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| SKA-Low Operations Scientist | Closing date: 2025-04-30
Contact: Heather |
A unique opportunity for a talented and motivated radio astronomer to play major roles in the scientific verification and operation of the world's largest low-frequency radio telescope. This role has a specific focus on expertise in the areas of Epoch of Rionisation, Cosmic Dawn, low frequency cosmology, or intensity mapping.
The SKA-Low Operations Scientist will be based at the Science Operations Centre in Perth, Australia.
Apply here: https://recruitment.skao.int/vacancy/skalow-operations-scientist-582036.html | | ▸ more | We are looking to recruit an Operations Scientist who will further enhance our growing SKA-Low Science Operations team, in particular with expertise in the areas of the Epoch of Reionisation, Cosmic Dawn, low frequency cosmology, or intensity mapping.
The SKA-Low Operations Scientists will have a unique opportunity to shape the operation of the SKA-Low Telescope through the sharing of their domain knowledge and expertise. During construction and early array deployment, they will assist with commissioning as well as plan and conduct science verification. The Science Operations team will verify the end-to-end science process, including proposal submission, scheduling, execution, data reduction and delivery.
Once the Telescope will be fully operational, the SKA-Low Operations Scientists will develop new capabilities, respond to new science directions and provide astronomical observing expertise to operators, ensuring the successful delivery of data for the key science objectives of the SKAO.
The SKA-Low Operations Scientist will be based at the Science Operations Centre in Perth, Australia.
They will collaborate with multidisciplinary SKAO colleagues and interact with the global science community to communicate progress. SKAO also has close contacts with universities in Australia, allowing for co-supervision of students and postdoctoral fellows.
The SKA-Low Operations Scientist will also have the opportunity to maintain an active research career, with up to 25% of their time available for personal research.
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.
There may be occasions where 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
Under the direction of the SKA-Low Senior Operations Scientist, the SKA-Low Operations Scientist will support science operations of the SKA-Low Telescope by:
*Contribute to the commissioning and science verification of array releases, including the development and implementation of test plans and procedures, with a particular focus on the Epoch of Reionisation, Cosmic Dawn, low frequency cosmology, or intensity mapping.
*Support the development and continual refinement of the science operational model for the SKA-Low Telescope, including the software needed.
*Provide user support to the scientific community including ensuring the broadest possible accessibility to SKA observing time and data.
*Effectively collaborate with SKAO Science Operations staff across the three sites; some travel to the SKA-Mid Telescope site in South Africa and SKAO Global Headquarters in the UK could be required.
*Optionally undertake a programme of personal research up to 25% of employed hours.
*Undertake other reasonable duties as directed.
Mandatory Knowledge, Skills and Experience
*A doctorate or equivalent experience in astronomy, physics, engineering, or closely related field.
*Expertise in radio astronomy techniques including in the acquisition, reduction and analysis of interferometric astronomical data.
*An appreciation, understanding of and demonstrated experience in the radio astronomy science cases motivating the SKA Observatory, in particular in the areas of the Epoch of Reionisation, Cosmic Dawn, low frequency cosmology, and/or intensity mapping.
*Demonstrated aptitude to undertake scientific facility operation, provide user support and translate the needs of the user to requirements and/or operational policies.
*Demonstrated aptitude to work collaboratively across disciplines, with engineers and scientists from a variety of cultures, contributing to an inclusive team environment.
*Demonstrated effective written and oral communication skills.
*An awareness of, and commitment to, equitable practices, including accessibility, to facilitate broad access to the Observatory.
Desirable Knowledge, Skills and Experience
*Experience with, or understanding of, ionospheric and direction-dependent calibration techniques relevant to the frequencies of the SKA-Low Telescope.
*Experience understanding and articulating the needs of a user (e.g. radio astronomer) to inform the development of requirements (e.g. through a series of use cases) and/or operational policies.
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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| PhD positions in stellar astrophysics at Uppsala University, Sweden | Closing date: 2025-04-04
Contact: Thomas Nordlander |
We are looking for up to three PhD students in astrophysics, with focus on Galactic archaeology, galaxy evolution, and stellar spectroscopy including accreted stellar populations, stellar ages, chemical evolution and the first stars.
The positions are fully funded and will cover purchase of computing equipment as well as research/conference travel. | | ▸ more | One successful candidate will primarily work with Dr. Diane Feuillet on identifying and characterizing stellar populations in the Milky Way using stellar kinematics, elemental abundances and stellar ages, with a focus on accreted stars in the halo and disk. The other successful candidate(s) will work with Dr. Nordlander towards understanding the early evolution of the Milky Way and the properties of the first stars, through spectroscopic analyses of metal-poor stars, stellar population analyses, and/or characterizing ancient supernovae using chemical abundance data.
We are looking for candidates with:
a strong interest to pursue research in stellar and/or galactic astrophysics,
good communication skills as well as good oral and written proficiency in English,
excellent study results,
a high level of creativity and thoroughness,
a structured approach to problem-solving,
and an ability to work both independently and in a team.
