whose members include UMBC, Hampton University, Howard University, and Caelum Research Corporation.
The OSCAR (Optical Systems Characterization and Analysis Research) project at GSFC researches, develops and applies parallel computational techniques to solve complex optical, imaging, and data analysis problems of interest to the NASA scientific and engineering communities. They involve the interplay of Computer Science, Image Processing, Optics, Applied Mathematics, Astronomy, and Earth Sciences. Computer resources will include a Beowulf cluster of hundreds of processors, a new Cray T3E, as well as workstations, PC’s and Macintoshes. The incumbent will study, model, simulate, and develop algorithms for wavefront sensing, optical control systems, interferometric and coronagraphic imaging systems for space applications. He will become directly involved in collaborating with scientists and engineers participating in NASA Space and Earth Science projects which may include the Next Generation Space Telescope, Terrestrial Planet Finder, and others.
Candidates must have excellent programming and numerical analysis skills and be well versed in applied mathematics and algorithm development. Parallel coding experience is desired, but not required. They should have had experience and understanding of one or more of the following: imaging science, image processing, and/or electro-optics, and have participated in developments for an aerospace environment.
Attention: , Departmental Secretary
UNIVERSITY OF OXFORD
MATHEMATICAL AND PHYSICAL SCIENCES DIVISION
DEPARTMENT OF PHYSICS
UNIVERSITY LECTURERSHIP IN ASTROPHYSICS IN ASSOCIATION WITH NEW COLLEGE
The department of Physics proposes to appoint a University Lecturer in Astrophysics with effect from October 1, 2001 or as soon as possible thereafter. The combined University and College salary will be according to age on a scale up to £39,564 per annum Preference will be given to applicants with a strong background in theoretical cosmology. However, well-qualified candidates in other areas of astronomy are also encouraged to apply. The Lectureship is associated with a Tutorial Fellowship in Physics at New College. Oxford University has a wide-ranging research programme in astronomy, astrophysics, cosmology and particle astrophysics. Highlights include telescope instrumentation; the scientific activities of the UK Gemini Support Group; galaxy and quasar surveys, and observational studies of large scale structure star formation; stellar evolution, X-ray binary and supernova theory; dark matter and microlensing; galaxy formation and evolution; cosmic microwave background radiation and early universe theory; and radio galaxies. Oxford is a major node of PPARC's STARLINK computing network. A 128 node BEOWULF computer system will be installed in Spring 2001. Further particulars of the post and more information on the research programme may be obtained from http://www-astro.physics.ox.ac.uk. Applications including a statement of research interests and teaching experience, curriculum vitae, a list of up to ten major publications, and the names of three referees should be sent to arrive no later than 31 March 2001 to Departmental Secretary, at the above address. Not more than two of the referees should be from the same institution and they should all be asked to send letters of reference directly to Prof. J. Silk at the same address to arrive by the closing date. U.K. applicants should submit six copies of their application, while overseas applicants need only submit one copy.
Attention: Phillip C. Stancil, Assistant Professor
Applications are invited for a postdoctoral position at The University of Georgia to conduct theoretical/computational research in molecular physics for astrophysical applications. The project involves the calculation of molecular line lists, photodissociation cross sections, and molecule-molecule collisional excitation rate coefficients for species of importance to Extrasolar Giant Planets (EGPs). The successful candidate will work closely with Phillip Stancil, Tim Heil, and Kate Kirby (CfA) for the production of such data, which will in some cases require the computation of potential energy surfaces. The project will also require close collaboration with Peter Hauschildt and Andres Schweitzer to test the results in advanced EGP models.
The initial appointment is for one year, possibly renewable for a second or more years depending on available funding and progress. Candidates should have a recent Ph.D. in physics, chemistry, or related field. Inquires and applications, including a CV, statement of research interests, and the names and addresses (no letters at this time, please) of three references, should be addressed (electronically if possible) to Phillip Stancil at the above address.
The application deadline is 31 March 2001, but the search will continue until a suitable candidate is identified. AAE/EOE.
Attention: Peter Brown, Assistant Professor
The Department of Physics and Astronomy at the University of Western Ontario has an immediate opening for a post-doctoral fellow. The successful candidate will work with Dr. Peter Brown of the meteor physics group in the area of observational planetary astronomy. This person will primarily conduct research relating to a new program of physical studies of small near-Earth asteroids (NEAs) being developed at UWO. In particular he/she will be charged with the observation and data reduction of seven color photometry of recently discovered NEAs using the UWO Elginfield 1.2m telescope. The position requires experience with the gathering of telescopic astronomical data and subsequent reduction. Knowledge of IRAF, Unix and experience with large-format CCDs is highly recommended, though not a strict requirement. The position will also offer the opportunity to engage in research work relating to radar meteor studies and/or orbital numerical simulation work with the UWO meteor physics group. The starting salary will depend on experience, but is expected to be approximately $35,000 CAD per annum. This is a two year position with the possibility of renewal for up to five years.
Candidates interested in additional information or wishing to apply are invited to submit a CV, a statement of research interests and contact details for three people willing to provide references before 30 March 2001 by email to Dr. Peter Brown (pbrown@julian.uwo.ca).
Attention: Sandra Abbey
Sr. Scientific Programmer (in Tucson): Develops and maintains computer systems that support the following applications: control of astronomical instruments; data acquisition, reduction and analysis; data storage distribution. Management and observatory administrative functions; electronic communication and document generation. Requires: MS in comp sci, math, engineering or physical science and 6 yrs scientific programming exp (or BS and 8), knowledge of FORTRAN, C, Unix or comparable languages. Reply by 30 March 2001 to Sandra Abbey, at the above address. Preference given to qualified Native Americans living in or near the Tohono O'Odham reservation. AAE/EOE.
