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| OSSSB@LSST: Outer Solar System Small Bodies in the era of LSST | Closing date: 2024-09-07
Contact: Jean-Marc PETIT |
The Vera C. Rubin Observatory will conduct the Legacy Survey of Space and Time (LSST)- the widest and deepest optical survey to date - over 10 years starting late 2025. It will repeatedly observe millions of Solar System small bodies (SSSBs) over this period.
By their large number, physical, compositional and dynamical characteristics of the various SSSB populations hold statistically significant clues on the origin and evolution of our Solar System.
The successful PostDoc will work on implementing dedicated detection and characterization algorithms in the LSST pipeline specilized for TNOs. | | ▸ more | The ASTRO team of UTINAM Institute, located on the western side of
lovely town Besançon (Franche Comte, FRANCE), as been and is still involved in
many major astronomical surveys of solar systeme and (sub-)stellar objects,
such as CFHT-LS, WEAVE, OSSOS, CLASSY, Gaia, GUCDS, CFBDS, EUCLID and LSST. In
these surveys, our team have played and is playing major roles in designing,
running and processing the data of the surveys.
We invite applications for a Post-Doctoral position in which the
candidate is expected to work 70-80% of her time on our activities in the
OSSSB @ LSST (Outer Solar System Small Bodies at LSST; pipeline preparation), and
the remaining time on science related to our research interests on TNO and
early solar system modelisation.
The Vera Rubin Observatory is a new large telescope which will achieve
first-light in early 2025. It will perform the Large Survey of Space and Time
(LSST) starting end of 2025 for a duration of 10 years. LSST will provide an
unprecedented snapshot of the Small Bodies of the Solar System which are to the
study of the solar system the equivalent of radiogenic isotopes to the study of
rocks.
OSSSB @ LSST will use the survey to better understand the populations of
OSSSBs by increasing by an order of magnitude the size of the known
sample. OSSSBs are the less evolved populations of the solar system and contain
invaluable clues on its formation and early evolution.
The full scientific exploitation of the OSSSB @ LSST survey requires to
provide 2 pieces of processing pipelines:
- detection: optimize and parallelize on GPU our detection algorithmes,
extensively used for our previous surveys, relying on 2 separate detection
methods to drasticvally decrease the number of false positives while retaining
a good efficeincy at limiting magnitude;
- characterization: since the survey CANNOT be complete at small sizes, we must
determine our detection efficiency as a function of observing parameters in
order to connect to the real populations; we plan to develop new Machine
Learning methods to process this huge dataset.
Our research interests are primarily:
- observation of TNOs, determining their size and orbital distirbutions;
- modelling the early evolution of the solar system, with dissipation of the
planetesimal disk;
- preparing for physical TNO binary observations with MICADO/E-ELT.
The position is funded by the Région Bourgogne-Franche Comté.
The starting date is October 2024, but applications to start weeks later, up
until Januray 2025, will be considered.
Funding is available for one year.
The net salary after tax deduction is approximately 2100 euros/month, including
medical insurance.
To apply please submit to Jean-Marc Petit (jean-marc.petit @ normalesup.org) a
curriculum vitae, a publication list, a summary of previous research, and a
statement describing how you plan to get involved in the team.
In addition, please arrange for two letters of recommendation to be sent to the
above address by the deadline of 7 September 2024.
Équipe ASTRO/UTINAM, UFC Besançon, 25000 Besançon, France
Category: Research, full time
Lab's web site: https://www.utinam.cnrs.fr/ and https://www.utinam.cnrs.fr/emploi/
[[Link to the scientific rationale of the OSSSB @ LSST proposal|https://www.utinam.cnrs.fr/wp-content/uploads/2024/07/ossos-petit_en.pdf]]
[[Link to a short presentation of OSSSB @ LSST|https://www.utinam.cnrs.fr/wp-content/uploads/2024/07/Presentation_projetGS_JMP_V1_en.pdf]]
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| Three postdoctoral positions in observational astrophysics, Warsaw, Poland | Closing date: 2024-09-10
Contact: Katarzyna Ma?ek |
The National Centre for Nuclear Research opens three postdoc positions in the field of observational astrophysics:
1. The search for low surface brightness galaxies,
2. Clustering of low surface brightness galaxies,
3. Smashing Galaxies into Dust. | | ▸ more | The Astrophysics Department of the NCBJ's Fundamental Research Division is dedicated to research in astrophysics and astronomy, mainly its observational aspects. The Division employs 19 people, including eight foreigners, at the rank of Assistant Professor and above. 9 PhD students from the Department of Astrophysics are trained in the Doctoral School of the NCBJ and the IChTJ. The Department of Astrophysics offers an active research environment at the highest international level.
