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Postdoctoral Research Associate (Physics/Astronomy) | Closing date: 2024-12-31 Contact: Human Resources |
The Department of Physics at Baylor University invites applications for a postdoctoral position in the area of observational cosmology and time-domain astrophysics. Applicants will work with Prof. Benjamin Rose to build the necessary tools and methods to take advantage of current and next generation experiments designed to probe cosmology. We are committed to building a group that is inclusive and representative of our community. For this reason, we strongly encourage applicants who come from groups that are historically underrepresented in the fields of physics and astronomy. | ▸ more | What You Will Do:
A successful candidate will work with Prof. Rose on the Roman Space Telescope and the Rubin Observatory Legacy Survey of Space and Time (LSST). Potential research topics include next generation pipeline development, photometric calibration of infrared telescopes, new techniques in statistical and image analysis, cosmology with Type Ia supernovae, developing follow-up strategies of variable and transient sources, innovative methods in image analysis for large surveys, and studies of astrophysical contributions to cosmological signals. Participation in some of the Roman Space Telescope, and the Rubin Observatory LSST DESC collaborations while at Baylor is expected.
More information on Prof Rose's research can be found at https://physics.artsandsciences.baylor.edu/person/dr-benjamin-rose.
These positions have an initial appointment for two years, renewable upon mutual agreement and availability of funding. The position can begin immediately, but is expected to begin by the start of the Fall 2024 semester. Candidates must have a Ph.D. by the date of appointment in astronomy, physics, or a relevant field. Applicants should prepare a cover letter, a current CV with a list of publications, a research statement of less than three pages describing past accomplishments and research goals, and arrange for three letters of recommendation to be sent. Applicants are encouraged to describe in their cover letter how their scholarship and experience would contribute to an inclusive community.
Required:
? PhD in Physics, Astronomy, or a closely related field
? Provide assistance with the preparation of project-related reports, manuscripts and presentations
? Conduct research design and oversee experiments
? Develop and establish experimental procedures
? Prepare and manage extensive databases
? Develop and implement research quality control procedures
? Analyze data and prepare reports; develop recommendations based on results
? Verify the accuracy and validity of data
? Work with highly technical and complex research instruments
? Perform all other duties as assigned to support Baylor's mission
? Ability to comply with University policies
? Maintain regular and punctual attendance
What You Can Expect:
Compensation & Benefits
As part of the Baylor family, eligible employees receive a comprehensive benefits package that includes medical, dental, and vision insurance, generous time off, and tuition remission. Baylor has a comprehensive benefits plan that supports you and your family's wellbeing and allows you to be a part of the life of a vibrant and active college campus. To learn more, go to https://www.baylor.edu/hr/index.php?id=949184.
Explore & Engage
Learn more about Baylor and our strategic vision, https://illuminate.web.baylor.edu/. Also, explore our great hometown of https://wacoheartoftexas.com/ and the many opportunities to https://waco.web.baylor.edu/waco-guides/waco-culture-guide.
About Us:
Baylor University is a private not-for-profit university affiliated with the Baptist General Convention of Texas. As an Affirmative Action/Equal Opportunity employer, Baylor is committed to compliance with all applicable anti-discrimination laws, including those regarding age, race, color, sex, national origin, military service, genetic information, and disability. Baylor?s commitment to equal opportunity and respect of others does not undermine the validity and effect of the constitutional and statutory protections for its religious liberty, including, without limitation, the religious organization exemption under Title VII of the Civil Rights Act of 1964, the religious exemption to Title IX of the Education Amendments of 1972, and the Free Exercise Clause of the First Amendment to the United States Constitution, among others. Baylor encourages women, minorities, veterans, and individuals with disabilities to apply. EEO/M/F/Vets/Disabled
To apply, visit https://apptrkr.com/5136613
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Postdoc position in Astronomy at NCBJ, Poland | Closing date: 2024-05-03 Contact: Katarzyna Ma?ek |
The National Centre for Nuclear Research (NCBJ) in Poland invites applications for a postdoctoral position in the Astronomy Division. The Astrophysics Division is dedicated to research in astrophysics and astronomy, focusing on observational works. The division covers a broad range of topics, including cosmology, gravitational waves, physics of galaxies, and the interstellar medium.
| ▸ more | The National Centre for Nuclear Research (NCBJ) in Poland invites applications for a postdoctoral position in the Astronomy Division. The Astrophysics Division is dedicated to research in astrophysics and astronomy, focusing on observational work. The division covers a wide range of topics, including cosmology, gravitational waves, the physics of galaxies, and the interstellar medium.