Attention: Robert Morse, Professor
The AMANDA collaboration invites applications from persons interested in spending approximately 13 months at the South Pole station, Antarctica, running the AMANDA, SPASE/VULCAN and RICE astrophysics experiments. Experience in Physics, Astrophysics, Electrical Engineering, or Computer Science is required, along with the ability to work and live successfully in a small group. Resourcefulness, self-motivation and ability to learn new skills are very important.
For more information, see the official Position Vacancy listings at http://www.ohr.wisc.edu/pvl/pv38808.html http://www.ohr.wisc.edu/pvl/pv38809.html (which include application details), contact Bob Morse (morse@alizarin.physics.wisc.edu), or visit our website, http://amanda.berkeley.edu
Attention: Philip E. Hardee, Professor
Candidates are sought for a research position in theoretical astrophysics with a duration of 2 - 3 years to start as early as Summer 2001. Salary will be commensurate with experience. Preference will be given to individuals having experience in relativistic computational hydrodynamics and MHD, particularly as it relates to relativistic jets in astrophysical systems. The theoretical/computational work should be relevant to current research projects on relativistic jets being conducted in Tuscaloosa and could be relevant to research projects involving analysis of data from BATSE (http://gammaray.msfc.nasa.gov/batse/), BeppoSAX, Chandra, and RXTE being conducted in Huntsville.
The sucessful candidate can spend time in residence either at the Physics & Astronomy Department on The University of Alabama campus in Tuscaloosa or at the National Space Science and Technology Center adjacent to the University of Alabama campus in Huntsville. The NSSTC consists of researchers from NASA Marshall Space Flight Center, the University of Alabama in Huntsville and the Universities Space Research Association.
A Ph.D. in astrophysics, astronomy or physics is required. Applicants should send vita, bibliography, statement of research interests, and names of three references to Prof. Philip E. Hardee at the above address, preferably before 30 April 2001. AAE/EOE.
Attention: Robert L. Mills, Director
Lowell Observatory seeks an experienced project manager to guide the planning, construction, and commissioning of a 4-meter-class, wide-field telescope to be built in Northern Arizona. Previous experience in management of a comparable telescope project is essential. Salary will be commensurate with experience and qualifications. To apply, send a cover letter, resume and the names and addresses of three professional references to R. Millis at the above address. Applications received by April 30 will be given full consideration. AAE/EOE.
Attention: Orgins Associateship
Applications are invited for a postdoctoral research associateship at DTM/CIW. The fellow will work with Alan Boss on theoretical models of mixing and transport processes in protoplanetary disks, with implications for the formation of planetary systems. The appointment is initially for one year, with a second year being contingent upon satisfactory progress on the research project.
DTM has an active group of researchers in this area. Alan Boss and George Wetherill lead the theoretical effort to understand the formation and evolution of stellar and planetary systems, while Paul Butler is active in the search for extrasolar planets. Conel Alexander and Larry Nittler perform laboratory studies of pre-planetary materials. Other DTM staff members include astronomers John Graham and Vera Rubin, and planetary scientist Sean Solomon. Carnegie is a lead member institution of the NASA Astrobiology Institute. Theoretical calculations are performed on the Carnegie Alpha Cluster.
Applicants should have a Ph.D. in a relevant field, experience with numerical hydrodynamics codes, and excellent computer skills. Applications should include a curriculum vita, a publication list, and three letters of reference to be sent directly to us by those familiar with your work. Applications should be submitted to the above address by 30 April 2001. EOE/AAE
Attention: Caltech Employment Department (Please reference PMA_2768)
The Palomar Observatory has an opening for a Computing Analyst to support current operations at the Observatory and to participate in construction of new instruments to be used at Palomar and at the Keck Observatory. The successful applicant will also take responsibility for organizing and maintaining the Palomar web site. Applicants must have a degree (astronomy, physics, engineering or computer science) plus commensurate experience (Bachelors degree plus 4 years experience or Masters degree plus 2 years experience) in instrument development programs with Unix, VxWorks, Solaris and Linux operating systems, and C, perl, and FORTRAN programming languages. Experience in developing programs for real-time control of instrumentation is highly desirable. Closing date is 15 April 2001.
Please send your resume referencing job code PMA_2768 to the above address. AAE/EOE.
Attention: S. Rawlings, Dr. (please reference DB01002)
UNIVERSITY OF OXFORD
Department of Physics
Research Assistant(s) in Astrophysics
Research Support 1A salary scale, £16,775 to £25,213
The Sub-department of Astrophysics invites applications for one or two PPARC-supported postdoctoral research positions in Observational Cosmology available from 1October 2001. Further particulars of the post and more information on the research programme may be obtained from http://www-astro.physics.ox.ac.uk. Research interests of members of the department include: large scale structure, gravitational lensing, galaxies and star formation at high redshift, AGN as cosmological probes and the physics of AGN and their jets. We particularly welcome applications from candidates with a proven record of research in these or related areas. The postholder will be expected to teach up to three hours per week during term.
Appointments will be made for two years with a possible extension to three years with a starting salary within the salary range above depending on skills and experience. Applicants should send a letter of application quoting reference DB01002 supported by a full curriculum vitae and ask two referees to write by the closing date of 31 March 2001 to Dr S. Rawlings, at the above address.
