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| Postdoc in Optical Time-Domain Data Processing | Closing date: 2025-01-28
Contact: Lukasz Wyrzykowski |
| The National Centre for Nuclear Research (NCBJ) invites applications for a Postdoctoral Researcher (Adjunct) position funded by the ACME Horizon Europe grant and led by prof. Lukasz Wyrzykowski. This 1+2 year position (with a 1-year probationary period) is offered within the growing BHTOM.space project ? a virtual global observatory for time-domain astronomy. | | ▸ more | Description of tasks:
- Manage and maintain the list of astronomical targets in the BHTOM system.
- Coordinate observation requests using a global telescope network.
Enhance the existing photometric data standardisation procedures in BHTOM.
- Pursue independent research in time-domain astronomy using observing time allocated through BHTOM.
- Participate in the scientific life of the Astrophysics Division, including attending meetings, seminars, and co-organizing workshops, conferences, and other events.
- Work in a research team under the supervision of the Principal Investigator (PI) and senior co-Investigators (co-Is) on tasks related to the implementation of the ACME grant.
- Analyse observational data, interpret results and prepare scientific publications and conference presentations related to the project.
- Promote research findings through various dissemination activities.
- (Co)-supervise and provide support to PhD and undergraduate students working on the project.
Requirements:
- A Ph.D. in astronomy, astrophysics, or a closely related field.
- Proven research experience, documented through publications and conference presentations.
- Strong expertise in photometric data processing and Python programming.
- A track record of publishing in peer-reviewed journals.
- Proficiency in spoken and written English.
Additional assets:
- Documented experience in international scientific collaborations.
- Documented skills in observation scheduling and telescope data management.
- Practical knowledge of Machine Learning techniques in astronomy.
- Knowledge of additional languages is considered an asset.
Required documents:
- Curriculum Vitae
- Full publication list
- A scan/copy of degree diploma
- Two references letters, arranged by applicants and directly submitted by the letter writers before the application deadline,
- Any other possible documents that might influence the assessment
- A cover letter that explains the motivating factors for considering the position (max. 1 pp)
We offer:
- Employment in one of the largest research Institute in Poland
- Good learning environment. Support of an experienced team
- Excellence with full research autonomy and being part of a diverse and supportive team of professionals
- External and internal trainings in hard and soft skills as well as participation in conferences
- Work in Polish and international networks with research institutes and industrial companies
- Employment based on an employment contract
- Stable working conditions without overtimes and friendly atmosphere
- A rich travel budget, including opportunities to visit partner institutes and observatories (e.g., in Italy, Greece, Spain, South Africa) and attend international conferences.
- Participation in cutting-edge time-domain astronomy projects (e.g. Gaia, LSST) and global collaborations (ACME, LCO)
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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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| Observing Programme Office Astronomer | Closing date: 2025-02-12
Contact: Vacancy |
The European Organisation for Astronomical Research in the Southern Hemisphere (ESO) is the foremost intergovernmental astronomy organisation in Europe and the world's most productive ground-based astronomical observatory. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries.
| | ▸ more | Main Duties and Responsibilities:
The Astronomer within OPO is responsible for supporting the preparation and selection of observing proposals, contributes to the formulation of time allocation policies, and assists in the development of a modern proposal handling system. This includes the study and implementation on AI-based algorithms to facilitate the distribution and review process. The OPO Astronomer will oversee the handling of the Phase 1 proposals and will support users during the Phase 1 proposal preparation and submission phase. They will prepare telescope time allocation statistics and monitor the performance of the Panel and Distributed Peer Review processes. Further to this, the OPO Astronomer will support the recruitment of the Observing Programmes Committee and Panel members, and will actively participate to the implementation of the upcoming Yearly Cycle and the Fast Track Channel. They will also be responsible for fostering strong key relationships and maintaining good communication with the following key stakeholders:
* Internal: Office of the Director General, VLT, VLTI and ELT Programme Scientists, User Support Department, Paranal Science Operations, Software Engineers, ESO Archive;
* External: Principal Investigators, Observing Programmes Committee, ESO Council, ESO Scientific Technical Committee, ESO Users Committee, Member-state institutes, High-level academic or governmental officials in the Member States.
As a member of the ESO Astronomy Faculty, the OPO Astronomer is expected and encouraged to conduct a strong personal research programme and to participate actively in the scientific life of ESO.
The tasks are not limited to the above and a flexible approach and willingness to adapt are required.
