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| Postdoctoral Position in Extragalactic Astrophysics at the University of Geneva | Closing date: 2026-09-06
Contact: Romain Meyer |
| We invite applications for a postdoctoral research position focused on the Epoch of Reionisation at the Department of Astronomy at the University of Geneva. The successful applicant will work on observational studies of the intergalactic medium at z>5 and galaxies/AGN in the epoch of reionisation in a new group led by Romain Meyer. | | ▸ more | The postdoctoral position will focus on observations of the IGM opacity and the ionising output of high-z galaxies, leveraging several PI-led JWST programmes (e.g. #7208, #11371) and VLT data (FORS2, MUSE, MOONS). The candidate will have the opportunity to conduct independent research for a fraction of their time, with access to large JWST collaborations (COSMOS-3D, FRESCO, EREBUS, JWST-OutThere) and access the VLT/MOONS and ELT/MOSAIC Consortia. The team will be initially composed of one postdoctoral researcher and two PhD students.
The position is initially for two years, with the possibility of extension for one year depending on funding and performance.
Computer equipment, travel funding and access to local HPC infrastructure is included.
The Department of Astronomy at UNIGE in Switzerland carry out research in the fields of extra-solar planets, stellar physics, high energy astrophysics, galaxy evolution and dynamics, and observational cosmology, providing a rich and vibrant research environment. Geneva is one of the most international and multicultural cities in Europe with a high quality of living, with the stunning Swiss/French Alps and Lake Geneva in close proximity.
Candidates should hold a PhD in Astrophysics or in a related field by the start of the position. We seek experience with JWST and/or VLT spectroscopy, and a solid background in high-redshift galaxies and/or IGM studies. Experience with simulation-based inference and Hierarchical Bayesian modelling is an asset. The successful applicant will become part of a dynamic environment and we especially look for team players with a high level of independence, reliability and scientific creativity.
Start date: Early 2027 (to be discussed).
We offer a competitive salary in agreement with the State of Geneva public sector and UNIGE standards.
Benefits include: Standard Swiss Social Security, Accident Insurance and Pension contributions, 30 day annual leave and special leave (maternity/paternity, etc..) in accordance with institutional standards.
The University of Geneva is an equal-opportunity employer and strongly encourages applications from candidates of all backgrounds.
The following application materials should be sent to Romain Meyer (romain.meyer @ unige.ch) by September 6, 2026 in a single PDF:
- A cover letter (1 page), including a statement on the AI use in drafting this application.
- A curriculum vitae (max. 4 pages).
- A list of publications
- A short research statement describing past achievements and future projects (max. 3 pages)
Additionally, the candidate should arrange for two letters of recommendation to be sent by September 6, 2026 to Romain Meyer (romain.meyer @ unige.ch).
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| PhD Position in Extragalactic Astrophysics at the University of Geneva | Closing date: 2026-09-06
Contact: Romain Meyer |
| We invite applications for a 4-year PhD position focused on the Epoch of Reionisation at the Department of Astronomy at the University of Geneva. The successful applicant will work on novel observational studies of the intergalactic medium at z>5 and the nature of the sources of reionisation in a new group led by Romain Meyer. | | ▸ more | The team will be initially composed of one postdoctoral researcher and two PhD students. The PhD position will leverage new JWST spectroscopy of galaxies in deep extragalactic fields and/or VLT observations from MUSE and the new-generation MOONS instruments. The candidate will be part of international JWST collaborations (COSMOS-3D, FRESCO, EREBUS, JWST-OutThere) and the MOONS Consortium.
The position is fully funded for 4 years. Computer equipment, travel funding and access to local HPC infrastructure is included.
The Department of Astronomy at UNIGE in Switzerland carry out research in the fields of extra-solar planets, stellar physics, high energy astrophysics, galaxy evolution and dynamics, and observational cosmology, providing a rich and vibrant research environment. Geneva is one of the most international and multicultural cities in Europe with a high quality of living, with the stunning Swiss/French Alps and Lake Geneva in close proximity.
Candidates should hold a Master degree in Astrophysics or in a related field (by the start of the PhD position), with some experience in research and Python. A background in extragalactic studies (especially JWST or VLT spectroscopy) is an asset. The successful applicant will become part of a dynamic environment and we especially look for team players with a high level of reliability and motivation to learn quickly.
Start date: January 2027 (negotiable).
We offer a competitive salary in agreement with the State of Geneva public sector and UNIGE standards.
Benefits include: Standard Swiss Social Security, Accident Insurance and Pension contributions, 30 day annual leave and special leave (maternity/paternity, etc..) in accordance with institutional standards.
The University of Geneva is an equal-opportunity employer and strongly encourages applications from candidates of all backgrounds.
The following application materials should be sent to Romain Meyer (romain.meyer @ unige.ch) by September 6, 2026, in a single PDF file:
- A cover letter (1 page max) detailing your academic background and the motivation for seeking a PhD in Astrophysics, as well as the contact details of two scientists willing to provide letters of recommendation (letters will be requested at a later stage).
- A short statement (1 page max) on your research experience so far, including a statement on the AI use in drafting this application.
- A curriculum vitae (max. 2 pages)
- A copy of Bachelor and Master academic record (exams & theses grades)
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| SKA-Mid Senior Operations Scientist | Closing date: 2026-09-14
Contact: Heather |
An ideal role for a radio astronomer with Observatory experience who is keen to contribute to, and play a leadership role in, the operational planning and Science Verification of the SKAO.
For more information and to apply, follow this link: https://recruitment.skao.int/vacancy/skamid-senior-operations-scientist-616343.html | | ▸ more | The SKAO Science Operations group is seeking to employ a talented and experienced SKA-Mid Senior Operations Scientist to join our team based at the SKAO Science Operations Centre in Cape Town, South Africa.
With SKA-Mid now in the construction and commissioning phases, planning for the operations of the SKA has entered an exciting phase. In order to support our planning, this role will play a key part in establishing the operational foundation of a world-leading radio astronomy facility. The successful candidate will have broad operational experience and we are seeking a scientist with substantial experience in the operation of astronomical facilities and a strong understanding of radio astronomy instrumentation, data processing and scientific analysis. Equally important is experience supporting a diverse user community and translating scientific requirements into effective operational practices.
The successful candidate will have the inclusive and collaborative leadership skills needed to successfully build, manage and develop a small team of operations scientists. Furthermore, the successful applicant will be comfortable balancing strategic planning with operational delivery, working across organisational boundaries, and coordinating activities involving scientific, engineering and software teams.
