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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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| TWO ERC-FUNDED PHD POSITIONS IN EXOPLANETS WITHIN THE "THIRSTEE" PROJECT | Closing date: 2025-01-15
Contact: Rafael Luque |
| We invite applications for two PhD 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. The PhD degree will be granted by the University of Granada. | | ▸ 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).
We are seeking a talented and highly motivated student to work at the frontier of the rapidly moving field of exoplanets. One of the students will contribute to the data reduction and analysis of JWST observations, developing new data modeling and noise mitigation techniques. The other student will contribute to the measurement of precise and accurate bulk densities of small planets using transit and radial velocity observations from state-of-the-art facilities worldwide.
All the information for each position and how to apply can be found here:
- PhD on Atmospheres:
https://www.iaa.es/empleo/erc-funded-phd-position-exoplanet-atmospheres-within-thirstee-project
- PhD on Exoplanet Characterization:
https://www.iaa.es/empleo/erc-funded-phd-position-exoplanet-characterization-within-thirstee-project
Please contact Dr. Rafael Luque (rluque @ uchicago.edu) for specific information about the positions.
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| Multiple PhD positions at the University of Bristol | Closing date: 2025-01-15
Contact: Dr Natasha Maddox |
| We are currently accepting applications for the 2024-2025 recruitment round, for start dates around September 2025. Here you can find information on our PhD Studentships, including descriptions of projects available, and details on how to apply. The deadline for applications is Wednesday, 15 January, 2025. | | ▸ more | The Astrophysics Group offers a limited number of fully funded PhD studentships for research projects in astrophysics, leading to a PhD degree from the University of Bristol. Funding sources include, but are not limited to, STFC and the University. Depending on the source of funding, the duration of the studentship ranges from 3.5 to 4 years.
We encourage applications from any suitably-qualified students (usually with a first class or upper second class degree in Physics or a related subject) from the UK or overseas. Our normal recruiting cycle for funded PhD places runs from October through January each academic year. Please check this website during that time for updates on which projects are available. Applications for funded studentships received outside this window will generally not be considered, unless specifically advertised as available.
Please follow the instructions on this webpage:
https://www.bristol.ac.uk/physics/research/astrophysics/postgrad/phd-studentships/
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| Research Associate in Data-Intensive Astrophysics | Closing date: 2024-12-01
Contact: Sotiria Fotopoulou |
| Applications are invited to a Postdoctoral Research Associate position, working in the application of machine-learning methods to the Euclid dataset with Dr Sotiria Fotopoulou at the University of Bristol. The position is full-time open-ended contract, with current funding until 31st December 2027. | | ▸ more | The project will be based on exploiting the Euclid dataset, as part of the EU-funded Euclid Legacy Science Advanced Analysis Tools (ELSA) project. The successful candidate will extend the functionality of the Active-learning dashboard AstronomicAL to include access to the Euclid archive, and apply Unsupervised Learning and anomaly detection methods to the first quick-look (Q1) and first data release (DR1) of the photometric and spectroscopic Euclid data.
We encourage applications from those interested in applying machine-learning methods and further exploiting large astronomical datasets. It is expected that the applicant will have a PhD (or that their viva/defence is already scheduled) prior to starting the position. Informal enquiries (not applications) can be made to Dr Sotiria Fotopoulou (sotiria.fotopoulou @ bristol.ac.uk).
Please submit a cover letter describing how your skills and experience would prepare you for this role, a CV, and research statement including information on your previous and current research. The research statement and cover letter should be no more than 2 pages each. Please also provide information for two referees who can comment on your research record and potential.
https://www.jobs.ac.uk/job/DKO087/research-associate
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| Postdoctoral Appointment in Space Science Research | Closing date: 2024-12-15
Contact: Joseph Romano |
| The South Texas Space Science Institute (STSSI) at the University of Texas Rio Grande Valley (UTRGV) in Brownsville announces the opening of two postdoctoral appointments in space science research, broadly defined. The successful candidates are expected to actively contribute to and expand the current research activities at UTRGV in space science technology development, gravitational-wave (GW) astronomy, optical, and radio astronomy, or experimental GW detector development. | | ▸ more | The STSSI is an interdisciplinary institute with active research in various areas of space and astrophysical science. We are particularly interested in hiring creative and motivated candidates who are at ease working both collaboratively and independently in a vibrant, interdisciplinary and synergistic group.
Specifically, we are looking for one postdoc to work in the STARGATE Space Technology Group 1 (SG1). The STARGATE SG1 group is specifically focused on experimental physics and technology development with space applications. Current areas of research include phased array development (with applications in spacecraft communication and radio astronomy); testing of materials, electronics, and systems in a simulated space environment; and laser systems for space communication, precision metrology, and gravity gradiometry (including applications for space and ground-based gravitational-wave detectors). The STARGATE project has extensive research equipment and facilities for electronics and antenna testing, printed circuit board fabrication, space environment simulation, rapid prototyping, and laser and optics research.
The research area for the second postdoc is more open-ended. We are looking for the strongest possible candidate to collaborate on research projects with members of STSSI in the areas of gravitational-wave astronomy (data analysis or source modeling), optical and/or radio astronomy, or experimental GW detector development.
Applicants should have a Ph.D. in Physics or a related field, and a strong interest in leading research efforts as part of STSSI. The postdoc will also have ample opportunity to assist in the supervision of undergraduate and graduate students involved in STSSI research projects.
Appointments are for 2 years with annual renewal contingent upon satisfactory progress and funding status. The anticipated start date of the position is either Summer or Fall 2025. Applications will be considered until the position is filled. Interested candidates should apply through the UTRGV job portal.
To apply, please submit your application via the UTRGV job portal at careers.utrgv.edu for Position Number SRGV7883 or careers.utrgv.edu/postings/44961.
Review of the applications will start January 15, 2025 and continue until the position is filled.
The University of Texas Rio Grande Valley is an Equal Employment Opportunity/Affirmative Action Employer.
It is the policy of The University of Texas Rio Grande Valley to promote and ensure equal employment opportunities for all individuals without regard to race, color, national origin, sex, age, religion, disability, sexual orientation, gender identity or expression, genetic information or protected veteran status.
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| 2+1 year Postdoc on the detection and characterisation of multi-planetary systems | Closing date: 2024-12-03
Contact: Adrien Leleu |
| Applications are invited for a 2+1 year postdoc position in the Geneva exoplanet group, to start in Spring 2025. Women and candidates from underrepresented groups in Astronomy are strongly encouraged to apply. Flexible work options and family friendly work hours are possible at the University of Geneva. | | ▸ more | 2+1 year Postdoc on the detection and characterisation of multi-planetary systems
Applications are invited for a 2+1 year postdoc position in the Geneva exoplanet group, to start in Spring 2025. Women and candidates from underrepresented groups in Astronomy are strongly encouraged to apply. Flexible work options and family friendly work hours are possible at the University of Geneva.
The researchers will join the group of Prof. Adrien Leleu that focuses on the characterisation of the architecture of resonant exoplanetary systems, with strong collaboration with Prof. Xavier Dumusque and Dr. Jean-Baptiste Delisle. The team of Prof. Leleu combines space-based photometry from the Kepler/K2, TESS, and CHEOPS space missions to discover new compact multi-planetary systems and characterise them by observing and modelling the dynamical interactions between the planets (keywords: Transit Timing Variations - TTVs, photo-dynamical models). The team is also strongly involved in the preparation of the upcoming ESA mission PLATO.
Overall the exoplanet group is composed of about 40 PhD students and postdocs, and 11 faculty members, specialised in radial-velocity measurements, transit photometry, exoplanet atmosphere characterization, direct imaging as well as instrumentation. The exoplanet group is also part of the Switzerland-wide network PlanetS (http://nccr-planets.ch/), specialised in all different fields of planetary sciences with a large focus on exoplanets.
The successful applicant will work on:
(1) The vetting and characterisation of multi-planetary systems candidates in long photometric time-series identified by RIVERS (Leleu et al 2021) : RIVERS searches for planetary candidates in the lightcurve of ~200,000 Kepler targets and ~140,000 TESS targets, and will be used for the PLATO mission. The vetting of these candidates consists in defining and applying criteria on individual candidates and the coherence of the system in which they are embedded. The characterisation of each system is then done using photo-dynamical models.
(2) The definition and calibration of robustness criteria for the masses obtained by TTVs and RVs (radial velocities), in the framework of the preparation for the PLATO mission. These criteria could rely on the trial of different sets of priors and/or noise models for each time series. These criteria will then be calibrated using well characterised systems, preferably characterised by both RVs and TTVs.
Relevant experience for this position are : time series analysis (photometry, radial velocity), statistics (vetting, model comparison, etc.). and orbital dynamics/TTVs. Prior experience in the two latter is not necessary but a plus, and the candidate should be interested in learning those during the Postdoc. The positions are open for a start in the spring of 2025. For more information about the position, interested candidates should directly contact Prof. A. Leleu.
The applicant should have obtained their PhD less than 5 years before the start of this contract. Applications (concatenated in a SINGLE PDF FILE) must contain:
-A cover letter including a short (2 pages max) research statement describing relevant experience, past achievements and future projects, as well as interest in the topic;
-A curriculum vitae;
-A publication list and specific contributions to each article.
-Names, positions and e-mail addresses of up to three persons of reference that could be contacted.
Applications shall be sent to Prof. A. Leleu (adrien.leleu @ unige.ch), with c.c. to Prof. Xavier Dumusque (Xavier.Dumusque @ unige.ch) and Dr Jean-Baptiste Delisle (Jean-Baptiste.Delisle @ unige.ch). Application received by December 3rd 2024 will receive full consideration.
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| Postdoctoral Positions in Star-Exoplanet connections at Leiden Observatory | Closing date: 2024-12-08
Contact: Aline Vidotto |
| Leiden Observatory invites applications for up to 2 postdoctoral positions to join the group of Aline Vidotto, whose research ranges from stellar outflows (stellar winds, coronal mass ejections), exoplanetary outflows (bulk atmospheric escape), magnetism (stellar and planetary), with a focus on star-planet interactions. For this position, we are particularly welcoming applicants with experience in numerical modelling, preferably associated to any of the topics aforementioned. | | ▸ more | The position is funded for 4 years, consisting of an initial appointment of 2 years plus an extension of 2 years contingent on satisfactory performance. Starting date is negotiable, but preferably before 1 September 2025. For more information about the position and how to apply, please visit
https://edu.nl/n9ckg
Leiden Observatory is a lively world-class university astronomy department that covers a wide range of science. We are the largest astronomy department in the Netherlands, with about 35 faculty members, 40 postdoctoral researchers, 30 support staff, 70 PhD students and 100 MSc students. Leiden itself, is a charming university town with international flair with easy connections to other European countries.
Leiden Observatory is dedicated to providing an inclusive, equitable, and supportive environment for everyone.
Interested candidates should upload their applications by 8 December 2024. The application should contain a cover letter, CV, publication list, and a statement of research experience and future research interests (2-3 pages). Please mention how the candidate?s past experience and his/her/their skills could complement the research carried out in Vidotto?s research group. Candidates should arrange for three reference letters to be submitted before the indicated deadline.
Benefits: The position comes with a competitive salary and comprehensive benefits including paid vacation, sick leave, disability insurance, maternity and parental leave, and social security and retirement benefits. Medical insurance is compulsory but not included and costs on average 150 euro/adult/month.
