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| Scientist / Optical Engineer in Optical Spectroscopy (m/f/d) at AIP in Potsdam | Closing date: 2022-02-11
Contact: Andreas Kelz |
The Leibniz-Institute for Astrophysics Potsdam (AIP) invites applications for a Scientific Researcher / Optical Engineer in Optical Spectroscopy (m/f/d) for the development of an optical fiber system for the Multi-Object Spectrograph of the European Extremely Large Telescope (ELT-MOSAIC).
For the development of a Multi-Object Spectrograph (MOS) for the Europe an Extremely Large Telescope (ELT), AIP is partnering with European wide consortia, and is in charge of the optical fiber system from the telescope to the spectrographs. | | ▸ more | The advertised position is to work with the team to undertake the technical R&D activities of the preliminary design study, to conduct measurements in the optical laboratories and to document the findings and results.
The Leibniz-Institute for Astrophysics Potsdam (AIP) is dedicated to astrophysical questions ranging from the exploration of our Sun to the evolution of the cosmos, supported by the development of research technology in the fields of spectroscopy. The AIP has many years of experience in the area of optical instrumentation for international telescope facilities, like ESO, LBT, HET or the Calar Alto observatory.
Former and current instrumentation projects include 4MOST, MUSE, PMAS, PEPSI and VIRUS; special focus is put on fiber coupled multi-channel and integral-field spectroscopy.
Your tasks
- Develop the p reliminary design of the optical fiber systems for ELT-MOSAIC
- Contribute to the optical and mechanical design
- Provide technical feedback on the top level requirements and the statement of work
- Define the interfaces to the other sub-systems
- Assembly and experimental evaluation of fiber cable prototypes
- Set up of optical test benches
- Measurements of optical fibers and micro optics
- Interaction with industrial partners
- Documentation of designs, experimental setups and measurement results
- Reporting to local and consortium project offices
Essential criteria
- Bachelor (or higher degree) in Physics, Optical Engineering or related discipline
- Proficiency an d experience in (fiber) optics and working in optical / physics laboratories
- Excellent communication skills in English, written and spoken
- Ability to communicate effectively with peer engineering staff
- Hands on experience in optics, e.g. optical design, optical test set ups, measurements
- Good general computer user skills (e.g. standard Office packages, Windows, or Linux)
Desired experience
- Programming skills (e.g. C++, IDL, MATLAB and/or LabView)
- A background in fiber optical techniques and / or development of astronomical instrumentation
- Experience in experimental and theoretical fiber optics and/or micro-optics is a plus
- Communication skills in German are a desirable
- Self motivation, creativity, flexibility and the ability to work alone and in a team are highly appreciated
Offering & Conditions
The AIP is an equal opportunity employer and strives to maintain a diverse, inclusive work environment and culture. AIP particularly encourages applications from women. Preference will also be given to people with disabilities with equal competence.
The position is offered on a fixed term contract of 24 months with a possible extension depending on performance and funding. Salary and social benefits are calculated based on the German public service scale. A salary level between E10 and E13 TV-L is envisaged, depending on qualifications and experience in relation to the position. Employer contributions to medical, parental leave, and retirement benefits are included. The position can be either full time or part time assignment.
AIP offers an open minded and cooperative working atmosphere in a modern working environment, very well equipped and located in the middle of a UNESCO World Heritage Site. The institute is located in the beautiful Potsdam-Babelsberg area, southwest of Berlin and has about 200 employees.
Application
To apply, please register at https://jobs.aip.de/rec001 and follow the instructions to upload pdf files of your curriculum vitae, documentation of your qualifications, and either references or contact information for (at least) two referees. Complete applications received by Feb. 10th, 2022 will receive full consideration, but review of applications will continue until the position is filled.
For further information or in case of questions, please contact bewerbung-2022-01 @ aip.de.
Please note that your application documents will be made available to the members of the selection committee and appropriate bodies within AIP. These documents will be kept for at least three months after the completion of the application process.