Previous experience of research and/or study in astronomy, experience with astronomical spectroscopy, study results, and programming or data analysis skills will be considered a merit. The quality of scholarly writing (project reports, theses, publications) will be given significant weight. Interviews and aptitude tests may be conducted as part of the selection procedure.
This is a four-year full-time employment. Extension up to a maximum total employment of five years is possible by including department duties such as teaching at a level of at most 20 %. The starting salary is 31,900 kr (roughly 2900 EUR), with annual increments.
Full instructions are provided in the online application system:
https://uu.varbi.com/en/what:job/jobID:795806/
Please note that applications must be submitted through the online application system.
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| Post-doctoral or researcher position in stellar astrophysics | Closing date: 2025-03-28
Contact: Lenka Cihakova |
| Applications are invited for a fixed-term researcher position in the Stellar Physics Department of the Astronomical Institute of the Czech Academy of Sciences. The successful applicant will work in the team of Dr. Michaela Kraus on modelling of stellar atmospheres and winds of pulsating blue supergiants. Advanced knowledge in handling non-LTE radiative transfer codes such as CMFGEN or PoWR is pre-requisite for the position. | | ▸ more | Submission: by email to sekretariat @ asu.cas.cz with the subject POSTDOC - KRAUS
Required application parts (all in PDF):
- cover sheet listing: full name, birth date, nationality, current position, short motivation (1/2 page maximum)
- curriculum vitae
- list of publications
- summary of the most significant research results achieved to date and proposed research project (2 pages max in total)
- recommendation letters (to be delivered separately)
Applicants must arrange for a minimum of two recommendation letters to be sent directly to the same electronic address as above. The letters may be issued up to 9 months before the application deadline.
The appointment is initially for one year; an extension until 31 December 2027 is expected upon satisfactory scientific performance. A necessary condition is to satisfy legal requirements for employment in the Czech Republic (EU member state). Salary will be based on the domestic level (cca 1800 EUR/month before taxes plus eventual bonuses; health insurance included). There is a possibility of staff accommodation in Ondrejov or private accommodation can be arranged. The employment may start immediately or based on negotiations. The most promising applicants may be invited for an online interview. Once the evaluation process is completed, all applicants will be notified.
Further information:
o https://www.euraxess.cz/ for details about the research employment and work conditions in the Czech Republic
o http://www.numbeo.com/cost-of-living/comparison.jsp to compare the cost of living
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| Maîtrise en 2026 au Planétarium de Montréal et IREx / 2026 M.Sc. at the Montreal Planetarium and IREx | Closing date: 2025-05-31
Contact: Jonathan Gagné |
*French follows*
The Montreal Planetarium, in collaboration with the Trottier Institute for Research on Exoplanets (IREx), affiliated with the Department of Physics of the Université de Montréal (UdeM), invites candidates to apply for an M. Sc. under the supervision of Jonathan Gagné on the detection and characterization of isolated planetary-mass objects (planemos) in nearby, young stellar associations.
The Masters' degree will start between January and April 2026 for 2 years. The stipend is 17k CAD/year.
Apply here / Appliquez ici: https://forms.gle/dehkVo6y25wqSduRA | | ▸ more | Apply here / Appliquez ici: https://forms.gle/dehkVo6y25wqSduRA
Jonathan Gagné is a researcher at the Montréal Planetarium, an adjunct professor at UdeM, and a member of IREx. His research revolves around characterizing the ages of stars, brown dwarfs, exoplanets, and planetary-mass objects (planemos), with a particular emphasis on:
? The discovery and characterization (membership, kinematics, age) of young stellar associations, notably using data from the Gaia space mission,
? The discovery and (spectral and kinematic) characterization of substellar objects, including brown dwarfs and planemos,
? The search for exoplanets using the radial velocity method, with a focus on exoplanets around young stars.
Jonathan is also interested in numerical methods for machine learning (e.g., Gaussian processes, extreme deconvolution, and other clustering algorithms), the compilation of large datasets using MySQL databases, data visualization, and the characterization of light pollution.
The master?s program lasts for two years, starting between January and April 2026, with a salary of CAD 17,000/year funded by Jonathan?s NSERC research grant. Candidates will be required to apply for NSERC and FRQNT master?s scholarships in fall 2025, which could increase their stipend to CAD 31,000/year (CRSNG) or CAD 24,000/year (FRQNT). The master?s internship could be extended (or converted) into a PhD position depending on interest and the availability of research funding after 2026.
The internship will take place in person at the Montréal Planetarium (located at 4801 Pierre-de Coubertin Ave, Montréal), where an office will be provided for the candidate near Jonathan?s office. Jonathan will be available most of the time during the week to work with the candidate. The candidate will also be encouraged to visit IREx (located at the MIL campus of UdeM at 1375 Thérèse-Lavoie-Roux Ave, Montréal, QC H2V 0B3) regularly for IREx coffee meetings, conferences, and collaborations.
Application Deadline: May 31, 2025
If you have any questions or concerns about your application, contact me at jonathan.gagne @ montreal.ca.