SKAO is working in partnership with SARAO for the construction and operation of the SKA-Mid Telescope, and this role will also interact with the SARAO MeerKAT Science Operations Team and support the coordination of activities on both telescopes under a joint team.
The appointee will be encouraged to carry out research up to 25% of employed hours. Appropriate support, including conference travel, will be provided.
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. These roles may be offered on a full-time, part-time or job share basis. Please raise your preference in your application.
Due to the locations involved in the SKA project, in particular the UK and Australia, 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. It will also require some domestic travel to the Karoo Site and occasional international travel.
Informal enquiries may be made to Shari Breen, SKAO Head of Science Operations and acting SKA-Mid Head of Science Operations (shari.breen @ skao.int).
Key Responsibilities
Under the direction of the SKA-Mid Head of Science Operations, the successful candidate will support the future science operations of the SKAO by:
-Recruit and manage a high performing and inclusive team of operations scientists, ensuring their continual development while motivating and mentoring staff to meet the current and future requirements of the Observatory;
-Provide input into the strategic direction of the SKA-Mid Science Operations team to support the SKAO in the delivery of an efficient and effective science program;
-Collaborate closely with the SARAO Science Operations team;
-In collaboration with the SKAO Head of Science Operations and the Global Science Operations team, contribute to the development and continual refinement of the Mid operations, commissioning and science verification plans, and in defining the requirements for early array releases and test procedures;
-Support the implementation of the SKA-Mid Science Verification and Operations plans, as the arrays are handed over from construction to operations;
-Effectively interface with the SKA user community, promote SKAO activities, gather community feedback, influence where appropriate, and facilitate appropriate support through the SKAO Helpdesk and other activities;
-Support the development of software needed to operate the SKA telescopes or necessary for the SKA user community;
-Effectively collaborate with SKA staff across the three sites (i.e. some travel to the SKAO telescope sites in Australia and/or South Africa will be necessary);
-Communicate openly, effectively and respectfully with internal and external stakeholders;
-Optionally undertake a programme of personal research up to 25% of employed hours;
-Undertake other duties as directed by the SKA-Mid Head of Science Operations.
Mandatory Knowledge
The post holder will have:
-A University PhD degree in Astronomy, Physics, Engineering, another closely related and relevant field, or equivalent qualification.
-Demonstrated ability to lead and manage a small team, fostering an inclusive and high-performing culture while effectively managing competing priorities, resources and deadlines in a dynamic operational environment.
-Demonstrated experience in scientific facility operations and user support, including translating user requirements into effective operational practices.
-Demonstrated ability to engage and influence diverse stakeholders, including scientists, engineers and external partners, through strong written and verbal communication skills.
-Expertise in radio astronomy techniques including in the acquisition, reduction and analysis of astronomical data.
-An awareness of, and commitment to, equitable practices, including accessibility, to facilitate broad access to the observatory.
Desirable Knowledge
-Expertise across a breadth of radio astronomy techniques, including one or more of, e.g. spectral line, Very Long Baseline Interferometry, beamforming techniques and/or time domain science (pulsars, fast transients).
-An appreciation and understanding of the science cases motivating the SKA Observatory.
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| CTAO and Synergy Programme Scientist | Closing date: 2026-09-15
Contact: Evelina Dietmann |
| The CTAO and Synergy Programme Scientist will provide scientific leadership for ESO's participation in CTAO. In return for the effort to operate CTAO-S, ESO will have 10% of the open time on the northern and southern arrays. They will also be responsible for optimising the multi-wavelength/multi-messenger use across ESO's facilities and with other leading facilities. | | ▸ more | The Programme Scientist is responsible for developing and maintaining a strategic vision for multi-wavelength synergistic use of ESO facilities, including advising on and developing strategic partnerships with other astrophysical facilities both ground based, and in space. In particular, the Programme Scientist is responsible for maintaining a strategic scientific vision for CTAO and contributing to ESO's overall policy and long-term planning. They maintain professional contacts at the highest level outside the Organisation and, as postholder, will be assigned to the role for the full duration of the CTAO Programme. In addition, the Programme Scientist serves as the primary interface between CTAO and the broader ESO user community.
The Programme Scientist works closely with colleagues across the Directorate for Science (DSC) to ensure synergies with ESO's existing facilities and the optimal scientific use of ESO's share of observing time on CTAO in support of the Programme's goals. They will closely monitor the evolving scientific priorities of the community within the rapidly advancing landscape of astronomical facilities projected for the 2030s and beyond and foster broad community engagement in planning for the best multi-wavelength/messenger use of ESO's facilities, identify emerging scientific areas, and promote synergetic use of ESO's facilities through working groups, community days, and workshops, in close coordination with the Offices for Science. They also monitor and assess the scientific effectiveness of multi-wavelength use of ESO's facilities, developing strategies to maximise its impact and establishing best practices for both scientific capabilities and operations.
Strong coordination with CTAO is essential. In collaboration with the Communications Department, the Programme Scientist identifies and promotes key science drivers and results. They also work closely with the Observing Programmes Office, particularly for initiatives such as multi-telescope time allocation processes, and the promotion of large surveys and synergies with other ESO facilities, including ALMA.
Together with the Director for Science and other Programme Scientists, they contribute to shaping the Organisation's scientific strategy and play an active role in decisions affecting the capabilities of current and future facilities. The CTAO and Synergy Programme Scientist reports regularly to the ESO Advisory and Governing Bodies, principally on CTAO.
Main Duties and Responsibilities:
-Work with the VLT, VLTI, ALMA and ELT Programme Scientists to ensure that scientific synergies between the facilities are identified and propose means to strengthen these where relevant.
-Provide the scientific leadership of the CTAO Programme at ESO.
-Contribute to the Governance of CTAO, representing ESO as required.
-Coordinate the scientific ESO CTAO activities with CTAO, in particular with the CTAO Project Scientist.
-Present ESO facilities to the CTAO user community to promote them and to increase the interest in the exploitation of emerging synergies.
-Advise the ESO Directors of Science, Programmes and Operations on the Programme's strategic scientific goals and assisting with the coordination and updating of observing modes to adapt to the paradigm shift introduced by CTAO.
-Consult the scientific community and ESO advisory committees in developing a scientific vision for CTAO and synergetic use of ESO facilities with facilities inside or outside of ESO.
-Report to ESO and its governing and advisory bodies on CTAO developments, challenges and scientific productivity.