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| Postdoc in Exoplanets - DTU Space | Closing date: 2024-12-20
Contact: Lars A. Buchhave |
| The Exoplanet Group at DTU Space is extensively engaged in the detection and characterization of exoplanets through observations and modelling. | | ▸ more | The Exoplanet Group at DTU Space at the Technical University of Denmark, situated in the greater Copenhagen area, invites applications from highly qualified individuals for two postdoctoral positions of three-year duration in exoplanet research. The Exoplanet Group at DTU Space is extensively engaged in the detection and characterization of exoplanets through observations and modelling. Our group has a particular interest in atmospheric studies of terrestrial and sub-Neptune exoplanets and extreme prevision radial velocities, but if you have interests in broader exoplanet areas, you are also encouraged to apply.
You will work with Prof. Lars A. Buchhave and Dr. Alexander Rathcke in the rapidly growing Exoplanet Group. At DTU Space, you will have access to data from world-class telescopes, including JWST, HST, ultra precise RV spectrographs (e.g., HARPS-N and EXPRES), and the VLT. Ongoing projects include characterizing terrestrial worlds with JWST (including several PI led programs) and scientific and technical work on the Second Earth Spectrograph (2ES, PI Buchhave, http://www.2es.dk) to discover Earth-mass planets, and work pertaining to the ESA Ariel Mission (co-PI Buchhave, https://arielmission.space). Additional information about the Exoplanet Group at DTU Space can be found at http://www.exoplanets.dk.
Responsibilities and qualifications
We are seeking talented and highly motivated researchers to work at the cutting edge of the rapidly moving research field of exoplanets. If you have previous experience in the mentioned areas of research, strong programming skills, and knowledge relating to data reduction and analysis and/or modelling of spectroscopic data, you are especially encouraged to apply. Flexibility and self-motivation are desired skills at DTU Space. In particular, the Exoplanet Group fosters a vibrant collaborative work environment, where collaboration with other group members is highly encouraged.
The above-mentioned projects will allow for you to work on a number of cutting-edge datasets, and you are encouraged to pursue independent research interests during the course of their postdoc.
As a formal qualification, you must hold a PhD degree (or equivalent).
The assessment of the applicants will be made by the end of December 2024 and shortlisted candidates will be invited to an interview in late January/early February. We expect to extend formal offers in mid-February 2025.
We offer
DTU is a leading technical university globally recognized for the excellence of its research, education, innovation and scientific advice. We offer a rewarding and challenging job in an international environment. We strive for academic excellence in an environment characterized by collegial respect and academic freedom tempered by responsibility.
Salary and terms of employment
The appointment will be based on the collective agreement with the Danish Confederation of Professional Associations. The allowance will be agreed upon with the relevant union.
The period of employment is 3 years. The starting date is flexible but would ideally commence in Q3-Q4 of 2025.
You can read more about career paths at DTU here.
Further information
Further information and inquiries about the position can be made to Prof. Lars A. Buchhave (buchhave @ space.dtu.dk) or Dr. Alexander Rathcke (rathcke @ space.dtu.dk). You can read more about the Exoplanet Group at www.exoplanets.dk and the DTU Space institute at www.space.dtu.dk.
If you are applying from abroad, you may find useful information on working in Denmark and at DTU at DTU ? Moving to Denmark.
Application procedure
Your complete online application must be submitted no later than 20 December 2024 (23:59 Danish time).
Applications must be submitted as one PDF file containing all materials to be given consideration. To apply, please open the link "Apply now", fill out the online application form, and attach all your materials in English in one PDF file. The file must include:
Application (cover letter)
CV
Academic Diplomas (MSc/PhD ? in English)
List of publications
Research statement describing your previous work and thoughts and ideas for future research (max 3 pages)
Shortlisted candidates will be asked to provide 2-3 reference letters to be emailed at a later date.
Applications received after the deadline will not be considered.
All interested candidates irrespective of age, gender, disability, race, religion or ethnic background are encouraged to apply. As DTU works with research in critical technology, which is subject to special rules for security and export control, open-source background checks may be conducted on qualified candidates for the position.
DTU Space
The Institute has about 200 employees and is located in the greater Copenhagen area at the Lyngby Campus of the Technical University of Denmark together with 19 other institutes within the technical sciences. In the Astrophysics & Atmospheric Physics Division of the Department of Space Research and Space Technology (DTU Space), current focus areas cover exoplanets, large-scale structure of the universe, physics of compact objects, space weather, upper atmosphere physics and cosmo-climatology, as well as development of instrumentation, in particular high-energy instrumentation, i.e. X- and gamma ray detectors and optics. The division is currently active in the operation of instruments and data analysis from three satellites. The division also runs four instrumentation laboratories and hosts a center for space weather research and forecasts.
Technology for people
DTU develops technology for people. With our international elite research and study programmes, we are helping to create a better world and to solve the global challenges formulated in the UN?s 17 Sustainable Development Goals. Hans Christian Ørsted founded DTU in 1829 with a clear mission to develop and create value using science and engineering to benefit society. That mission lives on today. DTU has 13,500 student
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| PhD in computational astrophysics and galaxy formation/evolution - Geneva University | Closing date: 2025-01-15
Contact: Melanie Habouzit |
| Applications are invited for a Ph.D. position (starting early Fall 2025) in computational astrophysics and galaxy formation/evolution at the Department of Astronomy of the University of Geneva (Switzerland), in the research group led by Melanie Habouzit. The position is fully funded by the SNSF Starting Grant "Constraining black hole origins with cosmological simulations?. | | ▸ more | The selected candidate will join a dynamic and passionate research group dedicated to understanding and constraining how massive black holes formed in the early Universe. The group performs and analyzes large-scale cosmological simulations of the Universe with new models for massive black hole formation. Our novel theoretical and computational framework is key in interpreting current observations of massive black holes and galaxies (e.g., from the James Webb Space Telescope) and future data from, for example, the Euclid, Roman, and Athena telescopes, and the LISA gravitational wave antenna.
The large Department of Astronomy of the University of Geneva offers a diverse research environment including theoretical and observational studies of black holes and galaxies, exoplanets, development of scientific software for space missions, and numerical simulations. The selected candidates will be part of the vibrant ?Extreme Universe? department. Geneva is one of the most international and multicultural cities in Europe with a high quality of living. Beautiful French and Swiss Alps within striking distance!
The position is for 4 years; remuneration is based on the University salary grid (Canton of Geneva). Generous funds for travel and computer equipment are included. The selected Ph.D. student will enroll in the Ph.D. programme of the Department and University (UniGE).
Applicants are expected to hold a Master degree (or equivalent degree) in Astrophysics/Astronomy or a closely related field, by the start of employment. Previous experience with extragalactic astrophysics, including observations, and/or cosmological simulations is desirable but not required.
How to apply: Applications must be submitted electronically in a single PDF to applications.habouzit @ gmail.com by January 15th (2025) and include (in the order listed below): a cover letter, a CV (maximum 2 pages), grades for the master degree (if not yet available, please send the grades of the previous year), a brief statement (maximum 2 pages) describing your research interests and experience. In addition, please arrange for 2 reference letters to be sent directly to applications.habouzit @ gmail.com by January 15th, 2025.
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| Lecturer (Teaching) in Observational Astrophysics at UCL, London | Closing date: 2024-11-15
Contact: Dr. Steve Fossey |
The Dept. of Physics & Astronomy at UCL invites applications for a Lecturer (Teaching) in Observational Astrophysics. The UCL Observatory (UCLO) is operated by the UCL Department of Physics and Astronomy, and used for teaching observational (laboratory) astrophysics to undergraduate students, and also engaging in public-outreach and research activities. The new Lecturer will be based at UCLO, and will work closely with UCLO staff and Astrophysics research colleagues, and with teaching staff in the Dept. of Physics and Astronomy.
| | ▸ more | Lecturer (Teaching) in Observational Astrophysics
Department of Physics & Astronomy, UCL
Location: London, UK
Salary: £52,487 -- £61,534 (Grade 8, inc. London weighting)
Closing Date: 15-Nov-2024
ABOUT US
UCL is one of the world's top universities based in the heart of London. UCL students taking Astrophysics-related degrees in the Department of Physics and Astronomy attend observational courses at UCL Observatory (UCLO, Mill Hill, NW London), which has a track record of astrophysics teaching, research activity and public engagement. UCLO hosts a team of academic teaching and technical staff with a broad range of expertise; and has strong links with academic research staff in the Dept's Astrophysics Group, who support the teaching and research function of UCLO, in the delivery of UCLO modules and research projects for undergraduate and masters-level students.
ABOUT THE ROLE
UCL invites applications for a Lecturer (Teaching) in Observational Astrophysics. The new Lecturer will be based at UCLO, and will work closely with UCLO and Astrophysics colleagues, and with teaching staff in Physics and Astronomy.
The successful candidate will be responsible for leading and assisting practical-class modules in observational astrophysics at UCL Observatory. They will design and develop course content and materials, translating advances in astrophysics to UCLO teaching, and developing effective assessment and feedback. They will supervise undergraduate and MSc-postgraduate student projects, making use of UCLO facilities. They will contribute to facility design and development at UCLO to extend the range of activities available to students.
Candidates will need to upload a CV (including a list of publications), and the contact information for three references. A full cover letter addressing how the candidate meets the person specification should also be included using the "Cover Letter" section of the online form.
Informal enquiries regarding the vacancy can be made to: Dr. Steve Fossey, s.fossey @ ucl.ac.uk
ABOUT YOU
The successful candidate will have a PhD in Astrophysics or closely related discipline and Fellowship of the Higher Education Academy (FHEA) or equivalent professional teaching qualification.
It is essential that you have experience of teaching astrophysics in a higher-education context, ideally within an observatory environment. You will also possess the knowledge and experience of techniques and technologies in observational astrophysics.
The ability to teach astrophysics to undergraduates and postgraduates at a high level and experience of supervising undergraduate or masters-level student research projects is key.
TO APPLY
Full details (job description and person specification) and the online application form are available at the UCL jobs page:
https://www.ucl.ac.uk/work-at-ucl/search-ucl-jobs/details?jobId=28551
WHAT WE OFFER
At UCL, we offer a competitive benefits package including 27 days annual leave plus six days (bank holidays are in addition), hybrid and flexible working, pension scheme, season ticket loan, cycle to work scheme, enhanced maternity/ paternity/ adoption pay, workplace nursery, employee assistance programme and much more!
For more information on our benefits, please visit our staff benefits webpage - https://www.ucl.ac.uk/work-at-ucl/reward-and-benefits
OUR COMMITMENT TO EQUALITY, DIVERSITY AND INCLUSION
As London's Global University, we know diversity fosters creativity and innovation, and we want our community to represent the diversity of the world's talent. We are committed to equality of opportunity, to being fair and inclusive, and to being a place where we all belong.
We therefore particularly encourage applications from candidates who are likely to be underrepresented in UCL's workforce. These include people from Black, Asian and ethnic minority backgrounds; disabled people; LGBTQI+ people; and for our Grade 9 and 10 roles, women.
