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EAS Job Directory
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| Postdoc in Exoplanets: EPRV Research and the Second Earth Spectrograph (2ES) | Closing date: 2025-01-09
Contact: Lars A. Buchhave |
| The Exoplanet Group at DTU Space at the Technical University of Denmark, situated in the greater Copenhagen area, invites applications from highly qualified individuals for a postdoctoral position of three-year duration in extreme-precision radial velocity research. | | ▸ more | The Exoplanet Group at DTU Space at the Technical University of Denmark, situated in the greater Copenhagen area, invites applications from highly qualified individuals for a postdoctoral position of three-year duration in extreme-precision radial velocity research.
You will work with Prof. Lars A. Buchhave (2ES PI) and the rapidly growing Exoplanet Group at DTU Space. At DTU Space, you will have access to data from world-class telescopes, including JWST, ultra-precise RV spectrographs (e.g., HARPS-N and EXPRES), and access to ESO facilities. Additional information about the Exoplanet Group at DTU Space can be found at http://www.exoplanets.dk, and more details about 2ES can be found at http://www.2es.dk.
Responsibilities and qualifications
We are seeking a talented and highly motivated researcher to work at the forefront of extreme-precision radial velocity science. The postdoc will be involved with one or more of the following activities: developing and implementing a data reduction pipeline for 2ES to achieve extreme RV precision; conducting laboratory testing and characterization of 2ES to ensure optimal performance and stability; integrating a Laser Frequency Comb (LFC) calibration source to ensure extreme long-term precision; developing and applying stellar activity mitigation techniques for solar-type stars; refining the target list for 2ES and conducting preparatory observations using other facilities; and contributing to the scientific and technical preparation for 2ES operations and the discovery of Earth-mass planets.
As a formal qualification, you must hold a PhD degree (or equivalent).
Application procedure
Your complete online application must be submitted no later than Friday, 9 January 2026 (23:59 Danish time).
To view the full announcement and to apply: Postdoc in Exoplanets:
EPRV Research and the Second Earth Spectrograph (2ES):
https://efzu.fa.em2.oraclecloud.com/hcmUI/CandidateExperience/en/sites/CX_2001/job/6296/?utm_medium=jobshare&utm_source=External+Job+Share
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| Postdoctoral Position in Black Hole Research and Experimental Astrophysics | Closing date: 2025-11-15
Contact: Dr. Linda Tacconi |
| This year we are focusing our search mainly on candidates whose interests are in studying the Galactic Center black hole with GRAVITY+. | | ▸ more | The Infrared Group of the Max Planck Institute for Extraterrestrial Physics invites applications from talented, ambitious graduating PhD students and postdoctoral researchers working on Galactic Center and black hole research. This research is supported by a major program of innovative instrumentation development. We have recently commissioned ERIS, a new diffraction-limited imaging and spectroscopic facility for the VLT. We are investing substantial developmental effort in interferometry and adaptive optics for ESO. We are the PI institute for GRAVITY and GRAVITY+, an ESO VLTI facility for precision astrometry and interferometric imaging of faint objects. We are also the PI institute for MICADO, the first-light instrument for the ESO ELT
This year we are focusing our search mainly on candidates whose interests are in studying the Galactic Center black hole with GRAVITY+. Strong candidates with experience in experimental astrophysics will also be considered for additional positions. Postdoc appointments can start anytime in 2026. Applicants should have a PhD in 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.
Please send a letter of application, a 2-3 page description of research interests, a CV including bibliography, and request three letters of reference to be sent directly to us by November 15, 2025 to 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.
The Max Planck Society is an equal opportunity employer. Applications from women, disabled people and minority groups are particularly welcome.
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| Postdoc in exoplanet science preparation for PLATO | Closing date: 2025-11-16
Contact: Hans Deeg |
| A postdoc position at the Instituto de Astrofísica de Canarias (IAC) has opened to work on science preparation for the PLATO mission, with an expected focus on circumbinary planets and/or ground-based photometric follow-up. | | ▸ more | The successful candidate will pursue activities related to PLATO science preparation, in the following fields (not necessarily in all of them):
- Detection and analysis of extrasolar planet systems, especially around binary stars.
- Analysis and interpretation of photometry from ground and space-based facilities.
- Development of analysis-tools for ground-based photometry.
- The availability to participate in outreach activities related to PLATO is appreciated.
A full description of the position plus submission guidelines can be found here: https://www.iac.es/en/employment/one-postdoctoral-contract-plato-exo-2025-ps-2025-074
The application deadline is 16 November 2025; the position has funding assured until the end of 2027.
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| Postdoctoral ERC Fellowship in Black Hole and Multiphase Astrophysics | Closing date: 2025-11-19
Contact: Massimo Gaspari |
| The ERC-CoG BlackHoleWeather is a cutting-edge initiative aimed at understanding how the feeding and feedback of supermassive black holes shape the evolution of galaxies, groups, and clusters, self-consistently linking macro- and micro-scales (Gaspari+20, Nat. Astron.). The successful candidate may contribute on the numerical side (by developing and exploring multiscale MHD simulations) or on the observational side, via the analysis of multi-wavelength data. Applications are equally welcome from both observational and numerical backgrounds, with the possibility to integrate both approaches. | | ▸ more | Numerical track: running and analyzing high-resolution 3D multiscale MHD simulations on GPUs (e.g., AMR codes such as AthenaPK and GAMER); implementing advanced microphysics (e.g., anisotropic conduction/viscosity, chemical networks, star formation, plasma physics); producing synthetic observables (X-ray, optical/IR, radio) and comparing them with observations.
Observational track: reducing and analyzing multi-wavelength datasets (e.g., JWST/HST, Chandra/XMM, ALMA/MeerKAT/LOFAR, MUSE); extracting physical and kinematic properties; performing quantitative comparisons with the MHD simulations.
Cross-cutting activities: publishing first-author scientific papers, presenting results at international conferences, collaborating with global partners (Princeton, MIT, NTU), playing a leading role within the BlackHoleWeather excellence team, mentoring students, engaging in problem-solving, and contributing to ERC deliverables (datasets and codes).
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* Application Details
The position is for 2+2 years, with renewal based on performance. The position may be later upgraded to tenure-track Assistant Professor. The starting date is preferred to be as soon as possible (negotiable).
* Application Instructions
Please submit via the PICA platform (ENG or ITA; see link/PDF below for details) the following:
1. full CV (dated and signed), including publication list and ~3 reference contacts;
2. Cover Letter tailored to this position;
3. brief Research Proposal (max 3 pages) specifying your preferred track (numerical/observational/combined), the methodology you plan to adopt, and deliverables aligned with BlackHoleWeather science;
4. key Publications (up to 10 uploaded PDFs);
5. Valid ID or passport (for non-EU residents).
Eligibility. Ph.D. in Astronomy/Astrophysics (or equivalent). Final-year Ph.D. candidates may apply, but the degree must be obtained before contract signing. Working language: English (Italian not required).
Deadline: 19 November 2025, 13:00 CET. Review begins immediately after the deadline; short-listed candidates will be invited to a remote interview discussing prior research and problem-solving experience, scientific output, and core knowledge.
If you have any questions about the position or application procedure, do not hesitate to write to Prof. Gaspari: massimo.gaspari @ unimore.it
You are welcome to send your CV to Prof. Gaspari for pre-screening, but note that complete formal applications must be submitted through the official portal: https://pica.cineca.it/unimore/cdr-2025-19
* Link to Online Application: https://shorturl.at/LmAQi
* Included Benefits
Research benefits: extensive dedicated funds for travel, workshops, and international conferences, plus substantial research and computing resources within the 2 million Euro ERC BlackHoleWeather project, providing an exceptional environment to develop independent ideas and collaborations.
Retirement benefits: full enrollment in Italy's national pension system (INPS), with the employer covering the majority of contributions and annual TFR severance fully funded by the university, ensuring long-term social-security coverage and end-of-contract benefits.
Healthcare benefits: comprehensive coverage through the Italian National Health Service with no premiums required; optional private health insurance may also be supported by the employer for international researchers.
* Compensation Notes
The salary ranks among the highest for research scientists in Italy, close to an assistant professor, and includes full employee benefits. The cost of living in Italy is 2-3x lower than in most Western countries, while Emilia-Romagna offers one of the highest quality-of-life standards in Europe, combining rich culture, excellent food, and affordable living.
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| Research position at the Astronomical Institute of the Czech Academy of Sciences | Closing date: 2025-11-20
Contact: Lenka Cihakova |
| Astronomical Institute of the Czech Academy of Sciences (CAS) invites applications for a research position in frame of the grant project "ESA space coronagraphy with Czech participation". The successful applicant is expected to contribute to analyses of coronagraphic spectral images of CMEs and eruptive prominences obtained by the Solar Orbiter/Metis and Proba-3/ASPIICS space coronagraphs. The programming experience using Fortran and IDL/Python is also expected in order to further develop the relevant spectral diagnostic tools. | | ▸ more | The successful applicant will join the Solar Department of the Astronomical Institute of the CAS, which resides in Ond?ejov (Central Bohemia, about 30 km from Prague). The project involves a close collaboration with the Metis and ASPIICS international teams.
The position is supported by a salary, which is based on the domestic standards (around 2400 EUR/month before taxes) and includes a health insurance. The applicant must hold a PhD degree. Applications can be submitted before finishing PhD, in which case a statement about the planned date of the defense should be included. The appointment is initially for one year (starting on 1 January 2026), with possible extension until 31 December 2027 depending on satisfactory scientific performance. For informal inquiries about the position please feel free to email pheinzel @ asu.cas.cz or gunar @ asu.cas.cz .
Applications containing a Cover Letter (describing the candidate?s scientific profile and why he/she is applying for this position), Curriculum Vitae, and the List of Publications should be submitted to info @ asu.cas.cz (cc to pheinzel @ asu.cas.cz), subject: GACR-research position.
The application deadline is 20 November 2025.
Candidates are encouraged to arrange for two recommendation letters that have to be sent to the same email addresses with the same subject.