The University is an Equal Opportunity Employer
Attention: Caltech Employment Department (Please referenceJOB CODE PMA_2769)
The Palomar Observatory has an opening for an Electronics Engineer to support current operations at the Observatory and participate in the construction of new instruments to be used at Palomar and the Keck Observatory.
Applicants must have a degree in engineering plus commensurate experience (Bachelors degree plus four years experience or Masters degree plus two years experience) designing and constructing instrument control systems. Familiarity with array-type detectors and controllers commonly used in optical and infrared astronomy and experience with computer-aided design and layout programs (ORCAD) is desirable.
Close date: 15 April 2001.
Please send your resume referencing JOB CODE PMA_2769 to the above address. Caltech is an AA/EOE employer. Women, minorities, veterans and disabled persons are encouraged to apply. AAE/EOE.
Attention: Melanie Stretton, Mrs
Applications are invited for a PPARC-funded postdoctoral research position to work on theoretical studies of the evolution of cosmological density fluctuations, the statistical properties of galaxy clustering and large-scale structure, and the relationship between the distribution of galaxies and that of gravitating matter in the Universe.
The successful candidate will join our existing PDRAs and research students in a burgeoning cosmology program (led by Professor Peter Coles, Dr Steve Maddox and Dr Frazer Pearce) which encompasses both theory and observation. This activity benefits from close interaction with the other members of the astronomy group at Nottingham (Professor Merrifield, and Drs Peletier and Aragon-Salamanca) whose interests span the range of extragalactic astrophysics, from detailed analyses of individual galaxies to the large-scale structure of the Universe, and combines observational studies with detailed theoretical modelling (see http://www.nottingham.ac.uk/physics/).
Candidates should have (or be about to complete) a PhD in a theoretical cosmology. We welcome applicants with either analytic or numerical expertise (or both).
The post is available for up to three years from 1 April 2001 or as soon as possible thereafter. It is supported by PPARC and the salary is on the RA1A scale, which currently starts in the range (GBP) 16,775 to 18,731, depending on age and experience.
Informal enquiries about the position may be addressed to Prof P.Coles, (Peter.Coles@nottingham.ac.uk) or Steve Maddox (Steve.Maddox@nottingham.ac.uk).
Candidates should send a letter of application, a CV including a brief description of research interests, and should ask two referees to write directly to Melanie Stretton, at the above address.
The closing date for completed applications is 31 March 2001.
Attention: Prof. Willy Kley
Applications are invited for a Post-Doc position in the Computational Physics group of the Institute of Astronomy and Astrophysics of the University of Tübingen (Germany), available immediately. The position is funded by the special research programme SFB 382 (Simulation of Physical Processes on High-Performance Supercomputers) by the German Science Foundation.
The topic of research will be in the field of Computational Astrophysics. The successful applicant will participate in the development of a programme for the solution of the equations of magnetohydrodynamics including radiation transport and self-gravitation.
Part of the work will include the parallelisation of the programme. A massively parallel PC-Cluster consisting of 192 individual processors is available within the group.
Astrophysical problems will include the study of turbulent accretion disks and the formation of planets.
The salary will be according to the German Public Service Tariffs (BAT IIa). Women and minorities are encouraged to apply.
Applications should be sent until 15 April 2001 to Prof. Dr. Wilhelm Kley at the above address.
Informal inquiries are welcome and should be directed to Dr. H. Klahr klahr@tat.physik.uni-tuebingen.de or Prof. Dr. W. Kley, kley@tat.physik.uni-tuebingen.de, Tel. +49 7071 29 74007
Attention: Richard G. French, Professor
The Wellesley College Astronomy Department seeks a 3/5 time leave replacement at the Assistant Professor level for the 2001/2002 academic year, beginning September 2001. Wellesley College, located near Boston, is a highly selective women's college of 2200 students with a history of excellence in astronomy. We are part of the Keck Northeast Astronomy Consortium (KNAC) of eight undergraduate astronomy departments. We are looking for applicants with a Ph.D. in astronomy or astrophysics and evidence of enthusiasm for and experience in undergraduate teaching in astronomy. The successful candidate will teach one course in the fall semester and two courses in the spring semester. Please visit http://www.astro.wellesley.edu for more information about Wellesley College and our department.
The leave replacement position includes full benefits. Candidates should submit a letter of application describing relevant work and teaching experience, a vita, and the names, e-mail addresses, and telephone numbers of three people who would be willing to write letters of recommendation upon our request. Review of applications will begin on 1 April 2001 and will continue until the position is filled.
Wellesley College encourages applications from women, minorities, veterans and candidates with disabilities. AAE/EOE.
Attention: The Personnel Officer, College of Sciences and Technology
Applications are invited for a postdoctoral fellow to work with Dr Tim Bedding on stellar oscillations. The project is to detect and interpret oscillations in solar-like stars using ground-based telescopes and to participate in the development of the Danish-led space telescope MONS (Measuring Oscillations in Nearby Stars).
Candidates must possess a PhD in astronomy or equivalent, show proven research ability, evidence of the potential for further development and evidence of ability to work co-operatively with others. Experience in developing and using software for reduction of astronomical data is essential.
Experience in stellar spectroscopy and/or photometry, particularly observations and analysis of stellar oscillations, is desirable, as are familiarity with IDL and expertise in time series analysis using Fourier transforms and related methods.
The position is full-time fixed term for one year, subject to the completion of a probation period for new appointees. There is the possibility of further offers of employment up to 1.5 years, subject to funding and need.