-Support public engagement and outreach, in collaboration with the -Communication Department, helping make the multi-wavelength use of ESO telescopes and their instruments accessible and inspiring to a diverse audience.
The above main duties and responsibilities are not exhaustive and will evolve. As a member of the ESO Astronomy Faculty, the CTAO and Synergy Programme Scientist is expected and encouraged to conduct an active astronomical research programme on a 50/50 basis.
Reports to:
Director for Science
Key Competences and Experience:
Essential Competences and Experience
-At least five years of experience in the field of physics, astronomy or closely related disciplines after PhD;
-Proven ability in developing a long-term scientific vision, understanding science requirements, and translating them into coherent plans;
-Proven experience using astronomical facilities in a multi-wavelength and multi-messenger environment, and knowledge of VHE gamma-ray astrophysics;
-Ability to think strategically, taking a long-term perspective and openness to new ideas, emerging scientific priorities, challenges and anticipating future needs or trends, while communicating a compelling vision for the future;
-Experience in collaborating to develop shared visions and scientific strategies for the future, within and beyond ESO, including the wider astronomical community;
-Effectively lead and inspire geographically dispersed, multicultural and interdisciplinary teams, fostering ownership, engagement and a professional, respectful working environment, and constructively addressing disagreement and conflict;
-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;
-An ability to create and formalise synergies inside and outside the Organisation ensuring that resources are used optimally, cost effectively and transparently;
-A strong record of personal research achievements, demonstrating international recognition appropriate to the career stage in optical and near-infrared or multi-wavelength astrophysics.
For more information: https://recruitment.eso.org/jobs/2026_0038
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| Postdoc Position: Planet-Forming Disks and Astrochemistry | Closing date: 2026-09-15
Contact: Peter Woitke |
| The Space Research Institute (IWF) of the Austrian Academy of Sciences in Graz, Austria, invites applications for a Postdoc position (f/m/x) within the research group led by Priv.-Doz. Dr. Peter Woitke. | | ▸ more | Your Role: You will prepare archival and new observational data (e.g., ALMA or JWST) for analysis and modelling, including high-quality data reduction, using ProDiMo to analyse and interpret these observations. Additionally, you will support and collaborate with international science teams preparing future ESA space missions.
Your Profile: Applicants must hold a PhD in Physics, Geophysics, Astrophysics, or a related field. You should have proven experience in astrochemistry in protoplanetary disks, ALMA/JWST data reduction, and an excellent publication record.
Our Offer & Application: The appointment is initially for 3 years, with potential extensions up to 6 years based on funding and performance. The position starts as early as November 1st, 2026, though a later start date can be agreed upon.
The application deadline is September 15, 2026, but the position remains open until filled. Apply online at https://www.oeaw.ac.at/jobs?jh=nkujljvb04425fl0u688i6lz2tk9dw7 or contact peter.woitke @ oeaw.ac.at for inquiries.
We are looking forward hearing from you!
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| ESA Research Fellowship in Space Science (Postdoctoral Fellowships) | Closing date: 2026-09-21
Contact: Victoria Grinberg |
| We are pleased to announce the 2026 Call for Applications for the European Space Agency's Research Fellowships in Space Science. We expect to hire ~9-10 postdoctoral fellows who will start their fellowship in fall 2027. | | ▸ more | ESA's postdoctoral Research Fellowship programme offers early-career researchers the possibility to carry out independent research in a variety of disciplines. Research Fellowships in Space Science offer the opportunity to contribute to ESA's endeavour to explore our Solar System and the Universe in the fields of heliophysics, planetary science, astrophysics, and fundamental physics.
ESA Research Fellow contracts have a maximum duration of three years. Projects initially last two years and are frequently extended to a third year upon submission of a dedicated proposal.
Research Fellowships in Space Science can be located at any of the following institutes:
- European Space Astronomy Centre (ESAC) in Villafranca del Castillo near Madrid, Spain
- European Space Research and Technology Centre (ESTEC) in Noordwijk, the Netherlands
- ESA Office at Space Telescope Science Institute (STScI) in Baltimore, Maryland, USA
The deadline for applications is 21 September 2026.
Detailed information and a link to the application portal can be found on the fellowship webpage: https://www.cosmos.esa.int/fellowship
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| Two open positions at Light Bridges: GPU-accelerated computing | Closing date: 2026-09-27
Contact: Miguel R. Alarcon |
We are hiring two PhD scientists to work on CORVUS, a project developing GPU-accelerated technology to detect fast-moving, very faint near Earth objects, with direct applications to planetary defence.
We are opening two broad, overlapping positions:
- Research Scientist · GPU-Accelerated Algorithms, leaning towards algorithm design and image processing.
- Computational Scientist · GPU Optimisation & Performance, leaning towards low-level performance and GPU optimisation. | | ▸ more | Light Bridges is a private company based in the Canary Islands. We operate the Two-meter Twin Telescope (TTT) and the Transient Survey Telescope (TST), together one of the world's most advanced robotic telescope facilities, at the Teide Observatory.
Full details of the project, contract conditions and how to apply: https://lightbridges.es/wp-content/uploads/2026/08/TwoPositions_LB-CORVUS.pdf
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| Instrument Scientist — Two-meter Twin Telescope | Closing date: 2026-09-27
Contact: Miguel R. Alarcon |
We are hiring an Instrument Scientist (PhD required) to join our Operations Team, working on the optical quality of our telescopes and the mechanical and optical design of parts for new instrumentation.
We are opening one position:
- Instrument Scientist · Optical Systems & Telescope Operations, leaning towards optical quality, instrument design and daily telescope operations. | | ▸ more | Light Bridges is a private company based in the Canary Islands. We operate the Two-meter Twin Telescope (TTT) and the Transient Survey Telescope (TST), together one of the world's most advanced robotic telescope facilities, at the Teide Observatory.
Full details of the project, contract conditions and how to apply: https://lightbridges.es/wp-content/uploads/2026/08/InstrumentScientist_LB-CORVUS.pdf
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| Postdoctoral positions in observational astrophysics at CNRS / IRAP, Toulouse, France | Closing date: 2026-09-30
Contact: Jean-Francois Donati |
| We invite applications for two 2+1yr postdoctoral positions in stellar and exoplanet research at the Institut de Recherche en Astrophysique et Planétologie (IRAP) located in Toulouse, France, within the SPIRou science consortium locally coordinated by Drs JF Donati and C Moutou. | | ▸ more | The first project aims at modeling the planetary systems and magnetic topologies of M dwarfs, monitored with the SPIRou near-infrared spectropolarimeter at the Canada-France-Hawaii Telescope (CFHT) since 2019 in the framework of the SPIRou Large Programs. The goal is to exploit SPIRou data collected for a few tens of M dwarfs of various masses, to (i) study the radial velocity curves and filter out activity to unveil / constrain their planetary systems , (ii) analyse the spectropolarimetric data with Zeeman-Doppler imaging (ZDI) to reconstruct the evolving stellar magnetic topologies and characterize the underlying dynamo processes.