Further information:
http://www.asu.cas.cz for the list of working groups at the Institute.
http://www.euraxess.cz for details about the research employment and work conditions in Czech Republic.
http://www.numbeo.com/cost-of-living/comparison.jsp to compare cost of living.
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| 7 PhD positions at the Kapteyn Astronomical Institute | Closing date: 2025-11-28
Contact: Kapteyn Institute |
| The Kapteyn Astronomical Institute of the University of Groningen in the Netherlands invites applications for at least 7 PhD positions in the areas of planet forming disks, exoplanet astronomy, dwarf galaxies and galactic archeology. | | ▸ more | Description:
The Kapteyn Astronomical Institute of the University of Groningen in the Netherlands invites applications for at least 7 PhD positions in the areas of planet forming disks, exoplanet astronomy, dwarf galaxies and galactic archeology:
- Two positions in the group of Prof. Inga Kamp working on planet forming disks.
- One position in the group of Dr. Quentin Changeat on the observation of exoplanet atmospheres.
- One position in the group of Dr. Tim Lichtenberg on simulations of the interior and atmospheric evolution of rocky exoplanets.
- One position in the group of Dr. Ting-Yun Cheng on dwarf galaxies and machine learning applications
- Two positions in the group of Prof. Else Starkenburg on the early Milky Way.
We seek excellent students with a strong background in the physical sciences who desire a PhD degree from a top European University. A successful candidate must hold an MSc or equivalent degree in Physics, Astronomy, Geoscience, Mathematics, Computational Science or a related field by the starting date of the position. Previous research experience and skills will be important criteria for the selection.
The University of Groningen is a university in which inclusion and equality are core values and we are constructively working on creating a socially safe environment. We therefore invite applicants from underrepresented groups in particular to apply. For more information: https://www.rug.nl/(...)rsity-and-inclusion/.
Compensation and Benefits:
These PhD student positions are paid according to the Collective Labour Agreement of Dutch Universities:
- a salary of ? 3,059 in the first year to a maximum of ? 3,881 gross per month in the final year (PhD salary scale), based on a full-time position
- a holiday allowance of 8% gross annual income
- an 8.3% year-end bonus
- a full-time position (1.0 FTE).
The selected PhD candidates will be first offered a temporary position of one year with the option of renewal for another three years.
Instructions:
Information on how to apply and more details on the positions can be found at https://www.rug.nl/research/kapteyn/vacatures/phd-positions
Please check this link carefully as potential new positions will be advertised there.
Application Deadline: 2025 Nov 28
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| Sustainability Manager | Closing date: 2025-11-28
Contact: Heather or Nasrin |
We are seeking an ambitious, strategic, and visionary Sustainability Manager to lead the next phase of our journey. You will drive the development and implementation of our sustainability strategy, embedding sustainable practices across all aspects of our global operations.
Apply here: https://recruitment.skao.int/vacancy/sustainability-manager-599174.html | | ▸ more | In this pivotal role, you will champion the SKAO?s sustainability agenda internally and externally, ensuring measurable progress in environmental stewardship, social value, and responsible governance. You will represent the SKAO at international fora, engage with governments, industry, research partners, and communities, positioning the SKAO as a model of sustainability in large-scale scientific collaboration.
You will work closely with experts across all directorates and sites of the SKAO, collaborating with multidisciplinary teams to embed sustainability principles into every aspect of the organisations work.
This is an unparalleled opportunity to influence the sustainability direction and outcomes of a globally significant scientific project and ensure long-term societal and environmental impact.
This role will be based at the SKAO Global Headquarters at the iconic Jodrell Bank Observatory, Cheshire, UK.
SKAO is committed to providing an inclusive and flexible working environment, meeting the requests of our Colleagues whilst also fulfilling the needs and objectives of the Observatory.
This role requires the post holder to work across different time zones and, in line with SKAO policy, flexible working hours will be supported in agreement with the line manager.
Key Responsibilities, Accountabilities and Duties
-Lead the development, delivery, and continuous improvement of the SKAO?s Sustainability Strategy and associated action plans.
-Act as the organisation?s senior sustainability ambassador, building networks and representing SKAO at international events, conferences, and global fora.
-Build and manage strong relationships with stakeholders, including SKAO colleagues, partner governments, regulatory authorities, local communities, research partners, and suppliers.
-Embed sustainability principles and improvements into organisational processes, including strategic planning, procurement, construction, and scientific operations.
-Collaborate with the Strategy and Impact Specialist to ensure high-quality ESG reporting and transparent communication aligned with global frameworks such as the UN SDGs and GRI.
-Monitor global sustainability trends, policy developments, and emerging risks, advising senior leadership on opportunities and potential challenges.
-Work with multidisciplinary teams to design and implement initiatives that reduce environmental impact, enhance climate resilience, improve social impact and create long-term value.
-Promote a culture of sustainability and continuous improvement across international, cross functional teams.
-Oversee sustainability budgets and resources, ensuring effective collaboration, transparency and accountability.
-Influence and engage internal stakeholders to align day to day operations with the SKAO?s sustainability ambitions.
Mandatory Knowledge, Skills and Experience
-Significant experience in a senior sustainability leadership role within a complex, multi-stakeholder or international organisation.
-Proven track record of designing, implementing, and measuring sustainability strategies that deliver tangible results.
-Exceptional communication and relationship-building skills, with the ability to represent the organisation at senior levels and in external fora.
-Strong knowledge of global sustainability frameworks, environmental science, ESG standards, and regulatory compliance.
-Advanced data analysis, reporting and performance management capabilities, including experience with sustainability metrics and tools.
-Excellent project management and organisational skills, with the ability to manage multiple priorities and teams.
-Demonstrated ability to influence and embed cultural change across diverse teams, disciplines, and geographies.
-Relevant professional qualifications or certifications (e.g., ISSP, IEMA, LEED).
Desirable Knowledge, Skills and Experience
-Previous experience within an intergovernmental organisation.
-Understanding of science, research, or engineering-based environments.
-Degree in Environmental Science, Sustainability, Engineering, or a related discipline.
Equality Diversity and Inclusion Statement
SKA Observatory recognises that our diversity is a strength. We aim to create a welcoming and inclusive environment where everyone feels they belong, and diverse perspectives and ideas thrive. As such, Equality, Diversity, and Inclusion are at the core of SKA Observatory?s agenda.
Our aim is to recruit and retain the most talented individuals, regardless of gender, race, disability, age, sexual orientation, marital status, religion, nationality or background.
Women have traditionally been under-represented in the fields of science and engineering; SKA Observatory welcomes and encourages female applicants.
Where applicants with a disability need facilities or adjustments to enable them to participate in the recruitment process, these will be provided.
SKA Observatory welcome all candidates, especially those from member countries.
The ?How to Apply? information contained within the SKA Observatory recruitment portal provides more detail regarding our application and selection approach.
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| ICCUB's Maria de Maeztu Postdoctoral positions and Fellowship | Closing date: 2025-11-30
Contact: Esther Pallares |
| The Institute of Cosmos Sciences of the University of Barcelona (ICCUB) invites applications for two postdoctoral positions and one ICCUB Postdoctoral Fellowship, offered under the framework of its Unit of Excellence Maria de Maeztu. All positions are funded for up to 3 years. | | ▸ more | The three scientific profiles are as follows:
- Position in Beyond the standard models of cosmology and particle physics: https://icc.ub.edu/node/1177163
- Position in Gravitational wave physics: https://icc.ub.edu/node/1177161
- Position in Quantum Resources for Science and Technology: https://icc.ub.edu/node/1177162
These positions are part of a dynamic and interdisciplinary research environment at one of Europe?s leading centers in cosmology, astrophysics, and particle physics. The Institute of Cosmos Sciences (ICCUB) at the University of Barcelona, established in 2006, focuses on cosmology, astrophysics, particle physics, quantum physics, and nuclear physics. With over 70 scientists, 20 engineers, and 90 postdoctoral researchers and PhD students (35% international), ICCUB collaborates internationally on projects like Gaia, LHCb, Virgo, MAGIC, CTA, and DESI. It also has an Advanced Technology Unit supporting experimental research requiring cutting-edge technology.
Requirements:
Applicants must hold a PhD in Physics, Astrophysics, or a closely related field by the start date of the contract, approximately in October 2026. We are looking for motivated researchers with a strong track record and a collaborative spirit.
Employment Terms:
Duration: up to 3 years
Start Date: Preferably by Fall 2026 (flexibility possible for parental or special circumstances)
Salary:
Maria de Maeztu Postdoctoral Positions: Approx. 36.360?/year (gross), including full social security and public healthcare coverage for the researcher, spouse or registered partner and children
ICCUB Postdoctoral Fellowship: Approx. 42.900?/year (gross), including full social security and public healthcare coverage for the researcher, spouse or registered partner and children
Research Support:
Fellowship: ?8,000/year for travel and training
Postdoctoral Positions: ?5,000/year for travel and training
Access to ICCUB?s advanced computational infrastructure, training programs, and career development resources
Equal Employment Opportunity Statement
ICCUB offers and promotes a diverse and inclusive environment and welcomes applicants regardless of age, disability, gender, nationality, race, religion or sexual orientation (for additional information please see the Diversity, Equity and Inclusion Commission. Job seekers in need of a reasonable accommodation to complete the application process should call or email secretaria @ icc.ub.edu with their request.
Application Process:
To apply, please complete the application form and provide contact details for three referees. After submission, you will receive instructions to upload the following documents:
Curriculum Vitae
Cover Letter
Research statement (max 4 pp) outlining research experience, interests, research plan and how the candidate?s profiles and research plan would fit with the scientific profile of the position(s)
Publication List
The contact of three Reference Letter writers (referees will be contacted directly)
Reference letters must be sent directly by the referees through the on-line application system (the system will contact these scientists you named, asking them to submit their letters of reference after a few working days). Applications will only be considered once at least two reference letters have been received.
Note: Applicants should select their preferred job offer.