The National Centre for Nuclear Research opens three postdoc positions in the field of observational astrophysics:
1. The search for low surface brightness galaxies
2. Clustering of low surface brightness galaxies
both under project MAESTRO No 2023/50/A/ST9/00579 "Barely Visible: Low Surface Brightness Universe in the LSST era," led by Prof. Agnieszka Pollo. (Agnieszka.Pollo @ ncbj.gov.pl), and
3. "Smashing Galaxies into Dust" financed by NCN project SONATA 19 No UMO-2023/51/D/ST9/00147 - "Smashing galaxies into dust" led by dr William Pearson (William.Pearson @ ncbj.gov.pl).
Link to the website of the Department of Astrophysics: https://www.ncbj.gov.pl/en/astrophysics-division
Link to the job offers:
https://www.ncbj.gov.pl/en/astrophysics-division/work-with-us
Please contact the PIs directly for further details.
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| SKA-Mid Commissioning Scientists | Closing date: 2024-08-30
Contact: Heather |
The SKA Observatory is seeking to appoint experienced and motivated radio astronomers to plan and execute the scientific commissioning of the SKA-Mid Telescope array. The post-holders will form the nucleus of a small group of commissioning astronomers primarily based in Cape Town, South Africa, with the possibility of the location at the headquarters in the UK being considered under exceptional circumstances. We are also open to secondments.
For more information and to apply click here: https://recruitment.skao.int/vacancy/skamid-commissioning-scientists-554732.html | | ▸ more | The Role
As part of the construction of the SKA-Mid Telescope, a team of commissioning scientists is needed for planning, executing, and analysing test observations. This recruitment aims to hire the first four roles with a 4-year Fixed Term Contract, with the team expanding over the next 12 months. Commissioning activities will commence immediately and will continue through to initial operations of the telescope.
Two skill sets are required: organisational and technical. Therefore we aim to fill four posts, including one Lead. Depending on applicants' experience, one of the other posts may be at the Senior level:
-Lead Commissioning Scientist: Manages the commissioning team. Capable of leading the group, planning and documenting tests, and organising interactions with external stakeholders.
-Senior Commissioning Scientist: Acts as technical lead for the group and mentor to less experienced members. Must have significant commissioning experience and a deep understanding of interferometric radio astronomy and system issues. Quite likely to prefer secondment.
-Commissioning Scientist: Familiar with the operation of radio interferometric arrays and with high potential to develop commissioning skills.
The Lead reports to the Head of System Science and the SKA-Mid Telescope Director. The remaining positions will handle specific technical areas under the Lead's direction.
Please indicate on your application whether you would like to be considered for the Lead Commissioning Scientist position.
Key Responsibilities, Accountabilities and Duties
The primary tasks of the Science Commissioning group are:
-Take responsibility for science commissioning tasks including but not limited to: planning, execution and analysis of test observations on the telescope array. The group will work closely with the System Science Group based at GHQ (UK), which has oversight of commissioning of both SKA Telescopes.
-Submit both written and verbal reports on the analysis done during the commissioning activities.
-Close collaboration with engineering (hardware and software) groups involved in construction to verify aspects of the system and to identify and suggest corrections as needed. There will be a particularly close interaction with the Assembly, Integration and Verification (AIV) Group based in Cape Town, South Africa to verify the top-level engineering requirements of the array.
-Maintain a close interaction with the Science Operations Group, in particular to support Science Verification.
-Create the documentation for commissioning test procedures, initially for the early deployment of SKA-Mid.
Further, the Lead Commissioning Scientist requires additional essential criteria, as follows:
-Lead the SKA-Mid Science Commissioning Group.
-Take responsibility for detailed planning of the science commissioning of the SKA-Mid Telescope.
-Oversee the development, execution and documentation of astronomical test procedures, initially for the early deployment of SKA-Mid.