The successful applicant will work on a research project that complements the work already conducted in the NCBJ Astrophysics Division.
The position is initially for a period of two years, with the possibility of an extension for a further year.
Applications are welcome by emailing the application directly to dr hab. Katarzyna Ma?ek (Katarzyna.Malek @ ncbj.gov.pl) before 2024-05-03.
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POSTDOC POSITION (F/M/X) Exoplanet atmospheres - links to observations | Closing date: 2024-05-15 Contact: Cosima Muck |
The Space Research Institute (IWF) of the Austrian Academy of Sciences (OeAW), Austria's leading non-university research and science institution, is offering a POSTDOC POSITION (F/M/X) in Exoplanet atmospheres - links to observations (full-time, 40h per week).
The successful candidate will be part of Prof Christiane Helling's research group Exoplanets: Weather & Climate (Complex Atmosphere Modelling) at the IWF which is part of the OeAWs effort to expand the theme of exoplanet research at the Space Research Institute (IWF) Graz. | ▸ more | Your profile:
- PhD in the relevant fields of astrophysics
- Experiences in interpreting ground based and space instrumentation data
- Experiences in 3D retrieval, polarimetry and/or gas-cloud radiative transfer modelling
- Experiences in scientific programming and publishing
Your tasks:
- Link complex modelling results (e.g., 3D atmospheres, cloud modelling) to observations.
- Scientific data interpretation (e.g., CHEOPS, JWST) and preparation for PLATO, Ariel, JWST and other future missions based on 3D GCM results.
- Publication and support in proposal writing activities.
The appointment may begin as early as June 01st, 2024 and will be for 2+1 years.
Applications must include a cover letter in addition to (1) curriculum vitae, (2) list of publications, (3) statement of the applicant's research experience (max 2 page) and a research plan (max 1 pages),
(4) certificates for full academic record, and (5) two letters of references. Please send the application in one PDF file, mentioning Job ID: IWF153PD123 to cosima.muck @ oeaw.ac.at no later than May 15th, 2024.
Inquiries about the position should be directed to Prof Dr Christiane Helling.
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POSTDOC POSITION in Exoplanet Atmosphere Cloud Modelling | Closing date: 2024-05-15 Contact: Cosima Muck |
The Space Research Institute (IWF) of the Austrian Academy of Sciences (OeAW), Austria's leading non-university research and science institution, is offering a POSTDOC POSITION (F/M/X) in Exoplanet Atmosphere Cloud Modelling (full-time, 40h per week).
The successful candidate will be part of Prof Christiane Helling's research group Exoplanets: Weather & Climate (Complex Atmosphere Modelling) at the IWF which is part of the OeAWs effort to expand the theme of exoplanet research at the Space Research Institute (IWF) Graz | ▸ more | Your profile:
- The applicant must hold a PhD in physics, astrophysics or geoscience or related areas.
- The successful candidate will benefit from a background in exoplanet and/or solar system cloud formation or chemistry modelling in diverse chemical environment.
- Experiences in programming are required.
- Past experiences in working with students will be beneficial.
Your tasks:
- The post holder will play a crucial role in working on our kinetic cloud formation model as part of our efforts in providing physical interpretations of observational data for space missions, for example, CHEOPS, JWST, PLATO, ARIEL, NEWATHENA, HWO. The post holder will be part of related space mission work packages
The appointment may begin as early as June 01st, 2024 and will be for 2+2 years.
Applications must include a cover letter in addition to (1) curriculum vitae, (2) list of publications, (3) statement of the applicant's research experience (max 2 page) and a research plan (max 1 pages),
(4) certificates for full academic record, and (5) two letters of references. Please send the application in one PDF file, mentioning Job ID: IWF143PD123 to cosima.muck @ oeaw.ac.at no later than May 15th, 2024.
Inquiries about the position should be directed to Prof Dr Christiane Helling.
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Postdoctoral position at the Gaia group at the ICCUB | Closing date: 2024-04-21 Contact: Lola Balaguer |
The Gaia group at the ICCUB offers a postdoctoral position at the Institute of Cosmos Sciences (ICCUB) of the University of Barcelona in the project SPACIOUS, funded by Horizon Europe. The postdoc will be part of the Gaia-UB group (https://gaia.ub.edu/) with about 25 scientists and engineers of the Gaia mission. | ▸ more | The SPACIOUS project aims to boost the scientific exploitation of ESA mission data by developing a computational framework for astrophysical research that requires Big Data and Data Mining technologies to be addressed, with special focus on the Gaia and Euclid missions.