Note: For questions regarding the application process, please contact Esther Pallarès at secretaria @ icc.ub.edu.
Deadline
Application deadline: November 30th, 2025
Review of applications will begin immediately after the deadline and will continue until all positions are filled.
Selection process:
The selection process consists of two phases: merit-based evaluation and an interview.
1. Merit-Based Evaluation
The Selection Committee will verify and assess the merits documented by the applicants. The maximum score for this phase is 80 points, distributed across the following categories:
Curriculum Vitae ? Maximum: 30 points
Alignment with the María de Maeztu Challenge ? Maximum: 30 points
Reference Letters ? Maximum: 20 points
2. Interview: maximum 20 points
Applicants who score at least 50 points in the merit-based evaluation will be invited to an interview. The interview will be conducted in English and may take place online via a video conferencing platform.
Funding:
These positions are financed by the State Agency for Research of the Spanish Ministry of Science, Innovation and Universities through the "Unit of Excellence María de Maeztu 04/2019-03/2031" awarded to the Institute of Cosmos Sciences, grant CEX2024-001451-M funded by MICIU/AEI/10.13039/501100011033.
The Unit of Excellence Maria de Maeztu recognition has been awarded by the Spanish Government in 2025 for the third time to the ICCUB, as a center with a highly competitive strategic research programmes in the frontiers of knowledge.
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| PhD student position in Star formation with machine learning at the University of Geneva | Closing date: 2025-11-30
Contact: Marc Audard |
We are looking for a candidate for a PhD position at the Department of Astronomy of the University of Geneva in the context of the newly funded Swiss National Science Foundation project "STARforM-Lens: Accretion in star formation through the lens of machine learning".
| | ▸ more | The star formation group at the University of Geneva, led by Dr Marc Audard, has an opening for a PhD position to work on the newly funded
project "STARforM-Lens: Accretion in star formation through the lens of machine learning, which aims to study star formation and its accretion across time with innovative machine learning techniques. The project aims to use the wealth of Gaia multimodal data (photometry, spectroscopy, radial velocities, astrometry, and time variability) together with complementary all-sky survey data at different wavelengths. The project will employ two distinct ML techniques: the first one aimed to scrutinise the long-term evolution of YSO accretion by boosting a very large database of panchromatic spectral energy distributions (SEDs) for young stellar objects with Gaia spectra, while the second technique will focus on the short-term accretion variability by modeling the heterogeneous data using a shared latent space.
The PhD student is expected to focus on the second technique, while collaborating on the other technique with a postdoc in Geneva and with the international team composed of Dr Kai Polsterer at the Heidelberg Institute for Theoretical Studies (HITS) in Germany and Dr Gabor Marton at Konkoly Observatory / CSFK in Hungary. Several secondments (typically a month per year) at HITS are planned. A taste and skills in astronomy and astrophysics, data science, and/or machine learning are required, together with the ability to work in small, international teams. The PhD student will furthermore have the opportunity to be integrated in the Coordination Unit 7 of the Gaia Data Processing and Analysis Consortium toward the final release DR5 planned for 2030.
The Department of Astronomy at the University of Geneva offers a modern and vibrant working environment, with a wide range of activities including theory, numerical simulations, observations and instrumental developments in the fields of exoplanets, stellar physics, galactic dynamics, observational cosmology, and high-energy astrophysics.
Applications are invited from candidates with a solid background in physics or astronomy and should consist of a cover letter explaining the motivation for seeking a PhD in astrophysics and especially the aforementioned research fields, a statement outlining any research experience so far (<1 page each), a CV, and a copy of the Bachelor and Master academic record (exams, theses, and grades). Candidates should also provide names and e-mail addresses of at least two references. Applications should be sent as a single PDF file to marc.audard @ unige.ch.
The position is for 4 years, contingent upon satisfactory performance, mutual agreement, and approval by the PhD committee; remuneration is based on the University salary grid (Canton of Geneva). Generous funds for travel and computer equipment are included. The selected Ph.D. student will enroll in the Ph.D. programme of the Department and University (UniGE).
Complete applications received by 30 November 2025 will receive full consideration, but the search will remain open until the positions are filled. Start date is negotiable. Preliminary inquiries may be addressed via e-mail to marc.audard @ unige.ch.
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| Postdoc position in Star formation with machine learning at the University of Geneva | Closing date: 2025-11-30
Contact: Marc Audard |
We are looking for a candidate for a postdoc position at the Department of Astronomy of the University of Geneva in the context of the newly funded Swiss National Science Foundation project "STARforM-Lens: Accretion in star formation through the lens of machine learning".
| | ▸ more | The star formation group at the University of Geneva, led by Dr Marc Audard, has an opening for a postdoc position to work on the newly funded
project "STARforM-Lens: Accretion in star formation through the lens of machine learning, which aims to study star formation and its accretion across time with innovative machine learning techniques. The project aims to use the wealth of Gaia multimodal data (photometry, spectroscopy, radial velocities, astrometry, and time variability) together with complementary all-sky survey data at different wavelengths. The project will employ two distinct ML techniques: the first one aimed to scrutinise the long-term evolution of YSO accretion by boosting a very large database of panchromatic spectral energy distributions (SEDs) for young stellar objects with Gaia spectra, while the second technique will focus on the short-term accretion variability by modeling the heterogeneous data using a shared latent space.
The postdoc is expected to focus on the first technique, while collaborating on the other technique with a PhD student in Geneva and with the international team composed of Dr Kai Polsterer at the Heidelberg Institute for Theoretical Studies (HITS) in Germany and Dr Gabor Marton at Konkoly Observatory / CSFK in Hungary. Long visits to HITS are planned. The postdoc will furthermore have the opportunity to be integrated in the Coordination Unit 7 of the Gaia Data Processing and Analysis Consortium toward the final release DR5 planned for 2030.
The Department of Astronomy at the University of Geneva offers a modern and vibrant working environment, with a wide range of activities including theory, numerical simulations, observations and instrumental developments in the fields of exoplanets, stellar physics, galactic dynamics, observational cosmology, and high-energy astrophysics.
Applications are invited from candidates with research experience on one or more of the following fields: star formation, data science, machine learning, together with the ability to work in small, international teams. Applications should consist of a cover letter, a statement outlining the candidates past research work as well as proposed future research directions (<3 pages) and a CV including a publication list. Candidates should also provide names and e-mail addresses of at least three references. Applications should be sent as a single PDF file to marc.audard @ unige.ch.
The initial appointment will be for one year, renewable annually, contingent upon satisfactory performance, mutual agreement, and availability of funds.
Remuneration is based on the University salary grid (Canton of Geneva). Generous funds for travel and computer equipment are included.
Complete applications received by 30 November 2025 will receive full consideration, but the search will remain open until the positions are filled. Start date is negotiable. Preliminary inquiries may be addressed via e-mail to marc.audard @ unige.ch.
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| ICCUB María de Maeztu Unit of Excellence PhD Fellowships (Pre-selection Call) | Closing date: 2025-11-30
Contact: Institut de Ciències del Cosmos de la Universitat de Barcelona |
| The Institute of Cosmos Sciences of the University of Barcelona (ICCUB), recognized as a Unit of Excellence under the Severo Ochoa and María de Maeztu program, the highest distinction awarded to research institutes or centers in Spain, is launching a pre-selection call for at least six PhD fellowships as part of its María de Maeztu Strategic Program. This initiative reflects ICCUB?s strong commitment to scientific excellence and the advancement of emerging research talent. | | ▸ more | The Institute of Cosmos Sciences of the University of Barcelona (ICCUB), recognized as a Unit of Excellence under the Severo Ochoa and María de Maeztu program, the highest distinction awarded to research institutes or centers in Spain, is launching a pre-selection call for at least six PhD fellowships as part of its María de Maeztu Strategic Program. This initiative reflects ICCUB?s strong commitment to scientific excellence and the advancement of emerging research talent.
This pre-selection aims to identify highly motivated national and international candidates interested in pursuing a PhD in one of ICCUB?s core research areas: cosmology, astrophysics, gravitational waves, quantum technologies, and particle physics. Selected candidates will be invited to participate in the official selection process conducted by the University of Barcelona, which is required for formal admission and hiring.
ICCUB offers a dynamic, interdisciplinary research environment that fosters international collaboration and innovation, supported by cutting-edge infrastructure and a vibrant academic community. Located in Barcelona, a global hub for science and technology, the institute provides an ideal setting for early-stage researchers to launch their scientific careers while enjoying a rich and multicultural lifestyle.
The institute is actively involved in several major international collaborations, including LHCb, DESI, and Euclid, and plays a leading role in gravitational wave experiments such as the Virgo Collaboration, the Einstein Telescope Collaboration, and the LISA Consortium. ICCUB also contributes to large-scale astronomical surveys like ESA-Gaia, Weave, and SDSS-IV, as well as electromagnetic follow-up missions across various wavelengths, including BlackGEM, MAGIC, and LST.
Opportunities at ICCUB:
The PhD fellows at ICCUB will benefit from a comprehensive and enriching training program designed to prepare them for successful careers in academia, industry, or scientific outreach. Each doctoral project is embedded within one of ICCUB?s strategic research challenges. Supervision is provided by experienced ICCUB researchers, often involving co-supervision to foster interdisciplinary perspectives and collaborative mentorship.
In addition to research, students will engage in a tailored training program that includes both technical and transferable skills: scientific seminars, ICCUB Colloquia, advanced instrumentation workshops, data science, research ethics, science communication, project management, and career development. ICCUB also encourages international mobility through short-term research stays at leading institutions worldwide, enhancing global scientific exchange and visibility.