The second project aims at modeling the magnetic topologies and accretion processes of pre-main sequence low-mass (T Tauri) stars, also monitored with SPIRou at CFHT since 2019. The goal is to analyze existing and future SPIRou data for a number of T Tauri stars of various masses, ages and accretion rates, to (i) model the spectropolarimetric data with ZDI, reconstruct the evolving stellar magnetic topologies and characterize the magnetospheric accretion processes taking place between the inner accretion disk and the stellar surface, and (ii) study the radial velocity curves and filter out activity to unveil and characterize potential close-in massive planets.
Forthcoming observations will also include, in addition to SPIRou near-infrared spectra, optical spectra simultaneously collected with the ESPaDOnS spectropolarimeter at CFHT, further broadening the panel of available diagnostics for both projects. The work will take place at IRAP with Drs JF Donati and C Moutou, starting Q4 2026 (preferably) or Q1 2027.
In addition to a PhD in astrophysics, the candidates must have a solid background in stellar spectropolarimetry and / or velocimetry to efficiently analyze spectra collected with SPIRou and ESPaDOnS.
The candidates should provide by 2026 September 30 the following documents (PDF only, via a file server):
* a motivation letter (<2p),
* a description of past and current research statements (<5p),
* a CV (<2p)
* a publication list,
* 3 reference letters sent by the mentors (same deadline)
to Drs JF Donati (jean-francois.donati @ cnrs.fr) and C Moutou (claire.moutou @ cnrs.fr).
Short-listed candidates will be invited for an on-line interview ~2 weeks after the deadline.
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| Postdoctoral Researcher in 21-cm Cosmology and Data Analysis for the Epoch of Reionization | Closing date: 2026-09-30
Contact: Florent Mertens |
| We are seeking a postdoctoral researcher to advance the search for the redshifted 21-cm signal from the Cosmic Dawn and Epoch of Reionization. The project will develop and apply new signal-recovery and foreground-mitigation methods to deep NenuFAR and LOFAR observations, with the goal of improving current constraints and moving toward a first detection. The work will directly feed into preparation for SKA-Low, within a team strongly involved in NenuFAR, LOFAR-EoR and SKA 21-cm science. | | ▸ more | Project
The detection and characterisation of the redshifted 21-cm signal from the Cosmic Dawn and Epoch of Reionization is one of the major goals of current low-frequency radio astronomy. NenuFAR and LOFAR are now providing increasingly deep observations targeting this signal, while SKA-Low will soon open a new regime of sensitivity.
The successful candidate will join the NenuFAR Cosmic Dawn and LOFAR-EoR projects and contribute to extracting the maximum cosmological information from these observations. A central challenge is to distinguish the faint 21-cm signal from astrophysical foregrounds and residual instrumental effects, which remain orders of magnitude brighter.
The project will develop new approaches to this problem, building on the signal-separation techniques already developed within the LOFAR and NenuFAR teams, including ML-GPR, while providing substantial freedom to investigate new ideas. The aim is both to improve the robustness and sensitivity of current NenuFAR and LOFAR analyses and to develop the methods that will be needed to exploit SKA-Low observations.
Activity
The work will involve formulating, testing and comparing new approaches to 21-cm signal recovery using low-frequency radio-interferometric data. Possible directions include improved modelling of astrophysical foregrounds and instrumental systematics, exploiting their spectral and temporal structure, and using realistic simulations to develop and validate new analysis strategies.
These developments will first be evaluated on simulations and may then be applied to NenuFAR Cosmic Dawn and/or LOFAR-EoR data. The successful candidate will contribute to the scientific interpretation of the results, their publication in international journals, their presentation at conferences, and interactions with the NenuFAR, LOFAR-EoR and SKA CD/EoR collaborations.
Candidate Profile
Applicants must hold a PhD in astrophysics, radio astronomy, signal processing, statistics, machine learning, or a related field.
Experience in data analysis, statistical modelling, signal processing, AI, or radio astronomy will be particularly relevant. Experience with LOFAR, NenuFAR, MWA, HERA, SKA, or Bayesian inference would be an asset but is not required.
Applications from candidates with backgrounds in signal processing, statistics, AI, or astrophysical data analysis are encouraged.
Research Environment
The position will be based at LUX, within the Cosmology and Galaxies team, which brings together expertise in radio data analysis, artificial intelligence, statistical inference and simulations of the 21-cm signal, including with the LICORICE code. The successful candidate will work under the scientific supervision of Florent Mertens and will be integrated into the NenuFAR Cosmic Dawn and LOFAR-EoR projects, in an international environment directly connected to SKA science preparation.
Position and Benefits
The appointment is for 24 months, with an expected starting date of 1 January 2027. The gross salary is €3,131–€4,341 per month, depending on experience.
Benefits include 44 days of annual leave, health coverage through the French national social security system complemented by employer-supported supplementary health insurance, 75% reimbursement of public-transport commuting costs, and a sustainable mobility allowance of up to €300 per year.
How to Apply
Applications should include a CV, a cover letter, a short research statement, and the names and contact details of two or three referees who may provide a recommendation.
Applications must be submitted through the CNRS Job Portal:
https://emploi.cnrs.fr/Offres/CDD/UMR8262-ELIBLA-005/Default.aspx?lang=EN
Application deadline: 30 September 2026.
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| Doctoral Researcher in Planet Formation with J. Drążkowska | Closing date: 2026-10-01
Contact: Joanna Drążkowska |
PhD project in Planet Formation at the Max Planck Institute for Solar System Research in Göttingen, Germany in the framework of the International Max Planck Research School for Solar System Science at the University of Göttingen and at TU Braunschweig
Subject: Vertically resolved modelling of dust evolution in a protoplanetary disk in the first comprehensive model that connects all stages of planet formation
Announcement: https://www.mps.mpg.de/phd/planet-formation | | ▸ more | PhD project in Planet Formation with J. Drążkowska at Max Planck Institute for Solar System Research in Göttingen, Germany
The Planet Formation Group is offering a PhD opportunity focused on vertically resolved modelling of dust evolution in a protoplanetary disk. Our research aims to build the first comprehensive model that connects all stages of planet formation, from micron-sized dust grains to fully formed planets, with a unique emphasis on leveraging evidence from Solar System materials.