/
Le Planétarium de Montréal, en collaboration avec l'Institut Trottier de recherche sur les exoplanètes (IREx) affilié au Département de physique de l'Université de Montréal (UdeM), invite les candidatures pour une maîtrise en recherche sous la supervision de Jonathan Gagné sur la détection et la caractérisation d'objets isolés de masse planétaire (planémos) dans les associations d'étoiles jeunes proches.
Jonathan Gagné est chercheur au Planétarium de Montréal, professeur associé à l'UdeM et membre de l'IREx. Ses champs de recherche sont centrés autour de la mesure de l'âge des étoiles, naines brunes, exoplanètes et planémos, et concernent principalement:
? La découverte et la caractérisation (membres, cinématique, âge) d'associations d'étoiles jeunes, notamment en utilisant les données de la mission spatiale Gaia,
? La découverte et la caractérisation spectrale et cinématique d'objets sous-stellaires, regroupant les naines brunes et les planémos,
? La recherche d'exoplanètes par la méthode des vitesses radiales, avec l'accent sur les exoplanètes autour d'étoiles jeunes.
Jonathan est aussi intéressé par les méthodes numériques d'apprentissage machine (par exemple les procédés Gaussiens, la déconvolution extrême et les autres algorithmes de regroupement), la collation de grands ensembles de données via l'utilisation de bases de données MySQL, la visualisation de données et la caractérisation de la pollution lumineuse.
La maîtrise est pour une durée de 2 ans, débutant entre janvier et avril 2026, avec un salaire de 17,000 $CAD/an fourni par la subvention de recherche CRSNG de Jonathan. Les candidat·e·s devront soumettre une demande de bourse de maîtrise auprès du CRSNG et du FRQNT à l'automne 2025, ce qui pourrait augmenter leur salaire à 31,000 $CAD/an (CRSNG) ou 24,000 $CAD/an (FRQNT). La maîtrise pourrait être prolongée (ou transformée) en stage doctoral selon l'intérêt et les fonds de recherche disponibles après 2026.
La maîtrise se produira en personne au Planétarium de Montréal (situé au 4801 Avenue Pierre-de Coubertin, Montréal), où un bureau sera mis à la disposition du·de la candidat·e à proximité du bureau de Jonathan, qui sera disponible la majorité du temps en semaine pour travailler avec le·la candidat·e. Le ou la candidat·e sera aussi encouragé·e à visiter l'IREx (situé au campus MIL de l'UdeM au 1375 Ave.Thérèse-Lavoie-Roux, Montréal, QC H2V 0B3) régulièrement pour les cafés IREx, conférences et collaborations.
Date limite pour l'application : 31 mai 2025
Si vous avez des questions concernant votre candidature, contactez-moi à jonathan.gagne @ montreal.ca.
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| Two post-doctoral positions in pipeline development for the ESO Extremely Large Telescope instruments METIS and MICADO. | Closing date: 2025-04-03
Contact: Norbert Przybilla |
Duration: 2 years
Number of Positions Available: 2
Could the duration be extended: Yes, if funding is available
Work Arrangement: In-Person
Location: Innsbruck / Austria | | ▸ more | The University of Innsbruck is the largest and most important research and education facility in Western Austria, located in the heart of the Alps. The Galactic Astrophysics group of Prof. Norbert Przybilla at the Institute for Astro- and Particle Physics invites applications for two post-doctoral positions to support development of data-reduction software packages for spectroscopic modes of the ESO ELT instruments MICADO and METIS.
Your tasks:
- independent project work for ESO ELT instrumentation projects
- participation in organizational and administrative tasks
Your profile:
- 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 through mid-infrared wavelength range and data analysis of astronomical instruments
- experience in 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
The appointment is for two years with the possibility of extension beyond that period contingent upon performance and availability of funding.
Compensation and Benefits:
The University of Innsbruck pursues a non-discriminatory employment policy and values equal opportunities, as well as diversity. Individuals from underrepresented groups are particularly encouraged to apply.
The minimum gross salary (stipulated by collective agreement for the universities of Austria) for this position is susceptible to increase depending on inflation and amounts to ? 4.933 per month (as of 2025), 14 salaries/year.
It also includes health and pension insurance (following the collective bargaining agreement of the university) and 5 weeks of holidays.
The University of Innsbruck voluntarily also offers several additional benefits like a grant for the local public transport, flexible working hours, a family-friendly working environment, and attractive training and development opportunities, see
https://www.uibk.ac.at/de/karriere/zusatzleistungen/
for more details.
Application Details / Instructions:
The application has to be submitted via the web portal of the University of Innsbruck, with the application deadline on April 3rd, 2025.
Required documents: cover letter including names and contact information for two references, who may be contacted for letters of recommendation, CV with publication list, a statement that describes all relevant experiences related to observations and development of data reduction software (maximum 2 pages).
Interested applicants should apply for both positions.