-Take responsibility for specific technical areas.
-Maintain close and effective collaboration with Engineering (AIV), Science Operations and System Science groups.
Research and Career Progression:
The duration of the commissioning phase is limited. At the end of the construction phase of the project the SKA-Mid Science Operations team will be recruiting more positions. Should applicants applying for this role possess the relevant skills, and these are tested at interview and assessment, then they may receive the offer of a permanent contract. Other applicants may receive offers for this role based on a 4-year fixed term contract but will of course have the opportunity to apply for further roles with the Observatory following the completion of their contract.
The appointees will be encouraged to carry out research in astronomy or astronomical instrumentation at a level commensurate with the requirements of the post (typically 25%) and in particular to exploit early opportunities with the SKA. Appropriate support, including conference travel, will be provided.
These roles are primarily based in Cape Town, South Africa, with occasional travel to the UK and Karoo. Applications to be based in the UK will be considered in exceptional cases.
SKAO is committed to providing an inclusive and flexible working environment: we believe you perform your best when you have a healthy work-life balance. We are open to discussing flexible working opportunities with these roles being offered on a full-time, part-time or job share basis. Please raise your preference in your application.
We encourage applications from under-represented groups such as women and individuals with disabilities, as well as open conversations during the recruitment process in relation to any specific requirements.
There will be occasions where these roles require the post holder to work across different time zones and, in line with SKAO policy, flexible working hours will be supported in agreement with the line manager.
Informal enquiries may be made to Robert Laing, Head of System Science (Robert.Laing @ skao.int).
Equality Diversity and Inclusion Statement
SKA Observatory recognises that our diversity is a strength. We aim to create a welcoming and inclusive environment where everyone feels they belong, and diverse perspectives and ideas thrive. As such, Equality, Diversity, and Inclusion are at the core of SKA Observatory?s agenda.
Our aim is to recruit and retain the most talented individuals, regardless of gender, race, disability, age, sexual orientation, marital status, religion, nationality or background.
SKA Observatory welcome all candidates, especially those from member countries.
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| Post-doctoral position in X-ray astronomy | Closing date: 2024-09-01
Contact: Jean Ballet |
We invite applications for a position in which the candidate is expected to work half-time on our activities in the XMM SSC consortium, and half-time on science related to our research interests.
Starting date: January 2025
| | ▸ more | AIM/Departement d'Astrophysique, CEA Saclay, 91191 Gif sur Yvette Cedex, France
Lab's web site: https://irfu.cea.fr/dap/en/
SSC web site: http://xmmssc.irap.omp.eu/
The astrophysics department at Saclay, which is situated 30 km south of Paris, is a major space astrophysics laboratory and is also involved in ground-based instrumentation.
Our institute played a major role in the hardware development and calibration of the EPIC MOS cameras on XMM Newton and participates in the SSC consortium that is responsible for the catalogue of XMM-Newton sources.
At high energies, the institute provides important contributions to Integral, Fermi, SVOM and the future Athena mission, as well as the HESS and CTA TeV instruments.
Other major projects are JWST/MIRI, Euclid, ELT/METIS, ARIEL.
Our activities in the XMM SSC consortium include the EPIC MOS data analysis software, the EPIC MOS in-flight calibration, background studies, screening the products generated by the data processing pipeline and testing the catalogue products.
Our research interests are primarily in three domains:
- supernova remnants (F. Acero, A. Decourchelle, J. Ballet), where our interests lie primarily around detailed spatially-resolved studies and modelling of nearby SNRs;
- multi wavelength observations of clusters of galaxies (G.W. Pratt);
- mining the XMM catalogue (J. Ballet).
The position is funded by the French space agency CNES.
The starting date is January 2025, but applications to start a few months later will be considered.
Funding is available for two years, with a possible extension for an additional year.
The net salary after tax deduction is approximately 2000 euros/month, including medical insurance.
To apply please submit to Jean Ballet (jballet @ cea.fr) a curriculum vitae, a publication list, a summary of previous research, and a statement describing how you plan to get involved in the team.
In addition, please arrange for two letters of recommendation to be sent to the above address by the deadline of 1 September 2024.