Contact
Dr Andreas Kelz
Head of 3D and Multi-Object Spectroscopy
Leibniz-Institut für Astrophysik Potsdam (www.AIP.de)
An der Sternwarte 16
D-14482 Potsdam
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| Systems Engineer (m/f/d) for astronomical instrumentation at AIP in Potsdam | Closing date: 2022-02-11
Contact: Andreas Kelz |
The Leibniz-Institute for Astrophysics Potsdam (AIP) invites applications for a Systems Engineer (m/f/d) for the development and support of astronomical instrumentation projects. The successful candidate will work on an advanced optical fiber system for the MOSAIC instrument for the European Extremely Large Telescope in collaboration with the local AIP project team and external partner network.
The MOSAIC project is now entering its Preliminary Design Phase which will conclude with a formal phase gate review. | | ▸ more | The Leibniz Institute for Astrophysics Potsdam (AIP) is dedicated to astrophysical questions ranging from the exploration of our Sun to the evolution of the cosmos, supported by the development of research technology in the fields of spectroscopy. The AIP has many years of experience in the area of optical instrumentation for international telescope facilities, like ESO, LBT, HET or the Calar Alto observatory.
Former and current instrumentation projects include 4MOST, MUSE, PMAS, PEPSI and VIRUS; special focus is put on fiber coupled multi-channel and integral-field spectroscopy.
Your tasks
- System functional and performance analysis:
- Perform and document system functional breakdown.
- Perform and document system performance analyses.
- Develop models and simulations as needed
- Requirements development and management:
- Derive performance requirements from top level requirements.
- Develop system operational and maintenance requirements.
- Manage system requirements.
- Prepare design trade off analyses.
- Define p reliminary verification plan.
- Create and distribute error budgets.
- Interfaces definition and management, Interface Control Documents (ICDs).
- Design documentation.
Essential criteria
- Bachelor (or higher degree in Engineering
- Proficiency in System Engineering tools and processes
- Excellent communication skills in English, written and spoken
- Ability to communicate effectively with peer engineering staff
- Basic understanding of optical fibre systems
Desired experience
- Formal degree in Systems Engineering.
- Experience in development, deployment and operation of optical instruments for astronomy.
- Experience with advanced fiber optic relay systems.
- Experience with engineering in international collaborations.
- Disciplined in quality and product assurance.
- Commun ication skills in German are a desirable
- Self motivation, creativity, flexibility and the ability to work alone and in a team are highly appreciated
Offering & Conditions
The AIP is an equal opportunity employer and strives to maintain a diverse, inclusive work environment and culture. AIP particularly encourages applications from women. Preference will also be given to people with disabilities with equal competence.
The position is offered on a fixed term contract of 24 months with a possible extension depending on performance and funding. Salary and social benefits are calculated based on the German public service scale. A salary level between E10 and E13 TV-L is envisaged, depending on qualifications and experience in relation to the position. Employer contributions to medical, parental leave, and retirement benefits are included. The position can be either full time or part time assignment.
AIP offers an open minded and cooperative working atmosphere in a modern working environment, very well equipped and located in the middle of a UNESCO World Heritage Site. The institute is located in the beautiful Potsdam- Babelsberg area, southwest of Berlin and has about 200 employees.
Application
To apply, please register at https://jobs.aip.de/rec002 and follow the instructions to upload pdf files of your curriculum vitae, documentation of your qualifications, and either references or contact information for (at least) two referees. Complete applications received by Feb. 10th, 2022 will receive full consideration, but review of applications will continue until the position is filled. For further information or in case of any
questions, please contact bewerbung-2022-02 @ aip.de.
Please note that your application documents will be made available to the members of the selection committee and appropriate bodies within AIP. These documents will be kept for at least three months after the completion of the application process.