Applicants are encouraged to contact Tim Bedding before applying.
Remuneration Package: $42,567 - $57,767 p.a. (which includes a base salary Level A $35,970 - $48,814 p.a., leave loading and up to 17% employer's contribution to superannuation).
Applications (five copies) should quote Reference no. A06/001263. They should address the selection criteria, and include a CV, a list of publications, and the names, addresses, e-mail, fax and phone number of three confidential referees. They should be sent to The Personnel Officer, at the above address.
The University is a non-smoking workplace and is committed to the policies and principles of equal employment opportunity and cultural diversity. The University reserves the right not to proceed with any appointment for financial or other reasons. AAE/EOE.
Attention: Giovanni Busarello, Dr.
We invite applications for a VIRMOS postdoctoral fellowship in extragalactic astronomy and cosmology at the Osservatorio Astronomico di Capodimonte (OAC) starting June 2001 (pending the approval of the Council of the Observatory). The fellowship is funded by the Italian Ministry of the University and Research and by OAC, as a part of a national project on "The VIRMOS-VLT survey: a key to the high redshift Universe".
The duration of the fellowship is one year, and is renewable for a second year.
The applicant should have experience in extragalactic astronomy and, in particular, in observational cosmology. The successful applicant will work at the OAC in Napoli, and will join the OAC group that is involved in the (local) project "Evolution of the global properties of galaxies".
The aim of the OAC project is to study galaxy evolution in the framework of the VIRMOS survey through the evolution of the scaling laws (e.g. fundamental plane) and through the evolution of the population parameters (e.g. spectral indices and colors). The successful applicant will be involved in the first phases of the VIRMOS survey and will be asked to contribute to observations, data analysis and interpretation.
The gross salary will be commensurate to experience, and will be in the range from 20000 to 24000 Euro, together with a suitable travel budget and computing support (please notice that taxes in Italy amount to 20% of the gross salary for a fellowship).
The applicant should send the Curriculum Vitae, a list of publications, and three letters of reference at the above e-mail address within 30 April 2001 (please use the subject "OAC VIRMOS Fellowship 2001").
Further information may be requested via e-mail at the above address.
Attention: Personnel Services (Please quote reference SK077/9148/01)
The Astronomy group in the School of Physics and Astronomy at the University of St Andrews invites applications for two postdoctoral positions in theoretical astrophysics. We are particularly interested in candidates working in one or more of the following areas: formation of stars, planets, and stellar clusters, protoplanetary disks, computational hydrodynamics or radiative transfer. You must have a Ph.D. and a demonstrated ability to pursue independent research. The positions are funded for three years on the UK salary scale 1A for Research Staff (sterling 16,775-25,213 per annum), and include support for travel and computing. High performance computing resources available to the group include the UK Astrophysical Fluids Facility, a 128 processor Origin 3000.
Application packs and further particulars are available from Personnel Services at the above address. Please quote reference SK077/9148/01. Closing date 1April 2001. Completed application forms, an outline of research interests and capabilities relevant to the post, a curriculum vitae including a list of publications and three letters of reference, should reach us by 1 April 2001.
We regret that applications cannot be made by email. However, informal enquiries may be addressed to Ian Bonnell (iab1@st-andrews.ac.uk) or Phil Armitage (pja3@st-andrews.ac.uk).
Attention: Ms. Mona Drexler
Computer Sciences Corporation (CSC) invites applications and resumes for a position at Goddard Space Flight Center. Work will support the X-ray and Gamma-ray Spectroscopy Facility that involves flight instruments on planetary missions (e.g., Mars Odyessy 2001) and related applications.
The successful candidate should posses an advanced degree in astronomy, physics, or a related field.
Major activities of this position are systems administration/network security, scientific programming, and the opportunity to do research connected with ongoing spaceflight missions.
Desirable skills and experience include:
* experience with systems administration functions in a Sun/UNIX environment
* scientific software development in Fortran, C, and IDL
* analysis and publication of data from spacecraft missions
* running large-scale Monte Carlo particle and photon transport codes
* development of websites
The candidate must be able to work well in a team environment.
Applicants should send a resume to the above address. The position will be filled as soon as a qualified candidate is found. For more information about careers at CSC, please visit our Website at http://www.csc.com. AAE/EOE.
Attention: William Metcalf, Chairman
The Department of Physics and Astronomy invites applications for an anticipated tenure-track position in astrophysics starting in fall 2001. Although the opening is at the level of an assistant professor, candidates with outstanding records will be considered for a more senior level position. Applicants must have a Ph.D. or equivalent degree in astronomy, physics, or a related field. The successful candidate is expected to teach at both the undergraduate and graduate levels and establish a vigorous research program. LSU has an ongoing research program in theoretical, observational, and experimental astrophysics, with involvement in ground-based and space-borne multiwavelength observations, involvement in several major neutrino, cosmic ray, and high energy astrophysics experiments, and an active gravitational wave detector group on campus. LSU is also located less than 30 miles from the Laser Interferometer Gravitational Wave Observatory (LIGO) Livingston laboratory. Preference will be given to candidates with a strong track record of research that complements these existing strengths and focuses on the astrophysics of compact objects, although exceptional candidates in all areas of astrophysics will be considered. Salary will be commensurate with qualifications and experience. Applicants should send a vita, a description of research interests and experience, and the names of three references to William Metcalf, at the above address. Application deadline is 31 March 2001 or until a suitable candidate is selected. AAE/EOE.