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| Postdoctoral position related to PLATO science | Closing date: 2024-08-05
Contact: Heike Rauer |
| The FU Berlin (Department of Geosciences/Planetary Sciences) cooperates with the Institute for Planetary Research of the German Aerospace Center (DLR) as part of the PLATO mission (PLAnetary Transits and Oscillations of stars). The mission aims to find and characterize extrasolar planets, including Earth-like planets. | | ▸ more | The FU Berlin (Department of Geosciences/Planetary Sciences) cooperates with the Institute for Planetary Research of the German Aerospace Center (DLR) as part of the PLATO mission (PLAnetary Transits and Oscillations of stars). The mission aims to find and characterize extrasolar planets, including Earth-like planets.
The PLATO Mission Consortium develops parts of the scientific payload, participates in the scientific operation of the payload, the scientific ground segment and ground-based follow-up observations to determine the mass, as well as in scientific mission planning and analysis.
The applicant supports the activities of the PLATO team regarding the creation of data production on the internal structure and evolution of detected planets
Job description:
The aim of this work package is to develop numerical models to provide information on the internal structure of exoplanets and study their evolution over time.
In addition to the primary parameters, information on planet interiors can be included in the PLATO planet catalogue and thus provide the scientific community with initial clues about the nature of the discovered planets as a basis for follow-up observations and further detailed modelling. Tasks include:
- Development of models to derive information about the internal structure and temporal evolution of planets from PLATO parameters.
- Development of an interface for the PLATO L2 and L3 database.
- Linking the results with theories on planet formation.
Please, submit your application as pdf-file by August 5, 2024 to plansec @ zedat.fu-berlin.de .
The expected starting date is not earlier than October 2024. The duration of the contract is limited until December 31, 2027.
Further details about the position can be found at:
https://www.fu-berlin.de/universitaet/beruf-karriere/jobs/english/GW-WiMi_PLATO-Katalog_Planetologie-2024.html
For further information, please contact Mrs Stefanie Pott (plansec @ zedat.fu-berlin.de / 030/838- 70575) or Heike Rauer (heike.rauer @ dlr.de).
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| University PhD assistant position in exoplanetary atmosphere simulations - University of Vienna | Closing date: 2024-07-30
Contact: Manuel Guedel |
| We invite applications for a 3-year doctoral (PhD) position in the area of exoplanet atmospheres at the Department of Astrophysics, University of Vienna. The Department of Astrophysics with currently around 100 members is part of the Faculty of Earth Sciences, Geography and Astronomy at the University of Vienna. | | ▸ more | Project and Tasks:
We are looking for a highly motivated and talented predoctoral researcher. You will work in the Star and Planet Formation group of Manuel Güdel in the field of planetary atmospheres and their evolution and collaborate closely with the exoplanetary atmospheres group of Sudeshna Boro Saikia in the same department. You will perform simulations of upper planetary atmospheres and their loss into space, contribute to the further development of corresponding simulation code including chemical networks and link it to atmospheric retrieval.
You will profit from interactions with a lively and diverse team engaging in research on planet formation in protoplanetary and debris disks, exoplanetary atmospheres and their evolution, solar system planetary evolution, and stellar astrophysics and magnetic activity.
- We expect you to finalize your dissertation agreement within 12-18 months.
- You work on your dissertation and its completion at the end of 3 years.
- You will join the Vienna International School of Earth and Space Sciences (VISESS, https://visess.univie.ac.at/).
- You hold courses independently within the scope of the provisions of the collective bargaining agreement.
Starting date preferably in September/October 2024
Funding: 75% position (30h/week) for 3 years
Job Classification in Collective Bargaining Agreement: §48 VwGr. B1 (predoc)
Your Profile:
- Completed Master's degree or Diploma in the field astrophysics or physics
- Basic knowledge of astrophysics
- Programming skills (Fortran is the main language of the project; Python, C, or C++ beneficial)
- Excellent command of written and spoken English
- Excellent abilities to work in a team and excellent communication skills
The University Offers:
- Salary: Job grading in accordance with collective bargaining agreement: §49 (3) lit. a (B1, predoc), https://personalwesen.univie.ac.at/en/jobs-recruiting/salary-scheme/
- Privileged access to the Vienna Scientific Cluster (VSC; https://vsc.ac.at/) super-computing facility.
- An interdisciplinary and international environment.
- Many opportunities for advanced learning/training.