Contact
Dr Andreas Kelz
Head of 3D and Multi Object Spectroscopy
Leibniz-Institut für Astrophysik Potsdam (AIP)
An der Sternwarte 16
D-14482 Potsdam
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| Time evolution of the star formation rate density in the early Universe | Closing date: 2022-03-01
Contact: Maciej Koprowski |
| The astronomy group at Nicolaus Copernicus University (Torun, Poland) invites applications for a PhD position in extragalactic astronomy, working on the determination of the time evolution of the star formation rate density in the early Universe out to redshifts as high as ~7. | | ▸ more | The project involves working with the observational data, collected with the state-of-the-art telescopes, like ALMA, JCMT, Herschel, Spitzer, Hubble, etc., using stacking techniques in order to quantify the contribution from faint galaxies, writing your own codes and summarising the results in the form of the scientific paper.
Torun is located in the heart of Poland and is renowned for its beautiful medieval town centre, its lively cultural scene and its vibrant student life. The institute is located some 15km north of the Torun city center in the Piwnice Observatory - home of the 32-m RT-4 radio telescope, being a part of the European VLBI network.
The position is fully funded for 3-3.5 years. We offer a scholarship of 3000 PLN per month, raising to 3500 PLN per month after the first half of the degree. In addition, the position has a generous funding available for conferences and research visits.
Applicants should have an MSc degree in astronomy or a closely related field and a good English speaking and writing skills. Previous experience with programming will be an advantage.
Application deadline is set for 1st of March 2022 and the project can start as early as 1st April 2022, but a later date can be negotiated. Applicants should submit their CV, a statement of the candidate's research interests, experience, and skills directly to mkoprowski @ umk.pl and arrange for two reference letters to be sent to the same address.
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| Time evolution of the star formation rate density in the early Universe | Closing date: 2022-03-01
Contact: Maciej Koprowski |
| The astronomy group at Nicolaus Copernicus University (Torun, Poland) invites applications for a PhD position in extragalactic astronomy, working on the determination of the time evolution of the star formation rate density in the early Universe out to redshifts as high as ~7. | | ▸ more | The project involves working with the observational data, collected with the state-of-the-art telescopes, like ALMA, JCMT, Herschel, Spitzer, Hubble, etc., using stacking techniques in order to quantify the contribution from faint galaxies, writing your own codes and summarising the results in the form of the scientific paper.
Torun is located in the heart of Poland and is renowned for its beautiful medieval town centre, its lively cultural scene and its vibrant student life. The institute is located some 15km north of the Torun city center in the Piwnice Observatory - home of the 32-m RT-4 radio telescope, being a part of the European VLBI network.
The position is fully funded for 3-3.5 years. We offer a scholarship of 3000 PLN per month, raising to 3500 PLN per month after the first half of the degree. In addition, the position has a generous funding available for conferences and research visits.
Applicants should have an MSc degree in astronomy or a closely related field and a good English speaking and writing skills. Previous experience with programming will be an advantage.
Application deadline is set for 1st of March 2022 and the project can start as early as 1st April 2022, but a later date can be negotiated. Applicants should submit their CV, a statement of the candidate's research interests, experience, and skills directly to mkoprowski @ umk.pl and arrange for two reference letters to be sent to the same address.
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| Three postdoctoral positions in asteroseismology of intermediate- and high-mass stars: clusters, binaries, and yields | Closing date: 2022-02-28
Contact: Conny Aerts |
| The Institute of Astronomy of KU Leuven in Belgium is looking for three junior post-doctoral researchers to join its asteroseismology research group for a period of 3 to 5 years each. All three projects involve Kepler/TESS photometry, Gaia astrometry, and asteroseismic modelling of intermediate- and high-mass stars. The three positions concern 1) gravity-mode asteroseismology of open clusters; 2) dynamical asteroseismology of eclipsing binaries and tidal evolution; 3) yield computations calibrated by asteroseismology and the chemical enrichment of galaxies. | | ▸ more | The Institute of Astronomy (IoA) of KU Leuven is a young and vibrant research group of some 90 scientists, engineers, and administrative staff, including 6 full-time and 3 part-time professors. The institute is an expertise centre in stellar and exoplanetary astrophysics and astronomical
instrumentation, and is active in several international consortia and collaborations, involving
telescopes at observatories worldwide and in space. Members of IoA have access to parallel
computing facilities at the Flemish Supercomputer Centre. The IoA is responsible for the organisation
of the Master of Astronomy & Astrophysics and the Advanced Master of Space Studies of the Faculty
of Science, and operates the 1.2m Mercator telescope at Roque de los Muchachos, La Palma
Observatory, Canary Islands. The institute has a long tradition in instrumental, observational,
computational and theoretical studies of stellar structure and evolution, with emphasis on stellar variability.