The position offered will be devoted, on the one hand, to the definition of scientific requirements for the framework, selection and preparation of the datasets to be used and scientific guidance for the technical development. On the other hand, it will supervise and manage the execution of several ?scientific challenges? included in the project; these challenges are key scientific projects requiring the use of large datasets that will be executed in the developed framework, becoming both test cases and a demonstration of performance. The position will also act as contact point and supervisor of the users of the system.
We will value previous work in the Gaia and/or Euclid missions; on the technical side, we require experience in programming and in astrophysical applications of data mining and big data techniques. We will also value experience in the use of Commercial Cloud resources and the management of software development projects.
Employment conditions:
The position is offered for 2.5 years. The contract is expected to begin around July 2024. Gross annual salary is about 30.000?, depending on the experience. This includes social security and public healthcare benefits, covering spouse and children.
Applicants should provide:
curriculum vitae
list of publications
letter of motivation including research experience and interests (2 pages max).
Applications should be done using this link before March 21st, 2024: https://forms.office.com/Pages/ResponsePage.aspx?id=qzwxosOxOk-7ESFXRH3btIoIot4FN6lHiSCx0AqqSpVUNDYwVlRXTExCSUc3UjJIVVc2SEFXWk5FOS4u.
Inquiries about the application submission can be directed to Lola Balaguer (lbalaguer @ fqa.ub.edu).
For inquiries about the scientific aspects, please contact Xavier Luri (xluri @ fqa.ub.edu).
About the Institute of Cosmos Sciences:
Relevant to the offered position, researchers of the institute have broad interests, including galactic dynamics, open and globular clusters, stellar physics, star formation, models of galaxy formation and evolution, the Large Magellanic Clouds, computational astrophysics, data
analysis, cloud computing.
The Institute of Cosmos Sciences is a research institute of the University of Barcelona. It is an interdisciplinary center dedicated to fundamental research in the fields of cosmology, astrophysics, and particle physics. In addition, the institute has a strong technology program through its participation in international collaborations in observational astronomy and experimental particle physics.
As part of the University of Barcelona, the ICCUB is a recipient of the European Commission?s HR Excellence in Research (HRS4R) Award, which recognises, among other achievements, respect for equal opportunities and the capacity to attract talent in a positive working environment that promotes the pursuit of successful research careers. The ICCUB respects the principles of open, transparent, merit-based selection. We strongly encourage women and underrepresented minorities to apply. For additional information please see the Diversity, equity and inclusion Commission.
The ICCUB is located in Barcelona, considered the 8th World's Best Cities 2022: one with near- perfect weather year-round, miles and miles of beaches, iconic parks, striking architecture and colorful neighborhoods that march to their own beat?artistic, sophisticated, bohemian. Moreover, it is a pole of attraction for the technology sector, a top choice to establish a company in this sector, and it hosts some of the world's major technological events, such as the Mobile World Congress and the Smart City Expo. In addition, Barcelona and its metropolitan area is a leading destination on the map of global technological ecosystems and
has infrastructures such as science parks, universities and the 22@ district.
SPACIOUS is a Horizon Europe HORIZON-CL4-2023-SPACE-01-71 project funded under grant agreement no. 101135205
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postdoc position for ERC grant in Warsaw | Closing date: 2024-04-30 Contact: Bozena Czerny |
Center for Theoretical Physics PAS invites applications for post-doctoral position in the project ERC-Synergy 'Sub-percent calibration of the extragalactic distance scale in the era of big surveys' (grant agreement No. [951549]). PI of the part of the project led by CFT is Prof. Bo?ena Czerny. Candidates with previous experience in astrophysics, and in particular in optical observations, preferentially of active galactic nuclei and in programming, are particularly welcome. Among the tasks will be modelling the expected continuum time delays in AGN, also from LSST. | ▸ more | Candidates should submit before April 30, 2024, the following documents to rekrutacja @ cft.edu.pl annotated with BC/02/2024 until 30 April 2024.
(1) The scientific CV, including the major scientific achievements, list of publications, participation in research projects and conferences, and the document must contain a statement: ?I consent to the processing of my data contained in the application documents?
(2) Personal questionnaire form (should be downloaded from the CTP web site)
(3) Three recommendation letters should be sent directly to rekrutacja @ cft.edu.pl (annotated BC/02/2024)
(4) Certified copy of the PhD diploma or the letter from the supervisor about the prospects for completion of the Thesis before the beginning of the employment.
(5) The signed RODO clause.