Application Details:
Please prepare your application as follows:
- a motivation letter (max. one page)
- a curriculum vitae with a list of publications and presentations (max. two pages)
- name, affiliation and email address of at least two referees (referees will be contacted
directly after the application deadline)
- bachelor´s and master´s diploma and transcripts
- Application deadline: 07/30/2024
Link to online application including full job ad (Job ID: 2514)
https://jobs.univie.ac.at/job/University-PhD-assistant-in-exoplanetary-atmosphere-simulations/1092160801/
If you have any questions, please contact Manuel Guedel, manuel.guedel @ univie.ac.at
The University of Vienna has an anti-discriminatory employment policy and attaches great importance to equal opportunities, the advancement of women and diversity: https://gleichbehandlung.univie.ac.at/en/ , https://personalwesen.univie.ac.at/en/culture-equality/diversity/ .
We lay special emphasis on increasing the number of women in academic positions among the academic and general university staff and therefore expressly encourage qualified women to apply. Given equal qualifications, preference will be given to female candidates.
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| PhD Opportunities in observational astrophysics (five positions) | Closing date: 2024-08-06
Contact: Katarzyna Ma?ek |
We invite applications for five PhD positions in observational astrophysics at the National Centre for Nuclear Research (NCBJ) in Poland.
The Department of Astrophysics of the NCBJ Department of Fundamental Research is involved in research in the fields of astrophysics and astronomy, mainly in their observational aspects. The department currently employs 19 staff members and 9 PhD students. Here is a list of employees: https://www.ncbj.gov.pl/en/astrophysics-division/employees | | ▸ more | The Department of Astrophysics focuses on Cosmology (including CMB, large-scale Structure of the Universe, dark matter, and gravitational lensing), Gravitational Waves (Multimessenger Astronomy), Galaxy Physics (galaxy formation and evolution, active galactic nuclei and quasars), and Astronomy of the Interstellar Medium (Star Formation, neutron stars, and white dwarfs).
Our PhD topics:
1. Gravitational lensing of the cosmic microwave background in the era of big surveys
2. Linking dust attenuation and radio data
3. Reliably identifying merging galaxies in large surveys
4. Properties of low surface brightness galaxies in the LSST era
5. Low surface brightness galaxies in the LSST era as a Big Data challenge
The webpage with a short description can be found here: https://www.ncbj.gov.pl/en/astrophysics-division/work-with-us
Rules and the instruction on how to apply are listed directly on the webpage of the doctoral school: https://gradschool.ncbj.gov.pl/
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| Two PostDoc positions in ELT pipeline development / University of Innsbruck | Closing date: 2024-07-19
Contact: Prof. Norbert Przybilla |
| The University of Innsbruck is the largest and most important research and education facility in Western Austria. The Galactic Astrophysics group of Prof. Norbert Przybilla at the Institute for Astro- and Particle Physics invites applications for two postdoctoral positions to support development of data-reduction software packages for spectroscopic modes of the ESO ELT instruments MICADO and METIS. | | ▸ more | Your tasks:
- independent project work for ESO ELT instrumentation projects
- participation in organizational and administrative tasks
Your profile:
- completed doctoral studies in astronomy or physics with a focus on astronomy/astrophysics
- experience in the research field of astronomy/astrophysics, preferably in observation-oriented astronomy and development of astronomical data reduction software
- experience in data acquisition, data reduction in the optical through mid-infrared wavelength range and data analysis of astronomical instruments
- experience in use of state-of-the-art astronomical software packages
- knowledge of ESO software standards for data reduction pipelines
- ability to work in a team with project groups at international level
- problem-solving skills
The appointment is for two years with the possibility of extension beyond that period contingent upon performance and availability of funding.
Compensation and Benefits:
The minimum gross salary (stipulated by collective agreement for the universities of Austria) for this position is susceptible to increase depending on inflation and amounts to ? 4.752 per month (as of 2024), 14 salaries/year.
It also includes health and pension insurance (following the collective bargaining agreement of the university) and 5 weeks of holidays. The University of Innsbruck voluntarily also offers several additional benefits like a grant for the local public transport, flexible working hours, a family-friendly working environment, and attractive training and development opportunities, see https://www.uibk.ac.at/de/karriere/zusatzleistungen/ for more details.