Available positions:
Detailed descriptions of the research projects and host groups can be found in the links
Building interacting quantum systems one atom at a time
Gravitational-wave physics
Gravitational-wave lensing
Fundamental Physics and Technology: From Gravitational Waves to Quantum Detectors
2 positions on Physics Beyond the standard cosmological model and the standard model of particle physics
Fellowship terms:
The fellowship includes funds for a predoctoral training contract for up to four years. The annual salary will be split into 12 monthly payments and distributed as follows:
The first year of PhD: 18.269,56 ?/year
The second and third year of PhD: 22.032,36 ? /year
The fourth year of PhD: 24.468,15?/year
Predoctoral contracts are renewed annually for up to 4 years. Renewal is subject to satisfactory performance in the PhD studies and related research activities. If the doctoral degree is obtained before the predoctoral fellowship ends, a Postdoctoral Orientation Period (POP) can be funded from the time the doctoral degree is obtained until the end of the predoctoral fellowship, with a maximum duration of 12 months (i.e. predoc contract + POP = max. 4 years in total).
The fellowship includes full social security coverage through the Spanish Social Security system, providing access to the Spanish public health care system and pension and unemployment benefits.
Up to 7.000? to cover the enrolment fees for the UB?s Physics doctoral program (for a maximum of 4 years) and carry out short stays in other institutions, companies or universities abroad. The research stays must have a minimum duration of one month and must be authorized by the doctoral supervisor/s.
For full details, refer to the 2024 ?Centros de Excelencia «Severo Ochoa» y Unidades «María de Maeztu»? call for proposals, within the Plan Estatal de Investigación Científica y Técnica y de Innovación 2021?2023 (Articles 10, 11, and 29).
Eligibility criteria:
The fellowships are addressed to graduate students of any nationality who fulfil the following eligibility criteria:
Applicants must hold a Bachelor?s and a Master?s Degree in Physics, Mathematics, Astronomy, Particle Physics, Cosmology, Electronics, Semiconductor Technology, Photonics, Quantum Technologies, Computer Science or a related discipline by September 2026
Be eligible for full-time enrollment in the UB Physics doctoral program for the 2026-2027 academic year by the time the fellowship starts, between September 2026 and January 2027.
Applicants must not hold a doctoral degree. Moreover, applicants are not eligible if they have benefited from a predoctoral training fellowship under the ?Plan Estatal de Investigación, Desarrollo e Innovación Tecnológica? or any of the previous Spanish National Plans by MICIU/AEI.
Applicants must have a thesis supervisor affiliated with the Institute of Cosmos Sciences.
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| Postdoctoral position in relativistic plasma astrophysics | Closing date: 2025-12-01
Contact: Benoit Cerutti |
| Applications are invited for a postdoctoral researcher position at IPAG, France. The successful candidate will join the research group led by Benoit Cerutti to conduct ab-initio plasma simulations of relativistic, magnetized outflows, with a particular focus on neutron star and black hole environments. | | ▸ more | The primary goal is to advance our understanding of plasma dynamics, including jet and wind launching, dissipation processes, and particle acceleration within these extreme astrophysical systems. The candidate will work with Zeltron, a state-of-the-art general relativistic, radiative particle-in-cell (PIC) code, and will have access to high-performance computing resources at both the French and European levels.
Candidates must hold a PhD in astrophysics or a closely related discipline, awarded within the past two years. Preference will be given to applicants with a strong background in computational astrophysics. The position is a two-year appointment, with an expected start date in 2026. The position will come with standard French healthcare benefits together with a generous research and travel budget.
Interested candidates should submit a curriculum vitae, publication list, and a brief statement of research interests, and arrange for up to three recommendation letters to be sent by December 1, to benoit.cerutti @ univ-grenoble-alpes.fr. Later applications will be considered until the position has been filled.
IPAG is a major French institute in astrophysical research under the supervision of both the CNRS and the University of Grenoble Alpes. The institute is located on the main University campus, nested in the heart of the French Alps, about 1 hour away from Lyon and 2 hours away from Geneva. IPAG has about 160 personnel active in fields as diverse as high-energy astrophysics, astrochemistry, exoplanets, star and planet formation, planetology and instrumentation.
The successful candidate will join the high-energy team (the Sherpas), a lively research group with a strong expertise in numerical plasma simulations (PIC and MHD), accretion disk, black hole magnetospheres and jets, pulsars, particle acceleration and radiative processes.
|
| Deputy Director of Gemini Observatory | Closing date: 2025-12-01
Contact: Amber Chasse |
| The International Gemini Observatory is seeking a Deputy Director to help lead an extraordinary team of scientists, engineers and other professionals to enable groundbreaking discoveries in astrophysics. Gemini?s twin 8.1-meter optical / infrared telescopes provide full-sky access from two of the world?s best astronomical sites, Maunakea, Hawai?i and Cerro Pachón, Chile. | | ▸ more | The Gemini Observatory is funded by an international partnership including Argentina, Brazil, Canada, the Republic of Korea, and the United States. Gemini is operated on behalf of its partners by the U.S. National Science Foundation?s National Optical and Infrared Astronomy Research Laboratory (NOIRLab), under a cooperative agreement with the Association of Universities for Research in Astronomy (AURA).
Essential Functions:
Management Oversight - Support and assist the Gemini Director in the discharge of their duties and assist with internal and external affairs of the Observatory.
Planning & Budget Management - Support the Director in the strategic planning of observatory affairs, preparation of the annual program operating plan and budget, and the reporting on the Cooperative Support Agreement with the NSF.
Communications and Governance - In partnership with Director and NOIRLab?s Communications, Education & Engagement (CEE) team support the Observatory?s strategic communications as well as internal and external communications.
Required Education/Experience/Skills/Abilities:
? PhD in astronomy or closely related field
? Knowledge of Spanish is an asset.
Skills Required:
? Internationally recognized scientist with broad interests beyond the field of research
? Familiarity with ground-based and/or space-based observatory operations
? Demonstrated strategic and analytical thinking skills
? Motivation and ability to identify and implement new strategic directions for the Observatory in a team environment
? Strong personnel-staff management skills
? Excellent written and oral communication skills
? Effective technical writing and public speaking communication skills
Experience Required:
? At least 7+ years of post-master?s and/or PhD experience as research scientist, astrophysicist, mechanical engineer, or other related scientific field-discipline.
? With a minimum of 3+ years of experience working in a leadership position (in a university, an observatory, and/or an equivalent science or research organization).
? Extensive experience in people, personnel-staff management, and leadership skills.
? Must have a valid Driver?s License; clean driving record; ability to drive a 4-wheel drive vehicle
Preferred Education/Experience/Skills/Abilities:
? Enthusiasm for scientific discoveries and for observational astronomy;
? Creativity, innovation, and a dedication to serving the community.
? Excellent people management skills and building high performance teams.
? Aptitude for dealing with strategic and tactical problems and issues.
? Ability to communicate with a wide variety of Gemini staff, Board members, oversight and advisory committee members, and users throughout the Gemini partnership
Physical Demands:
The physical demands described here are representative of those that must be met by an employee to successfully perform the essential functions of this job. Reasonable accommodations may be made to enable individuals with disabilities to perform the essential functions.
? Must be able to remain in a stationary position at least 50% of the time.
? Frequent need to move about inside the office environment to access files, office tools, attendance in a meeting room, etc.
? Constantly operates a computer and other office productivity tools that require fine motor skills, such as a calculator, copy machine, computer printer, etc.
? Frequent need to position self to maintain computer and related tools.
? Frequently moves technology equipment weighing up to 20 pounds throughout office locations.
? Constant communication with other individuals. Must be able to discern and exchange information as appropriate to the situation.
? Constant need to distinguish, discern, and identify a variety of objects and fine details with accuracy.
? Some travel may be necessary in or outside the contiguous United States including travel to the various observatory sites (Arizona, Chile and Hawai`i).
? Occasional work at high elevation summit sites may be required (summit elevations range from 6,800 feet to 14,000 feet)
The above statements are intended to describe the general nature and level of work being performed by individuals assigned to this position. They are not intended to be an exhaustive list of all duties, responsibilities and skills required by personnel so classified.
Salary Range
$171,000 - 195,000.
The final salary will depend on skills, qualification, experience and job location.
Salaries for positions hired in Chile meet Chile national market rates and internal scales for AURA.
AURA offers an excellent benefits package including paid time off and retirement contributions, competitive salary commensurate with experience, and a very attractive work environment. Details on benefits can be found at Benefits by Location - Aura Human Resources.
How to Apply
Apply by November 25, 2025, for priority consideration. This position will remain open until it is filled. Please submit a cover letter and a resume, PDF files preferred. Please name any attachments with the following format: LastName FirstName.
https://recruiting2.ultipro.com/SPA1004AURA/JobBoard/57b96f30-6a4b-42cc-8f73-d417a17b54e9/OpportunityDetail?opportunityId=ef790f4d-e225-41e3-b860-c781e1dcd15f
Individuals needing assistance with the employment process can request assistance at employment @ aura-astronomy.org
Equal Opportunity Employer
This employer is required to notify all applicants of their rights pursuant to federal employment laws. For further information, please review the Know Your Rights notice from the Department of Labor.
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| PhD position in BepiColombo, Mercury's space weather, and high-performance computing | Closing date: 2025-12-01
Contact: Riku Järvinen |
| We are seeking for a motivated doctoral researcher (PhD candidate) to work on the modelling of Mercury's space plasma physics in a BepiColombo related project. | | ▸ more | The position is part of the MErcury in the sOlar Wind (MEOW) ERC project at the Finnish Meteorological Institute. You will use our global particle-based space weather models to study the solar wind influence on Mercury and its environment and interpret observations from the BepiColombo mission. Alternatively, you can focus on the development of simulation methods for supercomputer environments, depending on your skills and interests.
Apply here:
https://valtiolle.fi/en/jobs/doctoral-researcher-space-weather-modelling-application-period-extended-16176/
More information:
https://planets.fmi.fi/
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| 2026 Trottier Postdoctoral Fellowship in Exoplanetary Science (IREx) | Closing date: 2025-12-04
Contact: Marie-Eve Naud |
| The Trottier Institute for Research on Exoplanets (IREx), affiliated with the Department of Physics of the Université de Montréal (Montréal, Canada) invites applications for the Trottier Postdoctoral Fellowship, which enables cutting-edge independent research in experimental, observational, or theoretical astrophysics applied to the study of exoplanets and related fields of astrophysics and astronomical instrumentation. | | ▸ more |
Starting Date: The successful applicant is expected to start between May and September 2026.