Attention: Sharon Tiebert, Administrator
The Far Ultraviolet Spectroscopic Explorer (FUSE) group at Johns Hopkins University is seeking astronomers interested in analyzing and interpreting scientific data from the FUSE satellite. FUSE is a high resolution ultraviolet spectrograph launched in June 1999 to study the interstellar and intergalactic medium, active galactic nuclei, and stellar and solar system phenomena. The reach of the telescope and data quality are unprecedented in this spectral region. Successful applicants will have access to Principal Investigator Team Guaranteed Time data, which comprises approximately half of the mission data. Applicants should have a Ph.D. in astronomy or physics and have demonstrated scientific accomplishments. Previous experience in studies of interstellar and intergalactic medium and astronomical spectroscopy is highly desirable. Applicants will be considered at both the Associate Research Scientist and Postdoctoral levels. Job duties for Associate Research Scientists normally include both research and observatory support functions; Postdoctoral positions are normally for research only. Appointees will have access to the Apache Point Observatory and data from the Sloan Digital Sky Survey. Additional information on the FUSE project may be obtained at http://fuse.pha.jhu.edu. Applicants should send a resume and arrange for three letters of reference to be sent as soon as possible to Ms. Sharon Tiebert at the address above. Review of applications will begin 1 April 2001 and will continue until the positions are filled. Johns Hopkins University encourages applications from women and minority candidates. AAE/EOE.
Attention: Verne V. Smith, Dr.
A postdoctoral research associate position is open, to commence after March 2001, to work on a project to help establish grid stars for the Space Interferometry Mission (SIM). The position will be for an initial appointment of one year, plus a second year pending satisfactory performance, with the possibility of a third year contingent on funding. The position will involve the observation, reduction, and analysis of photometric and spectroscopic data needed to establish a sample of halo K-giants to be used as grid stars by SIM. This database will also be used to investigate the chemical enrichment history of the halo. In addition, the researcher will have time to establish independent research programs.
Desirable experience includes CCD spectroscopic and photometric observational data reduction techniques and general software experience with UNIX and/or LINUX, IRAF, or IDL. Applicants should send a curriculum vita, a discussion of relevant experience and interests, bibliography, and the names and e-mail addresses of three scientists who are familiar with the applicants work to Verne Smith, at the address listed above. Applications will be reviewed until the position is filled. AAE/EOE.
Attention: Gerd Weigelt, Prof.
The Infrared Interferometry Group of the Max Planck Institute for Radioastronomy in Bonn (see http://www.mpifr-bonn.mpg.de/div/ir-interferometry/) invites applications for postdoctoral positions in the following fields:
The successful applicants are expected to work primarily on the observation and interpretation of the objects mentioned above. Applicants should have a Ph.D. and observational or theoretical experience in one of the above fields. The appointment is initially for one year, and is renewable for up to five years. Interested scientists should email a letter of application with a summary of relevant experience and research interests, a curriculum vitae, a list of publications, and two letters of recommendation to Gerd Weigelt at the above address.
Review of applications will begin on 1 April 2001 and continue until the positions are filled. The Max Planck Society is an equal opportunity employer.
Attention: Dr. Suzanne Madden,
The CEA, Saclay Astrophysics Department is inviting applications for two post-doctoral research associates to begin in the fall of 2001. The Astrophysics Department (Service d'Astrophysique) in Saclay, located 15 km south-west of Paris near several other astronomy centers, is a major space astrophysics laboratory and is also involved in ground-based instrumentation. The department is engaged in research projects which include extragalactic astrophysics, cosmology, solar physics, star formation and high energy astrophysics. Research activities are primarily in support of our contributions to space projects such as ISO, SOHO, XMM, INTEGRAL, GLAST and FIRST. Applicants who are particularly interested in X-ray studies of supernova remnants or galaxy clusters; stellar population studies or star formation/ISM in galaxies; physics of high energy, compact objects (e.g. microquasars); or stellar physics are invited to apply.
While these positions are initially for a period of one year, there is the usual possibility of extension for the second year. There is no restriction on nationality. Interested applicants, please send a cv, bibliography, description of research interests and arrange to have three letters of recommendations sent to Suzanne Madden at the above address by 20 April 2001.
Attention: NRAO HR Department (Please reference #SO2304)
Summary:
The Array Support Group of the Computer Division in Socorro, NM has an
opening for a Senior Programmer/Analyst to design and oversee
implementation of the proposed the Expanded VLA (EVLA) computing
systems, the core of which will be the real-time Monitor & Control
System.
Qualifications:
Organization: Computing Division, Array Support Group
Array Operations Center, Socorro, New Mexico
Benefits:
24 Vacation Days; 12 Holidays; Retirement Plan 401(a); Supplemental
Retirement Account 403(b); Health, Dental, Life, Long Term Disability,
and AD&D Insurance; Flexible Spending Accounts; Sick Leave; Tuition
Reimbursement.
To Apply:
Send resume to the NRAO HR Department, P.O. Box O, Socorro, NM 87801;
fax, (505) 835-7024; E-Mail, tmcbride@nrao.edu. Reference Req.
#SO2304. EEO/M/F/D/V.
The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
Attention: Erik Katsavounidis, Professor
The Laser Interferometer Gravitational-Wave Observatory (LIGO) project is an effort led by Caltech and MIT scientists to establish a gravitational-wave observatory, consisting of two facilities with laser interferometric detectors located at Hanford, WA and Livingston, LA. The project is sponsored by the National Science Foundation.