At the time of application, the candidates should either have a PhD degree, or will obtain a PhD degree before signing the job contract.
Related URLs: web site of the institute https://www.cft.edu.pl/
personal web site of Bozena Czerny: https://www.cft.edu.pl/pracownik/bczerny
job description in euraxess: https://euraxess.ec.europa.eu/jobs/205144
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The stellar-substellar limit in the large scale survey Euclid | Closing date: 2024-04-15 Contact: Celine Reyle |
The successful applicant will work on the identification of ultra cool dwarfs in Euclid fields, and may propose new identification techniques and explore the possibility of using the precise PSF of Euclid to identify close binaries. Other challenges can be addressed, such as to determine the luminosity function, infer the most likely low-mass end of the initial mass function and explore its degree of universality in different components of the Milky Way.
The candidate will be working with the international Euclid UCD group within the consortium, as well as the Gaia UCD team. | ▸ more | Euclid is a space mission led by the European Space Agency (ESA) to conduct a deep, single-epoch survey of 15,000 deg2 of sky with visible and near-infrared photometry and spectroscopy, and 40 deg2 multi-epoch very deep surveys. Its primary science goal is to investigate the geometry of the dark universe by mapping the distribution and shapes of galaxies. The unprecedented combination of sensitivity, areal coverage, spatial resolution, data homogeneity and spectral information will naturally be of tremendous benefit to other areas of astrophysics.
Ultra cool dwarfs (UCDs) are the lowest-mass, coldest, and faintest products of star formation. They are defined as objects with M7 and later spectral type objects. UCDs are of particular interest since they include both very low-mass stars that slowly fuse hydrogen, and brown dwarfs, which have insufficient mass to sustain hydrogen fusion in their cores, and cool down with time.
The Euclid wide survey will probe a very large volume and allow the detection of an unprecedented huge number of UCDs (> 1 000 000). The NIR colours are suitable to classify them, the only point-source contaminants being high redshift quasars. However, UCDs can be discriminated from QSOs thanks to the visible survey: UCDs VIS-NIR colours will be much redder or they will not be detected in the visible. Most of those with spectral type M7 to L5 have been discovered thanks to Gaia, completed by ground based or space telescopes in the NIR for the latter type brown dwarfs. With its deep and large cover in the NIR, Euclid is expected to complete the census and push the volume for L and T dwarfs.
Thanks to the depth of the NIR Euclid survey, we expect to use the UCDs as a probe of the oldest Milky Way populations and so learn more about the sub-stellar formation history at early times. In addition Euclid will offer a large sample of UCDs spanning a large metallicity range and open up a new window on the chemical evolution of the Milky Way.
Skills/Qualifications
Skill and experience required: The candidates will have a track record of research in a relevant area of expertise in astrophysics. The candidates will also have a record of submitting/publishing scientific research in leading astronomical journals, presenting their work at scientific conferences, workshops or seminars.
The candidates will ideally have some experience of working large scale surveys, and stellar populations, in particular low mass stars and brown dwarfs.
Specific Requirements
Applications should be sent to Céline Reylé and should be accompanied by PDF versions of a CV, a list of publications, and a personal statement/cover letter (maximum one side of A4 paper) explaining the motivation for applying, summarizing the research interests and the project. It should also include the contact details of two referees.
The position is funded by the Université of Franche-Comté, for 12 months, renewable.
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Postdoctoral Position at the Astronomical Institute of the Czech Academy of Sciences | Closing date: 2024-04-12 Contact: Lenka Cihakova |
The Astronomical Institute of the Czech Academy of Sciences (ASU) advertises a call for post-doc positions with the expected start in mid-2024. | ▸ more | ASU is a public research institution and the largest professional astronomical organization in the Czech Republic, located at Ondrejov observatory and in Prague. Successful applicants will collaborate with researchers in our scientific departments (theory, observation, and data analysis are all welcome). The Institute is involved in space programs of ESA and ground-based projects within ESO as well as its own observational projects. Experience in one of the subjects studied at ASU is valued but interesting independent new projects will be also considered.
The appointment is initially for one year; an extension for another year is expected upon satisfactory scientific performance. A necessary condition is to satisfy legal requirements for employment in the Czech Republic (EU member state). Salary will be based on the domestic level (cca 1450 EUR/month before taxes) and it includes health insurance. There is a possibility of institute accommodation in Ondrejov; in Prague private accommodation has to be arranged. The starting date of employment is expected to be 1st July 2024 and is slightly negotiable.