Job Portal:
https://lfuonline.uibk.ac.at/public/karriereportal.home?lang=en
Direct link to online Applications:
https://lfuonline.uibk.ac.at/public/karriereportal.details?asg_id_in=14890
https://lfuonline.uibk.ac.at/public/karriereportal.details?asg_id_in=14891
Application Deadline: 2025 Apr 03
Reference Code: MIP-14890, MIP-14891
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| 2025 Montreal Planetarium / UdeM / MITACS Postdoctoral Fellowship | Closing date: 2025-04-15
Contact: Olivier Hernandez |
The Montreal Planetarium, in collaboration with the Trottier Institute for Research on Exoplanets (IREx), affiliated with the Department of Physics of the Université de Montréal (UdeM), invites candidates to apply to a MITACS Elevate Postdoctoral Fellowship in observational astrophysics applied to the study of brown dwarfs, isolated planetary-mass objects and nearby, young associations.
The full job posting information can be found at: https://tinyurl.com/ys44bmnc
To apply, fill out the following form: https://tinyurl.com/pvppwvee | | ▸ more |
Eligibility: A PhD in physics, astronomy or related discipline is required at the time when the position starts. All areas of research related to brown dwarfs, young stars and related fields of astrophysics are eligible. Preference will be given to applicants within 5 years of obtaining their Ph.D. Applicants with career interruptions due to parental, medical or family leaves, or other causes are invited to mention it in their cover letter if so desired.
IMPORTANT: Once an applicant is selected by our committee, they must also successfully apply and obtain a MITACS Elevate Fellowship in collaboration with our team, given that half of the postdoctoral stipend will be paid by MITACS. Details can be found at: https://www.mitacs.ca/our-programs/elevate-students-postdocs/
The requirements specific to MITACS also apply to this announcement (see full job ad at URL in header for details).
Location: The position is held at the Montreal Planetarium, located at 4801 av. Pierre-de Coubertin in Montreal. IREx will also offer the successful applicant a visitor?s office at the MIL campus of Université de Montréal, located at 1375 ave Thérèse-Lavoie-Roux in Montreal.
Starting Date: The successful applicant is expected to start between June and September 2025.
Duration: The position will be held for a total of two years, with a possibility of renewal for a third year upon a successful extension request to MITACS.
Conditions: A stipend of 60,000 $CAD/year will be offered for two years (with a possibility of renewing for an additional year). Postdoctoral fellows are part of SERUM-POSTDOC union, and a collective agreement governs their working conditions. A full-time employee works 35 hours per week (140 hours spread over four-week periods). They are entitled to 23 vacation days and up to 8 sick days per year. They are also entitled to several holidays and social leaves, including parental leave.
Application: To apply, fill out the following form: https://tinyurl.com/pvppwvee
Your application must include, in a single PDF file:
- A cover letter (maximum 1 page)
- A curriculum vitae
- A list of publications: please clearly distinguish between peer-reviewed and - non-peer-reviewed articles.
- A statement of research interest (maximum 2 pages, references can be added in a 3rd page)
- You should also arrange to have three referees send a letter of reference to irex-applications @ umontreal.ca before the deadline. Please ask your referees to adopt the format YourLastName_HisHerLastName_Rec_MITACS.pdf
Deadline: Applications submitted by April 15th, 2025 will receive full consideration.
Once an applicant has been selected by our team, they will collaborate with the Montreal Planetarium and IREx to submit a MITACS Elevate Postdoctoral Fellowship before May 31, 2025. MITACS takes 6?8 weeks to review an application and accept or reject the application. The applicant will only be able to carry the Postdoctoral Fellowship if the MITACS application is successful.
About the Montreal Planetarium: The Montreal Planetarium initiated its astrophysics research branch in 2020, and has since hired two permanent researchers with growing teams of graduate-level researchers: Jonathan Gagné, an expert in brown dwarfs, young stars and exoplanets and adjunct professor at Université de Montréal, and Auriane Egal, an expert in the observation and modelling of meteor showers and adjunct professor at the University of Western Ontario.
The Montreal Planetarium is part of Space for Life, Canada?s largest natural science museum complex (the Biosphere, Biodome, Planetarium, Botanical Garden and Insectarium). The Planetarium?s mission, like that of the other Space for Life museums, is to bring people closer to nature, and it has a strong commitment to the diffusion of knowledge to the general public.
About IREx: IREx consists of a growing team of about 60 people working on a variety of observational, theoretical, and instrumental projects related to the study of exoplanets and other related fields of astrophysics. They work within several research institutions located in Quebec, Canada (Université de Montréal, McGill University, Bishop?s University, Montreal Planetarium of Space for Life, Université Laval). Our professors, researchers, and students are actively involved in large international projects related to the detection and characterization of exoplanets, notably the James Webb Space Telescope, the SPIRou and NIRPS spectrographs, and have privileged access to time and data from these instruments. More information on IREx?s research programs can be found on their website.
IREx also has a vibrant science education and outreach program led by astrophysicists who are seasoned science communicators. They believe in the importance of training scientists who have exceptional scientific research skills, but also outstanding communication skills. All the team is committed to bringing science to a wide audience in a variety of ways.