The successful applicants will be embedded in a team of asteroseismologists led by Conny Aerts,
Joris De Ridder, and Andrew Tkachenko. They will be working jointly on mapping the internal rota(on
and mixing profiles of stars as a function of their global stellar properties such as mass, age,
metallicity, initial angular momentum, and multiplicity. The selected postdocs are expected to take
up responsibilities in the supervision of BSc, MSc, and PhD students. They will receive ample training
in the writing of personal competitive project applications as an important aspect of their future career development.
The projects rely heavily on data from the Kepler/TESS and Gaia space missions, as well as from
ground-based spectroscopic surveys characterising stellar surface properties. The assembled time
series contain a tremendous amount of information, yet to be exploited jointly. As an overarching
aim, the three postdocs will work together with a group of PhD students to extract optimal
observables from data of non-radial pulsators assembled by the surveys and exploit them to improve
the theory of stellar structure and evolution.
The three projects cover a multitude of concrete aims and tasks to be done, requiring various skills.
Candidates wishing to apply for more than one posi(on are requested to express their order of
preference.
1) Gravity-mode asteroseismology of open clusters
The applicant will develop customized methods to extract optimal lightcurves from TESS full-frame
images of open clusters, by maximally eliminating instrumental effects in the Fourier domain and by
treating crowded fields. Thorough time series analysis will be carried out for all cluster stars to
identify and extract signatures of gravity-mode oscillations, rotational modulation and possible
binarity. The applicant will perform mode identification and model the identified modes of all
pulsators and all binaries per clusters jointly with their Gaia data, featuring the strongest set of
constraints on each member?s properties. The pioneering goal is to evaluate current stellar evolution
theory and to reveal empirical relations deduced from all observed properties of the cluster stars as
new recipes for stellar evolution predictions.
2) Dynamical asteroseismology of eclipsing binaries and tidal evolution
The applicant will extract optimally defined observables from the survey data to perform joint
modelling of photometric, spectroscopic, and astrometric time series of eclipsing binaries, with the
aim to deduce accurate dynamical masses and radii. The latter quantities will be used to deduce the
ages of the binaries for two large samples of intermediate- and high-mass stars, from stellar
modelling based on the latest evolutionary models of stellar interiors and atmospheres. This will lead
to an assessment of the so-called mass discrepancy of binary stars, pulsating and non-pulsating, in
terms of their metallicities, evolutionary stages, and orbital characteristics. From the multitude of
observational constraints, the theory of binary evolution will be re-evaluated and improved
with the aim to assess the effects of tides on internal rotation and mixing of stars, and of angular
momentum of the systems.
3) Yield computations calibrated by asteroseismology and the chemical enrichment of galaxies
The applicant will calibrate internal mixing profiles due to convection, rotation, magnetism, and
possible binarity from gravity-mode pulsators in the mass range [3,25] solar masses. This will be achieved
from asteroseismic modelling based on TESS, Gaia, and spectroscopy data. The asteroseismically
calibrated mixing profiles and the resulting He and C core masses during the main sequence (MS)
and post-MS evolution will be used to calculate new stellar models up to the remnant phase. The
corresponding chemical yield predictions will be computed with tools from the ChETEC INFRA
(https://chetec-infra.eu/) EU infrastructure (2021- 2026). These chemical yields will then be used to
assess the difference between asteroseismically calibrated yields and those for current models not
calibrated by asteroseismology. The final aim is to evaluate how much these differences impact
chemical evolution models of the galaxy and Magellanic Clouds.