You can read more about our commitment to Equality, Diversity and Inclusion here:
https://www.ucl.ac.uk/equality-diversity-inclusion/
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| Experimental Astro-Physicist (m/f/d, 100% E13 TV-L) | Closing date: 2024-11-15
Contact: Prof. Andrea Santangelo |
The position is expected to be filled from the 1 st of January 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 November 2024, 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/de/108817
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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| 11 PhD positions in astrophysics | Closing date: 2025-02-01
Contact: Antonis Georgakakis |
| 11 PhD positions on the feeding and feedback cycle of supermassive black holes are available at 10 astronomy groups across Europe from Sept 2025 as part of the Marie Sklodowska-Curie Action (MSCA) Doctorate Network TALES (Time-domain Analysis to study the Life-cycle and Evolution of Supermassive black holes). | | ▸ more | | A total of 11 doctorate research positions are available as part of the MSCA Doctorate Network TALES, (Time-domain Analysis to study the Life-cycle and Evolution of Supermassive black holes), a consortium of 10 astrophysics research groups, 8 industrial and 4 academic partners spread across Europe that aims to study the feeding and feedback cycle of supermassive black holes. The TALES doctorate candidates will (i) leverage time-domain astronomy observations from state-of-the-art facilities to map the structure of matter in the close vicinity of supermassive black holes, (ii) use novel analysis methods from the discipline of data science to maximise the information gain from the observations and (iii) develop new theories and models to interpret the data and learn about the physics of the life-cycle of black holes at the centres of galaxies. Parallel to the core research activities above, TALES aspires to implement an ambitious training programme on both technical and complementary skills that is tailored to the needs of the doctorate candidates and includes secondments to industrial and/or academic partners as well as specialised lectures and science communication events. Information about the 11 positions and application details can be found at https://euraxess.ec.europa.eu/jobs/280409 or the TALES webpage https://www.star.bris.ac.uk/TALES/
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| Astronomer - Group Head | Closing date: 2024-12-15
Contact: Evelina Dietmann |
| The Back-end Operations Department (BOD) is responsible for the management of science data from ESO's optical/near-infrared La Silla Paranal Observatory, as part of integrated end-to-end science operations. This includes the scientific and operational development of the ESO Science Archive, the generation of science data products for distribution through it, the collection, verification and archiving of data products from the community, and the scientific oversight of the reduction of ESO data. | | ▸ more | ESO copes with the increasing volume and complexity of the data generated at its facilities by providing its communities with the appropriate tools to process and calibrate it. These tools are, then, routinely used to generate processed data for publication in the ESO Science Archive. They are normally developed in close collaboration with the corresponding instrument-building consortia, to be then taken over and further developed by ESO in consultation with the wider community.
The successful candidate will lead a group responsible for assessing and improving the science quality of processed ESO data, and for generating suitably processed data for the ESO Science Archive. This includes working on any aspect that impacts the quality of processed data, e.g. frequency and nature of the calibrations, and research and development of suitable science data processing algorithms. This may include prototyping, while the production-grade implementation is the responsibility of software engineers in the ESO matrix structure. Duty travels to the ESO sites in Chile and relevant conferences/workshops are foreseen. As a Faculty Astronomer, you will be expected to balance your operational responsibilities with robust research portfolio contributing to the science community both in ESO and more widely.
Main Duties and Responsibilities:
Enhance the quality of processing of ESO raw data by:
-Assessing the quality of existing tools and data, both for direct and archival use.
-Exploring ways to enhance such quality, including processing algorithms and/or observing techniques, and/or calibration schemes.
-Prototyping solutions in commonly used programming/scripting languages, chiefly Python.
-Specifying user requirements and user stories for implementation of the chosen solutions by software engineers.
-Supervising and ensuring the generation of processed data for the ESO Science Archive.
Lead the Science Data Quality Group by:
-Supervising the work of the group members, a mix of Faculty Astronomers and Scientists. This includes assigning tasks to individual group members and performing the annual evaluations according to ESO standards and procedures.
-Coordinating with the reporting line the activities of the group within the ESO goals.
-Providing professional leadership and guidance for the group members, and ensure their alignment with the goals set by the Organisation.
-Acting as Job Manager of the pipeline software development activities.
-Liaising with other organisational units within the Back-end Operations Department, the DMO Division and, ESO at large. As a member of the ESO Astronomy Faculty, you will be encouraged and expected to carry out original research for up to 50% of their time.
Reports to:
The Head of the Back-end Operations Department.
Key Competences and Experience:
Essential Competences and Experience
-Experience with observations on a wide range of different telescopes and instruments, and the quality control of such observations.
-Hands-on experience with astronomical data processing and algorithms for a wide range of different data types. This includes a good understanding of limitations and trade-offs of methods.
-Practical understanding of the design of data reduction software and pipelines and their application for the needs of the science community.
-In depth knowledge of numerical and statistical methods as applied to astronomical data reduction.
-Excellent understanding of the user community of astronomical data, and of their needs in terms of raw and processed data.
-Strong cooperative skills to interface with other organisational units/teams.
-Critical thinking/problem solving skills.
-Excellent interpersonal, organization and communication skills.
-Demonstrable emotional intelligence in leading teams.
-Evidence of effectively developing a team through such techniques as coaching.
-Inclusiveness in dealing with people in a multicultural work environment.
Desirable Competences and Experience:
-Familiarity with ESO data and processing tools, mainly the pipelines and EDPS.
-Familiarity with the ESO Science Archive and other relevant astronomical data repositories/archives.
-Good understanding of software architecture and experience in working with software engineers to provide requirements for astronomical software projects.
-Experience with prototyping of astronomical algorithms in programming languages widely used in the astronomical community, e.g. Python.
-Familiarity with the common Python packages relevant to astronomy (astropy, numpy, matplotlib, pandas).
-Experience with graphical user interfaces for astronomy software.
-Experience with relevant Machine Learning algorithms, ideally applied to astronomy.
-Previous record in supervisory positions.
Qualifications:
PhD in Astronomy/Astrophysics, Physics or equivalent. An established track record of astronomical research and publication.
Language skills:
The position requires an excellent command of written and spoken English.
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, a CV, a publication list and a full research statement. Within your CV, please provide the names and contact details of three persons familiar with your work and willing to provide a recommendation letter upon request. Referees will not be contacted without your prior consent.
Deadline for applications is 15 December 2024.
Interviews are expected to start soon after this date.
|
| Astronomer - Back-end Operations | Closing date: 2024-12-15
Contact: Evelina Dietmann |
| The Back-end Operations Department (BOD) is responsible for the management of science data from ESO's optical/near-infrared La Silla Paranal Observatory, as part of integrated end-to-end science operations. | | ▸ more | This includes the scientific and operational development of the ESO Science Archive, the generation of science data products for distribution through it, the collection, verification and archiving of data products from the community, and the scientific oversight of the reduction of ESO data. ESO copes with the increasing volume and complexity of the data generated at its facilities by providing its communities with the appropriate tools to process and calibrate it. These tools are then routinely used to generate processed data for publication in the ESO Science Archive. They are normally developed in close collaboration with the corresponding instrument-building consortia, and are then taken over and further developed by ESO in consultation with the wider community.
You will take a leading role in assessing and improving the science quality of processed ESO data, and in generating suitably processed data for the ESO Science Archive. This includes working on any aspect that impacts the quality of processed data, e.g. frequency and nature of the calibrations, and research and development of suitable science data processing algorithms. This may include prototyping, while the production-grade implementation is the responsibility of software engineers in the ESO matrix structure. Duty travels to the ESO sites in Chile and relevant conferences/workshops are foreseen. As a Faculty Astronomer, you will be expected to balance your operational responsibilities with robust research portfolio contributing to the science community both in ESO and more widely.
Main Duties and Responsibilities:
Enhance the quality of the processing of ESO raw data by:
-Assessing the quality of existing tools and data, both for direct and archival use.
-Exploring ways to enhance such quality, including processing algorithms and/or observing techniques, and/or calibration schemes.
-Prototyping solutions in commonly used programming/scripting languages, chiefly Python.
-Specifying user requirements and user stories for implementation of the chosen solutions by software engineers.
Generate processed data for the ESO Science Archive by:
-Running the ESO pipelines for selected instrument modes to be ingested in the ESO Science Archive.
-Performing quality control on the resulting data streams.
-Following up data quality issues.
As a member of the ESO Astronomy Faculty, you will be encouraged and expected to carry out original research for up to 50% of your time.
Reports to:
The Head of the Science Data Quality Group.
Key Competences and Experience:
Essential Competences and Experience:
-Experience with observations on a wide range of different telescopes and instruments, and the quality control of such observations.
-Hands-on experience with astronomical data processing and algorithms for a wide range of different data types. This includes a good understanding of limitations and trade-offs of methods.
-Experience with the design of data reduction software and pipelines.
-Demonstrable understanding of numerical and statistical methods as applied to astronomical data reduction.
-Excellent understanding of the user community of astronomical data, and of their needs in terms of raw and processed data.
-Strong cooperative skills to interface with other organisational units/teams in a multicultural environment.
-Critical thinking/problem solving skills.
Desirable Competences and Experience:
-Familiarity with ESO data and processing tools, mainly the pipelines and EDPS.
-Familiarity with the ESO Science Archive and other relevant astronomical data repositories/archives.
-Good understanding of software architecture and experience in working with software engineers to provide requirements for astronomical software projects.
-Code prototyping in programming languages widely used in the astronomical community, e.g. Python.
-Familiarity with the most common Python packages relevant to astronomy (astropy, numpy, matplotlib, pandas).
-Experience with the design of graphical user interfaces for astronomy software.
-Experience with relevant Machine Learning algorithms, ideally applied to astronomy.
Qualifications:
PhD in Astronomy/Astrophysics, Physics or equivalent. An established track record of astronomical research and publication.
Language skills:
The position requires an excellent command of written and spoken English.
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, a CV, a publication list and a full research statement. Within your CV, please provide the names and contact details of three persons familiar with your work and willing to provide a recommendation letter upon request. Referees will not be contacted without your prior consent.
Deadline for applications is 15 December 2024.
|
| PhD position in observational solar physics at the University of Bern, Switzerland | Closing date: 2024-12-01
Contact: Lucia Kleint |
| The University of Bern hosts many domains of astronomy, from solar physics, to exoplanets, and satellite observations. The successful candidate will work in the space weather group, which focuses on understanding solar flares with machine learning, building astronomical instrumentation, and on researching the physics of the Sun. This position is part of a SERI-funded ERC CoG grant. | | ▸ more | Flares are eruptions on the Sun, which can influence the Earth by causing changes of satellite orbits, power outages, enhanced radiation, and aurora. However, solar flares can neither be reliably predicted, nor is their physics fully understood. The goal of this PhD project is to carry out research in observational solar physics, particularly by leading observations at the Swedish Solar Telescope (SST) to obtain new data of solar flares and to analyze these data to determine the structure of the solar atmosphere during flares.
The PhD student will learn about space weather, solar observations, solar data reduction, data analysis, radiative transfer, and modeling to interpret the solar atmosphere. The length of a PhD is typically 3-4 years. Support for conferences and collaborations is available.
Requirements:
- We are looking for highly motivated candidates with (or obtaining soon) a MSc in physics, astronomy, or a related topic.
- A strong interest in experimental work is desired, particularly in operating a telescope, analyzing astronomical data, and in programming.
- A background in programming in Python or IDL is desired.
- At least a basic knowledge of astronomy is required and knowledge of astronomical data analysis is beneficial.
- Strong verbal and written communication skills in English.
- Strong analytical abilities and problem solving/troubleshooting skills.
- Teamplayer who likes to work with other group members and students.
Appointment:
Starting in spring 2025, upon mutual agreement. Funding for maximally 4 years.
Application:
deadline: December 1, 2024, via email to L. Kleint, containing (as one pdf file):
- CV
- motivation letter for this specific PhD position
- a copy of BSc and MSc transcripts of courses and grades (scans of official transcripts are sufficient)
- if available, a pdf of or link to the Master's thesis (if emailed, please < 5 MB)
- Two letters of recommendation shall be sent before the application deadline directly by the referees to L. Kleint.