Key Competences and Experience:
Essential Competences and Experience
* Strong active research programme and robust publication record;
* Gained a minimum of one postdoctoral position in a scientific research institute;
* Experience at a large, international scientific facility;
* At least three years of demonstrated user experience with the ESO workflow, telescopes and instrumentation;
* Demonstrated experience with general Optical and NIR observing techniques;
* Proficiency in working with relational databases, SQL and Python scripting;
* Strong communication skills with the ability to interact effectively, respectfully, and with integrity, with internal and external stakeholders;
* Ability to deliver clear and concise written and verbal communications, identifying key issues, evaluating options, and proposing actionable solutions;
* Demonstrated capacity to build strong collaborative relationships with geographically dispersed teams and individuals from diverse cultural backgrounds.
The successful candidate will hold a PhD in Astronomy or equivalent.
Language skills:
Language skills:
Excellent command of the English language is essential. Additional knowledge of other European languages would be an advantage.
Remuneration and Contract:
ESO offers a competitive remuneration package, including pension, medical benefits, relocation support, and family-friendly policies. Detailed employment conditions are available at https://www.eso.org/public/jobs/conditions/intstaff/
Application:
If you are interested in working in areas of frontline science and technology and in a stimulating international environment, please visit http://www.eso.org for further details.
Applicants are invited to apply online at http://jobs.eso.org/. Applications must be completed in English and should include a motivation letter, and a CV containing a publication list and a research statement. Also required are the names and contact details of three scientists familiar with your work and willing to provide a recommendation letter. Referees will be automatically invited to submit a recommendation letter. However, applicants are strongly advised to trigger these invitations (using the web application form) well in advance of the application deadline.
Deadline for applications is 12 February 2025
Interviews are expected to start soon after this date.
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| Director General (DG) | Closing date: 2025-02-28
Contact: Vacancy |
| ESO operates world-class observing sites in northern Chile, including La Silla, Paranal, and Chajnantor (home to ALMA, in which ESO is a major partner). At Paranal, ESO runs the Very Large Telescope, one of the most advanced optical observatories globally, and is completing the 39-metre Extremely Large Telescope (ELT) on Cerro Armazones. The ELT, set to become "the world's biggest eye on the sky," will be fully integrated with Paranal operations. ESO is also a founding member of the Cherenkov Telescope Array Observatory (CTAO), the most sensitive high-energy gamma-ray observatory. | | ▸ more | At its Headquarters in Garching near Munich, Germany, ESO is now seeking to appoint a new Director General (DG) as the current DG's term concludes in August 2026.
Key Responsibilities
ESO has achieved a decade of remarkable scientific, technical, and organisational success, including expanding to 16 Member States, partnering with Australia, and advancing the ELT project. The new DG will build on this foundation, leading ESO to maintain its position as a global leader in astronomy. Key responsibilities include:
* Managing ESO's diverse programme and completing the ELT project.
* Supporting operations and upgrades of the La Silla-Paranal Observatory, the instrumentation programme, and international collaborations with ALMA and CTA.
* Overseeing ESO's strategy, including the Expanding Horizons initiative, and maintaining balanced budgets.
* Sustaining ESO's excellence in science, technology, and productivity.
Experience and Skills required
The successful candidate will:
* Hold a PhD in astronomy or a related field, with recognised excellence in observational astronomy.
* Demonstrate a proven ability to develop and implement vision and strategy.
* Possess effective leadership and management experience within an international astronomical organisation or institute.
* Have expertise in leading large programmes, managing resources efficiently, and fostering a motivated workforce.
* Strong political and diplomatic skills are essential to maintaining and strengthening ESO's relationships with Member States, Chile, Australia, the international community, and key stakeholders. A commitment to sustainability, inclusivity, and diversity is expected, alongside a focus on financial, environmental, and personnel resource management.
Language and contract details
Exceptional communication skills and fluency in English are essential, with knowledge of Spanish and / or German an asset. The position, based in Garching near Munich, is a full-time post with an initial fixed five-year term, renewable once for a set period subject to performance and organisational needs. The DG is expected to live in the general Munich area. Regular travel to Chile and other international locations is required.