In a cover letter please indicate the working group that you intend to join and provide the exact date of PhD defense. Applicants should contact an Institute researcher with whom they wish to work for further information, to define a joint research programme and to discuss the starting date. This is considered to be an important part of the proposal.
Applications shall contain: Cover Letter, Curriculum Vitae, List of Publications, Summary of Research Plans). Submit the application by email to: info @ asu.cas.cz , with subject "POSTDOC 2024", attach a single PDF that will include all required parts.
Applications can be submitted before finishing PhD, in which case a statement from the supervisor stating the planned date of the defense should be included. Successful candidates must hold PhD degree in the field and present a certificate of that by 26th of April 2024. Preferences will be given to early-stage researchers.
Please arrange for the minimum of two recommendation letters to be sent directly to the same electronic address as above. The letters may be issued up to 6 months before the application deadline.
To receive full consideration, the application deadline is 12th of April 2024 till the end of the day (Prague/Europe timezone). The receipt of applications will be acknowledged by email. Once the evaluation process is completed, successful applicants will be notified (short list will be preselected within 2 weeks from the application deadline).
Further information:
o https://asu.cas.cz/en for the list of working groups at the Institute
o https://www.euraxess.cz/ for details about the research employment and work conditions in Czech Republic
o http://www.numbeo.com/cost-of-living/comparison.jsp to compare cost of living
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ESA Archival Research Visitor Programme | Closing date: 2024-04-30 Contact: Guido De Marchi |
To increase the scientific return from its space science missions, the European Space Agency (ESA) welcomes applications from scientists interested in pursuing research projects based on data publicly available in the ESA Space Science Archives (https://www.cosmos.esa.int/web/esdc). | ▸ more | The ESA Archival Research Visitor Programme is open to scientists, at all career levels, affiliated with institutes in ESA Member States and Collaborating States. Early-career scientists (within 10 years of the PhD) and PhD students are particularly encouraged to apply. We encourage applications from women and minorities. The evaluation process is anonymised to ensure equal opportunities for all applicants.
During their stay, visiting scientists will have access to archives and mission specialists for help with the retrieval, calibration, and analysis of archival data. In principle, all areas of space research covered by ESA science missions can be supported.
Residence lasts typically between one and three months, also distributed over multiple visits. Research projects can be carried out at ESAC (Madrid, Spain) and at ESTEC (Noordwijk, Netherlands). To offset the expenses incurred by visitors, ESA covers travel costs from and to the home institution and provides support for lodging expenses and meals.
Applications received before 1 May 2024 will be considered for visits in autumn and winter 2024/2025.
For further details, including areas of research and contact information, please refer to:
https://www.cosmos.esa.int/web/esdc/visitor-programme
or write to the programme coordinators at arvp @ cosmos.esa.int
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Postdoctoral position in time domain astronomy | Closing date: 2024-04-07 Contact: Dr. Liliana Rivera Sandoval |
The Department of Physics and Astronomy at the University of Texas Rio Grande Valley (UTRGV) invites applications for a postdoctoral researcher in time domain astronomy. The successful applicant will work with Assistant Professor Liliana Rivera Sandoval on multiwavelength studies of compact binaries, as well as other types of transients detected through a TESS survey. The candidate will work mainly with TESS data complemented with data from other observatories. Previous experience with any of these instruments/data is not mandatory. | ▸ more | Candidates must possess a Ph.D. in Astronomy/Astrophysics or a closely related field by the starting date. Preferred qualifications include experience in one or more of the following areas: compact objects, binaries, transient astronomy, data analysis in any wavelength, pipeline development, computational astronomy, and experience with astronomical surveys.
Applications will start to be reviewed on 8 April 2024, but evaluation of applications will continue until the position is filled. The appointment is for two years, starting fall of 2024, but the exact date is negotiable. The position is for the Brownsville campus.
Complete applications should include a letter of interest, curriculum vitae, research statement (maximum 3 pages), and 3 references who could give letters of recommendation at a later stage. The documents should be submitted through UTRGVs portal
https://careers.utrgv.edu/postings/42031.
Questions and informal inquiries about the job should be sent to Dr. Liliana Rivera Sandoval at liliana.riverasandoval @ utrgv.edu.
About UTRGV:
It is UTRGVs vision to be one of the nations leaders in higher education, its premier Hispanic-serving institution, and a highly engaged bilingual university, with exceptional educational, research, and creative opportunities that serve as catalysts for transformation in the Rio Grande Valley and beyond. UTRGV is an equal opportunity and equal access institution committed to excellence. Over 91% of the students enrolled at UTRGV identify as Hispanic, making UTRGV one of the top 3 universities with the highest percentage of Hispanic students. For additional information about the university, please visit our website. For information about the Department see https://www.utrgv.edu/physics/about/index.htm.