As construction of the project is nearing completion and first physics data taking is expected to begin in year 2001, the MIT group in LIGO is seeking to fill two post-doctoral positions whose primary role will be in the analysis of LIGO data. LIGO's data analysis system uses modern object oriented computing methods and languages that includes parallel computational methods.
The MIT group has strong interest in pursuing searches for astrophysical sources of gravitational waves that includes bursts from supernovae, stochastic background as well as for signals from unmodeled sources while keeping involvement in analyses of data for diagnostic and detector characterization purposes. The instrument is expected to run for extended periods without interruptions as soon as it reaches its design sensitivity of gravitational wave strain 10^-21 near 100Hz. It is expected then to be part of a network of gravitational wave and neutrino detectors detectors; data analysis will involve techniques to combine data from a network of detectors.
Expertise related to astrophysical gravitational wave source modeling, data analysis environments within complex experiments, object-oriented and parallel computing, as well as novel signal processing techniques will be useful. Candidates must possess a Ph.D. in physics or astrophysics and have demonstrated ability related to the above research activities.
Please submit application material to: Dr. E. Katsavounidis, at the above address. MIT is a non-smoking enviroment. AAE/EOE.
Attention: The Personnel Officer
A PhD or equivalent in physics, astrophysics, applied mathematics, or related area is essential, as is proven research capacity and expertise in scientific computation and analytic and numerical modelling. Evidence of fruitful collaboration with observers and an understanding of interstellar scintillation and radio astronomical techniques are desirable.
Full time, fixed term for one year, subject to completion of a probation period. Possibility of further offers of employment up to one year, subject to funding and need.
Applicants should quote reference no. A06/001260 and include a short description of their research experience and background in their application, their best two papers, and significant evidence of analytic and computing skills.
Remuneration Package: AU$42,567 - AU$57,767 pa (including base salary, leave loading and superannuation).
Attention: Director's Office,
The fellow will take part in the activity (observational, interpretative, and theoretical) of the Arcetri Observatory in one or more of the following fields: search and statistical analysis of supermassive black holes in the nuclei of nearby galaxies (both quiescent and active); investigation of the properties of obscured AGNs (local and at high redshift) by means of infrared, optical and X-ray data; cosmological evolution of AGN/supermassive black holes. Applicants should have a strong previous experience in the relevant areas and are expected to work in close collaboration with the Arcetri staff.
The gross yearly salary will be in the range of 40-50 Million Lire. The fellowship will be granted for two years (subject to an evaluation of performance after the first year). The fellowship will not entail social benefits or medical insurance, but the fellow will be requested to cover himself/herself with basic medical insurance. No special application forms are required. The applicants should send a CV (including date of birth, PhD, nationality, e-mail address), list of publications, a summary of past activity (1 page) and a one-page statement of research interests, in connection with the areas of activity listed above. They should also arrange that at least two letters of reference are sent independently. Applications and letters of reference should arrive in Arcetri no later than 30 April 2001. The starting date should be 1 September 2001, but different dates can be considered.
Attention: Michael Rowan-Robinson, Prof
(1) In extragalactic infrared astronomy and cosmology, to participate in the Group's programme of far infrared and submillimetre surveys, their multi-wavelength follow-up, and studies of galaxy formation and the star formation history of the universe, with a strong role in the SWIRE Legacy Survey Programme on SIRTF.
(2) In the Group's PLANCK team, to work on the design of the time-line data processing for the PLANCK HFI instrument. The Group has a strong scientific interest in the PLANCK all-sky point-source survey at 350-1300 microns.
(3) In the Group's HERSCHEL team, to work on the design of the data processing for the HERSCHEL SPIRE instrument. The Group has a strong scientific interest in cosmological surveys with HERSCHEL.
For all four posts a PhD and a strong research background in extragalactic astrophysics is essential. Experience in far infrared or submillimetre work would be an advantage. At least one post will be at the top end of the salary range and would involve some management responsibility for the PLANCK and/or FIRST work. One of the four posts would have a 50% role in computer system and network support within the Group, and for this post computing experience would be essential.
Applications, including a cv, list of publications and the names of two referees (who should be asked to send their references to the same address), should be sent to Prof M.Rowan-Robinson, Astrophysics Group, Imperial College, Prince Consort Rd, London SW7 2BZ (mrr@ic.ac.uk) by 31 March 2001.
Imperial College is striving towards Equal Opportunities
Attention: Joseph S. Miller, Director (Please refer to provision # T00-30 in your reply)
RANK: Postgraduate Researcher Step IV to Step VIII
SALARY: $35,124 - $41,736
MINIMUM QUALIFICATIONS: PhD or equivalent in Astronomy or Physics or a closely related field, relevant refereed publications, and experience with galaxy data reductions and analysis and/or adaptive optics. Must be able to work independently yet collegially in a team environment.
TERM OF APPOINTMENT: Two years, with possible extension to three, contingent on availability of funding.
POSITION START DATE: 1 September 2001 (negotiable).
URL FOR MORE INFO: DEEP – http://deep.ucolick.org
CfAO – http://www.ucolick.org/~cfao
APPLICATION MATERIALS: Send vita, two-page summary of relevant experience and plans, and three or more letters of recommendation (all letters will be treated as confidential documents) to Postgraduate Researcher Recruitment c/o UCO/Lick, Office of the Director at the above address. Please refer to provision # T00-30 in your reply.
CLOSING DATE: All materials must be received no later than March 31, 2001.