The Montreal Planetarium and IREx advocate for diversity, inclusion, and employment equity
We strongly encourage applications from women, visible and ethnic minorities, Indigenous people, persons with disabilities and people of all sexual orientations and gender identities to apply. With the support of the IREx and Space for Life?s EDI committees, we are committed to the professional integration of people from groups that are traditionally underrepresented in the physics research community.
If you have any questions about this fellowship application, please contact Olivier Hernandez, olivier.hernandez @ montreal.ca
If you have any questions about IREx, please contact Marie-Eve Naud, marie-eve.naud @ umontreal.ca
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| Postdoctoral Position in Galactic Archaeology | Closing date: 2025-05-31
Contact: Nadège Lagarde |
| We invite applications for one postdoctoral position at the Bordeaux Laboratory for Astrophysics, France, to work on the characterisation of old Galactic stellar populations. | | ▸ more | The successful candidate will join the research team led by Dr N. Lagarde and work on PRIMA (PRobing the origIns of the Milky WAy's oldest stars), a project funded by the French National Research Agency (ANR) and the Swiss National Science Foundation (SNSF). PRIMA is an international collaboration with a team led by Prof. C. Charbonnel at the Department of Astronomy of the University of Geneva, Switzerland.
PRIMA focuses on the Galactic structures hosting the oldest stars of the Milky Way, namely the halo, thick disc, and globular clusters (GC), which are key tracers of the Galaxy's merger history. The project employs stellar population synthesis models to simulate the present-day stellar content of the Milky Way, combining state-of-the-art stellar evolution models with Galactic formation scenarios. By comparing simulated mock catalogues with multi-wavelength survey data, including Gaia data combined with spectroscopic and asteroseismic constraints, PRIMA offers a unique perspective on Galactic evolution. Unlike other approaches, it eliminates selection biases in data analysis and accounts for internal stellar processes that alter chemical abundances and impact stellar lifetimes. The project aims to disentangle in situ and ex situ origins of old stars and to assess the effects of mergers and secular evolution (e.g., radial migration) on Galactic stellar populations, including globular clusters and their escaped stars.
The postdoctoral researcher based in Bordeaux will focus on characterising and dating merger events in the halo and thick disc, using the Besançon Galactic Model (BGM), a well-established Galactic stellar population synthesis tool. We seek a highly motivated and creative researcher capable of developing new strategies to interpret Galactic surveys and correct for selection biases to better understand the oldest stellar populations of the Milky Way. We welcome applications from candidates with expertise in observational, theoretical, or computational astrophysics, particularly in the fields of stellar and Galactic evolution. The ideal candidate has good knowledge of English and solid programming skills. We treasure diversity in the Prima collaboration and strive to foster an inclusive, collegial and supporting environment where anyone can feel welcome and valued regardless of background or identity.
Position Details
- Duration: 2 years
- Starting Date: Autumn 2025 (flexible within reasonable limits)
- Location: Laboratoire d'Astrophysique de Bordeaux, University of Bordeaux, France
- Benefits: Full health insurance and social security coverage (as per French law)
- Funding: Support for travel to international conferences and collaborations
Application Process
Applicants should submit the following documents in a single PDF file:
1) Curriculum Vitae (including a list of publications);
2) Research statement (max. 4 pages) outlining past achievements, research interests, and envisioned contributions to PRIMA;
3) PhD diploma (or an official statement confirming its expected completion date).
Additionally, at least two letters of recommendation should be sent directly by the referees.
Send all applications and information requests to nadege.lagarde @ u-bordeaux.fr.
The review of applications will start immediately and will continue until May 31, 2025 or until the position is filled. The hiring process and the working relationship will adhere to the principles of diversity and inclusion upheld by our parent institutions.
The full announcement can be found at the following link: https://perso.astrophy.u-bordeaux.fr/~nlagarde001/Postdoc_position.pdf
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| Studentship at the European Southern Observatory | Closing date: 2025-04-20
Contact: Evelina Dietmann |
| The European Southern Observatory (ESO) offers an exceptional opportunity for PhD students to conduct research in a dynamic and scientifically rich environment. Our Studentship Programme allows students to work at one of the world's leading observatories for a period of one to two years. | | ▸ more | Are you a PhD student looking to immerse yourself in one of the world's most dynamic scientific environments? The ESO Research Studentship Programme offers an unparalleled opportunity to join the vibrant community of one of the leading observatories on the planet for up to two years.
Why ESO? ESO is Europe?s premier intergovernmental astronomy organisation, home to approximately 110 staff astronomers, 40 Fellows, and 40 PhD students. Our team conducts cutting-edge research across a broad range of fields, from exoplanets to cosmology, in a collaborative and stimulating setting that?s hard to match.
Elevate Your PhD Experience with a Studentship at the European Southern Observatory (ESO)
Who Can Apply? We welcome applications from students enrolled in PhD programmes in astronomy or related scientific fields. As an ESO student, you will work on your doctoral project under the guidance of your home university supervisor while benefiting from the co-supervision of an ESO staff astronomer. You will spend a minimum of six months in Chile or one year in Germany, with a maximum stay of two years. Positions are available at ESO?s headquarters in Garching, near Munich (Germany) and in Santiago (Chile), with special opportunities for students from Chilean universities.