Salary:
Based on the regulations of the University of Bern, starting at 47 kCHF/year
Contact:
Prof. Dr. Lucia Kleint (email lucia.kleint @ unibe.ch). See https://www.aiub.unibe.ch/about_us/jobs/index_eng.html
|
| PhD position at the University of Hamburg in Cosmology x Artificial Intelligence | Closing date: 2024-11-15
Contact: LUISA LUCIE-SMITH |
Research Associate for the Project "Cluster of Excellence Quantum Universe" as PhD student in the field of Astrophysics and Artificial Intelligence.
Institution: Faculty of Mathematics, Informatics and Natural Sciences, Department of Physics, Hamburg Observatory, Cluster of Excellence "Quantum Universe"
Salary level: EGR. 13 TV-L
Start date: 01.01.2025, the initial fixed term is three years
Application deadline:15.11.2024 | | ▸ more | The Cluster of Excellence "Quantum Universe" performs research to understand mass and gravity at the interface between quantum physics and cosmology. The research team includes leading scientists from mathematics, particle physics, astrophysics, and cosmology at the University of Hamburg and DESY.
Your responsibilities
Duties include academic services in the project named above. Research associates may also pursue independent research and further academic qualifications.
The PhD will be conducted under the supervision of Prof. Luisa Lucie-Smith at the Hamburg Observatory. The research will involve developing explainable AI models for cosmology, aiming to improve our ability to model the large-scale structure of the Universe in light of upcoming galaxy surveys.
Doctoral research associates will become members of the Quantum Universe Research School (QURS), which provides academic and soft skills training, as well as career planning support. In addition, they will receive individual budgets to facilitate the attendance of summer schools and conferences, and to support other educational measures. Additional travel money for project-specific duties will be provided by the hosting research groups. Doctoral research associates may participate in teaching at the University and in the organization of the Cluster via an early career council.
Your profile
A university degree in a relevant field.
- Excellent English communication skills are required.
- Excellent candidates will have prior knowledge of astrophysics and/or cosmology, ideally in the form of an undergraduate thesis project.
- Experience in computer programming, especially in Python, is desired.
- Excellent candidates will have interest and/or prior experience in modern machine learning and deep learning approaches.
- Successful candidates are expected to pursue a PhD in Physics at the University of Hamburg. The regular duration of a PhD at the Department of Physics is three years.
We offer
Universität Hamburg?University of Excellence is one of the strongest research educational institutions in Germany. Our work in research, teaching, educational and knowledge exchange activities is fostering the next generation of responsible global citizens ready to tackle the global challenges facing us. Our guiding principle "Innovating and Cooperating for a Sustainable Future" drives collaboration with academic and nonacademic partner institutions in the Hamburg Metropolitan Region and around the world. We would like to invite you to be part of our community to work with us in creating sustainable and digital change for a dynamic and pluralist society.
The Free and Hanseatic City of Hamburg promotes equal opportunity. As women are currently underrepresented in this job category at University of Hamburg according to the evaluation , HambGleiG), we encourage women to apply for this position. Equally qualified and suitable female applicants will receive preference.
Severely disabled and disabled applicants with the same status will receive preference over equally qualified non-disabled applicants.
Instructions for applying
Contact
Prof. Dr. Luisa Lucie-Smith
luisals @ mpa-garching.mpg.de
Location
Gojenbergsweg 112
21029 Hamburg
Application deadline
15.11.2024
Use only the online application form to submit your application with the following documents:
- cover letter
- CV
- copies of degree certificate(s)
If you experience technical problems, send an email to bewerbungen @ uni-hamburg.de.
Please apply at this link on the University website:
https://www.uni-hamburg.de/en/stellenangebote/ausschreibung.html?jobID=9728003f7d174feb4c7335ae59aa96839d7de847
|
| Postdoctoral Positions in Holographic Applications to Gravitational Waves | Closing date: 2024-11-30
Contact: Esther Pallares |
| The Institute of Cosmos Sciences at the University of Barcelona (ICCUB) is now offering four postdoctoral positions funded by Prof David Mateos? ERC Advanced Grant. | | ▸ more | Selected candidates will collaborate with Profs David Mateos, Jorge Casalderrey-Solana and other members of the group on applications of Holography to Cosmology and Astrophysics, with a focus on Gravitational Waves.
Topics of interest include cosmological phase transitions, baryogenesis, neutron star mergers, spacetime singularities and holography with dynamical boundary gravity. Prior knowledge of holography is not required.
Faculty members at the ICCUB working on related areas include Ruxandra Bondarescu, Pablo Bueno, Roberto Emparan, Bartomeu Fiol, Jaume Garriga, Cristiano Germani, Raul Jimenez, Alessio Notari and Jorge Russo.
For information about research at the ICCUB, visit http://icc.ub.edu
Appointments will begin in the Fall of 2025 or earlier for a period of 3 years. The salary includes social security and public health care benefits, covering spouse and children. We offer flexible working hours and family reconciliation.
The deadline for applications is November 30th 2024.
The University of Barcelona is part of a group of European institutes with a centralized system of postdoctoral applications. Candidates should apply through the following website, choosing Barcelona as one of their preferred institutes: https://itf.fys.kuleuven.be/postdoc-application/
Equal Employment Opportunity Statement
The ICCUB is an equal employment opportunity employer. The ICCUB promotes a diverse and inclusive environment and welcomes applicants regardless of age, disability, gender, nationality, race, religion or sexual orientation. We strongly encourage women and underrepresented minorities in physical sciences to apply. For additional information please see the Diversity, equity and inclusion Commission.
About the Institute of Cosmos Sciences:
The Institute of Cosmos Sciences is a research institute of the University of Barcelona. It is an interdisciplinary center dedicated to fundamental research in the fields of cosmology, astrophysics, and particle physics. In addition, the institute has a strong technology program through its participation in international collaborations in observational astronomy and experimental particle physics.
As part of the University of Barcelona, the ICCUB is a recipient of the European Commission?s HR Excellence in Research (HRS4R) Award, which recognises, among other achievements, respect for equal opportunities and the capacity to attract talent in a positive working environment that promotes the pursuit of successful research careers. The ICCUB respects the principles of open, transparent, merit-based selection. We strongly encourage women and underrepresented minorities to apply. For additional information please see the Diversity, equity and inclusion Commission.
The ICCUB is located in Barcelona, considered the 8th World's Best Cities 2022: one with near-perfect weather year-round, miles and miles of beaches, iconic parks, striking architecture and colorful neighborhoods that march to their own beat?artistic, sophisticated, bohemian. Moreover, it is a pole of attraction for the technology sector, a top choice to establish a company in this sector, and it hosts some of the world's major technological events, such as the Mobile World Congress and the Smart City Expo. In addition, Barcelona and its metropolitan area is a leading destination on the map of global technological ecosystems and has infrastructures such as science parks, universities and the 22@ district.
|
| 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
|
| Connecting the properties of MOONS galaxies and AGN with their large-scale environment | Closing date: 2024-11-30
Contact: Manuela Magliocchetti |
| A postdoctoral (1+1) position is available in Rome (Italy) at the Institute of Space Astrophysics and Planetology (IAPS-INAF) focussed on studies of the Large-Scale Structure of the Universe and the environment traced by galaxies and AGN within the MOONS GTO survey. | | ▸ more | We have just opened a postdoctoral position in Rome (Italy) at the Institute of Space Astrophysics and Planetology (IAPS-INAF) focussed on studies of the Large-Scale Structure of the Universe and the environment traced by galaxies and AGN within the MOONS GTO survey.
Project Overview:
MOONS is the new Multi-Object Optical and Near-infrared Spectrograph for the Very Large Telescope (VLT) at ESO which combines, for the first time, the collecting power of an 8-m telescope, 1000 fibres with individual robotic positioners, and both low- and high-resolution simultaneous spectral coverage across the 0.64-1.8 ?m wavelength range.
The MOONS GTO extragalactic survey (MOONRISE) with its 190 nights of observations will obtain key spectroscopic information for about half a million of AGN and galaxies at 0.9 < z < 2.6, as well as for a few thousand galaxies around the epoch of reionisation (z ~ 6?8). Amongst the many scientific goals, such a large statistics will also provide the unprecedented opportunity to investigate the Large Scale Structure of the Universe and the environments inhabited by galaxies and AGN in previously poorly explored redshift intervals and therefore also test assumptions embedded in various cosmological simulations and models.
The successful applicant will contribute to both the preparatory science for the MOONS GTO and scientific exploitation of the first data. In particular, he/she will deal with assessing the effects of the survey footprint and strategy on the photometric and spectroscopic catalogues for MOONRISE in order to successfully reconstruct both the environment and the Large-Scale Structure traced by galaxies and AGN up to the highest redshifts reachable by MOONS. Such analysis will then be used by the research fellow for his/her scientific purposes. The first part of the work will be carried out with the help of simulations and photometric catalogues already available to the MOONS collaboration, while the second part will make use of real MOONS data.
The work will be carried out at IAPS under my supervision and in collaboration with MOONS scientists, mainly in the person of Dr Olga Cucciati (OAS-INAF).
Eligibility Criteria:
By the deadline of the present call (November 30th 2024), applicants must have:
? A PhD in Astronomy or Astrophysics or equivalent Ph.D. issued by an Italian (or foreign) Advanced Studies Institute or University
or
? A master degree (or second Laurea degree if issued by an Italian University) in Physics, Astronomy, Astrophysics or Sciences of the Universe together with at least 3 years of documented research experience in scientific activities related to this call and obtained after the degree.
and
? A good knowledge of the English language
Application Details:
? A link to the announcement (both in English and Italian) and to the application forms (Allegato 1 and 2 for Italian speakers; Annex 1 and 2 for non-Italian speakers), as well as detailed instructions on the application procedure, can be found at: http://www.inaf.it/it/lavora-con-noi/assegni-di-ricerca/assegno-per-lo-svolgimento-di-attivita-di-ricerca-dal-titolo-201cconnessione-tra-le-proprieta-di-galassie-ed-agn-osservate-con-moons-e-la-loro-struttura-su-larga-scala201d-per-le-esigenze-del-progetto-201cthe-moons-extragalactic-survey201d
? The deadline for application is: November 30th, 2024
? Applications must be submitted by one of the following ways:
a) certified e-mail addressed to the certified mailbox areaconcorsi.iaps @ pec.it;
b) for Italian and foreigner citizens who do not have a certified mailbox (PEC), ordinary email addressed to areaconcorsi.iaps @ pec.it;
c) registered letter with acknowledgement of receipt or certified express courier addressed to: IAPS - Istituto di Astrofisica e Planetologia Spaziali ? Via Fosso del Cavaliere 100, 00133 Roma (post marks do not count).
Applications received by ordinary or certified mailbox, whose holder is different from the applicant, will be considered inadmissible. The applications must be delivered by reporting on the envelope or in the e-mail subject the following sentence: ?Application selection 2024-11-AR? ? IAPS ? Istituto di Astrofisica e Planetologia Spaziali ? AREA CONCORSI.
Required Application Material:
1. A signed copy of the application form (Annex 1 or Allegato 1 for Italian speakers);
2. A signed copy of Annex 2 (or Allegato 2 for non-Italian speakers);
3. A ?Curriculum vitae?, signed and dated by the applicant including a list, if applicable, of grants and fellowships held in the past or in progress;
4. A copy of a valid identity document (ID card or passport);
5. A list of publications;
6. Any other qualification, working task, research activity for public and private institutions and publications that the applicant deems appropriate to submit;
7. The list of all documents submitted.
Important:
The position is available for one year, extendable to a second year subject to performance review.