Requirements, offer, and online application tool via:
https://www.kuleuven.be/personeel/jobsite/jobs/60088185?hl=en&lang=en
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| Two Postdoctoral Fellowship Positions in the Centre for Astrophysics Research at the University of Hertfordshire | Closing date: 2022-02-20
Contact: Prof. Kristen Coppin |
| We are seeking to appoint two promising early-career researchers to lead original investigations in any area of theoretical or observational astrophysics that will complement active areas of research in the Centre for Astrophysics Research (CAR) at the University of Hertfordshire. | | ▸ more | Details of CAR staff research interests/activities and facilities may be found here: https://www.herts.ac.uk/research/centres/car. CAR also has strong links and overlapping interests with the Centre of Data Innovation Research (CoDIR; https://www.herts.ac.uk/research/centres/codir), a relatively new research centre that combines data science and machine learning expertise from astrophysics and computer science and addresses cross-disciplinary research questions.
The postholder will have a good track record of scientific research in their area of expertise, including leading projects and submitting/publishing their work in refereed astronomical journals. Whilst this is an independent fellowship, there is an expectation that the successful candidate(s) will start new or strengthen existing collaborations with members of CAR, including leading/collaborating on external grant bids, helping out with some light departmental teaching, and should be prepared to contribute more generally to the general research environment.
Candidates should have (or submitted for) a PhD in astronomy/astrophysics before taking up the posts, which are available from August 1, 2022 and should be taken up (ideally) no later than October 1, 2022. The starting salary is expected to be Ł34,304 per annum, incrementing annually, with a higher salary possible based on previous postdoctoral experience. The fellowship duration is for 3 years on a full-time basis (1 FTE), but the possibility of fractional / part-time working will also be considered.
For further details please see our recruitment website (https://www.herts.ac.uk/staff/careers-at-herts; JobID 039075), where you will also need to submit your application by February 20 2022 including a CV, list of publications, a research proposal for the duration of the fellowship (making sure to indicate how your proposed research is complementary to CAR, and not exceeding two sides of A4 paper), and the contact details of two referees willing to write on your behalf.
Informal enquiries can be directed to Prof Kristen Coppin (Director of CAR, k.coppin @ herts.ac.uk)
Included Benefits:
The Centre for Astrophysics Research group is is a thriving research group of ~60 academic staff, research fellows and postgraduate students and is part of the Department of Physics, Astronomy and Mathematics. The department takes pride in the diversity of its staff, and holds both an IoP Juno Champion and an Athena-Swan Silver award. We encourage applications from all individuals meeting our essential criteria, irrespective of gender or membership of underrepresented groups.
The UH vision is to transform lives and UH is committed to Equality, Diversity and Inclusion and building a diverse community. UH offers a range of employee benefits including generous annual leave and discounted Sports Village memberships, personal and professional development and family-friendly policies. #GoHerts
A standard package of benefits will be provided for successful candidates, including funding for travel and equipment expenses.
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| JUNIOR GROUP LEADER (F*M) in Space Instrumentation | Closing date: 2022-03-31
Contact: Cosima Muck |
| The Space Research Institute (IWF) is with about 100 employees from twenty nations one of the largest institutes of the Austrian Academy of Sciences (OeAW). The institute is located in the Victor Franz Hess Research Center of OeAW in the south of Graz. The IWF also operates a world-leading satellite laser ranging station at the Lustbühel Observatory. | | ▸ more | Job ID: IWF184JGL121
The Space Research Institute (IWF) is with about 100 employees from twenty nations one of the largest institutes of the Austrian Academy of Sciences (OeAW). The institute is located in the Victor Franz Hess Research Center of OeAW in the south of Graz. The IWF also operates a world-leading satellite laser ranging station at the Lustbühel Observatory. The Space Research Institute invites applications for a position as
JUNIOR GROUP LEADER (F*M)
in Space Instrumentation
(full-time, 40h per week)
We invite ambitious candidates who are interested in technology development for new and existing fields of scientific instruments at the IWF. We strive for a tight collaboration between instrumentation and space science as we understand instrumentation as science enabler.