The University of Innsbruck pursues a non-discriminatory employment policy and values equal opportunities, as well as diversity. Individuals from underrepresented groups are particularly encouraged to apply.
Application Details:
The application has to be submitted via the web portal of the University of Innsbruck.
Required documents: cover letter including names and contact information for two references, who may be contacted for letters of recommendation, CV with publication list, a statement that describes all relevant experiences related to observations and development of data reduction software (maximum 2 pages).
Reference Codes: MIP-14262, MIP-14263
Links to the online applications:
https://lfuonline.uibk.ac.at/public/karriereportal.details?asg_id_in=14262
https://lfuonline.uibk.ac.at/public/karriereportal.details?asg_id_in=14263
Applicants are asked to apply to both positions.
Application Deadline: 2024 Jul 19
Contact for inquiries:
Professor Norbert Przybilla
norbert.przybilla @ uibk.ac.at
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| Two postdoctoral positions in solar and stellar physics at HIT Shenzhen, China | Closing date: 2024-09-31
Contact: Valery Nakariakov |
| Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen (HIT Shenzhen), China is hiring two postdoctoral researchers to address impulsive energy releases in the solar and stellar atmospheres, for a duration of two years. The working language will be English. The project is jointly led by Professor Valery Nakariakov (University of Warwick, UK) and Professor Ding Yuan (HIT Shenzhen). | | ▸ more | Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen (HIT Shenzhen), China is hiring two postdoctoral researchers for a duration of two years.
The postdocs will address the fundamental physical processes responsible for impulsive energy releases in the solar and stellar atmospheres, such as flares and coronal mass ejections (CME). The main emphasis will be put on the quasi-periodic pulsations in flares, the role of oscillatory processes in CMEs, and the exploitation of the solar-stellar analogy.
The project is jointly led by Professor Ding Yuan (HIT Shenzhen) and Professor Valery Nakariakov (University of Warwick, UK). The project is dedicated to analysis of data obtained with modern EUV, X-ray, white light, and radio observational facilities, analytical studies, and high-performance numerical simulations, including forward modelling of plasma emissions.
The postdocs will be based at the dynamic and cosmopolitan Shenzhen campus of Harbin Institute of Technology, located in one of the most modern and advanced cities in China. The annual salary is around 240k RMB.
The candidates shall possess a PhD in solar physics, astrophysics, plasma physics, machine learning or related field. Experience in numerical simulation of plasma processes is a strong plus. Applicants shall send an e-mail with a CV, publication list and references (at least two) to yuanding @ hit.edu.cn. The position will remain open until filled, with priority for applications received before end of August. Feel free to reach out with any informal inquiries to V.Nakariakov @ warwick.ac.uk.
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| Professor in experimental planetary science (in situ mass spectrometry) | Closing date: 2024-08-01
Contact: Christoph Mordasini |
| The Division of Space Research and Planetary Sciences within the Physics Institute of the University of Bern has an opening, as of 2025, for a Professor in Experimental Physics (100%) in space instrumentation for experimental planetary science, field of in situ mass spectrometry. | | ▸ more | The Division is one of the leading research groups in the field of space instrumentation for experimental Solar System exploration and is looking for a professor in the field of planetary in situ mass spectrometry or a related field. The initial hiring level can range from assistant professor tenure track to full professor according to qualifications (open rank). The position will be filled in coordination with another open professorship in experimental planetology (field of remote sensing) at the Division. This inter-dependence may influence the finally available rank.
The successful candidate is expected to have or further develop an excellent and internationally recognized track record in the development, construction, and exploitation of scientific instrumentation flying on major spacecraft missions. The successful candidate's research program will constitute a central part of the Division's core research activities and represent the field of space research nationally and internationally. It will complement existing research activities both at the University and within the Swiss and international landscapes. The successful candidate will be part of a vibrant Division and Institute interacting in research, education, outreach, and administration as a member of the physics faculty. The Division offers excellent conditions in terms of laboratory infrastructure, engineering, and manufacturing capabilities to build space-grade hardware.
We expect an outstanding academic record including successful acquisition of third-party funds, demonstrated expertise in instrument development, a strong international network in space research including multiple links to space agencies, excellent social skills, and leadership qualities. The person will teach at BSc. and MSc. level, including lecturing basic physics courses in German for which non-German speakers will be given the necessary time to become competent in the language.