The annual gross salary is 28,000 Euros. Funds will be available for trips related to the project and computing resources.
For any question or further clarification, please contact me at manuela.magliocchetti @ inaf.it
|
| 2025 Trottier Postdoctoral Fellowship in Exoplanetary Science (IREx) | Closing date: 2024-12-04
Contact: Marie-Eve Naud |
| The Trottier Institute for Research on Exoplanets (IREx), affiliated with the Department of Physics of the Universite de Montreal (Montreal, Canada), invites applications for the Trottier Postdoctoral Fellowship in experimental, observational, or theoretical astrophysics applied to the study of exoplanets, which enables forefront independent research related to exoplanets. All areas of exoplanet research will be considered. | | ▸ more | The Trottier Institute for Research on Exoplanets (IREx), affiliated with the Department of Physics of the Universite de Montreal (Montreal, Canada), invites applications for the Trottier Postdoctoral Fellowship in experimental, observational, or theoretical astrophysics applied to the study of exoplanets, which enables forefront independent research related to exoplanets. All areas of exoplanet research will be considered.
Starting Date: The successful applicant is expected to start between May and September 2025.
Duration: The position is for two years, renewable for a third year subject to performance and availability of funds.
Application: Applicants should submit a cover letter (optional, max 1 page), a CV, a list of publications, and a statement of research interests (max 2 pages), and should arrange to have three referees send a letter of reference to irex-applications @ umontreal.ca by December 4th, 2024 for full consideration.
Full description of the position plus submission guidelines can be found here: https://exoplanetes.umontreal.ca/en/job/2025-trottier-postdoctoral-fellowship/
|
| Postdoctoral Fellowships in Astrophysics | Closing date: 2024-11-14
Contact: Massimo Gaspari |
| We are seeking two exceptional Postdoctoral Fellows to join cutting-edge research on understanding black hole mechanisms across all scales. The successful candidates will be deeply involved in modeling and analyzing astrophysical processes within cosmic halos, including the intracluster, circumgalactic, and interstellar medium, by using magneto-hydrodynamic (MHD) simulations. Their research will also involve comparing simulations with multiwavelength observations from major telescopes such as JWST, Chandra, XMM, HST, ALMA, and MUSE. | | ▸ more | Strong programming skills (e.g., C++, Python, Cuda) are highly desirable, as the role involves the development of state-of-the-art 3D MHD simulations with major astrophysical codes (e.g., Athena++, GAMER, FLASH). Expertise in high-performance computing, especially GPU-based systems, and familiarity with AGN feeding/feedback and gas processes - turbulence, magnetic fields, dust/cooling, chemistry - are significant assets.
The successful candidates will have a leading role in the ERC BlackHoleWeather team, benefiting from world-class resources and extensive opportunities for international collaboration, including partnerships with major institutions like Princeton, MIT, NASA, and NTU. These Fellowship positions offer a rare opportunity to contribute to groundbreaking theoretical and observational advancements in modern astrophysics, pushing the boundaries of our knowledge of black holes and galaxies coevolution throughout cosmic time.
----------
* Application Details
The positions are for 3 years, with yearly formal renewal. An additional 2 years may be available for those demonstrating excellence. One position may be later upgraded to tenure-track Assistant Professor. The starting date is preferred to be as soon as possible (negotiable).
* Application Instructions
Applicants should follow the below link (ENG or ITA). The core of the application is simple, i.e. upload:
1) a complete CV (with at least 3 reference contacts);
2) a Research Statement (especially in relation to BlackHoleWeather topics; see Gaspari+20, Nature Ast.);
3) a Publication List (web links are sufficient; e.g., ADS, Google Scholar);
4) a Cover Letter tailored for the position.
Reference letters are not required in the formal application, although they might be asked in a second stage.
Preferred education degree: Ph.D. in Astronomy/Astrophysics.
Note: don't worry about the "decree" PDF and related lengthy Italian admin text (e.g., Italian language is not a requirement; 12 months of research includes ongoing Ph.D. studies). The selection committee will focus on the above four documents and excellence of the candidates.
Review of the applications will begin soon after the (extended) deadline of November 14, 2024 (1pm CEST). Subsequently, short-listed candidates will be invited for an online interview.
If you have any questions about the position or application procedure, do not hesitate to write to Prof. Gaspari: massimo.gaspari @ unimore.it
You are welcome to send your CV to Prof. Gaspari for pre-screening, but note that complete formal applications must be submitted through the below online portal PICA.
* Link to Online Application: https://pica.cineca.it/unimore/2024-adrs255
* Included Benefits
Research benefits: the position comes with extensive dedicated funds for travel to meetings and workshops/conferences, as well as substantial funds for equipment (the ERC BlackHoleWeather team is based on a 2 million Euro funding).
Retirement benefits: majority of pension (2/3) paid by the employer (+22% of salary).
Healthcare benefits: fully covered by the Italian National System (no insurances required).
* Compensation Notes
The salary is in the top bracket for research scientists in Italy. Moreover, the compensation is income tax free (0% IRPEF). As such, the net salary is comparable to that of an Italian Associate Professor.
Note: costs of living in Italy are substantially lower than those in other Western countries (e.g. 2-3x compared with USA). Quality of life in Emilia Romagna is consistently ranked among the highest in Italy and Europe.
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| PhD position: Identification of past major dust-producing events within our Solar System (MfN Berlin) | Closing date: 2024-11-22
Contact: Jenny Feige |
| As part of the ERC funded project NoSHADE we seek a talented PhD candidate to join our interdisciplinary team at the Museum für Naturkunde (Natural History Museum) in Berlin, Germany. The focus is on analysing micrometeorites from time-resolved sedimentary records and link them to specific cosmic events, such as collisions among asteroids or comet break-ups. | | ▸ more | The overarching goal of the NoSHADE (Novel Perspectives on our Solar System History recorded in the Atacama Desert) project funded by the European Research Council (ERC, 101077668) is to collect traces of cosmic dust from Atacama Desert sedimentary records reaching back >10 million years and link them to specific cosmic events (https://www.youtube.com/watch?v=R9SzMdAGtVk).
Within our Solar System, cosmic events such as asteroid collisions or comet break-ups release interplanetary dust particles that encounter Earth and become part of sedimentary records as micrometeorites. To identify past major dust-producing events in our Solar System the focus is on analysing the micrometeorite types and fluxes over time, as well as reconstructing their exposure ages and origins by quantifying the content of cosmogenic radionuclides.
We offer
- Working in a dynamic interdisciplinary team with scientific excellence in astrophysics and geology and extensive professional networking opportunities.
- Excellent infrastructure in an attractive working environment.
- Exciting field work experience.
A detailed description on the tasks and requirements, as well as more information on the application process are available here:
https://jobs.museumfuernaturkunde.berlin/jobposting/0650feb50f3522e6a573ee4465c6ac565f6fef880
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| PhD position: Detection of supernova isotopes in Atacama Desert sediments (MfN Berlin) | Closing date: 2024-11-22
Contact: Jenny Feige |
| As part of the ERC funded project NoSHADE we seek a talented PhD candidate to join our interdisciplinary team at the Museum für Naturkunde (Natural History Museum) in Berlin, Germany. The focus is on deciphering past nearby Supernovae that left traces on Earth in the form of radioactive isotopes. | | ▸ more | The overarching goal of the NoSHADE (Novel Perspectives on our Solar System History recorded in the Atacama Desert) project funded by the European Research Council (ERC, 101077668) is to collect traces of cosmic dust from Atacama Desert sedimentary records reaching back >10 million years and link them to specific cosmic events (https://www.youtube.com/watch?v=R9SzMdAGtVk).
Particularly, Supernovae occurring in our Solar neighborhood leave trace amounts of characteristic radionuclides on Earth (e.g. Fe-60). Such isotopic fingerprints mirror the various types of interstellar matter our Solar System encountered in the past as well as nucleosynthesis processes in massive stars. To identify the quantity, timing, locations and types of past nearby Supernova events, the focus is on searching for anomalies of long-lived radionuclides in the sedimentary records.
We offer
- Working in a dynamic interdisciplinary team with scientific excellence in astrophysics and geology and extensive professional networking opportunities.
- Excellent infrastructure in an attractive working environment.
- Exciting field work experience.
Detailed descriptions on the tasks and requirements, as well as more information on the application process are available here:
https://jobs.museumfuernaturkunde.berlin/jobposting/4e4eb3cb8a01ebdfdeee2368ecfed09bb76fd3af0
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| Postdoctoral Fellowship in Meteor Astronomy at the Astronomical Institute of the Czech Academy of Sciences | Closing date: 2024-11-10
Contact: Jiri Borovicka |
| The Group of Meteor Physics at the Astronomical Institute of the Czech Academy of Sciences in Ondrejov, Czech Republic, invites application for a postdoctoral position, which will be open from January 1, 2025 in the scope of the project "Detailed insight into the properties of meteor showers" funded by the Czech Science Foundation. | | ▸ more | The successful candidate will work under the leadership of Dr. Jiri Borovicka (jiri.borovicka @ asu.cas.cz) on the analysis and interpretation of data from the cameras of the European Fireball Network and other meteor cameras operated by the Group. The possible specific topics include orbital integration and search for parent bodies of meteor showers, analysis of meteor spectra, or modeling of meteoroid atmospheric fragmentation on the basis of meteor data (light curves, deceleration, morphology).
Astronomical Institute is a Public Research Institution and the largest professional astronomical organization in the Czech Republic. It is located at the Ondrejov Observatory near Prague (see http://www.asu.cas.cz/en/). The European Fireball Network is the world?s longest operating fireball network. It has been modernized in the recent years.
The appointment is initially for one year; an extension for another year (until the end of 2026) 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) and it includes health insurance. There is a possibility of institute accommodation in Ondrejov. The starting date of employment is expected to be 1st of January 2025, but it is negotiable.
Successful candidates must hold PhD degree not older than 8 years at the time of start of the employment (in case of maternity leave or long-term illness, these periods are not counted into the limit). Applications can be submitted before finishing PhD, in which case a statement from the supervisor stating the planned date of the defense should be included.
Applications must contain Curriculum Vitae, list of publications, and a specification of the research topic the applicant plans to contribute to. The applications are to be submitted by email to:
info @ asu.cas.cz.
Please, arrange for a minimum of two letters of reference to be sent directly to the same electronic address as above. The letters may be issued up to 9 months before the application deadline.
To receive full consideration, the application deadline is 10th of November 2024 till the end of the day (Prague/Central Europe timezone). The receipt of applications will be acknowledged by email. Once the evaluation process is completed, applicants will be notified about the result. The institute reserves the right not to take any of the candidates.
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| Postdoctoral position in extragalactic radio astronomy | Closing date: 2024-11-25
Contact: Shane O'Sullivan |
| We invite applications for a postdoctoral position of two years duration at Universidad Complutense de Madrid (UCM) to work with Prof. Shane P. O'Sullivan on extragalactic radio surveys related to cosmic magnetism science. | | ▸ more | The postdoctoral researcher will work with data from ongoing radio polarization surveys, such as the LOFAR Two-Metre Sky Survey and the ASKAP-POSSUM survey, to constrain the properties of cosmic magnetic fields across a wide range of physical scales and use the results to test models for their origin. They will also be involved in the preparation for future projects with the Square Kilometre Array (SKA) telescope, which Spain is a full member of.