UCSC IS AN AFFIRMATIVE ACTION/EQUAL EMPLOYMENT OPPORTUNITY EMPLOYER WOMEN AND MINORITIES ARE ENCOURAGED TO APPLY
Inquiries regarding the University's equal employment opportunity policies may be directed to: Equal Employment Opportunity/Affirmative Action Office at, University of California, Santa Cruz, CA 95064; (831) 459-2686. Under Federal law, the University of California may employ only individuals who are legally able to work in the United States as established by providing documents as specified in the Immigration Reform and Control Act of 1986.
If you need assistance due to a disability please contact the Academic Human Resources Office at 350 McHenry Library (831) 459-4300. This position description is available in alternate formats, which may be requested from Academic Human Resources at (831) 459-4300.
UCSC's annual security report includes statistics for the previous three years concerning reported crimes that occurred on campus; in certain off-campus buildings owned or controlled by UCSC; and on public property within, or immediately adjacent to and accessible from the campus. The report also includes institutional policies concerning campus security, such as policies concerning alcohol and drug use, crime prevention, the reporting of crimes, sexual assault, and other matters. You can obtain a copy of this report by contacting the UCSC Police Department at (831) 459-2231 or by accessing the following web site: http://www2.ucsc.edu/police/reports.html
VISIT OUR WEB SITE AT http://www2.ucsc.edu/ahr/academic.htm
Attention: Dr. George Nickas, Chair, Physics Search
Attention: Edie Alton L-413
The successful candidate will conduct a vigorous and innovative program of research in planetary science aligned with current and planned projects in solar system observation, theory and data analysis ongoing at IGPP. This includes infrared imaging of solar system bodies using the state-of-the-art adaptive optics systems at the Lick and Keck Observatories, modeling and theory of planetary atmospheres and surfaces, and analysis of infrared spectra of solar system bodies. Projects are also ongoing at IGPP to investigate extrasolar planetary systems and brown dwarfs, and to survey outer solar system bodies.
Postdoctoral Researchers at IGPP have access to LLNL's unique resources, University of California Lick Observatory and, in collaboration with IGPP staff members or UC faculty, Keck Observatory. IGPP has a modern unix network and access to LLNL's supercomputer facilities. IGPP hosts collaborators from the UC, other academic institutions, and an extensive postdoctoral and visitor program.
This position requires either a recent Ph.D. in Planetary Science, or a recent Ph.D. in Astronomy or Astrophysics with research experience in planetary science. It also requires effective communication skills, and evidence of scientific publication in refereed journals. Experience in spectroscopy is highly desirable.
LLNL offers a challenging work environment and a competitive salary/benefits package. To be considered, referemce Dept. AJAH311PH, send a cover letter, curriculum vitae, and contact information for three references to Edie Alton L-413, at the above address or visit our website at http://www-igpp.llnl.gov/. Review of applications will begin 15 March 2001. We are an equal opportunity employer with a commitment to workforce diversity.
For more information about this position and the Laboratory, visit us on the web at www.llnl.gov/jobs.
Attention: William Taylor, Chair
Attention: Mary Ellen Barba
Attention: Human Resources
The position is for one year, renewable for up to a total of three years, depending on performance and continued funding. Funding is available for two years and the candidate will be expected to help secure funds for a third year.
Candidates should possess a PhD in astrophysics or a related field by the date of appointment and experience in observational astronomy, particularly infrared spectroscopy. There are no restrictions on citizenship.
STScI, located on Johns Hopkins University Campus in Baltimore, Maryland, offers an excellent benefit package, competitive salaries, and a stimulating work environment. The minimum salary is $41,900; however, STScI’s pay is commensurate to the year of Ph.D.
Applicants should send a cover letter with position applying for, curriculum vitae, bibliography, and one-page statement of research to the address below. They should also arrange for three letters of recommendation to be sent directly to the same address. Completed applications received by 31 March 2001 are assured full consideration. Women and members of minority groups are strongly encouraged to apply. EOE/AA/M/F/D/V.
Attention: A. Lewis, Personnel Office
The AIPS++ Project has a job vacancy at the National Radio Astronomy Observatory headquarters in Socorro, New Mexico. The duties will be to participate in the development of advanced visualization capabilities in AIPS++ building on top of the existing Display Library and other AIPS++ infrastructure. Development will focus on the display of information in two complementary domains, connected by a transform (such as Fourier transform or self-calibration) that is itself implemented in the AIPS++ Library. The position is funded by a grant from the NSF and is funded for two years.
Substantial experience in astronomical data reduction is required. Experience with radio-interferometry, and visualization is desirable. Knowledge of C++, Unix and experience of working in a large distributed software project would both be advantageous. Pursuit of research in either astronomy or astronomical techniques is expected (25% time).
Socorro is a small historic town (pop. 9000) in the mid Rio Grande valley of New Mexico. More information can be obtained from the Socorro Home Page at http://www.socorro.com.
Applicants should provide: letter of application, a current curriculum vitae, and the names of three references whom we may contact as necessary. Application materials should be addressed to A. Lewis, Personnel Office, NRAO, P.O. Box 0, Socorro, NM 87801-0837 or alewis@nrao.edu.
Further information is available for both the AIPS++ Project and the NRAO from the NRAO Home Page http://www.nrao.edu.