Candidates are expected to hold a PhD in physics or a related field and must be able to teach physics classes. The University of Bern values diversity and is committed to equal opportunities; applications are welcome from all suitably qualified candidates who meet the stated criteria. The University of Bern has set the aim of increasing the percentage of women in leading academic positions and thus strongly encourages female scientists to apply for the position. Applications proposing job sharing will also be considered. The University of Bern has signed the DORA declaration and will apply its principles to the recruiting process. Remuneration is in accordance with the personnel regulations of the Canton of Bern.
Applications should include: Letter of motivation, Curriculum vitae, List of publications, List of courses taught, List of third-party funds raised, List of contribution to space missions and instrument developments, Information on further academic activities including science management, Research plan for the first 5 years.
The application documents must be submitted by 1. August 2024 electronically in a single PDF file (smaller than 10 MB) to the Dean's Office (email: applications.natdek @ unibe.ch ), Sidlerstrasse 5, 3012 Bern, Switzerland, including this completed online questionnaire:
https://www.space.unibe.ch/about_us/jobs/questionnaire/index_eng.html
where also additional information on the position can be found. The contact person for inquiries is Prof. Christoph Mordasini, Executive Director of the Division of Space Research and Planetary Sciences: jobs.space @ unibe.ch
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| Professor in experimental planetary science (remote sensing) | Closing date: 2024-08-01
Contact: Christoph Mordasini |
| The Division of Space Research and Planetary Sciences within the Physics Institute of the University of Bern has an opening, as of 2025, for a Professor in Experimental Physics (100%) in space instrumentation for experimental planetary science, field of remote sensing. | | ▸ more | The Division is one of the leading research groups in the field of space instrumentation for experimental Solar System exploration and is looking for a professor in the field of planetary remote sensing or a related field. The initial hiring level can range from assistant professor tenure track to full professor according to qualifications (open rank). The position will be filled in coordination with another open professorship in experimental planetology (field of in situ mass spectrometry) at the Division. This interdependence may influence the finally available rank.
The successful candidate is expected to have or further develop an excellent and internationally recognized track record in the development, construction, and exploitation of scientific instrumentation flying on major spacecraft missions. The successful candidate's research program will constitute a central part of the Division's core research activities and represent the field of space research nationally and internationally. It will complement existing research activities both at the University and within the Swiss and international landscapes. The successful candidate will be part of a vibrant Division and Institute interacting in research, education, outreach, and administration as a member of the physics faculty. The Division offers excellent conditions in terms of laboratory infrastructure, engineering, and manufacturing capabilities to build space-grade hardware.
We expect an outstanding academic record including successful acquisition of third-party funds, demonstrated expertise in instrument development, a strong international network in space research including multiple links to space agencies, excellent social skills, and leadership qualities. The person will teach at BSc. and MSc. level, including lecturing basic physics courses in German for which non-German speakers will be given the necessary time to become competent in the language.
Candidates are expected to hold a PhD in physics or a related field and must be able to teach physics classes. The University of Bern values diversity and is committed to equal opportunities; applications are welcome from all suitably qualified candidates who meet the stated criteria. The University of Bern has set the aim of increasing the percentage of women in leading academic positions and thus strongly encourages female scientists to apply for the position. Applications proposing job sharing will also be considered. The University of Bern has signed the DORA declaration and will apply its principles to the recruiting process. Remuneration is in accordance with the personnel regulations of the Canton of Bern.
Applications should include: Letter of motivation, Curriculum vitae, List of publications, List of courses taught, List of third-party funds raised, List of contribution to space missions and instrument developments, Information on further academic activities including science management, Research plan for the first 5 years.
The application documents must be submitted by 1. August 2024 electronically in a single PDF file (smaller than 10 MB) to the Dean's Office (email: applications.natdek @ unibe.ch ), Sidlerstrasse 5, 3012 Bern, Switzerland, including this completed online questionnaire:
https://www.space.unibe.ch/about_us/jobs/questionnaire/index_eng.html
where also additional information on the position can be found. The contact person for inquiries is Prof. Christoph Mordasini, Executive Director of the Division of Space Research and Planetary Sciences: jobs.space @ unibe.ch
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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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