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Postdoctoral Positions in Experimental Infrared/ Submillimeter Astrophysics (m/f/d) | Closing date: 2024-03-31 Contact: Prof. Dr. Frank Eisenhauer |
The positions will be in the area of experimental astrophysics, focusing on MICADO and next generation interferometry. Postdoc appointments will start as soon as possible in 2024. Applicants should have a PhD in physics, astronomy or related field before starting. | ▸ more | The Max Planck Institute for Extraterrestrial Physics (MPE) in Garching (near Munich), Germany, is a world-leading institute which develops and operates state-of-the-art astronomical instruments for both ground-based and space-based applications. MPE is divided into four major research areas. The Infrared Group of the Max Planck Institute for Extraterrestrial Physics invites applications from talented, ambitious graduating PhD students and postdoctoral researchers in experimental astrophysics. Our front-line research focuses on near-IR-millimeter high-resolution imaging and spectroscopy of the Galactic Center, and of star forming galaxies in the early Universe. We lead studies of star formation, gas content, physical properties and dynamics of galaxies, and black-hole formation and evolution. This research is supported by a major program of innovative instrumentation development. We are investing substantial developmental effort in interferometry and adaptive optics for ESO. We are the PI institute for GRAVITY, a unique ESO VLTI instrument for precision astrometry and interferometric imaging of faint objects, and are leading the major upgrade to GRAVITY+. We are also the PI institute for MICADO, the first-light instrument for the 39-meter ESO ELT, which will come online later this decade. We have recently commissioned ERIS, a new diffraction-limited imaging and spectroscopic facility for the VLT, and are undertaking a 5-year ERIS guaranteed time program on z~2 galaxy dynamics and the Galactic Center.
Postdoctoral Positions in Experimental Infrared/ Submillimeter Astrophysics (m/f/d)
Job Code: 03/2024
The positions will be in the area of experimental astrophysics, focusing on MICADO and next generation interferometry. Postdoc appointments will start as soon as possible in 2024. Applicants should have a PhD in physics, astronomy or related field before starting.
The salary and full social benefits are based on the German TVöD scale for public employees (E14 for postdocs), depending on experience.
The full-time position is initially for three years and then a possibility for an extension (WissZeitGesetz), depending on mutual agreement.
The Max Planck Society is an equal opportunity employer. Applications from women, disabled people and minority groups are particularly welcome.
Your application:
Please send a motivational letter of application and a CV including bibliography to (https://recruitingapp-5257.de.umantis.com/Vacancies/589/Application/CheckLogin/2?lang=eng) by March 31st, 2024. We also require three letters of reference to be sent directly to us (irjobs @ mpe.mpg.de).
The search will continue until suitable candidates are found. For scientific enquiries about the positions, please contact Linda Tacconi (Linda @ mpe.mpg.de) or Frank Eisenhauer (Eisenhau @ mpe.mpg.de) .
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Postdoctoral position in observational extragalactic astrophysics | Closing date: 2024-04-01 Contact: Damien Hutsemekers |
Applications are invited for a postdoctoral position in observational extragalactic astrophysics at the STAR institute of the University of Ličge (Belgium), to work in collaboration with Drs. D. Hutsemékers and D. Sluse. The research activities encompass AGN physics, in particular polarization, galaxy-scale strong / milli / micro-lensing of quasars, distribution of dark matter in galaxies, and cosmic large-scale groups hosting quasars. The candidate is expected to contribute to one (or several) of those research fields. | ▸ more | The STAR Institute gathers more than 100 researchers carrying out cutting-edge research in extragalactic astrophysics, gravitational waves, astro-particles, planetology, stellar physics, and instrumentation. It has direct access to the full suite of ESO observing facilities, and excellent computing facilities.
Applicants should have a doctorate in astrophysics or a related discipline, obtained no more than five years ago at the starting date of the contract. In addition, the candidate cannot have spent more than 24 months as a resident in Belgium during the last three years. A good command of English or French is required.
Applicants should submit a CV, publication list, and a research statement (containing a report on previous and current research activities and expertise as well as a research project, within three pages maximum, one single pdf file), via email to dsluse @ uliege.be before April 1st. Two letters of recommendation should be independently sent to the above e-mail address. Late applications will be considered until the position is filled. The position is initially for two years, with possible extension of up to three years in exceptional cases. It comes with a competitive salary, benefits, and generous travel funding. The successful candidate is expected to start on September 1st, 2024, with some flexibility, but in any case no later than December 1st.