Your profile:
- PhD in engineering or physics/astrophysics
- Experiences in development of space-qualified instrumentation and related engineering disciplines: electrical, electronics, mechanical, software, quality assurance as well as other engineering fields which fit to the scientific activities of the institute
- Proven track record in development of at least one spaceborne instrument or in leading subunit development or in being responsible for one of the mentioned engineering fields
- Proven track-record in project and in people management
Your tasks:
- Leading an existing research group with focus on instrument development and development support in direct link with the IWF?s research activities
- Management (jointly with senior engineers of the research group) of already existing projects (Router and Data Compression Unit for PLATO and IWF?s contribution for SXI aboard SMILE to be finalised; Digital Processing Unit for MANiaC aboard Comet Interceptor and IWF?s contribution for the Wide Field Imager aboard ATHENA under preparation)
- Initiation of new developments in accordance with the scientific core activities of IWF
- Technical and financial proposal writing and reporting
- Coordination of all activities to fulfil technical and schedule requirements
- Supervision of group members, incl. PhD students and PostDocs
- Publication activities
The appointment begins as early as September 01, 2022 for initially 4 years with the option for tenure track. More senior applicants can be offered the position of a group leader for an initial duration of 6 years with a tenure-track option. We offer an annual gross salary of ? 54.661,32 for a junior group leader according to the collective agreement of the Austrian Academy of Sciences. Group leaders expect a higher enumeration.
Applications must include a cover letter, their curriculum vitae, list of publications, a statement of the applicant's research experience (2 pages) and a research plan (1 page), certificates for full academic record, and the full contact information for two references letters. Please send the application as one PDF file, to cosima.muck @ oeaw.ac.at, mentioning Job ID: IWF184JGL121, no later than 31 March 2022. Inquiries about the position should be directed to Cosima Muck.
The Austrian Academy of Sciences (OeAW) pursues a non-discriminatory employment policy and values equal opportunities, as well as diversity. Individuals from underrepresented groups are particularly encouraged to apply.
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| Ten CATA Postdoctoral Fellowships in observational, theoretical, and computational astrophysics | Closing date: 2022-02-25
Contact: Prof. Ezequiel Treister |
| The Center for Astrophysics and Applied Technologies (CATA) calls for applications to the CATA postdoctoral research fellowship program, covering the areas of observational, theoretical, and computational astrophysics. CATA is a large government-funded astronomical Center that ? incorporating 12 member universities across 6 provinces, 40+ professors, 50+ postdoctoral researchers, and 70+ graduate students ? provides a vibrant, dynamic, and productive international astronomical research environment. We welcome applications across all scientific areas. | | ▸ more | The postdoctoral research fellowships are anticipated to be funded initially for two years with a one-year extension subject to a performance evaluation. Successful fellowship applicants are expected to carry out independent research in close collaboration with one or more faculty members of CATA, and develop research at any of the CATA member universities, including Universidad de Chile, Pontificia Universidad Católica de Chile, Universidad de Concepción, Universidad Andrés Bello, and Universidad Diego Portales, amongst others. Successful fellows will have privileged access to the Chilean 10% time allocation on all telescopes in Chile, as well as Chilean access to membership in selected large surveys (e.g., LSST, SDSSV). CATA fellows will have access to supercomputers and GPU clusters, as required by their projects. In addition, CATA fellows will have access to CATA-provided administrative support, as well as the opportunity to explore the varied and striking natural landscapes of Chile, from high deserts to lush rainforests.
CATA scientific areas include:
Area 1 - Cosmology and Galaxy Formation: Goals in this area include cosmological simulations of galaxy formation and large-scale structure properties, as well as the study of the CMB observables.