Duration: The position is for two years, renewable for a third year, subject to performance and availability of funds.
Eligibility requirements: A PhD in physics, astronomy or a related discipline is required when the position starts. Preference will be given to applicants who have obtained their Ph.D. within the last 3 years. Applicants with career interruptions due for example to parental, medical, or family leaves, are invited to mention this in their cover letter if desired.
Conditions: The remuneration includes an annual salary of CAD 65,000 (full-time), maximum research funds of CAD 10,000 per year (for travel, publication, etc.), and a one-time allowance of up to CAD 2,000 for moving expenses to Montreal.
Application: Applicants should submit a cover letter (optional, max 1 page), a statement of research interests (max 2 pages), and a CV incl. a list of publications. They should also arrange to have three referees send a letter of reference to irex-applications @ umontreal.ca (format ApplicantName_RefLastName_Rec_IREx.pdf) by December 4th, 2025, for full consideration.
Full description of the position plus submission guidelines can be found here: https://exoplanetes.umontreal.ca/en/job/2026-trottier-postdoctoral-fellowship/
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| Two PostDoc positions in pipeline development for ESO ELT instruments (University Assistant) ***EXTENDED DEADLINE*** | Closing date: 2025-12-10
Contact: Prof. Norbert Przybilla |
In the framework of our contribution to the ESO ELT instrumentation project for MICADO and METIS we offer two PostDoc positions for the pipeline development
| | ▸ more | University Assistant - PostDoc positions (40 hours/week)
Institute for Astro- and Particle Physics
University of Innsbruck / Austria
Start date/duration:
as soon as possible
for 2 years
Main tasks:
- Independent project work for ESO ELT instrumentation projects (in particular pipeline development)
- teaching courses
- participation in organizational and administrative tasks
Required qualifications:
- Completed doctoral studies in astronomy or physics with a focus on astronomy/astrophysics
- Experience in the research field of astronomy/astrophysics, preferably in observation-oriented astronomy and development of astronomical data reduction software, experience in data acquisition, data reduction in the optical to mid-infrared wavelength range and data analysis of astronomical instruments
- High programming skills in Python and C
- Use of state-of-the-art astronomical software packages
- Knowledge of ESO software standards for data reduction pipelines
- Ability to work in a team with project groups at international level
- Problem-solving skills.
Our offer:
With us, you can expect exciting tasks, flexible working hours, a family-friendly working environment, attractive training and development opportunities, a paid lunch break, a meal allowance and much more!
The minimum gross salary (stipulated by collective agreement) for this position amounts to EUR4.933 per month (14 times, as of 2025).
More general information on the positions and benefits:
https://www.uibk.ac.at/de/personalabteilung/wissenschaftliches_personal/profile/#post-doc
https://www.uibk.ac.at/en/career/additional-benefits/
Application:
We are looking forward to receiving your online application by 10.12.2025 stating the codes MIP-15436 and MIP-15437 via the job portal from the University of Innsbruck:
https://lfuonline.uibk.ac.at/public/karriereportal.details?asg_id_in=15436
https://lfuonline.uibk.ac.at/public/karriereportal.details?asg_id_in=15437
We kindly ask candidates to apply to both positions.
General:
The University of Innsbruck emphasizes equal opportunities and diversity in its personnel policy.
The University of Innsbruck strives to increase the percentage of women and thus expressly encourages women to apply. This is particularly true for leading positions and scientific job offers. In case of under-representation women with the same qualifications will be given priority.
The University of Innsbruck bears the "We are inclusive" seal of approval. We therefore expressly invite qualified individuals with disabilities and/or chronic illnesses to apply.
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| Postdoctoral Position in Astronomical Instrumentation for the PLANETES Project | Closing date: 2025-12-14
Contact: Sylvestre Lacour |
| PLANETES, recently funded by the European Research Council, aims to advance exoplanet science by pushing the limits of the VLT Interferometer (VLTI). | | ▸ more | This instrumental project is directly aligned with the ongoing upgrade of the VLTI infrastructure, including the recent commissioning of GRAVITY+ (https://www.eso.org/public/news/eso2519/). The project addresses technological challenges critical to the next generation of interferometric instruments: development of photonic components for shorter wavelengths; on-sky testing of a new large-format APD detector; and implementation of a novel metrology system to enable microarcsecond astrometry. Over the duration of the project, we plan to validate the concept at the Paranal Observatory in Chile. More details on the project are available here: https://exogravity.obspm.fr/planetes
A postdoctoral position, based at ESO Headquarters in Garching, Germany, is offered to support this project. The successful candidate will focus on the development and validation of the new metrology system while working in close collaboration with the PLANETES team and ESO experts. The postdoctoral researcher will join the research group and report to the PLANETES Project Manager and to the ESO Head of the Office for Science in Garching. The postdoctoral supervisor will be the PLANETES Principal Investigator, Sylvestre Lacour, based at ESO Headquarters in Garching.
The researcher?s main responsibility will be to develop, integrate (at Paranal), and test the new metrology system, including the following tasks:
-Implement a metrology test bench, including installation of an ultra-stable ytterbium laser and integration with long single-mode fibres.
-Demonstrate nanometre-level optical-path measurements and vibration-correction capabilities under realistic conditions.
-Work with VLTI specialists to adapt the bench design into a deployable system for the Paranal Auxiliary Telescopes.
-Specify optical and electronic subsystems and assess operational aspects for long-term deployment.
-Participate in the installation, commissioning, and performance validation of the system at the Paranal Observatory.
-Pursue independent research, preferably in areas related to optical metrology, interferometry, or astronomical instrumentation.
Qualifications and experience
Key competencies and experience include at least three years in the development of instrumentation for optical metrology, long-baseline interferometry, or, more generally, optical instrumentation for astronomy. Required are expertise in operating and handling lasers and optical systems?particularly those related to interferometry?experience in optical assembly, alignment and experimental characterisation, and proficiency in Python for developing analysis and simulation tools for optical instrumentation. Understanding of optical-interferometry principles applied to astronomy is considered an asset.
The successful candidate will hold a completed PhD in astronomy, physics, or optical instrumentation, ideally with a specialisation in optical interferometry, prior to taking up the position. An excellent command of English, both written and spoken, is required.
Contract and benefits
The position is funded for 36 months. The successful candidate will receive a Fellow contract in line with the ESO Fellow stipend rates and benefits as outlined at https://www.eso.org/public/jobs/conditions/fellows/. Please note that a second Fellow contract at ESO through alternative programmes is not foreseen.
Location
The position is based in Garching near Munich, Germany, with duty trips to the Paranal Observatory in Chile.
Application
Applications should include :
-A CV (including personal data, education, skills, and expertise).
-A statement of research interests (maximum two pages).
-A one-page motivation letter titled ?Why I should join the PLANETES project.?
-The names and contact details of three referees, each of whom has agreed to be contacted during the selection process.
Please send the above directly to the project office at planetes.jobs @ sympa.obspm.fr.
Applications must be received by 14 December 2025 midnight. The selection process will begin shortly after the deadline, with interviews expected to take place in January 2026. The starting date is flexible but should be between February and November 2026.
We regard diversity as an asset within a team and welcome applicants with diverse backgrounds and experiences.
For further information, contact: Sylvestre Lacour (sylvestre.lacour @ eso.org).
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| Research Associate in Cosmology and Gravitation (Fixed Term) | Closing date: 2025-12-15
Contact: James Parke |
| Applications are invited for a Postdoctoral Research Associate position in cosmology within the Stephen Hawking Centre for Theoretical Cosmology/GR group at the Department of Applied Mathematics and Theoretical Physics. | | ▸ more | Candidates should be qualified to undertake research in the areas of the CMB, large-scale structure and early universe cosmology. Although all qualified candidates will be considered, we are particularly interested in candidates who can undertake work on higher-order correlators from Simons Observatory CMB data, notably CMB bispectra in combination with other cosmological probes, to gain new insights about inflation and fundamental theory.
The successful candidate will work primarily with Professors James Fergusson and Paul Shellard, as well as academic staff across the Relativity and Gravitation group (Challinor, Gratton, Sherwin, Cranmer, Hartnoll, Moore, Pajer, Reall, Santos, Sperhake, Wall and Warnick) and research staff and PhD students. There are close links with the HEP group and the AI Infosys Lab in DAMTP, and the Kavli Institute for Cosmology (https://www.kicc.cam.ac.uk).
The position is expected to be available on or soon after 1 September 2026, but the start date is flexible. Applicants should have, or be about to obtain, a PhD in a relevant area of theoretical physics, and to have an established track record of original research and experience of working in collaboration.
Duties will include developing and conducting individual and collaborative research objectives, proposals and projects. For data reduction aspects of this project, you will be expected to have computational experience, preferably on HPC systems with knowledge of parallelisation techniques and GPU programming. You will be expected to plan your own research, with guidance if required, and to assist in the preparation of funding proposals. You must be able to communicate material of a technical nature. You may be asked to assist in the supervision of student projects and development of skills and deliver seminars relating to the research area.
Further information about CTC can be found at https://www.ctc.cam.ac.uk and the GR Group at https://www.damtp.cam.ac.uk/research/gr/
Fixed-term: The funds for this post are available for 2 years in the first instance.
Details of how to apply or submit informal enquiries can be found here:
https://www.cam.ac.uk/jobs/research-associate-in-cosmology-and-gravitation-fixed-term-le47448
|
| University of Texas Rio Grande Valley-South Texas Space Science Institute-POSTDOC [#31071, SRGV8615] | Closing date: 2025-12-15
Contact: Joseph Romano |
| The South Texas Space Science Institute (STSSI) at the University of Texas Rio Grande Valley (UTRGV) in Brownsville, TX announces the opening of one postdoctoral appointment in space science research, broadly defined. The successful candidate is expected to actively contribute to and expand the current research activities at UTRGV in space science technology development, gravitational-wave (GW) astronomy, optical and radio astronomy, or experimental GW detector development. | | ▸ more | The STSSI is an interdisciplinary institute with active research in various areas of space and astrophysical science (https://www.utrgv.edu/stssi/). We are particularly interested in hiring creative and motivated candidates who are at ease working both collaboratively and independently in a vibrant, interdisciplinary and synergistic group.