ESO offers a competitive remuneration package, including pension, medical benefits, relocation support, and family-friendly policies. Detailed employment conditions are available at https://www.eso.org/public/jobs/conditions/intstaff/
Application Process
Interested candidates should send a brief CV and letter of motivation to Fiona Brazil, ESO Head of Human Resources, at HOHR @ eso.org by Friday, 28 February 2025. General inquiries on the role may be directed to Professor Tom Ray, ESO Council President, at tr @ cp.dias.ie.
In-person interviews for shortlisted candidates will be held in early May, with final interviews scheduled for October. Applicants will participate in assessment activities during the selection process. The selected candidate is expected to join in the first half of 2026 for a handover period.
ESO values diversity and is committed to equal opportunities, encouraging applications from all qualified candidates. Recruitment preference will be given to nationals of ESO Member States, Australia, and Chile.
For more information about ESO, please visit www.eso.org.
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| Postdoctoral Position (m/f/x) in Intensity Mapping and Machine Learning at the MPIfR Bonn, Germany | Closing date: 2025-01-27
Contact: Prof. Dr. Jonathan Pritchard |
| The MPIfR is recruiting a postdoctoral researcher to join the new research group of Prof. Jonathan Pritchard. The scientific focus of the group is radio cosmology and machine learning, in particular the combination of intensity mapping in 21 cm and other atomic lines, with CMB and other large surveys, to learn about the epoch of reionization, cosmic dawn, and cosmology. | | ▸ more | The successful candidate will have scientific interests, qualification and skills matching these aims. They will be expected to conduct a dynamic research program targeting these core scientific objectives, in collaboration with Prof. Pritchard.
As part of this research, the selected candidates will be expected to take part in the project-based efforts of the group, with themes including:
1. Statistical inference of cosmology & astrophysics from 21cm intensity maps with SKA
2. Joint simulation and modelling for line intensity mapping and 21cm experiments
3. Development of novel machine learning techniques for intensity mapping experiments
Necessary criteria:
- A PhD in physics, astronomy or a related field by the appointment date
- A good proficiency in scientific writing supported by previously written research articles/thesis/etc.
- Experience in programming, modifying, and testing numerical software
- Experience with research in cosmology or astrophysics
Desirable criteria (one or more of):
- Experience with research in 21cm cosmology, intensity mapping or reionization
- Experience working with machine learning/data science techniques
Application Process:
Interested and qualified individuals are encouraged to apply by submitting the following:
- curriculum vitae
- list of publications
- research statement
Arrange to have at least two letters of recommendation sent to jpritchard @ mpifr-bonn.mpg.de
Please submit your application through the MPIfR application portal given the link below and arrange for reference letters by Jan 27, 2025.
https://jobs.b-ite.com/en/jobposting/aff3898c2a075a826e0ab47a02fbd1b7d6cc677f0/apply
Terms of Employment:
The initial appointment is for two years with the possibility of further extension for one year after review. The preferred start date is 1 October 2025, but this is open to discussion. Dedicated funds will be made available for the postdoc to present their work in national and international conferences. Remuneration is within the framework of the German wage agreement for the public service (TVöD-Bund) in level 13, which includes comprehensive healthcare coverage and social benefits.
The Max Planck Society is committed to increasing the number of individuals with disabilities in its workforce and therefore encourages applications from such qualified individuals. Furthermore, the Max Planck Society seeks to increase the number of women in areas where they are underrepresented and therefore explicitly encourages women to apply.
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| ERC postdoc (3-yr): Large-scale structure, AGN and/or clusters with radio data | Closing date: 2025-01-31
Contact: Francesco de Gasperin |
We are inviting applications for one postdoc in the framework of the Ultra Low Frequency Universe project funded by the ERC Consolidator Grant ULU. The duration of the contracts is 3 years and it will be based at the Institute of Radioastronomy (IRA INAF) in Bologna, Italy.
Main research topics include: the physics of galaxy clusters, AGN, ICM, and cosmic ray acceleration processes | | ▸ more | The successful candidate will have the chance to work with the LOFAR telescope and other SKA precursors and pathfinders to study the Universe at the lowest frequencies with emphasis on the physics of galaxy clusters, AGN, ICM, cosmic ray acceleration processes and the development of novel techniques for big data analysis.