Dust coagulation and transport are typically studied in a 1-dimensional framework, as most of the dust mass is confined to the protoplanetary disk midplane. However, scattered-light observations show that many disks are vertically puffed up and their surfaces exhibit substructures different from those seen at millimeter wavelengths. Our group has been developing the publicly available 2-D Monte Carlo code mcdust, which resolves dust evolution in both radial and vertical dimensions. This project assumes further development of the mcdust code in order to address disk vertical structure and its interplay with the midplane. Depending on the interests of the candidate, the project may include:
- Self-consistent thermochemical modeling, for example using the Dust and Lines code (DALI) to investigate the feedback between disk thermal structure and dust composition and evolution.
- Including external disk photoevaporation, for example using the Python Utility For Fuv Irradiated disc deNsities (PUFFIN) to study the formation of the youngest planetesimals and comets.
- Including dust aggregate electrostatic charging and its impact on dust coagulation.
Due to the nature of this project, preference will be given to candidates with experience in Fortran and Python code development.
Please direct all inquiries about the project to Joanna Drążkowska.
https://www.mps.mpg.de/planetary-science/erc-planetoids
https://www.mps.mpg.de/phd/application
https://www.mps.mpg.de/phd/online-application
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| PhD position in astrochemistry and machine learning at University College Dublin | Closing date: 2026-10-01
Contact: Marie Van de Sande |
| We invite applications for a PhD position in astrochemistry and machine learning at the School of Physics at University College Dublin, Ireland. You will work with Dr Marie Van de Sande on the ERC Starting Grant ASHES on dust formation in the outflows of asymptotic giant branch (AGB) stars. | | ▸ more | Position details
• 4-year PhD
• Fully funded (€30,000/year, tax-free)
• Start date: January 2027
• Application deadline: 1 October 2026
Project background
Stars like our Sun will go through an AGB phase near the end of their lives, losing their outer layers by means of a stellar outflow and enriching the interstellar medium with the building blocks for the next generation of stars and planets. To study how the chemistry is affected by the dynamics of the outflow, 3D hydrochemical models are essential. Machine learning is crucial to make this possible: by emulating, rather than calculating the chemistry, an on-the-fly hydrochemical model can finally be built.
What you will do
You will optimise the proof-of-concept emulator MACE by postprocessing Phantom SPH models of AGB binary interactions. While generating the training dataset using snapshot models, you will already be able to determine how different binaries affect the outflow’s chemistry. Coupling the emulator to Phantom, your on-the-fly hydrochemical model will then demonstrate how chemistry is affected by the dynamics. In the next stage, you will train the emulator on a novel chemical reaction network that includes dust formation. This will give us the first 3D and time-dependent overview of how dust formation is affected by AGB stars and their companions.
As part of ASHES, you will interact with all aspects of astrochemistry: chemistry, computational modelling, and astronomical observations. You will start alongside another PhD student, with two postdocs joining the group later. There are ample opportunities for attending conferences, workshops, and research stays.
Who we are looking for
The project is suitable for a student with a degree in physics or astronomy and a genuine interest in building skills in coding (Python and Fortran), machine learning, data analysis, and visualisation. Prior experience in chemical modelling or hydrodynamical modelling is a strong advantage, but not a strict requirement.
Application instructions
Applications should include a CV (including personal data, education, skills, and expertise), a one-page motivation letter, and the names and contact details of two references. Please send the documents to marie.vandesande @ ucd.ie before 1 October 2026.
Inquiries
If you have any questions, contact Dr Marie Van de Sande at marie.vandesande @ ucd.ie
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| Doctoral Researcher in Star-Planet Interactions with E. Ilin | Closing date: 2026-10-01
Contact: Ekaterina Ilin |
PhD project in Star-Planet Interactions at the Max Planck Institute for Solar System Research in Göttingen, Germany in the framework of the International Max Planck Research School for Solar System Science at the University of Göttingen and at TU Braunschweig
Subject: Confirming and characterizing magnetic star-planet interaction through time-resolved X-ray observations.
Announcement: https://www.mps.mpg.de/phd/star-planet-interactions | | ▸ more | PhD project in Star-Planet Interactions with E. Ilin at Max Planck Institute for Solar System Research in Göttingen, Germany
The soon-to-be established research group on star-planet interactions is offering a PhD opportunity, focused on confirming and characterizing magnetic star-planet interaction through time-resolved X-ray observations.
In recent years, exoplanetary science has undergone a major shift -- moving from exoplanet detection towards understanding star-planet systems as a whole, including the host star, interplanetary medium and galactic context. Specifically, tidal and magnetic interactions between planets and their host stars have been recognized to be able to modulate the evolution of both, including the atmospheric evolution of the planet and its habitability. The newly established research group led by Dr. Ekaterina Ilin seeks a PhD student with an interest in stellar magnetism and/or exoplanetary science to develop novel ways of detecting and characterizing the mutual influence of stars and planets with a focus on the influence of planets in short orbits on the magnetism of their host stars.
Individual systems with emission suspected to be planet-induced have been reported at X-ray, optical, and radio wavelengths, but confirmation and characterization has been difficult: the decisive test is whether the emission recurs on the planetary orbital period. The project applies it to both new and archival XMM-Newton observations of systems with known or suspected planet-induced emission. Depending on the interests of the candidate, the project may also include:
- Extension to radio and optical diagnostics to test different interaction scenarios
- Extension to low mass binary interactions at optical wavelengths
- Development of empirically motivated models of magnetic interaction, and predictions for how to distinguish them observationally.
- Design and submission of observing proposals, including target selection from the interaction candidates identified within the project.
Due to the nature of this project, preference will be given to candidates with experience in the reduction and analysis of X-ray, radio or other time-series data, and in scientific programming in Python.
You will work in a newly formed team of two postdocs and a PhD student, led by the PI (Ekaterina Ilin), and collaborate closely with both postdocs, who will be working primarily on a large optical photometric survey of young stars in search of interacting systems. The student is expected to present at workshops and international meetings in both the stellar and exoplanet communities.