Specifically, we are looking for the strongest possible candidate to collaborate on research projects with members of STSSI in the areas of gravitational-wave astronomy (data analysis or source modeling), optical and radio astronomy, experimental GW detector development, or technology development with space applications. Current experimental research areas within STSSI include phased array development (with applications in spacecraft communication and radio astronomy); testing of materials, electronics, and systems in a simulated space environment; and laser systems for space communication, precision metrology, and gravity gradiometry (including applications for space and ground-based gravitational-wave detectors).
Applicants must have a Ph.D. in Physics or a related field, and a strong interest in leading research efforts as part of STSSI. The postdoc will also have ample opportunity to assist in the supervision of undergraduate and graduate students involved in STSSI research projects.
Appointment is for 2 years with annual renewal contingent upon satisfactory progress and funding status. The anticipated start date of the positions is either Summer or Fall 2026. Applications will be considered until the position is filled. Interested candidates should apply through the job portal (posting number SRGV8615): https://careers.utrgv.edu/postings/49123
Applicants should submit a cover letter, curriculum vitae, and research statement in job portal.
Applicants should also arrange to have three letters of recommendation emailed directly to Dr. Joseph Romano at joseph.romano @ utrgv.edu prior to the application deadline.
Candidates are encouraged to apply as soon as possible. The deadline for full consideration is set for December 15, 2025. This deadline may be subject to extension, if necessary.
For all application related questions, please contact Dr. Joseph Romano at joseph.romano @ utrgv.edu.
Review of applications will start January 15, 2026 and continue until the position is filled.
The University of Texas Rio Grande Valley is an Equal Employment Opportunity/Affirmative Action employer.
It is the policy of The University of Texas Rio Grande Valley to promote and ensure equal employment opportunities for all individuals without regard to race, color, national origin, sex, age, religion, disability, sexual orientation, gender identity or expression, genetic information or protected veteran status.
|
| Fixed-term researcher position on "Dynamics of galaxies at high z" at INAF, Florence, Italy | Closing date: 2025-12-15
Contact: Federico Lelli |
| The Arcetri Astrophysical Observatory (INAF, Florence, Italy) is advertising a fixed-term researcher position for two years, with the possibility of renewal for more years. The successful candidate will work with Dr. Federico Lelli and his research team on the dynamics of galaxies at high z, as well as on other subjects of common interest. | | ▸ more | JOB DESCRIPTION: The successful candidate will study the dynamics of galaxies at high z, analyzing multi-wavelength observations (from ALMA, JWST, and the VLA) and/or comparing them with the predictions from cosmological simulations. In particular, the researcher will join the TRICEPS international collaboration, led by Dr. Federico Lelli (https://www.lellifederico.com/), which is studying a sample of massive galaxies at z=4-5.
INSTITUTE DESCRIPTION: The Arcetri Astrophysical Observatory is part of the Italian National Institute of Astrophysics (INAF). It is located on the Arcetri hill in the surroundings of Florence, near the town where Galileo was exiled and spent the last years of his life. The observatory has strong ties with the Department of Physics and Astronomy of the University of Florence and hosts a large international group working on galaxies and cosmology (see https://sites.google.com/inaf.it/exagal). The observatory also hosts research groups working on star formation, stellar evolution, exoplanets, Solar System, high-energy astrophysics, and instrumentation. The observatory is very active in outreach and education.
SALARY AND BENEFITS: The researcher position is at the same entry level of a permanent INAF researcher (gross salary of 38465/year) and comes with extra benefits, such as full access to the Italian public healthcare system, pension funds, maternity/paternity leave, parental leave, and more.
ELIGIBILITY: By Italian law, to apply to this type of position, the candidate must (1) be a citizen of the European Union (EU), or (2) be a relative of citizens of the EU so that the candidate is eligible for a permanent residence permit, or (3) hold a long-term residence permit in the EU by the application deadline, or (4) have the legal status of refuge or subsidiary protection.
In addition, by the application deadline, the candidate must hold a PhD in Astronomy or Physics, or have three years of documented research expertise after the M.S. degree.
REQUESTED EXPERTISE: The following expertise will be assessed by the selection committee: (1) general knowledge of models of galaxy formation and evolution; (2) knowledge of analysis techniques of radio/submm interferometric data and/or optical/NIR photometry and/or optical/NIR spectroscopy; (3) knowledge of analysis techniques of cosmological simulations of galaxy formation and evolution; (4) knowledge of numerical techniques and/or software to model galaxy dynamics.
HOW TO APPLY: The application must be sent by the deadline of 23:59 CET on 14 December 2025 using the PICA webportal (https://pica.cineca.it/login). For technical and/or practical help, it is highly recommended to contact Federico Lelli (federico.lelli @ inaf.it). Basic guidelines:
After registering to the webportal, use the following code: 2025INAFRIC-OAA-Triceps-012. On the webportal, complete all parts and upload the following documents:
(1) Curriculum vitae (CV)
(2) Research statement (max 5 pages, font 12 pt, single line spacing)
(3) Full list of publications
(4) Five top publications that the committee will individually evaluate (the candidate may either upload the pdf files of the published papers, or a list with active weblinks to the papers)
For legal reasons, the CV of the applicant must be signed and report the following statement at the end:
"Le informazioni contenute nel presente "curriculum vitae et studiorum" sono rese sotto la personale responsabilità del sottoscritto, ai sensi degli articoli 46 e 47 del Decreto del Presidente della Repubblica 28 dicembre 2000, numero 445, e successive modifiche e integrazioni, consapevole della responsabilità penale prevista dall'articolo 76 del medesimo Decreto per le ipotesi di falsità in atti e/o dichiarazioni mendaci."
After providing the requested information and uploading the requested documents on the portal, the applicant must either (1) electronically sign the application using a certified software, or (2) save a pdf copy of the full application, sign it, and upload the signed pdf copy on the portal together with a copy of a valid document (ID card or passport).
CONTACTS: For any information (scientific and/or technical) send an email to federico.lelli @ inaf.it
|
| Assistant Professor in Astrophysics | Closing date: 2025-12-15
Contact: Director - HR |
| Manipal Academy of Higher Education (MAHE), Manipal an Institution of Eminence Deemed to be University invites applications from potential candidates across the globe for faculty position at Manipal Centre for Natural Sciences (MCNS), Centre of Excellence, Manipal, a constituent unit of MAHE, Manipal. | | ▸ more | Candidates with strong research experience in astrophysics are encouraged to apply. Experience with multiwavelength observations, astronomical data analysis, astronomical instrument design and development, would be highly desirable. The MCNS research group in Astrophysics is particularly seeking candidates with experience in one of the following areas: accretion in compact binary systems, physics of active galactic nuclei and sun and solar system physics.
Successful candidates will join the astrophysics research team at MCNS, working with students and postdocs. Since MCNS does not have large astronomical observational facilities, they are encouraged to make maximal
use of national and international facilities in pursuit of their research.
For more details, visit: https://manipal.edu/mcns-manipal.html
Eligibility:
- Minimum of 3 years of Post-Doctoral experience at a reputed institution and an excellent publication record.
- Teaching experience at the postgraduate level, mentoring research students and demonstrated ability to write successful proposals for external research grants, will be accorded additional weightage.
The subject field in the email must contain: ASSISTANT PROFESSOR - MCNS
Eligible candidates may apply with a detailed CV, Statement of Research and copies of certificates in support of qualification, experience and research publications via email on or before Dec 15th 2025 to jobs @ manipal.edu
Director - HR
Manipal Academy of Higher Education (MAHE)
Madhav Nagar, Manipal 576104, Karnataka, India
e-mail: jobs @ manipal.edu
Phone: +91 820-2923433
|
| 2year postdoctoral position in the observations of exoplanet atmospheres at high and low resolution in Toulouse - France | Closing date: 2025-12-18
Contact: Florian Debras |
| 2-years funding for a postdoctoral position in Toulouse, France dedicated to exoplanet atmospheres, starting between November 2025 and March 2026. The post doctoral research will gather archival data and perform new observations of a small sample of exoplanet atmospheres with SPIRou in order to understand as precisely as possible the multi dimensional structure of exoplanet atmospheres. | | ▸ more | | The first goal of this post doctoral position is to gather the archival data from high and low resolution observation of exoplanet atmospheres for 3/4 planets, and provide the best constraints possible by combining observations from all available sources. The second goal is to prepare and plan the observations of these targets with SPIRou @ CFHT, in the context of the PLANETS large program, that was allocated 280 nights of observation over two years. This position is provided in the context of the Exo-ATMO ANR-funded proposal, and includes travel for national and international conferences and buying a computer if need be. It will be complemented by a PhD student working jointly with the post doctoral researcher on exploiting the data to provide 3D constraints on the selected exoplanet atmospheres.
|
| 2 year postdoctoral position in the observations of exoplanet atmospheres at high and low resolution | Closing date: 2025-12-18
Contact: Florian Debras |
| 2-years funding for a postdoctoral position dedicated to gathering archival data and performing new observations of a small sample of exoplanet atmospheres with SPIRou in order to unlock the multi dimensional barrier. | | ▸ more | | The first goal of this post doctoral position is to gather the archival data from high and low resolution observation of exoplanet atmospheres for 3/4 planets, and provide the best constraints possible by combining observations from all available sources. The second goal is to prepare and plan the observations of these targets with SPIRou @ CFHT, in the context of the PLANETS large program, that was allocated 280 nights of observation over two years. This position is provided in the context of the Exo-ATMO ANR-funded proposal, and includes travel for national and international conferences and buying a computer if need be. It will be complemented by a PhD student working jointly with the post doctoral researcher on exploiting the data to provide 3D constraints on the selected exoplanet atmospheres.
|
| Postdoctoral position in interacting binary stars | Closing date: 2025-12-20
Contact: Viktoriya Momchilova |
| We invite applications for a postdoctoral research position within the ERC-funded program 2SStars - The Role of Binary-Stripped Stars: from Atomic Scales to Cosmic Dawn. The postdoc will join an active research team led by Dr. Ylva Götberg (www.ylvagotberg.com) at the Institute of Science and Technology Austria (ISTA). | | ▸ more | Application Deadline: 23:59 CET, December 20, 2025
We invite applications for a postdoctoral research position within the ERC-funded program 2SStars - The Role of Binary-Stripped Stars: from Atomic Scales to Cosmic Dawn. The postdoc will join an active research team led by Dr. Ylva Götberg (www.ylvagotberg.com) at the Institute of Science and Technology Austria (ISTA). Our group uses both observational and computational approaches to investigate the physics of envelope-stripped stars. We explore how stripped stars can be used to understand binary interaction, gravitational wave and supernova transients, stellar interiors, and sources of ionizing radiation. We maintain strong international collaborations, and the postdoc will be encouraged to engage in these and expand their scientific network.