The successful candidate will become part of the Extragalactic Astrophysics and Astronomical Instrumentation group of UCM (GUAIX), as well as the Institute of Particle Physics and the Cosmos (IPARCOS). See https://guaix.ucm.es/home/science/cosmic-magnetic-fields for more details.
Applicants must have a PhD in Astrophysics and some experience in radio astronomy.
Interested candidates should email their CV (including the names of two referees), a motivation letter (max. 1 page) and a summary of their research to date (max. 1 page) to s.p.osullivan @ ucm.es by 25 November 2024. The earliest start date will be mid-Feb 2025.
Salary: 30-35k including social security costs (access to Spanish public health system). Research funds are also available for travel, computing and publications.
Applications are especially encouraged from people from underrepresented groups.
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| Warwick PhD Prize Scholarships in Astrophysics | Closing date: 2025-01-08
Contact: Warwick Astronomy Admissions Team |
The University of Warwick's Astronomy & Astrophysics group is seeking talented PhD applicants for our Warwick PhD Prize Scholarships in Astrophysics. Applications are due by January 8th, 2025.
The scholarships are open to national and international applicants and all are welcome to apply. All successful applicants will have a full stipend plus allocations for travel and computing.
All projects are here https://warwick.ac.uk/fac/sci/physics/research/astro/postgraduate_phd/ and our Frequently Asked Questions are here: https://warwick.ac.uk/fac/sci/physics/research/astro/postgraduate_phd/faq | | ▸ more | Potential projects span a wide range of research areas including exoplanet discovery, characterisation and evolution, protoplanetary and debris discs, white dwarfs and planetary remnants, stellar populations, transients and explosive astrophysical phenomena, and space situational awareness.
Applicants are encouraged to contact the project supervisors for further information on the projects here:?https://warwick.ac.uk/fac/sci/physics/research/astro/postgraduate_phd/
Warwick is an internationally recognised centre of research excellence. Our group takes leading roles in many major ground and space-based projects, including the Gravitational-wave Optical Transient Observer (GOTO), Next Generation Transit Survey (NGTS), PLAnetary Transits and Oscillations of stars (PLATO) telescope, CHaracterising ExOPlanet Satellite (CHEOPS), Sloan Digital Sky Survey (SDSS), WHT Enhanced Area Velocity Explorer (WEAVE) spectrograph, 4-metre Multi-Object Spectrograph Telescope (4MOST), and Dark Energy Spectroscopic Instrument (DESI).
We also run state-of-the-art computer simulations to develop theoretical models using the university's modern super-computing facilities, and are experts in the exploration of large and heterogenous data sets, adopting novel techniques including machine learning.
The Astronomy & Astrophysics group is part of the Physics Department at Warwick; both the department and the university hold Athena SWAN Silver awards, a national initiative to promote gender equality for all staff and students. The Physics Department is also a Juno Champion, which is an award from the Institute of Physics to recognise our efforts to address the under-representation of women in university physics and to encourage better practice for all. The Astronomy & Astrophysics group also hosts monthly equitea forums to break down barriers faced by all under-represented groups in science:?https://warwick.ac.uk/fac/sci/physics/research/astro/seminars/equitea/
Warwick is an excellent place to begin your scientific career, where you will be exposed to a wide range of research topics. You will be immersed in a friendly, collaborative and supportive environment with nearly 40 fellow astronomy PhD students, working with and learning from experts in very different areas. Personal development is a priority, and incoming PhD students will be invited to join our network of international collaborators, lead projects, and present their work on international platforms.
More information about the Warwick Astronomy & Astrophysics Group can be found here:?https://warwick.ac.uk/fac/sci/physics/research/astro/?and more information about the local area can be found here:?https://nam2022.org/warwick/local-area
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| Postdoctoral Positions in Experimental and Observational Infrared/ Submillimeter Astrophysics (m/f/d) | Closing date: 2024-11-15
Contact: Linda Tacconi |
| This year we are focusing our search mainly on candidates whose interests are in studying black holes over cosmic time with GRAVITY+. | | ▸ more |
The Infrared Group of the Max Planck Institute for Extraterrestrial Physics invites applications from talented, ambitious graduating PhD students and postdoctoral researchers. Our front-line research focuses on near-IR-millimeter high-resolution imaging and spectroscopy of the Galactic Center, and of star forming galaxies in the early Universe. We lead studies of star formation, gas content, physical properties and dynamics of galaxies, and black-hole formation and evolution. This research is supported by a major program of innovative instrumentation development. We have recently commissioned ERIS, a new diffraction-limited imaging and spectroscopic facility for the VLT, we are the PI institute for GRAVITY and GRAVITY+, the ESO VLTI instrument for precision astrometry and interferometric imaging of faint objects, and we are also the PI institute for MICADO, the first-light instrument for the ESO ELT.
Postdoctoral Positions in Experimental and Observational Infrared/ Submillimeter Astrophysics (m/f/d)
Job Code: 19/2024
This year we are focusing our search mainly on candidates whose interests are in studying black holes over cosmic time with GRAVITY+. Strong candidates whose interests mesh with our other research fields in experimental astrophysics and galaxy evolution will also be considered for additional positions. Postdoc appointments can start anytime in 2025. The duration of the positions are for 3 years with a possibility of extension for one or two years, according to current German labor law, Applicants must have a PhD in astronomy or related field before starting. The salary and full social benefits are based on the German TVöD scale for public employees (E14 for postdocs), depending on experience.
Please send a letter of application, a 2-3 page description of research interests, a CV including bibliography, and request three letters of reference to (https://recruitingapp-5257.de.umantis.com/Vacancies/619/Application/CheckLogin/2?lang=eng) by November 15, 2024 the search will continue until suitable candidates are found.
For scientific enquiries about the positions, please contact Linda Tacconi - linda @ mpe.mpg.de or Frank Eisenhauer - eisenhau @ mpe.mpg.de.
The Max Planck Society is an equal opportunity employer. Applications from women, disabled people and minority groups are particularly welcome.
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| Astronomer / Instrument Project Scientist | Closing date: 2024-11-08
Contact: Evelina Dietmann |
| ESO is engaged in the operation and construction of a number of optical and infrared instruments for its observatories. The Instrument Project Scientist follows the development and construction phases of new instruments supporting and nurturing its science goals, ensuring that the top-level requirements are fulfilled and that the operational scenarios are commensurate with the scientific needs and the constraints of the observatory. | | ▸ more | The development of the instruments may either be carried out by a consortium of universities and institutes, working in collaboration with ESO, or by an internal team at ESO. The Project Scientist is a prime contact for the associated consortia/institutes, as well as for the ESO science community at large when it comes to prepare for and advertise the science.
We are looking for an enthusiastic and outstanding scientist with a strong expertise in optical and/or near-infrared spectroscopy. The successful applicant will be assigned to follow one or more instruments at any given time. Two state-of-the-art instruments are presently considered: the prime objective for the Instrument Project Scientist would be to support and follow the ELT optical/near-infrared spectrograph ANDES and the integral-field spectrograph BlueMUSE for the VLT as a potential secondary project. ANDES is a high-spectral-resolution instrument for the ELT that has the potential to greatly impact our understanding of the cosmos and exoplanets. BlueMUSE is a new integral-field spectrograph, complementing the very successful MUSE spectrograph operating at bluer wavelengths. Both instruments will serve a broad community of scientists addressing topics from planets, Galactic and extragalactic systems, to the high-redshift universe and fundamental physics.
Main Duties and Responsibilities:
- Provides strong scientific leadership to the assigned instrument projects within ESO;
- Acts as the principle scientific contact to the instrument consortium;
- As a member of the ESO Astronomy Faculty, will be expected and encouraged to conduct a strong personal research programme and to participate actively in the scientific life of ESO;
- Liaises with ESO's scientific community on issues related to the instruments under their responsibility;
- Develops, owns and maintains the scientific requirements for the assigned instruments;
- Works closely with the ESO Project Managers, and System Engineers to ensure the implementation of the scientific requirements;
- Coordinates and connects with the relevant Programme Scientist(s) on the related instruments and projects;
- Supports testing, commissioning and early operations. Specifically: preparation for the science operation during design, manufacturing/assembly/integration and testing and commissioning of the instrument in close cooperation with the observatory;
- Participates in progress meetings and instrument reviews;
- Tracks the evolving requirements for the assigned instruments emerging from the community;
- Interacts closely with the observatory and data management teams on operational aspects.
The tasks are not limited to the above and a flexible approach and willingness to adapt are required.
Reports to:
Head of the Project Science Department.
Key Competences and Experience
Essential Competences and Experience:
- Demonstrated experience and strong involvement in the key phases of the development of at least one astronomical instrumentation project (initial/final design, system testing, or commissioning and early operations);
- Experience with the planning, execution, analysis and publication of scientific research arising from said instrumentation;
- Active research programme and robust publication record;
- Understanding of the science requirements on instruments and strategies for their realisation;
- Ability to provide scientific and strategic vision and leadership to geographically dispersed multi-cultural/multi-disciplinary teams within a cost-constrained programme;
- Proficiency in relevant data reduction methods and tools;
- Ability to motivate and inspire others; strong influencing skills;
- Cooperative team player;
- Ability to work in a clear and structured manner producing meaningful reports to supervisors and presentations to ESO governing bodies;
- Provides clear, concise and timely oral and written communication, identifying the key issues, examining options, and proposing a way forward;
- Ability to effectively communicate at all levels and across disciplines within the organisation and with the community;
- Ability to negotiate with external scientists and instrument builders to achieve ESO's goals.
Desirable Competences and Experience:
- Significant expertise in spectroscopy (optical, near-infrared) and in particular with high-resolution spectroscopy and/or integral-field units (IFUs);
- Good knowledge of adaptive optics techniques, in particular SCAO;
- Broader experience following instrument development over most if not all phases from initial design to final commissioning.
Qualifications:
Ph.D. in astronomy, physics or equivalent.
Language skills:
Excellent command of the English language is essential.
Remuneration and Contract:
We offer an attractive remuneration package including a competitive salary, comprehensive pension scheme and medical, educational and other social benefits, as well as financial help in relocating your family and support to place your child/children in daycare.
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 https://recruitment.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 by the deadline. 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 8 November 2024.
Interviews are expected to start soon after this date.
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| ALMA Regional Centre Astronomer | Closing date: 2024-11-16
Contact: Evelina Dietmann |
| The ALMA Regional Centre (ARC) department at ESO provides the interface between the European ALMA Users Community and the ALMA observatory in Chile. In coordination with the ARCs in the other ALMA partner regions, the ARC at ESO promotes and provides support of the highest standards to the ALMA user community and to ALMA observatory global operations. | | ▸ more | The ESO ARC provides important services for the development and operation of ALMA, including software development and testing, Call for Proposals and observation preparations, participation in observing shifts at the ALMA observatory, delivery of quality-assured data products for principal investigators and archive users, and optimisation of capabilities. ALMA is also currently undergoing an ambitious upgrade - the Wideband Sensitivity Upgrade (WSU) - and the ARC is heavily involved in the planning and investigations needed to transition to WSU Operations at around the end of the decade.
The ARC at ESO is looking for an astronomer with a strong research profile in radio and/or millimetre astronomy. As a member of the ESO ARC and of the ESO Faculty, you will be given the opportunity to interact with other researchers at ESO and contribute to ESO's diverse scientific life. You should demonstrate scientific drive and vision to conduct high-impact independent research. Furthermore, you should have a strong interest in maximising ALMA's scientific output by leading operations support and user support tasks. As the ARC astronomer you will contribute to core ARC duties, in particular quality assurance, in coordination with colleagues at the ESO ARC, the European ARC network and the other ALMA partners, as well as to tasks leading to the optimisation of science operations. Expertise areas that are currently under-represented among the ESO faculty are encouraged. For an overview of the science expertise in Garching see here.