Please direct all inquiries about the project to Ekaterina Ilin.
https://www.mps.mpg.de/phd/application
https://www.mps.mpg.de/phd/online-application
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| Full Professor Position(s) in Astronomy at the Instituto de Alta Investigación, Universidad de Tarapacá (Chile) | Closing date: 2026-10-02
Contact: Ezequiel Treister |
| The Instituto de Alta Investigación (IAI) at the Universidad de Tarapacá (UTA), Chile, invites applications for at least one Full Professor position, open to all areas of astronomy and astrophysics. The successful candidate(s) will join a growing multi-disciplinary research center with privileged access to major observatories: VLT, ALMA, Gemini, Rubin, and more, and will help shape UTA's new PhD program in astronomy. | | ▸ more | Candidates must possess a Ph.D. in astronomy, astrophysics, or a related field and demonstrate a strong record of independent research, a minimum of 12 years of experience in academic functions, (co)authorship of at least 25 peer-reviewed WOS Q1 publications, and at least 5 successful funding applications, of which two or more should be as principal investigator. Ideal candidates will also have a solid track record in one or more of: (i) leading international research projects, (ii) teaching at the undergraduate or graduate level for at least 10 semesters, (iii) advising research projects of undergraduate and graduate students, and (iv) designing and/or leading substantial outreach or academic management projects.
The selected candidate(s) will join the IAI, a multi-disciplinary excellence research center currently including six astronomers, based in the University offices in Santiago, Chile. The search is open to all areas of astronomy and astrophysics, and may consider synergies with current Institute members and/or new research areas. More on the IAI Astronomy group: https://astroiai.github.io/home/en/index.html
At the Full Professor level, minimum expectations are:
(i) at least six Q1-indexed articles annually,
(ii) maintaining one or more active externally-funded projects as PI,
(iii) establishing collaborations with national and international centers of excellence, and
(iv) sponsoring postdoctoral fellows (e.g., FONDECYT, ALMA, COMITE MIXTO).
Selected candidate(s) are also expected to contribute to establishing a new world-class PhD program in astrophysics within the next two years.
Benefits: highly competitive salary depending on qualifications; performance bonuses; an annual research operational allocation; funding for research/support personnel; access to reserved telescope time at VLT, La Silla, Gemini, Magellan, CTIO, SOAR, Rubin, APEX, ALMA, and future facilities (CTA, ELT, GMT); privileged access to the UTA HPC cluster (96 Nvidia H200 GPUs).
Applications should include a cover letter, CV, a complete list of awarded projects and WOS publications, a statement of research interests for the next five years, and contact information for at least three references.
Submit via: https://form.jotform.com/262074237310650.
Review of applications begins Friday, October 2, 2026, and continues until the position is filled.
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| Tenure-track Faculty Position in Observational Massive Star and Compact Object Binary Science | Closing date: 2026-10-04
Contact: dr. Nathalie Degenaar, chair of the search committee |
| Do you work in the field of observational massive star and compact object binary science? Are you interested in contributing to a diverse and collaborative research and teaching community? Then join us at the Anton Pannekoek Institute for Astronomy (API) of the University of Amsterdam (UvA)! | | ▸ more | The Anton Pannekoek Institute for Astronomy (API) of the University of Amsterdam (UvA) is seeking to hire an assistant professor in high-energy astrophysics. We especially welcome applications from experts in multi-wavelength and time-domain observational astronomy that connect to new and future facilities such as SKA, CTA, NewAthena, and ELT. The candidate will lead a research program focused on the roles of binary star systems with massive stars, stellar-mass black holes and neutron stars, as laboratories for binary evolution, extreme gravity, accretion, particle acceleration and feedback. The new staff member is expected to play an active role in positioning the API within the Dutch and global data science communities and/or instrumentations programs, and to connect their research to other focus areas at the Anton Pannekoek Institute.
For all details about this position, our organization and the application procedure, please visit the job announcement on the UvA webpage.
Information about the API:
https://api.uva.nl/
UvA job posting and application link:
https://werkenbij.uva.nl/en/vacancies/tenure-track-faculty-position-in-observational-massive-star-and-compact-object-binary-science-netherlands-15403
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| Sirius Fellowship in Astrophysics Program at ISTA | Closing date: 2026-10-15
Contact: Postdoctoral Office |
Call for applications
The Institute of Science and Technology Austria (ISTA) has launched a new astronomy and astrophysics fellowship program, the Sirius Fellowship in Astrophysics, for exceptional postdoctoral scientists. | | ▸ more | Call for applications
The Institute of Science and Technology Austria (ISTA) has launched a new astronomy and astrophysics fellowship program, the Sirius Fellowship in Astrophysics, for exceptional postdoctoral scientists.
The fellowship is a three-year fully-funded position (guaranteed for two years, with the third year contingent on review), with a research and travel budget of 25,000 EUR per year. Up to two fellowships will be funded in the 2026 call.
The fellowship will provide postdocs with the freedom to establish their own research program in any area of astronomy, astrophysics and cosmology.
ISTA offers an enabling and collaborative environment in the outskirts of Vienna, with dedicated mentorship from excellent, established astrophysics faculty members. For more information about the astrophysics research groups at ISTA, see: https://astro.ista.ac.at/
Application deadline: October 15, 2026 (14:00 CEST)
Offers will be sent out to successful candidates by January 2027.
For further information and to submit your application, please visit our website:
https://ista.ac.at/en/education/postdocs/sirius-fellowship
Eligibility Requirements:
- Applicants must have had their PhD awarded no more than 6 years before the commencement of the fellowship.
- Researchers already employed at ISTA are not eligible for the fellowship.
- Following the initial evaluation round, top-ranked candidates must be available for a remote interview between Nov 16-18, 2026.
- Successful Fellows must begin their employment at ISTA on or around 1 September 2027.
Benefits:
Internationally competitive salary (min. 76,986 EUR gross per year)
Annual research and travel budget of 25,000 EUR
Cutting-edge and state-of-the-art resources: scientific service units (e.g. scientific computing clusters)
Open, collaborative, interdisciplinary research environment
Enabling framework in which to develop interdisciplinary skills
Teaching within ISTA encouraged (but not required), aiming to create the most conducive environment for the creation and transfer of knowledge
Access to optional Scientific integrity and leadership training, as well as career development support
Joining ISTA’s global networks of exceptional, pioneering researchers
All employees enjoy Austria’s social security benefits
Equity, Diversity & Inclusion (EDI)
At ISTA, equity, diversity and inclusion are core values that we see as essential for creating and disseminating new knowledge and for taking science into new directions. ISTA strives for a diverse community with an open, inclusive culture where scientists and staff of all backgrounds, regardless of age, gender, ethnicity, cultural background, religion, sexual orientation, and physical disabilities, can work and learn together.