Ready to Apply? If you are eager to enhance your PhD journey with an extended stay at ESO, visit ESO Studentship Employment Conditions for details on employment conditions and benefits. https://www.eso.org/public/jobs/conditions/students/
Apply online at ESO Recruitment. https://recruitment.eso.org/
Deadline: 20 April 2025.
Applications will be reviewed as soon as the deadline passes.
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| ESA Archival Research Visitor Programme | Closing date: 2025-04-30
Contact: Guido De Marchi |
| To increase the scientific return from its space science missions, the European Space Agency (ESA) welcomes applications from scientists interested in pursuing research projects based on data publicly available in the ESA Space Science Archives (https://www.cosmos.esa.int/web/esdc). | | ▸ more | The ESA Archival Research Visitor Programme is open to scientists, at all career levels, affiliated with institutes in ESA Member States and Collaborating States, although we will also consider strong applications from outside those states. Early-career scientists (within 10 years of the PhD) and PhD students are particularly encouraged to apply. We encourage applications from women and minorities. The 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 before 1 May 2025 will be considered for visits in autumn and winter 2025/2026.
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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| Chief Scientist | Closing date: 2025-04-13
Contact: Heather |
The Chief Scientist will have a strong record of astronomical research, a deep understanding of modern, state-of-the art astronomical facilities with extensive experience of radio astronomy interferometry. The appointee must be globally recognised as a leading researcher in their field, and have a demonstrable record of shaping scientific thinking across a broad community. They will be expected to communicate well and effectively across the Observatory and the SKAO?s science community.
Apply here: https://recruitment.skao.int/vacancy/chief-scientist-579979.html | | ▸ more | The Chief Scientist will be based at the SKAO Global Headquarters at the iconic Jodrell Bank Observatory, Cheshire, UK, and will be part of the executive team reporting to the Director-General. International travel will be required.
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.
Key Responsibilities, Accountabilities and Duties
The Chief Scientist will:
-Champion the scientific capabilities and accomplishments of the SKA Observatory;
-Be the primary face of science to the SKAO science community, the SKAO Council, and to the Science and Engineering Advisory Committee, and be responsible for actively shaping the Observatory science strategy;
-Have responsibility for the co-ordination of the scientific priorities for the SKA Observatory Development Plan, and the development of the Science Roadmap (through consultation including community workshops with the science community and expert advisory groups);
-Act as the Science ?Head of Profession? for the Observatory:
-Mentoring scientific staff (all PhD scientists with a research component to their role), cultivating their professional growth and participating in promotion reviews; and
-Advocating for the scientific interests and research time of all scientific staff;
-Work with the Director of Operations to maximise the overall scientific return of the Observatory;
-Effectively promote the values and culture of the SKA Observatory, within the Observatory, in relations with partner organisations and in the global SKA scientific community;
-Establish and oversee an SKAO post-doctoral research programme;
-Conduct their own independent research.
Mandatory Knowledge, Skills and Experience
-A PhD in astronomy or physics and an international reputation in astronomy;
-A strong track record of research in astronomy;
-An understanding of the science enabled by the SKAO, with in depth knowledge of the environment and context for developing SKAO as an advanced scientific facility;
-A deep technical understanding of astronomical techniques, including extensive experience of radio interferometry;
-A track record of leadership with scientific research groups;
-A strategic thinker, with a track record of working across international, diplomatic and cultural boundaries to build commitment to a common science strategic vision;
-Advanced communication and influencing skills demonstrating an ability to build consensus within diverse stakeholders with potentially conflicting views;
-A track record of acting as a role model and building an environment that supports organisational values, including a demonstrable commitment to Equity, Diversity and Inclusion.
Desirable Knowledge, Skills and Experience
-Familiarity with the SKA project;
-High-level experience of operating in large-scale international scientific organisations and/or observatories.
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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| PhD position: Galactic archeology through stellar spectroscopy | Closing date: 2025-03-23
Contact: Henrik Jönsson |
| One PhD-position in astrophysics is available at Malmö University, Sweden, with application deadline March 23rd 2025, and approximative starting date of September 2025. | | ▸ more | The PhD project focuses on so-called Galactic archaeology, where high-resolution stellar spectroscopy is the primary method. This means, in general terms, that spectroscopic data from individual stars, collected using large international telescopes, are used to investigate how specific parts of our galaxy, the Milky Way, have formed and evolved.
The project offers some flexibility depending on your previous experience but is expected to focus mainly on the local Galactic disk and/or globular clusters. The thesis will be built around one or more "medium-sized" sub-projects, where the research is niched by using rigorous, classical analysis methods to study thousands of stars - a methodology that is relatively uncommon. You will work together with your supervisor and colleagues to carry out both the practical analysis of stellar spectra, where elemental abundances of the stars are determined, as well as the scientific interpretation of the results: what do the measured elemental abundances reveal about the evolution of the stellar population and, in a broader perspective, the Galaxy?