Main Duties and Responsabilities
- Play a key role in the ALMA processes targeting the optimisation of the scientific products that come out of this world-leading facility; this task includes, but is not limited to, co-managing both manual and pipeline data reduction runs, overseeing reprocessing efforts, and contributing to the pipeline weblog review process and its optimisation;
- Perform general ARC duties, including answering Helpdesk tickets, contributing to testing of tools and playing a proactive role in the improvement of user documentation;
- Undertaking Astronomer-on-Duty shifts in Chile;
- Constructively work together with other ARC staff and ALMA operations staff around the globe;
- As a member of the ESO Astronomy Faculty, you will be expected and encouraged to conduct a strong personal research programme and to participate actively in the scientific life of ESO and interact with other parts of the wider organisation;
- The tasks are not limited to the above and a flexible approach and willingness and capability to adapt is required.
Reports to:
The post holder reports to the Head of the ALMA Regional Centre (ARC) Department. The ARC is a department of currently 13 highly skilled and motivated staff and is part of the ESO ALMA Support Centre (EASC) division.
Key Competences and Experience:
Essential Competences and Experience
- Active astronomical research at least at postdoctoral level with a solid publication record and continuing high-impact research activity in astronomy;
- Practical experience with astronomical radio/millimetre observing techniques and data analysis;
- Excellent cross-disciplinary communication skills, both oral and written;
- Demonstrated ability to work effectively in a team, have an eagerness to contribute to team performance, and a positive approach toward building links across teams in an international multi-cultural environment.
- Pro-active approach to contribute ideas for improvement and future developments.
- Flexibility in adapting to changes of requirements and priorities as well as of assignments.
- Good time management and prioritisation skills.
- Open and friendly attitude to interact with a variety of users.
Desirable Competences and Experience
- Work experience with Python and CASA;
- Experience with advanced interferometric or single-dish data techniques
Qualifications:
Essential educational level: PhD in Astronomy, Physics or equivalent.
Language skills:
Excellent working knowledge of English.
Remuneration and Contract:
We offer an attractive remuneration package including a competitive salary, comprehensive pension scheme and medical, educational and other social benefits, as well as financial help in relocating your family and support to place your child/children in daycare.
ESO aims to support members of personnel in maintaining a good work-life balance (https://www.eso.org/public/jobs/conditions/intstaff/#work-life-balance) between their professional and private life. ESO is also committed to offering family-friendly support (https://www.eso.org/public/jobs/conditions/intstaff/#family-friendly-support), creating a work environment and policies which allow staff to balance their professional and private responsibilities through flexible working arrangements and financial support for families.
The contract is for a fixed term duration of three years and is subject to successful completion of the probation period. There may be a possibility of extension(s) subject to individual performance and organisational requirements, and as defined in the applicable policies and staff rules and regulations. For any further information, please visit ESO's conditions of employment *https://www.eso.org/public/jobs/conditions). Please note that the contract policy and in particular the regulations concerning fixed-term and indefinite contracts are currently under review which may lead to changes in the contractual conditions applicable to this position.
Duty Station:
Garching near Munich, Germany with occasional duty trips to ESO/ALMA sites in Chile.
Career Path: V
Application:
If you are interested in working in areas of frontline technology and in a stimulating international environment, please visit http://www.eso.org and https://www.almaobservatory.org/en/home/ for further details.
Apply online at http://jobs.eso.org/.
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| PhD position in galactic Astrophysics | Closing date: 2024-11-01
Contact: Gina Panopoulou |
We invite applications for a PhD position at the Division of Astronomy and Plasma Physics at Chalmers University of Technology. Join our dynamic research team to explore the role of magnetic fields and cosmic rays in shaping the interstellar medium of galaxies, and contribute to advancing our understanding of galactic astrophysics. | | ▸ more | Project description
You will work in the group of Asst. Prof. Gina Panopoulou. The group specializes in observational studies of interstellar magnetism as part of the division of Astronomy and Plasma Physics. The research project will involve the use of observations from radio telescopes probing magnetic fields and cosmic rays. The main aim will be to develop methods for inferring the properties of these galactic components from observations. The methods will be tested on existing magneto-hydro-dynamical simulations of galaxies.
Major responsibilities
conduct research (data analysis, software development, writing publications, studying literature, presenting at conferences),
complete courses in Astrophysics as well as transferable skills courses,
collaborate within international networks (e.g. SKA).
Research in the division covers a broad range of topics, including interstellar medium, star formation, galaxy evolution, evolved stars and exoplanets. PhD education at Chalmers offers a wide range of opportunities for career development, providing connections to astronomers in diverse fields, training in pedagogy, leadership, research ethics and an engaging and supportive work environment. As part of the PhD education, students conduct research and complete coursework covering advanced topics in Astrophysics.
To apply, visit the Chalmers vacancies page:
https://www.chalmers.se/en/about-chalmers/work-with-us/vacancies/?rmpage=job&rmjob=13222&rmlang=UK
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| PhD scholarship in Exoplanets - DTU Space | Closing date: 2024-11-18
Contact: Lars A. Buchhave |
| The Exoplanet Group at DTU Space at the Technical University of Denmark, situated in the greater Copenhagen area, invites applications for PhD a scholarship in exoplanet research. The Exoplanet Group is extensively engaged in the detection and characterization of exoplanets through observations and modelling. Our group has a particular interest in atmospheric studies of terrestrial and sub-Neptune exoplanets and extreme prevision radial velocities, but candidates with interests in broader exoplanet areas are also encouraged to apply. | | ▸ more | The successful candidate will work with Prof. Lars A. Buchhave and Dr. Alexander Rathcke in the rapidly growing Exoplanet Group. At DTU Space, the candidate will have access to data from world-class telescopes, including JWST, HST, ultra precise RV spectrographs (e.g., HARPS-N and EXPRES), and the VLT. Ongoing projects include characterizing terrestrial worlds with JWST (including several PI led programs) and scientific and technical work on the Second Earth Spectrograph (2ES, PI Buchhave, http://www.2es.dk) to discover Earth-mass planets, and work pertaining to the ESA Ariel Mission (co-PI Buchhave, https://arielmission.space). Additional information about the Exoplanet Group at DTU Space can be found at http://www.exoplanets.dk.
Responsibilities and qualifications
We are seeking a talented and highly motivated student to work at the cutting edge of the rapidly moving research field of exoplanets. Applicants with previous experience in the mentioned areas of research, strong programming skills and knowledge relating to data reduction and analysis and/or modelling of spectroscopic data are especially encouraged to apply. Flexibility and self-motivation are desired skills at DTU Space. In particular, the Exoplanet Group encourages a vibrant collaborative work environment, where collaboration with other group members is highly encouraged.
The above-mentioned projects will allow for the successful applicant to work on a number of cutting-edge datasets, and the successful applicant is encouraged to pursue independent research interests during the course of their PhD.
You must have a two-year master's degree (120 ECTS points) or a similar degree with an academic level equivalent to a two-year master's degree. Candidates who are in the process of getting their degree can apply but must have a master's degree by the time of employment.
Approval and Enrolment
The scholarship for the PhD degree is subject to academic approval, and the candidate will be enrolled in one of the general degree programmes at DTU.
For information about our enrolment requirements and the general planning of the PhD study programme, please see DTU's rules for the PhD education.
The assessment of the applicants will be made by the end of November 2024 and shortlisted candidates will be invited to an interview. We expect to extend formal offers in December 2024.
We offer
DTU is a leading technical university globally recognized for the excellence of its research, education, innovation and scientific advice. We offer a rewarding and challenging job in an international environment. We strive for academic excellence in an environment characterized by collegial respect and academic freedom tempered by responsibility.
Salary and appointment terms
The appointment will be based on the collective agreement with the Danish Confederation of Professional Associations. The allowance will be agreed upon with the relevant union. The period of employment is 3 years.
The starting date is flexible but would ideally commence in Q1 of 2025.
You can read more about career paths at DTU here.
Further information
Further information and inquiries about the position can be made to Lars A. Buchhave (buchhave @ space.dtu.dk) or Alexander Rathcke (rathcke @ space.dtu.dk).
You can read more about the Exoplanet Group at www.exoplanets.dk and the DTU Space institute at www.space.dtu.dk.
If you are applying from abroad, you may find useful information on working in Denmark and at DTU at DTU ? Moving to Denmark.
Furthermore, you have the option of joining our monthly free seminar ?PhD relocation to Denmark and startup ?Zoom? seminar? for all questions regarding the practical matters of moving to Denmark and working as a PhD at DTU.
Application procedure
Your complete online application must be submitted no later than 18 November 2024 (23:59 Danish time).
Applications must be submitted as one PDF file containing all materials to be given consideration. To apply, please open the link "Apply now", fill out the online application form, and attach all your materials in English in one PDF file.
The single PDF file must include:
A letter motivating the application (cover letter)
Curriculum vitae
Grade transcripts and BSc/MSc diploma (in English) including official description of grading scale
Research statement describing your previous work and thoughts and ideas for future research (max 3 pages)
Shortlisted candidates will be asked to provide 2-3 reference letters to be emailed at a later date.
You may apply prior to obtaining your master's degree but cannot begin before having received it.
Applications received after the deadline will not be considered.
All interested candidates irrespective of age, gender, race, disability, religion or ethnic background are encouraged to apply.
DTU Space
The Institute has about 200 employees and is located in the greater Copenhagen area at the Lyngby Campus of the Technical University of Denmark together with 19 other institutes within the technical sciences. In the Astrophysics & Atmospheric Physics Division of the Department of Space Research and Space Technology (DTU Space), current focus areas cover exoplanets, large-scale structure of the universe, physics of compact objects, space weather, upper atmosphere physics and cosmo-climatology, as well as development of instrumentation, in particular hih-energy instrumentation, i.e. X- and gamma ray detectors and optics. The division is currently active in the operation of instruments and data analysis from three satellites. The division also runs four instrumentation laboratories and hosts a center for space weather research and forecasts.
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https://efzu.fa.em2.oraclecloud.com/hcmUI/CandidateExperience/en/sites/CX_1/job/4073/?utm_medium=jobshare
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| Postdoctoral Position in Dynamics of Planetary Systems | Closing date: 2024-11-10
Contact: Alexandre Correia |
| The Centre for Physics of the University of Coimbra (CFisUC), Portugal, invites applications for a research position in Dynamics of Planetary Systems under the CEEC FCT 2024 program. Applicants can be researchers of all nationalities, who have the potential to develop innovative research and have a relevant scientific CV in Astrophysics. | | ▸ more | Description:
The successful applicant is expected to do research in one of the following topics: solar system dynamics, TNOs, planetary formation and evolution, dynamics of multi-planetary systems. Applications by researchers working on other research topics related to the field of solar system or exoplanets will also be evaluated.
Qualifications:
PhD in Astrophysics or similar already concluded.
Application deadline: November 10th, 2024
Expecting starting date: 2nd half of 2025, to be agreed upon with the successful candidate.
Host institution: CFisUC, Department of Physics, University of Coimbra, PORTUGAL (EU).