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| Postdoc for Astronomical Observing Programs at the University of Vienna | Closing date: 2026-10-15
Contact: Stefan Meingast |
| The Leopold Figl Observatory for Astrophysics, operated by the Department of Astrophysics of the University of Vienna, hosts the largest optical telescope in Austria (1.5 m). Within the Figl 2030 project, the observatory is building up a major observing program for the follow-up and characterization of transiting extrasolar planets. We are looking for a postdoctoral researcher to join the team behind this program. You will work in close collaboration with colleagues at the Department of Astrophysics, in particular Univ.-Prof. Dr. João Alves and Dr. Stefan Meingast. | | ▸ more | The Leopold Figl Observatory for Astrophysics, operated by the Department of Astrophysics of the University of Vienna, hosts the largest optical telescope in Austria (1.5 m). Within the Figl 2030 project, the observatory is building up a major observing program for the follow-up and characterization of transiting extrasolar planets. We are looking for a postdoctoral researcher to join the team behind this program. You will work in close collaboration with colleagues at the Department of Astrophysics, in particular Univ.-Prof. Dr. João Alves and Dr. Stefan Meingast.
Your working place:
The Department of Astrophysics with currently around 100 members is part of the Faculty of Earth Sciences, Geography and Astronomy at the University of Vienna.
You will be at the center of the Figl 2030 project, which dedicates a large share of the observing time of the 1.5 m Leopold Figl telescope to the photometric follow-up of transiting exoplanet candidates identified by space missions such as TESS and PLATO. This includes false-positive screening and the refinement of transit parameters. The telescope is currently being upgraded with a new wide-field camera system. You will be based at the University Observatory in Vienna and help build up the observing program, including taking observations yourself. The team observes mostly remotely from Vienna, with occasional work at the telescope on Mitterschöpfl.
The position is set for 48 months, with a preferred starting date of January 1, 2027.
Your future tasks:
Active participation in research, teaching & administration, which means:
As part of a team, you help establish and operate observing programs — in particular those related to exoplanet research — at the 1.5 m Leopold Figl telescope.
You build up your research profile in time-domain science with room for independent projects and collaborations.
You participate in the commissioning and science verification of the new wide-field camera system.
You develop, maintain, and document the data reduction and photometry pipelines required for high-precision time-series photometry.
You help coordinate the observatory’s participation in international follow-up programs (e.g., for NASA’s TESS mission).
You lead and participate in scientific publications in peer-reviewed journals and present results at international meetings.
You contribute to the outreach activities.
You can (co-)supervise Bachelor and Master students and involve students in the observations.
You can hold courses independently within the scope of the provisions of the collective bargaining agreement.
Your profile:
Must-haves
A PhD degree in astronomy, astrophysics, or a closely related field, completed by the starting date.
Experience with optical astronomical observations.
Experience with high-precision photometry and/or time-series analysis.
Research experience in observational astronomy, demonstrated through publications appropriate to your career stage.
Solid programming skills (e.g., Python) and experience with astronomical data processing.
Fluency in English (spoken and written).
A category B driver’s license (Austrian Führerschein B or an equivalent from another country), or the willingness to obtain one before or shortly after the start of the position.
Good-to-haves
Experience with exoplanet transit observations and light curve modeling.
Experience with telescope operations, instrument commissioning, or remote observing.
Experience with infrared astronomical observations.
Hands-on technical or engineering experience, for example with observatory hardware, instrumentation, electronics, or mechanical systems, whether from astronomy or another field.
Experience in the supervision of students and in public outreach.
Knowledge of German.
Your working style is independent, structured, and solution-oriented. You thrive in collaborative, international teams and enjoy tackling technical challenges in dynamic environments. You are a team player and have good social and communicative skills.
What we offer:
Inspiring working atmosphere: You have the opportunity to work within a dedicated team on forefront science, while profiting from the international environment in the Department of Astrophysics. We have privileged access to the Austrian Scientific Computing (ASC) super-computing facility. As a member state of ESO and ESA, Austria has access to their first-class observing facilities, and the Department of Astrophysics is a partner in three instrument consortia for ESO’s Extremely Large Telescope (ELT), currently under construction.
Work-life balance: Our employees enjoy flexible working hours. Upon agreement, hybrid working hours within Austria might be possible up to a certain extent.
Good public transport connections: Your working place, the University Observatory, is located in the middle of the natural monument Observatory Park in the lively city of Vienna with outstanding public transport.
Internal further training & Coaching: Opportunity to deepen your skills on an ongoing basis. There are over 600 courses to choose from – free of charge.
Fixed-term contract and fair salary: The basic salary of EUR 5.014,30 (14 times a year) increases if we can credit professional experience.
Equal opportunities for all: We look forward to diverse personalities in the team!
It is that easy to apply:
With your CV including a list of publications
A letter of motivation
A brief description of your research interests
Contact details of references who may be contacted regarding your application
With your PhD certificate
Via our job portal/ Apply now - button
https://jobs.univie.ac.at/job/Postdoc-for-Astronomical-Observing-Programs-at-the-Leopold-Figl-Observatory/1433430933/
If you have any questions, please contact:
Stefan Meingast
stefan.meingast @ univie.ac.at
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| Postdoctoral researcher position in Space Physics/Astrophysics at the Space Research Centre PAS in Warsaw, Poland | Closing date: 2026-10-17
Contact: Pawel Swaczyna |
| The Space Research Centre of the Polish Academy of Sciences in Warsaw is seeking a motivated postdoctoral researcher to conduct research on the local interstellar medium surrounding the heliosphere. The successful candidate will participate in modeling possible interaction scenarios in the local interstellar medium and how these scenarios are reflected in the distribution of interstellar neutral atoms observable by dedicated instruments on the IBEX and IMAP missions. The researcher will join the team led by Paweł Swaczyna. | | ▸ more | More information and application procedure: https://pawelswaczyna.com/postdoc
Gross salary: 13 263 PLN/month (subject to personal income tax and social security deductions).
Period of employment: 12 months, with extension up to a total of 48 months, contingent upon satisfactory research progress.
Place of work: Bartycka 18a, Warsaw, Poland.
Start date: 1 November 2026 – 30 April 2027 (to be negotiated with the selected candidate).