The postdocs will be based at the Institute of Radio astronomy (IRA - INAF) in the city of Bologna (Italy) and they will be part of the quickly growing group of low-frequency radio astronomers at IRA (further info: https://www.ulu.radio). The candidates will have the chance to interface with the large astronomical community (>200 people) present in Bologna (including those working at IRA INAF, OAS INAF and UniBO department). The candidates will be part of the LOFAR collaboration and will have privileged access to data. The candidate will have access to state-of-the-art computing facilities and to large survey data from MeerKAT, LOFAR and other telescopes. Funding for computing and travel will be available and strong international collaborations are expected with the possibility of extended periods abroad. The position come with no teaching duties. A PhD in astronomy, physics, or equivalent is a requirement.
The application must include:
- CV
- Filled annex A and B (see website)
- A copy of the ID card
- Copy of phd certificate valid in Italy (or any master certificate with documented declaration to have at least 3 yrs of research experience, including the PhD period)
- Signed list of the attached material
Details about the positions, as well as instructions on the application procedure, deadlines, and requirements are available at this link: https://www.ulu.radio/positions
Interested candidates are encouraged to get in touch with the PI of the project for further information and questions on the application procedure (Francesco de Gasperin <fdg @ ira.inaf.it>).
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| Two 5-year ERC-funded positions in computational astrophysics | Closing date: 2025-01-26
Contact: Ondrej Pejcha |
| We invite applications for two postdoctoral positions in the area of computational astrophysics in the research group of Dr. Ondrej Pejcha (http://utf.mff.cuni.cz/~pejcha/). | | ▸ more | The successful candidates will pursue original research aligned with the group's interests leading to high-impact publications, lead the development of advanced computational tools utilizing the discontinuous Galerkin method, conduct multi-dimensional simulations of fundamental processes in binary stars (mass transfer and mass loss, accretion, explosions, pulsations, turbulence, mixing, etc.), apply simulation results to specific types of binary systems (tidally-deformed or mass-transferring stars, chemically-homogeneous gravitational wave progenitors, classical novae, Type Ia supernovae, circumbinary disks around supermassive black holes, etc.), and engage in the group's scientific activities, with optional opportunities to mentor students.
We encourage candidates with diverse research profiles, from computational tool development to broadly interpreted astrophysical theory, to apply. Previous experience with hydrodynamics in astrophysics and/or the discontinuous Galerkin method is advantageous but not required. Applicants must have a PhD in astronomy, computational physics, or a related field by the start date of the appointment.
The research group has access to a dedicated computer cluster, which will be soon expanded with new GPU-enhanced nodes. The group has been successful in applying for time on national supercomputing infrastructure with postdocs and students leading the proposals. The group is connected to observational efforts in time-domain astronomy as part of the All-Sky Automated Survey for Supernovae and other theoretical and observational collaborations.
The positions are financed from ERC Consolidator grant "ROGALLO". Each position will be initially awarded for one-two years, but extensions up to a total of five years are possible given mutual interest and satisfactory performance. Funds for travel and invitation of guests are available. Informal inquiries are welcome (pejcha @ utf.mff.cuni.cz).
To apply, please submit structured CV, list of scientific and publication activity, and motivation letter to positions @ matfyz.cuni.cz by the application deadline and with the reference code 202501-PD-MFF-UTF-101 in the Subject. Please make sure that two recommendation letters sent directly by the referees are received at the same email address by the deadline. Official job advertisement page is at https://cuni.cz/UKEN-1573.html?&pracid=202501-PD-MFF-UTF-101
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| ERC Research Fellow in Extrasolar Atmospheres at Trinity College Dublin | Closing date: 2025-01-06
Contact: Johanna Vos |
| We invite applications for a 3-year Research Fellow position in the area of Extrasolar Atmospheres at Trinity College Dublin (TCD), Ireland. The successful candidate will join Prof. Johanna Vos?s research group in the School of Physics. The position will focus on the study of giant extrasolar worlds and is funded by the ERC Starting Grant Exo-PEA (Exometeorology: Probing Extrasolar Atmospheres). | | ▸ more | We invite applications for a 3-year Research Fellow position in the area of Extrasolar Atmospheres at Trinity College Dublin (TCD), Ireland. The successful candidate will join Prof. Johanna Vos's research group in the School of Physics. The position will focus on the study of giant extrasolar worlds and is funded by the ERC Starting Grant Exo-PEA (Exometeorology: Probing Extrasolar Atmospheres).
The candidate will work towards the goals of the ERC project, which aims to disentangle extrasolar weather processes such as clouds, winds and aurorae. The ideal candidate will have expertise in observational and/or theoretical studies of brown dwarfs and/or giant exoplanets. The candidate will have access to multiple observational datasets from world-class facilities including the James Webb Space Telescope and Very Large Array. Applicants must have a PhD in Astrophysics or related field, or have satisfied the requirements of a PhD by the time of appointment.