Type of contract: 3 year Contract
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APPLICATION PROCEDURE:
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Job Reference: CEEC-FCT-24
Language: English
Candidates should contact Prof. Alexandre Correia (acor @ uc.pt) before November 10th, 2024, with the following documents:
1. CV (including publication list)
2. A brief research plan (maximum 3 pages)
3. Name and contact of 2 scientists who can provide a letter of recommendation.
4. Motivation letter
The pre-selected candidate will get the support from the CFisUC to apply to the CEEC program.
Contacts and further information:
Alexandre Correia:
http://faculty.uc.pt/uc44419
University of Coimbra:
https://www.uc.pt/en/fctuc/df
FCT Program:
https://www.fct.pt/en/concursos/concurso-estimulo-ao-emprego-cientifico-individual-7-edicao
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| PhD positions at the International Max Planck Research School for Astronomy & Astrophysics, Bonn Cologne | Closing date: 2024-11-01
Contact: IMPRS A&A Office |
| The International Max Planck Research School (IMPRS) for Astronomy & Astrophysics is a joint structured Ph.D. program of the Max Planck Institute for Radioastronomy (MPIfR, Bonn) and the Universities of Bonn and Cologne. At one of the most vibrant astronomy centers in Europe, several PhD positions are available for talented students nearing the end of their Master's degree (or equivalent) in physics or astrophysics. The teaching language is English. Application deadline is November 1st, 2024. | | ▸ more | Program Details:
+ Appointments are for 3 years, starting at any time in 2025.
+ Starting annual gross salary: ~45,756 Euro; with attractive benefits.
+ The IMPRS for A&A has 60+ Ph.D. students from 22 countries.
+ Supervision by world-leading experts at the MPIfR and the Universities of Bonn and Cologne.
+ Research on a wide range of cutting-edge topics in observational and theoretical astrophysics.
+ Access to world-class observing facilities at a wide range of wavelengths.
+ Career development workshops, advanced lecture courses, soft skill seminars.
+ Funding for travel and research.
The application deadline is November 1st, 2024. For more information visit https://imprs.mpifr.de. To apply electronically, visit https://imprs.mpifr-bonn.mpg.de.
Institution:
Max Planck Institute for Radio Astronomy
Department:
International Max Planck Research School (IMPRS)
Number of Positions Available:
18
Duration:
3 Years
Work Arrangement:
In-Person
Location(s):
Bonn, Cologne
Germany
Compensation Range:
25,978 to 27,201 Euros
(The compensation range is based on net values after taxes and other deductions. The precise values depend on the tax class and the choice of health insurance. The range before deductions is 45,756 - 49,287 Euros.)
Included Benefits:
Remuneration is based on the German collective agreement for the public sector (TVöD-Bund), level 13, which includes comprehensive health care and other social benefits such as contributions to a pension fund, accident insurance, sick leave and 30 days of vacation per year. In addition, our school has special agreements with daycare providers and counselors, and offers German classes.
The Max Planck Society is committed to increasing diversity in its workforce and encourages applications from individuals with disabilities. The society also seeks to increase female representation in underrepresented areas and strongly encourages women to apply.
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| POSTDOCTORAL POSITIONS (m/f/x) IN ASTROPHYSICS | Closing date: 2024-11-10
Contact: Prof. Dr. Yuri Kovalev |
| The Max Planck Institute for Radio Astronomy (MPIfR) is seeking postdoctoral researchers to join the MuSES (Multi-messenger Studies of Extragalactic Super-colliders) project led by Prof. Yuri Kovalev and funded by the European Research Council (ERC Advanced Grant No. 101142396). It will be conducted over five years starting January 1, 2025. | | ▸ more | MuSES (https://www.mpifr-bonn.mpg.de/muses) aims to explore the link between black holes, accretion disks, and their surrounding medium. Using advanced multi-messenger astrophysics, we seek to advance our understanding of black holes, relativistic outflows, cosmic ray production, and high-energy neutrino emission.
Project Objectives:
1. Observational studies of AGN jet geometry, collimation and acceleration:
- Measurements of jet shapes from parsec-scale images.
- Multi-year kinematics and model analysis to probe the acceleration of relativistic plasma in jets.
- Developments of new automated algorithms for VLBI model-fitting, kinematics measurements and robustness assessment.
2. Probing the physical mechanism of neutrino production on the basis of multi-messenger blazar data:
- Study of parsec-scale properties of neutrino-selected blazar candidates on the basis of regular VLBI observations of complete samples and neutrino-triggered followup experiments.
- Reconstruction of physical conditions in AGN jets including properties of newly ejected relativistic ejections potentially associated with high-energy neutrino events.
- Statistical and modeling analysis of radio-to-gamma-ray variations in relation to high-energy neutrino events to search for a possible connection between electromagnetic synchro-compton flares and neutrino arrival times and energies.
To achieve these goals, the MuSES team will combine a range of radio-to-gamma-ray observations, particularly VLBI, and high-energy neutrino data. They will conduct multi-frequency polarization observations of blazars and AGNs with the Very Long Baseline Array (VLBA) within the ongoing MOJAVE (https://www.cv.nrao.edu/MOJAVE/index.html) project and other dedicated VLBA experiments at cm and mm wavelengths.
We seek researchers whose scientific interests align with one or more of these objectives. Experience in any of the following areas is desirable but not strictly required: radio interferometry techniques and VLBI, modern methods of electromagnetic or multi-messenger statistical data analysis, AGN jet simulations.
Postdocs will have the opportunity to join the KM3NeT neutrino collaboration (https://www.km3net.org/) as full members and participate in neutrino telescope activities, including observations, data processing, and analysis as an integral part of the multi-messenger MuSES project.
Additionally, the International Max Planck Research School for Astronomy and Astrophysics (IMPRS, http://www.mpifr-bonn.mpg.de/imprs/) offers opportunities for collaborative research with PhD students, including their supervision and teaching within the MuSES project.
Application Process:
Interested and qualified individuals should submit the following:
- A curriculum vitae.
- A list of publications
- A research motivation letter (maximum of four pages long, including figures and references, and formatted with 12 pt. font) addressing at least one of the MuSES objectives.
Applicants should also arrange for three letters of recommendation to be sent to the MPIfR application portal (https://jobs.b-ite.com/jobposting/83d61e9862bc5f2b70f5d3974efcf5ff9b24a6c70)
Terms of Employment:
The initial appointments are for two (2) years with the possibility of extension upon review. Remuneration is based on the German wage agreement for the public service (TVöD-Bund), level 13, which includes comprehensive healthcare coverage and other social benefits.
The Max Planck Society is committed to increasing diversity in its workforce and encourages applications from individuals with disabilities. The society also seeks to increase female representation in underrepresented areas and strongly encourages women to apply.
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| ESA Archival Research Visitor Programme | Closing date: 2024-10-31
Contact: Guido De Marchi |
| To increase the scientific return from its space science missions, the European Space Agency (ESA) welcomes applications from scientists interested in pursuing research projects based on data publicly available in the ESA Space Science Archives (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 November 2024 will be considered for visits in spring and summer 2025.
For further details, including areas of research and contact information, please refer to:
https://www.cosmos.esa.int/web/esdc/visitor-programme
or write to the programme coordinators at arvp @ cosmos.esa.int
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| Post-doctoral position in numerical astrophysics | Closing date: 2024-12-01
Contact: Prof. Daniel Ceverino |
| We offer a postdoctoral position at Universidad Autonoma Madrid (Spain) to work with Prof. Daniel Ceverino on simulations of clumpy galaxies at high redshifts and the formation of star clusters within giant clumps. Applicants must have a PhD in Astrophysics and some expertise in galaxy formation simulations and/or star formation processes. The appointment will initially be for 2 years, starting in April 2025, with the possibility of further extension depending on funding availability. | | ▸ more | | Interested candidates should submit their cv with a list of publications to the email address daniel.ceverino @ uam.es by December 1, 2024. In addition they should arrange two letters of recommendation to be submitted at the same address
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| Postdoctoral Research Associate (Physics/Astronomy) | Closing date: 2024-12-31
Contact: Human Resources |
| The Department of Physics at Baylor University invites applications for a postdoctoral position in the area of observational cosmology and time-domain astrophysics. Applicants will work with Prof. Benjamin Rose to build the necessary tools and methods to take advantage of current and next generation experiments designed to probe cosmology. We are committed to building a group that is inclusive and representative of our community. For this reason, we strongly encourage applicants who come from groups that are historically underrepresented in the fields of physics and astronomy. | | ▸ more | What You Will Do:
A successful candidate will work with Prof. Rose on the Roman Space Telescope and the Rubin Observatory Legacy Survey of Space and Time (LSST). Potential research topics include next generation pipeline development, photometric calibration of infrared telescopes, new techniques in statistical and image analysis, cosmology with Type Ia supernovae, developing follow-up strategies of variable and transient sources, innovative methods in image analysis for large surveys, and studies of astrophysical contributions to cosmological signals. Participation in some of the Roman Space Telescope, and the Rubin Observatory LSST DESC collaborations while at Baylor is expected.
More information on Prof Rose's research can be found at https://physics.artsandsciences.baylor.edu/person/dr-benjamin-rose.
These positions have an initial appointment for two years, renewable upon mutual agreement and availability of funding. The position can begin immediately, but is expected to begin by the start of the Fall 2024 semester. Candidates must have a Ph.D. by the date of appointment in astronomy, physics, or a relevant field. Applicants should prepare a cover letter, a current CV with a list of publications, a research statement of less than three pages describing past accomplishments and research goals, and arrange for three letters of recommendation to be sent. Applicants are encouraged to describe in their cover letter how their scholarship and experience would contribute to an inclusive community.
Required:
? PhD in Physics, Astronomy, or a closely related field
? Provide assistance with the preparation of project-related reports, manuscripts and presentations
? Conduct research design and oversee experiments
? Develop and establish experimental procedures
? Prepare and manage extensive databases
? Develop and implement research quality control procedures
? Analyze data and prepare reports; develop recommendations based on results
? Verify the accuracy and validity of data
? Work with highly technical and complex research instruments
? Perform all other duties as assigned to support Baylor's mission
? Ability to comply with University policies
? Maintain regular and punctual attendance
What You Can Expect:
Compensation & Benefits
As part of the Baylor family, eligible employees receive a comprehensive benefits package that includes medical, dental, and vision insurance, generous time off, and tuition remission. Baylor has a comprehensive benefits plan that supports you and your family's wellbeing and allows you to be a part of the life of a vibrant and active college campus. To learn more, go to https://www.baylor.edu/hr/index.php?id=949184.
Explore & Engage
Learn more about Baylor and our strategic vision, https://illuminate.web.baylor.edu/. Also, explore our great hometown of https://wacoheartoftexas.com/ and the many opportunities to https://waco.web.baylor.edu/waco-guides/waco-culture-guide.
About Us:
Baylor University is a private not-for-profit university affiliated with the Baptist General Convention of Texas. As an Affirmative Action/Equal Opportunity employer, Baylor is committed to compliance with all applicable anti-discrimination laws, including those regarding age, race, color, sex, national origin, military service, genetic information, and disability. Baylor?s commitment to equal opportunity and respect of others does not undermine the validity and effect of the constitutional and statutory protections for its religious liberty, including, without limitation, the religious organization exemption under Title VII of the Civil Rights Act of 1964, the religious exemption to Title IX of the Education Amendments of 1972, and the Free Exercise Clause of the First Amendment to the United States Constitution, among others. Baylor encourages women, minorities, veterans, and individuals with disabilities to apply. EEO/M/F/Vets/Disabled
To apply, visit https://apptrkr.com/5136613
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