Application deadline: 17 October 2026
Questions about the position can be directed to Paweł Swaczyna at pswaczyna @ cbk.waw.pl
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| PhD positions at the International Max Planck Research School for Astronomy & Astrophysics, Bonn & Cologne | Closing date: 2026-10-30
Contact: Gunther Witzel |
| The International Max Planck Research School (IMPRS) for Astronomy & Astrophysics opens its Call for Applications on 15 September, 2026. | | ▸ more | The International Max Planck Research School (IMPRS) for Astronomy & Astrophysics is a joint structured Ph.D. program of the Max Planck Institute for Radioastronomy (MPIfR, Bonn) and the Universities of Bonn and Cologne. At one of the most vibrant astronomy centers in Europe, several PhD positions are available for talented students nearing the end of their Master's degree (or equivalent) in physics or astrophysics. The teaching language is English. Program Details: Appointments are for 3 years, starting at any time in 2027. Starting annual gross salary: ~40617 Euro; with attractive benefits. The IMPRS for A&A has 70+ Ph.D. students from 20+ countries.
Supervision by world-leading experts at the MPIfR and the Universities of Bonn and Cologne. Research on a wide range of cutting-edge topics in observational and theoretical astrophysics. Access to world-class observing facilities at a wide range of wavelengths. Career development workshops, advanced lecture courses, soft skill seminars. Funding for travel and research.
The Max Planck Society is committed to increasing diversity in its workforce and encourages applications from individuals with disabilities. The society also seeks to increase female representation in underrepresented areas and strongly encourages women to apply. Compensation and Benefits CompensationType:
The application deadline is October 30th, 2026.
More information: https://www.mpifr-bonn.mpg.de/en/imprs
Online Application: https://imprs.mpifr-bonn.mpg.de
Inquiries IMPRS A&A Office
Email: imprs @ mpifr-bonn.mpg.de
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| EXECUTIVE DIRECTOR Canada-France-Hawaiʻi Telescope Corporation | Closing date: 2026-10-31
Contact: Céline Reylé |
| The Canada-France-Hawaiʻi Telescope Corporation (CFHT) invites applications and nominations for the position of Executive Director. This is an exceptional opportunity for a visionary scientific and organizational leader to guide one of the world’s premier astronomical observatories through a pivotal chapter in its history — one that demands both scientific ambition and a deep, genuine commitment to the people and places of Hawaiʻi. | | ▸ more | The successful candidate will bring:
• A graduate degree (Master’s or doctoral level) in astronomy, astrophysics, engineering, or a closely related field, or equivalent demonstrated leadership experience in a science or technology-intensive organization.
• Broad knowledge of astronomy, including familiarity with optical and infrared observational techniques and instrumentation.
• Demonstrated experience managing a scientific research facility, technical organization, or comparable institution in a team-oriented, international environment.
• Very strong communication skills and a proven ability to inspire, motivate, and make compelling public presentations; demonstrated skills in institutional and international relations.
• The ability to think and act strategically, with a track record of translating vision into results.
• Demonstrated cultural competency and a genuine commitment to equity, diversity, and inclusion, with experience engaging authentically across diverse communities — a quality of particular importance given CFHT’s responsibilities on Maunakea.
Applications should be submitted electronically to the CFHT Search Committee and must include a curriculum vitae and the names and contact information of at least three references who may be contacted for confidential evaluations. Information about CFHT is available at www.cfht.hawaii.edu. Applications can be submitted at this link: https://cfht.applicantpro.com/jobs/. Prospective applicants with questions about the position or the search process are encouraged to contact the Search Committee at positioninfo @ cfht.hawaii.edu.
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| ESA Archival Research Visitor Programme | Closing date: 2026-10-31
Contact: Guido De Marchi |
| To increase the scientific return from its space science missions, the European Space Agency (ESA) welcomes applications from scientists interested in pursuing research projects based on data publicly available in the ESA Space Science Archives (http://www.cosmos.esa.int/web/esdc). | | ▸ more | The ESA Archival Research Visitor Programme is open to scientists, at all career levels, who are affiliated with institutes in ESA Member States and Cooperating States. All visits must comply with the ESA security directives, which may necessitate additional checks. Early-career scientists and PhD students are particularly encouraged to apply. We encourage applications from women and minorities. The peer-review evaluation process is anonymised to ensure equal opportunities for all applicants.
During their stay, visiting scientists will have access to archives and mission specialists for help with the retrieval, calibration, and analysis of archival data. In principle, all areas of space research covered by ESA science missions can be supported.
Residence lasts typically between one and three months, also distributed over multiple visits. Research projects can be carried out at ESAC (Madrid, Spain) and at ESTEC (Noordwijk, Netherlands). To offset the expenses incurred by visitors, ESA covers travel costs from and to the home institution and provides support for lodging expenses and meals.
Applications received by 31 October 2026, 23:59 UTC, will be considered for visits in spring and summer 2027.
For further details, including areas of research and contact information, please refer to
https://www.cosmos.esa.int/web/esdc/visitor-programme
or write to the programme coordinators at arvp @ cosmos.esa.int
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| PhD positions in space and astrophysics in Braunschweig, Germany | Closing date: 2026-10-31
Contact: Yasuhito Narita |
The Technical University Braunschweig is looking to recruit one or two doctoral researchers to work on space and astrophysics at the Institute for Theoretical Physics:
https://www.tu-braunschweig.de/stellenangebote/wimi/wissenschaftliche-mitarbeiterin-bzw-wissenschaftlichen-mitarbeiter-m/w/d-zum-thema-weltraum-und-astrophysik-institut-fuer-theoretische-physik
The positions require both German and English language skills. | | ▸ more | Prof. Dr. Yasuhito Narita at the Institute for Theoretical Physics is looking for a doctoral researcher to work on
- Fundamental plasma processes (waves, turbulence, shock waves, magnetic reconnection)
- Modeling (the Sun and solar wind, magnetospheres, small bodies)
- Plasma astrophysics (stars and galaxies, gravitational waves, compact objects)
- Numerical experiments using high-performance computers (Sun, planets, and comets)
- Development and maintenance of numerical codes
- Participation in international space programs at ESA/JAXA/NASA (Solar Orbiter, BepiColombo, Comet Interceptor, JUICE, Plasma Observatory, HelioSwarm)
- Assistance with the scientific journal *Earth, Planets and Space*.
- Teaching (various tasks, in German)
Initial appointment for three years, salary EG 13 TV-L ,75%
Please follow the instruction to apply at https://www.tu-braunschweig.de/stellenangebote/wimi/wissenschaftliche-mitarbeiterin-bzw-wissenschaftlichen-mitarbeiter-m/w/d-zum-thema-weltraum-und-astrophysik-institut-fuer-theoretische-physik
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