The research environment is highly international, with members who have broad experience in both small-scale, classical projects and large-scale surveys. As a natural consequence of the international character of the work, you will be expected to actively participate in international conferences and workshops, conduct observations at world-leading telescopes, and, if interested and possible, participate in shorter international research exchanges.
Read more and apply here:
https://web103.reachmee.com/ext/I005/1015/job?site=7&lang=UK&validator=e5819a4704cd849685049472c0c17895&job_id=3828
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| Infrared Spectroscopy of Brown Dwarfs and/or Ultracool Dwarfs | Closing date: 2025-05-01
Contact: Stanimir Metchev |
| Prof. Stanimir Metchev at the Department of Physics & Astronomy and the Institute for Earth and Space Exploration at Western University in London, Ontario invites applications for a Postdoctoral Associate to lead analysis of JWST observations and preparations for the proposed POET Canadian space astronomy mission. | | ▸ more | The successful applicant will analyze infrared spectroscopic data with JWST MIRI or with high-dispersion spectrographs on ground-based telescopes. The JWST investigations focus on brown dwarf atmospheres and their chemical and cloud content. The ground-based programs seek a complete characterization of the ultracool dwarf population in the solar neighbourhood in preparation for the proposed transit-exoplanet mission POET (Photometric Observations of Extrasolar Transits), co-led by Metchev. POET has been identified as a top space astronomy priority in the Canadian Astronomy Long Range Plan 2020-2030 (LRP2020).
Background in spectroscopy or time series analysis would be advantageous. Further information about Prof. Metchev?s research can be found at:
https://physics.uwo.ca/people/faculty_web_pages/metchev.html
The successful applicant will be expected to actively pursue additional ground- or space-based observations in support of the above programs. The position also offers an excellent opportunity for additional collaboration with Metchev's team in the fields of optical time-domain astronomy (transiting exoplanets or stellar occultations) or telescope instrumentation (robotic observatories, infrared instrumentation). Western has access to all Canadian national telescopes, including Gemini, CFHT, ALMA, and a slew of 1-2 metre-class telescopes. Metchev's team regularly uses JWST, TESS, Hubble, NOIRLab and ESO telescopes, and the NASA/IRTF.
Remuneration is CA $70,000 per year. Western University provides a competitive benefits package (https://www.uwo.ca/hr/benefits/your_benefits/pda/index.html) for postdoctoral associates, including vision, dental, annual vacation leave, paid parental leave, and pre-negotiated annual raises. Postdoctoral Associates at Western are members of the Public Service Alliance of Canada (PSAC) union. The position is in-person at Western, with possibility of flexible hours. A CA $3,000 allowance for moving expenses, visa or security clearance fees, is also available from Prof. Metchev. The start date is flexible, but preferably no later than July 1, 2025. The appointment is for up to three years, contingent on annual progress reviews and availability of funds.
Candidates must have a doctoral degree in Astronomy or a related field, received within five years of the start of the appointment. Accommodations will be
made for career interruptions or other extenuating circumstances when evaluating
applications. Candidates should submit a CV, a 2-3-page statement of research experience and interests, and the names of three references directly to Prof. Metchev (smetchev @ uwo.ca). The position is open until filled. For full consideration, complete applications should be received by April 1, 2025. For further information, please contact Prof. Metchev.
About Western University.
Western ranks as one of Canada's top research-intensive universities. From fundamental to applied discovery and other scholarly activities, its scholars advance knowledge that provides tangible benefits for the economic, social, health and cultural development of citizens in London, in Canada and around the world.
Western Values Diversity.
The University invites applications from all qualified individuals. Western is committed to employment equity and diversity in the workplace and welcomes applications from women, members of racialized groups, Indigenous persons, persons with disabilities, persons of any sexual orientation, and persons of any gender identity or gender expression.
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| Assistant / Associate Professorship in Data-Driven Radio Astronomy / Cosmology | Closing date: 2025-04-15
Contact: Metuka |
Assistant / Associate Professorship in Data-Driven Radio Astronomy / Cosmology
DEPARTMENT/LOCATION: Department of Physics, West Cambridge
SALARY: £46,485 - £58,596 (Grade 9) or £62,098 - £65,814 (Grade 10)
REFERENCE: KA44612
CATEGORY: Academic
PUBLISHED: 15 January 2025
CLOSING DATE: 15 April 2025
We are seeking a University Assistant / Associate Professor in Data-Driven Radio Astronomy / Cosmology. | | ▸ more | Modern radio astronomy/cosmology, powered by advances in big data analysis, is at the forefront of studies to unlock the answers to some of the most fundamental physics questions of our time. We are looking for a talented early career scientist to promote and develop ambitious programmes aimed at investigating the universe via radio observations. The successful candidate will be expected to lead the development of advanced data analysis for radio astronomy/cosmology (e.g. statistical analysis, machine learning, etc), in collaboration with observational/experimental activities in Cambridge. In particular, the global astrophysics community is eagerly awaiting the start of scientific observations of the Square Kilometre Array Observatory, commonly known as SKA, the largest and most powerful radio telescope ever to exist, currently under construction. The role holder will have the opportunity to take a leading role in our existing SKA activities and grants (e.g. SKA development grants). Furthermore, we expect the successful candidate to be well-placed to lead development efforts for SKA Phase II, expected to start within the coming years.