We particularly welcome applicants with expertise in hot star spectral modeling, binary population synthesis, nebular spectral modeling, or in designing and planning observational surveys. We seek candidates who are motivated by the science of envelope-stripped stars and eager to contribute creatively to the field of interacting binaries. We are committed to fostering an inclusive, supportive, and respectful research environment. We welcome applications from scientists of all backgrounds and identities, and we particularly encourage individuals from underrepresented or historically marginalized groups in astronomy to apply.
The expected starting date is September 2026 (flexible) and the position is for two years. The position includes funds available for necessary equipment purchases, travel resources, and publication costs. It is a fully paid employment contract with standard benefits, including health care, paid leave, and social security coverage.
Your profile:
- PhD in Astrophysics completed within the past 5 years
- Background in stellar astrophysics research; theoretical, computational or observational
- (Preferred qualifications) Experience with hot star research and binary evolution
Application documents:
- Cover letter detailing your interest and how you meet the criteria for this position (max 1 page)
- Research statement outlining your past and current research (max 3 pages)
- CV
- Publication list
- List of three referees that may be contacted for reference letters
To submit your application please email: Viktoriya.Momchilova @ ista.ac.at
Give the email the subject 'Application, Postdoc in Interacting Binaries' and attach your documents as one combined PDF labeled by your surname (e.g., SURNAME_interacting_binaries.pdf).
For questions regarding the position, please send an email directly to both Ylva Götberg (Ylva.Gotberg @ ista.ac.at) and Viktoriya Momchilova (Viktoriya.Momchilova @ ista.ac.at).
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| Warwick PhD Prize Scholarships in Astrophysics | Closing date: 2025-12-31
Contact: Warwick Astronomy Admissions Team |
The University of Warwick's Astronomy & Astrophysics group is seeking talented PhD applicants for our Warwick PhD Prize Scholarships in Astrophysics. Applications are due by January 13th, 2026.
The scholarships are open to national and international applicants and all are welcome to apply. All successful applicants will have a full stipend plus allocations for travel and computing.
All projects are here: https://warwick.ac.uk/fac/sci/physics/research/astro/postgraduate_phd/ and our Frequently Asked Questions are here: https://warwick.ac.uk/fac/sci/physics/research/astro/postgraduate_phd/faq/ | | ▸ more | Potential projects span a wide range of research areas including transients and explosive astrophysical phenomena, stellar populations, white dwarfs and planetary remnants, protoplanetary and debris discs, and exoplanet discovery, characterisation and evolution.
Applicants are encouraged to contact the project supervisors for further information on the projects here: https://warwick.ac.uk/fac/sci/physics/research/astro/postgraduate_phd/
Warwick is an internationally recognised centre of research excellence. Our group takes leading roles in many major ground and space-based projects, including the Gravitational-wave Optical Transient Observer (GOTO), Sloan Digital Sky Survey (SDSS), PLAnetary Transits and Oscillations of stars (PLATO) telescope, Next Generation Transit Survey (NGTS), CHaracterising ExOPlanet Satellite (CHEOPS), WHT Enhanced Area Velocity Explorer (WEAVE) spectrograph, 4-metre Multi-Object Spectrograph Telescope (4MOST), and Dark Energy Spectroscopic Instrument (DESI).
We also run state-of-the-art computer simulations to develop theoretical models using the university's modern super-computing facilities, and are experts in the exploration of large and heterogenous data sets, adopting novel techniques including machine learning.
The Astronomy & Astrophysics group is part of the Physics Department at Warwick; both the department and the university hold Athena SWAN Silver awards, a national initiative to promote gender equality for all staff and students. The Physics Department is also a Juno Champion, which is an award from the Institute of Physics to recognise our efforts to address the under-representation of women in university physics and to encourage better practice for all. The Astronomy & Astrophysics group also hosts monthly equitea forums to break down barriers faced by all under-represented groups in science: https://warwick.ac.uk/fac/sci/physics/research/astro/seminars/equitea/
Warwick is an excellent place to begin your scientific career, where you will be exposed to a wide range of research topics. You will be immersed in a friendly, collaborative and supportive environment with over 30 fellow astronomy PhD students, working with and learning from experts in very different areas. Personal development is a priority, and incoming PhD students will be invited to join our network of international collaborators, lead projects, and present their work on an international platforms.
More information about the Warwick Astronomy & Astrophysics Group can be found here: https://warwick.ac.uk/fac/sci/physics/research/astro/ and more information about the local area can be found here: https://nam2022.org/warwick/local-area
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| Postdoctoral position in cosmology and machine learning | Closing date: 2026-01-01
Contact: Guilhem Lavaux |
| Applications are invited for a postdoctoral position in large-scale-structure cosmology at the Institut d'Astrophysique de Paris (IAP). The group is tightly connected to the Euclid survey and leads several of its key analyses. The Large-Scale Structure group notably develops state-of-the-art Bayesian inference and machine-learning tools for interpreting large-scale-structure data. | | ▸ more | Applications are invited for a postdoctoral position in large-scale-structure cosmology at the Institut d'Astrophysique de Paris (IAP). The IAP, located in central Paris, is an internationally recognised centre for fundamental research in astrophysics, cosmology and high-performance computing. The institute comprises about 150 researchers, engineers, technicians, administrative staff, postdoctoral researchers and PhD students. It is tightly connected to the Euclid survey and leads several of its key analyses. The Large-Scale Structure group notably develops state-of-the-art Bayesian inference and machine-learning tools for interpreting large-scale-structure data.
The successful candidate will join this vibrant team to develop and apply simulation-based Bayesian and AI methods for the scientific exploitation of Euclid early-data releases, in particular galaxy clustering, and to produce synthetic galaxy catalogs. The position is a 36-month fixed-term contract (full-time) with a negotiable start date that must occur before the end of 2026. The gross monthly salary ranges from 2800 euros to 3500 euros, depending on qualifications.
The working language of the team is English. Applicants must hold a PhD in physics, astrophysics or a closely related field and have no more than three years of post-doctoral experience (or equivalent research experience). We seek candidates with strong expertise in cosmology, Bayesian statistics and/or data-driven methods, and excellent scientific writing and presentation skills in English. Experience with high-performance computing or machine learning is a plus.
Please submit a CV, cover letter, list of publications, an approximately three-page research proposal and up to three letters of recommendation via the online portal: https://shlink.aquila-consortium.org/postdoc-iap-apply. The letters must be uploaded through https://shlink.aquila-consortium.org/postdoc-iap-1. Direct any enquiries to Guilhem Lavaux (guilhem.lavaux @ iap.fr) and Florent Leclercq (florent.leclercq @ iap.fr).
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| ELT Programme Scientist | Closing date: 2026-01-15
Contact: Evelina Dietmann |
| The ELT Programme Scientist provides the overall scientific leadership for the ELT and its suite of instruments. The role encompasses all scientific aspects of the ELT Construction Programme, covering the telescope itself, and the development of its instruments under the ESO Instrumentation Programme. | | ▸ more | A key responsibility is to ensure strategic and scientific alignment between these two programmes. The Programme Scientist is charged with developing strategies to maximize the scientific performance of both the telescope and its instruments currently under development, shaping plans for future instrumentation, advising operations, and overseeing telescope and instruments commissioning and science verification. In addition, the Programme Scientist serves as the primary interface between the ELT, the instrument Consortia, and the broader user community. By closely monitoring the evolving scientific priorities of the community within the rapidly advancing landscape of astronomical facilities projected for the 2030s and beyond, the Programme Scientist ensures that the ELT delivers world-leading optical and infrared capabilities to drive major astrophysical discoveries. We are seeking an experienced senior scientist with a strong technical background to provide authoritative scientific leadership and advice across both the ELT telescope Construction and Instrumentation Programmes, in coordination with the other ESO Programme Scientists (VLT, VLTI, ALMA, CTA) to enable scientific synergies.
Main Duties and Responsibilities:
-Provide scientific leadership to the ELT Construction Programme and ensure that the telescope will be scientifically exploited to the best of its capabilities;
-Guide the scientific development of ELT instruments through sound scientific leadership within the ESO Instrumentation Programme, helping ensure they meet their science goals;
-Act as a strategic and scientific connector between the Telescope and its suite of Instruments across both Programmes, ensuring that their combined performance offers the highest possible scientific return;
-Oversee and maintain the ELT Observatory Top Level Requirements, working closely with the ELT Construction Programme Manager to ensure these are integrated throughout the construction phase;
-Collaborate closely with the Instrumentation Programme Manager to maintain, evolve and develop the ELT Instrumentation Plan;
-Provide advice to the Instrumentation Programme Manager to ensure that the necessary design trade-offs made on the Programme are carried out within an appropriate science-driven context. Provide science-based guidance on design decisions, helping to set clear and balanced scientific priorities in this context;
-Lead the scientific verification of the telescope performance and the commissioning and science verification of the instruments;
-Engage with the Community to optimise the usage of ESO optical and near-infrared telescopes, together with other ESO Programme Scientists;
-Prepare and give briefings to communicate progress and challenges to ESO governing bodies and committees as needed;
-Inform the Director for Science about ELT developments, challenges and scientific productivity;
-Support public engagement and outreach, in collaboration with the Communication Department, helping make the scientific goals and results of the ELT and its instruments accessible and inspiring to a diverse audience.