The selection procedure will be in accordance with the regulations of the University of Ličge. Our institutional policy is based on diversity and equal opportunities. We select candidates based on their qualities, regardless of age, sexual orientation, origin, beliefs, disability, or nationality. More details on the position can be found at https://shorturl.at/jKR48
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Postdoctoral Positions in Experimental Infrared/ Submillimeter Astrophysics (m/f/d) | Closing date: 2024-03-31 Contact: Prof. Dr. Frank Eisenhauer |
Postdoctoral Positions in Experimental Infrared/ Submillimeter Astrophysics
The positions will be in the area of experimental astrophysics, focusing on MICADO and next generation interferometry. Postdoc appointments will start as soon as possible in 2024. Applicants should have a PhD in physics, astronomy or related field before starting.
The full-time position is initially for three years and then a possibility for an extension (WissZeitGesetz), depending on mutual agreement. | ▸ more | The Max Planck Institute for Extraterrestrial Physics (MPE) in Garching (near Munich), Germany, is a world-leading institute which develops and operates state-of-the-art astronomical instruments for both ground-based and space-based applications. MPE is divided into four major research areas. The Infrared Group of the Max Planck Institute for Extraterrestrial Physics invites applications from talented, ambitious graduating PhD students and postdoctoral researchers in experimental astrophysics. Our front-line research focuses on near-IR-millimeter high-resolution imaging and spectroscopy of the Galactic Center, and of star forming galaxies in the early Universe. We lead studies of star formation, gas content, physical properties and dynamics of galaxies, and black-hole formation and evolution. This research is supported by a major program of innovative instrumentation development. We are investing substantial developmental effort in interferometry and adaptive optics for ESO. We are the PI institute for GRAVITY, a unique ESO VLTI instrument for precision astrometry and interferometric imaging of faint objects, and are leading the major upgrade to GRAVITY+. We are also the PI institute for MICADO, the first-light instrument for the 39-meter ESO ELT, which will come online later this decade. We have recently commissioned ERIS, a new diffraction-limited imaging and spectroscopic facility for the VLT, and are undertaking a 5-year ERIS guaranteed time program on z~2 galaxy dynamics and the Galactic Center.
Postdoctoral Positions in Experimental Infrared/ Submillimeter Astrophysics (m/f/d)
Job Code: 03/2024
The positions will be in the area of experimental astrophysics, focusing on MICADO and next generation interferometry. Postdoc appointments will start as soon as possible in 2024. Applicants should have a PhD in physics, astronomy or related field before starting.
The full-time position is initially for three years and then a possibility for an extension (WissZeitGesetz), depending on mutual agreement.
We offer:
? Fair payment according to your qualifications and professional experience in accordance with the collective agreement for the public service (TVöD).
? Company pension scheme (VBL).
? Family service at the Garching research campus.
? Private accident insurance financed by the employer.
? Underground station U6 directly in front of the institute.
? Canteen in the immediate vicinity.
? Reduced rates for certain insurance policies.
? Free parking on the institute grounds.
The Max Planck Society is committed to increasing the number of individuals with disabilities in its workforce and therefore encourages applications from such qualified individuals.
Furthermore, the Max Planck Society seeks to increase the number of women in those areas where they are underrepresented and therefore explicitly encourages women to apply.?
Your application:
Please send a motivational letter of application and a CV including bibliography to (https://recruitingapp-5257.de.umantis.com/Vacancies/589/Application/CheckLogin/2?lang=eng) by March 31st, 2024. We also require three letters of reference to be sent directly to us (irjobs @ mpe.mpg.de).
The search will continue until suitable candidates are found. For scientific enquiries about the positions, please contact Linda Tacconi ? Linda @ mpe.mpg.de or Frank Eisenhauer ? Eisenhau @ mpe.mpg.de.
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Head of the ALMA Regional Centre | Closing date: 2024-03-30 Contact: Evelina |
Owing to an internal reorganisation and the resulting strengthening of the ESO ALMA Support Centre Division (EASC) in the Directorate of Operations at the Headquarters in Garching near Munich, Germany, we are looking to fill the position of Head of the ALMA Regional Centre . | ▸ more | The ALMA Regional Centre (ARC) Department of the EASC is a central link between ESO and the ESO ALMA user community and provides services to the ALMA observatory. The ARC supports the ESO users and the ALMA Observatory in coordination with the ARCs in the other ALMA partner regions. Besides the support of ALMA users, the ESO ARC provides other important services for the development and operation of ALMA, including software development and testing, Call for Proposals and observation preparations, participation in observing shifts at the ALMA observatory, data quality assurance (QA2), optimization of capabilities and work on calibrator database data. ALMA is also currently undergoing an ambitious upgrade - the Wideband Sensitivity Upgrade (WSU) - and the ARC is heavily involved in the planning and investigations needed to transition to WSU Operations at around the end of the decade.