The successful candidate will also become part of the Trinity Astrophysics Group, a friendly and vibrant environment where world-leading research on exoplanet systems/atmospheres, supernovae, pulsars, and light pollution takes place. Trinity?s campus is located at the heart of Dublin, which hosts a number of other astrophysics research institutes with an active community in Star and Planet Formation+Exoplanets. Trinity has access to ESO and ESA facilities such as ALMA, JWST, HST, the VLT, and soon the ELT, as well as both EU and Irish research career development opportunities, with multiple ERC, Marie-Curie and Royal Society URF fellowship awardees in the group. The successful applicant will contribute to the supervision of students and have the opportunity to gain teaching experience within the School of Physics.
The full-time position is available for three years, with a nominal start date of September 1st, 2025. The starting salary will normally be in the range E46,305-E50,168 depending on qualifications and experience, plus benefits and funding for travel and relocation costs. The group has access to dedicated computing servers and high-performance computing facilities through Trinity's Research IT and the Irish Centre for High-End Computing (ICHEC).
Applicants should submit a cover letter, a CV with publication list, two letters of recommendation (max 2-pages), and a (max 3-page) research statement. Complete applications received by the application deadline of January 6th, 2025 will receive full consideration. Applications from traditionally under-represented minorities in physics and astronomy are particularly welcome.
Applications, references, as well as any queries, can be submitted via email to astrojobs @ tcd.ie - please include Extrasolar Atmospheres Research Fellow application in the subject heading.
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| ERC Research Fellow in Exoplanetary Systems at Trinity College Dublin | Closing date: 2025-01-06
Contact: Luca Matrà |
| We invite applications for a 3-year Research Fellow position in Exoplanetary Systems at Trinity College Dublin (TCD), Ireland. The successful candidate will join Prof. Luca Matrà's E-BEANS ERC-funded research group, with the overarching goal of understanding the potential for young Earth analogues to be provided with volatile molecules in the latest stages of formation. | | ▸ more | The candidate's work will be in the broad areas of exocometary belts and/or detection of exoplanets in these systems and/or volatile delivery mechanisms. The group is leading large collaborations including the REASONS survey and the ARKS ALMA Large program, and benefits from multiwavelength expertise with HST, VLT/CRIRES+ and JWST data. The group also has access to dedicated computing servers and high-performance facilities.
Applicants must have a PhD in Astrophysics or related field, or have satisfied the requirements of a PhD. Preference will be given to applicants with expertise specific to the areas described above, but consideration will be given to candidates more broadly experienced with circumstellar disks and/or exoplanets and/or planet formation, both theory and observations.
The candidate will actively contribute to and interact with the group and the broader Trinity Astrophysics Group, a friendly and vibrant environment researching exoplanet systems/atmospheres, supernovae, pulsars, and light pollution, currently including three ERCs, as well as Marie-Curie and Royal Society fellowship awardees.
The full-time position is available for three years starting on September 1st, 2025 (negotiable). The starting salary will normally be in the range EUR 46,305-48,896 depending on qualifications and experience, plus benefits and funding for travel and relocation costs.
Applicants should submit a cover letter, a CV with publication list, two letters of recommendation (max 2-pages), and a research statement (max 3-pages). Complete applications received by the application deadline of January 6th, 2025 will receive full consideration. Applications from traditionally under-represented minorities in physics and astronomy are particularly welcome.
For full details, please see: https://tinyurl.com/5n77ucnk
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| TWO ERC-FUNDED POSTDOC POSITIONS IN EXOPLANETS WITHIN THE "THIRSTEE" PROJECT | Closing date: 2025-01-15
Contact: Rafael Luque |
| We invite applications for two postdoc positions in exoplanets at the Instituto de Astrofísica de Andalucía (IAA-CSIC) located in Granada (Spain) within the ERC-funded "THIRSTEE" project led by Dr. Rafael Luque. The desired starting date is Fall 2025. | | ▸ more | THIRSTEE aims to decipher the enigmatic nature and origin of planets with sizes between Earth and Neptune, also known as sub-Neptunes. The project is based on state-of-the-art observations using a multi-technique approach combining transit, radial velocity, atmospheric characterization, and novel statistical analyses. The THIRSTEE team at IAA-CSIC will be composed of three PhD students and two postdocs, and will have frequent interactions with collaborators of the THIRSTEE project in other institutions worldwide (incl. USA, UK, and Spain).