As a member of the ESO Astronomy Faculty, the ELT Programme Scientist is expected and encouraged to conduct an active astronomical research programme on a 50/50 basis.
Key Competences and Experience:
Essential Competences and Experience
-Ability to think strategically, taking a long-term perspective and openness to new ideas, challenges and anticipating future needs or trends;
-Experience in supporting and leading geographically dispersed, multicultural and interdisciplinary teams, with an inclusive and respectful approach to team dynamics;
-Experience collaborating to develop shared visions and scientific strategies for the future, both within ESO and the wider astronomical community;
-In-depth knowledge of astrophysical instrumentation, along with experience in facility commissioning and operations;
-Ability to inspire and support others, fostering a positive and motivating team environment;
-Strong written and oral communication skills, with the ability to present complex ideas clearly and constructively, and to facilitate informed decision-making;
-A proactive approach to constructively suggest improvements to established ways of working to create positive change;
-Excellent communication and diplomatic skills, allowing to effectively communicate and establish trust at all levels within the organization, the instrument Consortia and with the community;
-A strong record of personal research achievements, demonstrating international recognition appropriate to the career stage in optical and near-infrared astrophysics research;
-Willingness to spend considerable time in Chile during ELT Commissioning.
Desirable Competences and Experience
-Experience in project leadership including familiarity with project management principles and/or experience contributing to complex, multi-stakeholder scientific projects;
-Experience in community liaison and/or community leadership;
-Understanding of science policy, funding structures, or strategic planning in large-scale research organisations;
-Ability to navigate between technical, scientific, and organisational priorities, and to find common ground among diverse perspectives;
-Experience with the ELT and its operational aspects.
Qualifications:
PhD in astronomy, physics or equivalent.
Language skills:
The position requires a full working knowledge of English, both oral and written.
If you are interested in working in areas of frontline science and technology and in a stimulating international environment, please visit http://www.eso.org for further details.
Applicants are invited to apply online at http://jobs.eso.org. (further details are available on the ESO career portal)
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| ERC-funded postdoctoral position in computational binary star astrophysics | Closing date: 2026-01-25
Contact: Ondrej Pejcha |
| We invite applications for postdoctoral position in the area of computational binary star astrophysics in the research group of Dr. Ondrej Pejcha. | | ▸ more | The successful candidate will pursue original research using multi-dimensional simulations of binary stars, contribute to code development, and engage in the group's scientific activities with optional opportunities to mentor students.
We encourage candidates with diverse research profiles, from broadly interpreted astrophysical theory to computational tool development to apply. Experience with hydrodynamics in astrophysics, especially stellar convection, turbulence, and magnetohydrodynamics, is advantageous but not required. Applicants must have a PhD in astronomy, computational physics, or a related field by the start date of the appointment.
The research group has access to a dedicated computer cluster, which will be soon expanded with new nodes. The group has been successful in applying for time on national supercomputing infrastructure with postdocs and students leading the proposals. The group is connected to observational efforts in time-domain astronomy. Group website is at https://utf.mff.cuni.cz/~pejcha/
The positions are financed from ERC Consolidator grant "ROGALLO". The position will be initially awarded for one year, but extensions up to a total of five years are possible given mutual interest and satisfactory performance. Funds for travel and invitation of guests are available. Informal inquiries are welcome (ondrej.pejcha @ matfyz.cuni.cz).
Full employee benefits provided by the Czech state and Charles University: health insurance (no or very small co-pays), 25 vacation days, 5 personal development days, contributions to state pension fund, subsidized meals, parental leave, discounts for sports & wellness, Czech language classes, etc.
Please submit CV, list of publications, and statement on past research and future interests to ondrej.pejcha @ matfyz.cuni.cz by the application deadline and with the reference code ROGALLO26PD in Subject. Please make sure that 3 recommendation letters sent directly by the referees are received at the same email address by the deadline. The position will remain open until filled.
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| Professor in Planetary Sciences | Closing date: 2026-01-31
Contact: Prof. Dr. Christoph Mordasini |
The Division of Space Research and Planetary Sciences of the Physics Institute, University of Bern, Switzerland, invites applications for a full-time position as a Professor in Planetary Sciences.
The Division is a leading institute in space research and is looking for a Professor of Experimental Physics in the field of planetary science for Solar System exploration. The initial level of tenure can range from assistant professor tenure track to full professor depending on qualifications (open rank). | | ▸ more | We invite applications from candidates who conduct outstanding research, teaching, mentorship, and leadership in any area of experimental planetary science. Areas of research could include, but are not limited to, the properties, origin and evolution of planets and minor bodies in the Solar System, the search for and emergence of life beyond Earth, the composition of surfaces and atmospheres, ongoing physical and chemical surface and sub-surface processes and the evolution of planetary interiors. A diverse spectrum of approaches and methodologies is welcome, including, but not limited to, the analysis and modelling of space probe datasets, instrumentation and flight hardware development, experimental, observational and laboratory techniques, comparative planetology or the involvement, development and leadership in space missions.
The successful candidate's research program will constitute a defining part of the Division's research activities. It will complement existing research initiatives locally and within the Swiss and international landscape. The successful candidate will become a member of the faculty of science and of the Division directorate, playing a vital role in a large and dynamic Division that is strongly engaged in research, education, and outreach programs.
The Division values internationality and boasts a longstanding tradition in planetary research and space missions. It provides excellent conditions in terms of infrastructure like laboratories, engineering and manufacturing capabilities to build space-grade hardware, but also through a rich and vibrant scientific environment that includes the Division, the interdisciplinary Center for Space and Habitability of the University of Bern, and the International Space Science Institute in Bern.
We anticipate an excellent academic record including the successful acquisition of third-party funds, a strong international network in space research, as well as excellent social skills. We seek suitable candidates who have the potential and/or skills in transformational leadership and who foster a conducive research culture. The successful candidate will also possess a strong record and/or commitment to excellence in teaching, advising and mentorship.
Candidates are expected to hold a PhD in planetary sciences, physics, geophysics, astrophysics or a related field. In line with its commitment to fostering an inclusive academic environment, the University of Bern actively seeks to increase the proportion of women and other underrepresented groups in leadership positions. We warmly encourage such candidates to apply. Applications involving job sharing or part time will be considered. As a signatory of the DORA declaration, the University applies its principles to ensure fair and transparent recruitment.
The University of Bern provides a comprehensive set of research, teaching, and grant application support services. It offers attractive working conditions with various support mechanisms, like family assistance, personal coaching, and career development. The University is situated in a central location within the city of Bern which is renowned for its high quality of life. An attractive salary package and organisational retirement plan are provided by the renumeration scheme of the Canton of Bern. Extensive relocation support, onboarding assistance, and a start-up package are available to facilitate the transition into academic and personal life in Switzerland and the initiation of new research projects.
Applications should include:
- Letter of motivation (max. 3 pages)
- Curriculum Vitae (max. 5 pages)
- List of publications
- List of courses taught (max. 2 pages)
- List of third-party funds raised (max. 1 page)
- DEI-statement outlining past and planned future contributions (max. 1 page)
- Research plan for the first 5 years (max. 10 pages excluding references)
The application documents should be submitted by 31 January 2026 electronically in a single PDF file to the Dean's Office (email: applications.natdek @ unibe.ch), including the completed online questionnaire which can be found here: https://www.space.unibe.ch/about_us/open_positions/index_eng.html
For inquiries, please contact Prof. Christoph Mordasini, Executive Director of the Division of Space Research and Planetary Sciences (jobs.space @ unibe.ch).
https://www.space.unibe.ch
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| Postdoctoral position on modeling magnetic topologies of M dwarfs at IRAP / Toulouse France | Closing date: 2026-01-31
Contact: Jean-Francois Donati |
| We invite applications for a 2-3yr postdoc position on modeling magnetic fields of M dwarfs at the Institut de Recherche en Astrophysique et Planétologie (IRAP) located in Toulouse, France, within the SPIRou science consortium coordinated by Drs JF Donati and C Moutou in Toulouse. | | ▸ more | This project aims at modeling the evolving magnetic topologies of M dwarfs, monitored with the SPIRou near-infrared spectropolarimeter at the Canada-France-Hawaii Telescope since 2019 in the framework of the SPIRou Large Programs. More specifically, the goal is to exploit an advanced version of Zeeman-Doppler imaging incorporating temporal evolution, to the existing and future SPIRou data collected for a few tens of M dwarfs of various masses, to infer fresh constraints on the dynamo processes operating in largely and fully convective stars. The work will take place at IRAP with Drs JF Donati and C Moutou, starting Q1 2026.
The candidates must have a solid background in stellar magnetic fields and spectropolarimetry, to efficiently analyse data sets collected with SPIRou using the tomographic technique of Zeeman-Doppler imaging, and to reconstruct the parent magnetic topology at the surface of the star. Experience in velocimetry is also welcome.
The candidates should provide the following documents (PDF only, accessible via a file server) by 2026 Jan 31 :
* a motivation letter (max 2 pages),
* a description of past and current research statements (max 5 pages),
* a CV (max 2 pages)
* a publication list,
* 3 reference letters to be sent directly by the mentors (same deadline)
to Drs JF Donati (jean-francois.donati @ irap.omp.eu) and C Moutou (claire.moutou @ irap.omp.eu). Short-listed candidates will be invited for an on-line interview ~2 weeks after the deadline.
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