The ARC in ESO's member states is organised as a coordinated network of nodes distributed across Europe. The central ARC is located at ESO Headquarters in Garching and carries the responsibility for all the core ARC activities as well as the coordination of the additional science support provided by the regional nodes and centres of expertise. ARC nodes have been set up in Italy, Germany, France, the Netherlands, the United Kingdom, Czech Republic and Sweden.
As we celebrate 10 years since the inauguration of ALMA we are looking for the next Head of the European ARC to build upon our catalogue of success. In this exciting role you will not only work with staff at ESO but also with colleagues in the other parts of our ARC network. You will also interact with the Science Operations teams in Chile, East Asia and North America.
You will be the interface between the community and Science Operations and with the Head of the ESO ALMA Support Centre you will drive ALMA forward determining what it will do and how it will interact with its users. Leading the ARC in Europe you will grow your team and motivate them to help build on the impressive results we have achieved so far.
In summary you will be the face of ALMA Science Operations in Europe and be an active member of the ALMA global middle management team. With significant challenges in 2024 and beyond you will also play an integral role in the planning for the WSU and helping to drive the strategy for the ESO ALMA Support Centre Division. You will be key in ALMA's continuing success.
The position is in the ESO Faculty and up to 50% of your time will be spent in scientific research. You must have a strong research profile in radio and/or millimetre astronomy. As a member of the ESO Faculty, you will be given the opportunity to interact with other researchers at ESO and contribute to ESO's diverse scientific life. You must be able to show us your scientific drive and vision to conduct high-impact research to be considered for this post.
Main Duties and Responsibilities:
Manage the ARC department of the EASC Division;
Manage the ARC department budget;
Manage ESO ARC staff and oversee all ESO ARC activities with a deputy appointed by the Head;
Keep the oversight and responsibility of the ARC node activities in Europe, maintain the strategic view of the evolution of the ARC network and lead the changes, together with the ARC network coordinator;
Liaise with the Heads of ALMA computing, engineering and development at ESO and ALMA stakeholders both within and external to ESO as required;
Report on the ESO share of ALMA Operations, ESO ARC and European ARC network activities at the ESO Users Committee (UC), the ALMA European Science Advisory Committee (ESAC), and the Scientific Technical Committee (STC);
Participate in and contribute to EASC division management meetings, playing an integral role in development of division strategy;
Coordinate activities of ESO fellows with duties in the ARC;
Attend, or delegate within the ARC Department, ALMA science operations meetings (including the ALMA Integrated Science Operations Team), Joint Operations meetings and subsystem scientists' meetings when required;
Contribute to the ESO Quarterly Report, Annual Report, ALMA highlights and other reports as needed;
Maintain a proactive overview of and involvement in the ARC website and ESO ARC Newsletters;
Availability and willingness to travel to the JAO in Chile is required, as well as to the ALMA Partner sites in East Asia and North America.
Reports to:
Head of the ESO ALMA Support Centre (EASC) Division.
Key Competences and Experience:
Essential Experience
At least 6 years of experience post PhD;
Experience in science operations (and particularly a radio interferometer) or equivalent;
Experience with, and positive attitude towards, providing user support and services;
Experience with the coordination and management of a geographically distributed teams;
Familiarity with ALMA or similar instruments on a technical and operational level.
Competencies
Motivating teams and leading with strategic vision;
Excellent and demonstrable interpersonal and cross-disciplinary communication skills with a strong ability to work both within and simultaneously lead a team;
In-depth understanding of ALMA operations and a distributed network of data reduction or knowledge of operations of other large astronomical facilities;
Ability to build and maintain effective links with peers within ESO, ALMA and with the user community;
Self-driven, critical thinker with the capacity to provide clear, concise and timely oral and written communications, reports and specifications and with excellent problem-solving skills;
Ability to make and justify decisions under operational stress, and proactively act and/or react quickly when confronted with, or in anticipation of, unexpected situations or challenges;
Ability to design and implement departmental procedures and workflows;
Please see https://recruitment.eso.org/jobs/2024_0007 for more information.
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