Attention: Physics and Astronomy Search Committee (#R2312), c/o Bates College Secretarial Services
The Department of Physics and Astronomy at Bates College seeks to fill a leave replacement position for two and one-half years, beginning January 1, 2002. Applicants must demonstrate potential for teaching excellence in a vigorous undergraduate program and welcome the opportunity for close interaction with serious students. Applications are encouraged from candidates that can teach non-calculus astronomy courses with weekly labs, as well as upper level courses in physics or astrophysics. Teaching may include working with seniors on research projects. Bates College is a highly selective liberal arts college of approximately 1,600 students, located in Maine, two and one-half-hours north of Boston. Review of applications begins 1 March 2001, and will continue until the position is filled. To apply, please submit a letter of application, curriculum vitae, graduate transcripts, and the names of three references.
Bates College values a diverse college community and seeks to assure equal opportunity through a continuing and effective Affirmative Action program. AAE/EOE.
Attention: Sandra Abbey, Human Resources Manager
Attention: Dr. R. Michael Rich, Research Astronomer
The successful candidate has access to the 3.0m telescope at Lick Observatory, and collaborative opportunities with Rich and other UC faculty at the 10-m Keck telescopes in Hawaii. Proven ability to do point-spread fitting photometry with ALLFRAME or an equivalent software package is essential; experience with NICMOS data would be useful. the PI has a proven record of placing postdoctoral researchers and Ph.D. students in long term positions. Funding is assured for one year, and further renewal is subject to funding and performance. Applications from minority and woemn candidates are strongly encouraged. We will begin considering applications on 15 April 2001 and will continue until the position is filled. Applications should include a CV, description of relevant experience, and the names of three references. AAE/EOE.
Attention: Geoffrey W. Marcy, Professor
The successful candidate will (1) Conduct a search for extrasolar planets using the 3m and coude auxiliary telescopes at Lick Observatory, (2) write software and test hardware needed for the planet search project, (3) optimize PSF description and implement innovations to improve velocity precision, (4) run spectral analysis to derive stellar metallicities, (5) analyze chromospheric activity and correlate characteristics with the presence of extrasolar planets, (6) write software to derive Keplerian fits in multiple-planet systems, (7) write research proposals and papers, (8) assist students (graduate and undergraduate) and postdocs in Marcy's research group, and (9) serve as project manager for our SIM key science project. IDL is the necessary language for software, especially in (2) and (6) above.
Minimum qualifications include (1) Ph.D. in astronomy or physics; (2) at least three years of postdoctoral experience; (3) demonstrated ability to work with astronomical observations and data reduction on Sun Unix workstations and various PCs; and (4) knowledge of current problems related to extrasolar planets and a demonstrated competence in their solution.
Please send a resume, list of publications, and copies of two recent publications (preprints or reprints) by 30 April 2001 to Prof. Geoffrey Marcy, at the above address. Include the names and addresses of two persons who could be contacted for reference letters. AAE/EOE.
Attention: Leo Blitz, Director
The position will be available starting April 2001. Applicants should send a resume, detailing relevant experience to Leo Blitz, director. Applications will be accepted until the position is filled, and we will make an initial review of all application recieved by 31 March 2001. The salary will be commensurate with experience. Women and minorities are particularly encouraged to apply. AAE/EOE.
Attention: Director's Office
Further information can be found at www.nrao.edu on these positions and others.
Applications should be sent to the Director's Office, NRAO, 520 Edgemont Road, Charlottesville VA 22901-2475 and should include: a letter with a presentation of qualifications for the position, a description of research interests and plans, the names of five scientists who may serve as references, and a curriculum vitae. All application materials received at the above address by 15 April 2001 will receive full consideration.
The National Radio Astronomy observatory is operated by Associated Universities, Inc. (AUI) under cooperative agreement with the National Science Foundation. The NRAO is an equal opportunity employer (M/F/H/V).
Attention: Director's Office
The appointment is expected for an initial period of three years, with the possibility of an eventual permanent appointment, including AUI tenure. In exceptional cases, a more senior initial appointment may be considered. The appointment will be made at NRAO's Green Bank WV site with responsibility for development of the Green Bank Telescope's capabilities at millimeter wavelengths. Applicants should have a record of experience and accomplishment in millimeter instrumentation.
Applications should be sent to theDirector's Office, at the above address and should include: a letter with a description of research interests and plans, a presentation of qualifications for the position, a curriculum vitae, and the names of five scientists who have been asked to send letters of reference directly to the NRAO. All application materials and supporting letters received at the above address by 15 April 2001 will receive full consideration.
NRAO is operated by Associated Universities, Inc. (AUI) under cooperative agreement with the National Science Foundation. The NRAO is an equal opportunity employer (M/F/H/V). AAE/EOE.
Attention: Human Resources Department
Qualifications:
Benefits: 12-24 Vacation Days; 12 Holidays; Retirement Plan 401(a); Supplemental Retirement Account 403(b); Health, Dental, Life, Long Term Disability, and AD&D Insurance; Flexible Spending Accounts; Sick Leave; Tuition Reimbursement
To Apply: Send resume to the National Radio Astronomy Observatory HR Department, at the above address. AAE/EOE.
Attention: Employment,
Cutting-edge technology projects include a laser beacon, adaptive optics systems, and an interferometer that joins the two Keck telescopes to work as a single unit.
Opportunities exist for
*Electronics Engineer
*Electronics Technician
*Mechanical Engineer
*Mechanical Technician
*Optics Engineer
*Optics Technician
*Laser Optics Engineer
*Laser Technician
*Software Engineer
*Instrument Scientist
*Interferometry Optics Engineer
For more information, visit our Web site at www2.keck.hawaii.edu:3636
Fax (808-885-4464) or mail resumes, references,
and salary history to the above address. EOE/M/F/D/V