The candidates must have a background on the analysis and interpretation of exoplanet data. One postdoc will contribute to the analysis of the guaranteed radial velocity data of transiting sub-Neptunes and development of new projects. Another postdoc will contribute to the analysis of the JWST observations already granted to the team and the development of new proposals and projects aiming to understand the atmospheric and interior composition of sub-Neptunes. Both postdocs will also be involved in the mentoring of the PhD students of the group.
All the information for each position and how to apply can be found here:
- Postdoc on Atmospheres:
https://www.iaa.es/empleo/erc-funded-postdoc-position-exoplanet-atmospheres-within-thirstee-project
- Postdoc on Exoplanet Characterization:
https://www.iaa.es/empleo/erc-funded-postdoc-position-exoplanet-radial-velocity-observations-within-thirstee-project
Please contact Dr. Rafael Luque (rluque @ uchicago.edu) for specific information about the positions.
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| Experimental Astro-Physicist (m/f/d, 100% E13 TV-L) | Closing date: 2025-01-15
Contact: Prof. Andrea Santangelo |
The position is expected to be filled from the 1 st of March 2025 and the initial appointment will
be for 3 years. The position is a ?wissenschaftliche Mitarbeiterstelle?, remuneration is in
accordance with pay grade E13 (100%) of the German public-sector collective agreement TV-L. | | ▸ more | The planned work will take place as part of the ATHENA project, one of the candidates for ESA?s
large observatories. Tasks comprise different aspects of electronics development, which are
carried out by the high energy astrophysics section of the institute. The successful candidate is an
outstanding experimental physicist with a Doctoral title in Astrophysics / Physics or with a very
good Master degree (or equivalent) with a focus on electronics.
We require a solid background in digital electronics development and substantial experience in
the layout of PCBs. We expect a deep knowledge of FPGA related workflows and familiarity with
hardware description languages like VHDL and the respective development environments (Xilinx,
Microchip). In addition, candidates should be experienced in the design- and manufacturing-
processes for multi-layer PCBs with current layout software tools. Presentation and
documentation of the work results in project meetings across Europe is another essential part of
the assignment. A background in space research or additional knowledge in the fields of
microcontrollers, embedded systems and ethernet protocols is considered an asset.
The High Energy Astrophysics Group of IAAT has a wide range of interests, including experimental
developments in X-ray and TeV Astronomy. Main projects include eROSITA, ATHENA, H.E.S.S., CTA,
eXTP, THESEUS, HERMES and GIFTS. We are conducting data analysis and modelling of multi-
wavelength observations of galactic compact sources, supernova remnants, and for indirect dark
matter search.
The University of Tübingen is committed to equal opportunity and diversity. Applications from
equally qualified candidates with disabilities will be given preference. We invite qualified women
to apply. The position is generally suitable for part-time work.
Applications, including a full curriculum vitae, motivation letter, list of publications and the names
and email addresses of at least two references, should be sent, as soon as possible and not later
than the 15 th of January 2025, via e-mail (single pdf preferred), to the head of the section high
energy astrophysics: Prof. Andrea Santangelo, andrea.santangelo @ uni-tuebingen.de
The responsibility for the employment lies with the administration of the University of Tübingen.
For further information: Prof. Andrea Santangelo, +49 7071 29-76128, andrea.santangelo @ uni-
tuebingen.de
Related links:
The link to the job ad on the university pages: https://uni-tuebingen.de/en/university/careers/newsfullview-job-advertisements/article/experimental-astro-physicist-m-f-d-e13-tv-l-100/
A link to the group webpage:
https://uni-tuebingen.de/fakultaeten/mathematisch-naturwissenschaftliche-fakultaet/fachbereiche/physik/institute/astronomie-und-astrophysik/astronomie-hea/forschung/prof-santangelo-abteilung-hochenergieastrophysik/
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| 162153 Tenure Track Assistant Professor of Origin of Life Research | Closing date: 2025-01-15
Contact: Professor Anders Johannes Hansen |
| The University of Copenhagen seeks to appoint a tenure track assistant professor to commence 1 June 2025 or as soon as possible thereafter. | | ▸ more | The University of Copenhagen seeks to appoint a tenure track assistant professor to commence 1 June 2025 or as soon as possible thereafter.