The role holder will be a world-class researcher in one of the following areas (corresponding to Science Working Groups for the SKA project): Cosmology, Epoch-Of-Reionization, Gravitational Waves, Pulsars, and Transients.
The role holder will be based in the Department of Physics in the Astrophysics Group, located in the Battcock Centre for Experimental Astrophysics and the Kavli Institute for Cosmology in Cambridge.
Data-driven science and radio astronomy/cosmology with the SKA are areas of very active research in Cambridge, with scientists leading several ongoing projects and the development of new facilities that are expected to be ground-breaking in this research field.
Applicants should have a PhD in physics (or a related discipline), a strong record of relevant research, and must show evidence of enthusiasm and ability to teach a wide range of Physics courses successfully at both undergraduate and master's level.
Appointment will be based on merit alone. As a signatory of DORA, the University is committed to assessing research on its own merits rather than on the basis of the journal, in which it is published.
Please ensure that in the Upload section of the online application, you provide: a Curriculum Vitae (CV); a full list of publications - please highlight up to 5 papers where you have made the most significant personal contributions, with up to 4 lines of text for each such paper; a research proposal no longer than 3 pages, including half a page description of how your research plans might fit with existing activities at the Department of Physics and the wider University; a one-page statement on your approach to teaching and how you believe you can contribute to the Department's teaching programme at undergraduate and graduate level; the contact details of three referees - please make your referees aware they will be contacted shortly after the closing date.
Shortlisted applicants will be informed at the end of April 2024. They will be invited to visit Cambridge in May/June 2025 for a departmental visit, informal discussions with faculty, to give a presentation and attend a formal interview.
The position is available from 1st September 2025. There is some flexibility on the start date, which can be negotiated at the appointment stage.
Click the 'Apply' button below to register an account with our recruitment system (if you have not already) and apply online.
Informal enquiries are welcome and should be directed to Dr Eloy de Lera Acedo.
Please quote reference KA44612 on your application and in any correspondence about this vacancy.
The University actively supports equality, diversity and inclusion and encourages applications from all sections of society.
The University has a responsibility to ensure that all employees are eligible to live and work in the UK.
Apply Here: https://app.webrecruit.co/JobSeeker/ApplyOnline?jobid=131540&boardid=6197
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| PhD and Postdoctoral research position on star-forming galaxies | Closing date: 2025-03-17
Contact: Daniel Schaerer |
| The University of Geneva, Switzerland, announces a PhD and postdoctoral position on star-forming galaxies in the framework of the Swiss-French collaborative project "speXion" co-funded by the SNSF and ANR. | | ▸ more | The overall goals of speXion are to understand extremely metal-deficient galaxies, their radiation fields including up to X-rays, the feedback processes dominating these galaxies, and their contribution to cosmic reionization. The collaboration will use multi-wavelength observations from JWST, HST, XMM, Chandra, VLA, and other facilities, and state-of-the-art spectral modeling tools.
The Post-doc will work on available multi-wavelength observations of metal-poor star-forming galaxies at low- and intermediate redshift, analyze and interpret interstellar medium signatures of these galaxies. The candidate will also be encouraged to develop an independent research programme. The PhD student will primarily work on the modeling and interpretation of multi-wavelength data, including their overall SEDs and emission lines, and observations from high-to-low energies (X-rays to radio).
Both candidates will primarily work in Geneva with the group of Prof. Daniel Schaerer, within the Swiss-French collaboration co-lead by Drs. Vianney Lebouteiller (CEA, Saclay) and Hakim Atek (IAP, Paris), and with other international collaborators.
The Geneva Observatory carries out observational, interpretative and theoretical research in the fields of extra-solar planets, stellar physics, high energy astrophysics, galaxy evolution, and observational cosmology.
The appointments will start in sept-oct 2025. The duration is up to three years for the post-doc, and 4 years for the PhD. Qualified candidates are encouraged to send the following their application including the following content in a *single pdf* file via email to daniel.schaerer @ unige.ch :
- Post-doc: CV, publication list, description of research experience and interests, contact information of 3 references
- PhD student: CV, motivation letter, course transcripts, and contact information of 2-3 references
Applications received by March 17, 2025 will receive full consideration.
Informal enquiries with Daniel Schaerer (daniel.schaerer @ unige.ch) are welcome.
For information on the research teams visit
https://www.unige.ch/sciences/astro/starbursts/en/
https://irfu.cea.fr/en/dap/lfemi/star-formation-and-interstellar-medium/
http://www.iap.fr/recherche/groupes/groupes-1.php?nom=galaxies&langue=en
Included Benefits:
Standard Swiss Social Security, Accident Insurance and Pension contributions.
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