Job description
The Globe Institute invites applications for a tenure track assistant professorship in Origin of Life research at the Centre for Star and Planet Formation.
The Centre for Star and Planet Formation is a multidisciplinary research centre focused on understanding the formation of planetary systems, including the Solar System, using a multidisciplinary approach that combines astronomy, astrophysics and cosmochemistry. Globe Institute is a recently established department at the Faculty of Health and Medical Sciences, University of Copenhagen. Globe aims for interdisciplinary research, teaching and outreach and therefore has a strong focus on developing transformative science across our planet?s history.
The successful candidate is expected to lead original scientific research into addressing fundamental questions in the origin of life and/or the connection between the metabolism of a young biosphere and the early planetary conditions. It is an important requirement that the candidate?s research profile complements our existing research groups at StarPlan who focus on understanding planet formation, planetary composition, and the volatile budgets of rocky planets. We further expect candidates to have a strong interest in multidisciplinary approaches to the origin of life that span several disciplines at StarPlan and/or Globe Institute (such as biology, chemistry, geology, geochemistry, cosmochemistry and planetary astrophysics). A start-up package will be provided. The candidate will be supported in actively applying to secure external funding to building and expanding the research group. Potential to successfully apply for external funding is an important assessment criterion.
The tenure track assistant professor?s responsibilities will primarily consist of:
research, including publication/academic dissemination
research-based teaching
sharing knowledge with society
participation in formal pedagogical training programme for assistant professors
The tenure track assistant professor?s performance will be evaluated through annual evaluations. Furthermore, the tenure track assistant professor will be evaluated in a mid-track appraisal.
After no more than six years of employment and on condition of a positive final appraisal, the tenure track assistant professor will be employed as associate professor. Read more about tenure track at the University of Copenhagen here: http://employment.ku.dk/tenure-track/tenure-track-at-ucph/
Required qualifications
Six overall criteria apply for assistant professor appointments at the University of Copenhagen. The six criteria (research, teaching, societal impact, organisational contribution, external funding and leadership) are considered a framework for the overall assessment of candidates. Find information about each criterion here: https://employment.ku.dk/faculty/criteria-for-recognising-merit.
Furthermore, each applicant must be able to document:
A PhD degree or similar qualifications within the subject area
Research experience within the field of the position
The tenure track assistant professor must have an academic standing showing internationally competitive research, and/or have internationally recognized high potential to make a future impact.
The assistant professor is also required to possess good interpersonal and communicative skills.
Place of employment
The place of employment is at the Section for Star and Planet Formation, Øster Voldgade 5-7, 1350 Copenhagen K.
About Globe Institute
The Globe Institute is part of the Faculty of Health and Medical Sciences at the University of Copenhagen. The Institute?s main purpose is to address basic scientific questions through interdisciplinary approaches. The institute operates at the intersection of natural and medical sciences and the humanities. Information on the institute can be found at: http://www.globe.ku.dk/.
The Globe Institute is committed to creating an inclusive and diverse environment where employees and students can belong and thrive. See website for more information. All qualified applicants will receive full consideration. Candidates who, through their research, teaching, and/or service, contribute to diversity and competencies of our Institute are encouraged to apply. The University of Copenhagen strives to offer a family friendly and flexible working environment with a sustainable balance between work- and private life, including parental leave schemes (up to 47 weeks for both parents) and up to six weeks of paid holidays per year. Researchers that have not been tax liable in Denmark for the last 10 years can apply for a special (reduced) tax scheme. The university offers a variety of services for international researchers and accompanying families.
Terms of employment
The position is permanent and the average weekly working hours are 37 hours per week.
Salary and other terms and conditions of appointment are set in accordance with the Agreement between the Ministry of Taxation and AC (Danish Confederation of Professional Associations) or other relevant professional organisations.
The position is covered by the Job Structure for Academic Staff at Universities 2020.
Questions
For further information, please contact Head of Department Professor Anders Johannes Hansen (ajh @ sund.ku.dk) or Professor Anders Johansen (anders.johansen @ sund.ku.dk).
Foreign applicants may find the following links useful: http://www.ism.ku.dk/ (International Staff Mobility).
Application due
1/15/2025
Application
Please read the full job description and apply at the university homepage
https://candidate.hr-manager.net/ApplicationInit.aspx?cid=1307&ProjectId=162153&DepartmentId=19217&MediaId=4638
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