Area 2 - Supermassive Black Holes and Energetic phenomena: Concentrates on observational studies of supermassive black hole growth using current and planned facilities (Vera Rubin, E-ELT, GMT, EHT, VLT-MOONS, 4MOST), as well as energetic phenomena using the Cherenkov Telescope Array (CTA) and the Southern Wide-field Gamma-ray Observatory (SWGO).
Area 3 - Galaxies: The research focus is the formation and evolution of galaxies and AGN, including the effects of the environment, across cosmic time throughout the electromagnetic spectrum, with significant involvement in current and upcoming surveys like the Rubin Observatory LSST, S-PLUS, SDSS-V, LAGER, PHANGS-JWST, and the ALMA Large Programme CRISTAL.
Area 4 - Local Universe: Research will focus on areas of fundamental stellar astrophysics, Galactic stellar populations, Milky Way and Local Group structure and evolution, and galaxy formation and evolution in the nearby Universe (at the group/cluster level).
Area 5 - Star and Planet formation: Current hiring priorities include: early science exploitation of the SDSS-V Local Volume Mapper (LVM) program; exploitation of ALMA data of forming clusters and specifically the kinematics (via e.g. the ALMA-IMF Large Program); observational programs (e.g., ALMA, VLT, Magellan) focused on the chemistry and evolution of planet-forming disks and young planets.
Area 6 - Exoplanets & Astrobiology: Aims to observationally and theoretically tackle current questions related to the formation and evolution of the solar system and exoplanets, with the goal of exploring the origins of rocky planets and the possible extension of life beyond Earth.
Area 7 - Theoretical Astrophysics: Focuses on simulations in the context of star formation, astrochemistry, and magnetic fields; supermassive black hole and star cluster formation; stellar dynamos, stellar and black hole mergers as well as machine learning techniques.
Applicants should declare (see below for requested materials) which science area(s) they envision working in. Research programs that exploit multi-area synergy are encouraged. We also encourage applicants to make early contact with CATA professors working on their area(s) of interest.
Applicants should submit here the following materials as a single pdf file: a brief cover letter; a CV including exact or expected Ph.D. date; a publication list; a research statement (max. 3 pages) describing past and future proposed CATA research; an optional 1-page technical skills statement; and the names of three contacts for letters of recommendation.
CATA is committed to equal opportunity and diversity in the workforce. Women and minorities are strongly encouraged to apply.
Included Benefits:
Generous research budget, and administrative support (e.g. for visa processing and relocation), and support for health insurance.
Related URLs:
Application form
Description of CATA Scientific Areas
Announcement and Position Description
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| Astronomy Data Science Engineer | Closing date: 2022-01-26
Contact: Mark Allen |
The selected candidate will work within the Strasbourg astronomical Data Centre (CDS) to provide data science expertise for the operation of the EOSC Future Project.
| | ▸ more | The selected candidate will work within the Strasbourg astronomical Data Centre (CDS) to provide data science expertise for the operation of the EOSC Future Project.
Activities:
The selected candidate will provide expertise for the use of data access techniques and visualisation tools for the EOSC Future Science Projects in the area of multi-messenger astrophysics. This will involve the application of techniques for the indexation of astronomical data using the standards and tools that have been developed in the astronomical Virtual Observatory framework, in particular the Hierarchical Progressive Survey (HiPS) and Multi-Order Coverage map (MOC) systems. The activities also include the development and presentation of training materials for the use of astronomy data interoperability systems in the European Open Science Cloud (EOSC). This work will involve interaction with the technical and scientific staff of the CDS as well as with the ESCAPE and EOSC Future partners.
Skills:
The role would suit candidates with a research background with strong skills in data science techniques.
- Expertise in astronomical data analysis or data science.
- Expertise with astronomical data (observational or simulation).
- Experience with Python language tools and notebooks.
- Experience with Virtual Observatory tools.
- Experience with astronomical visualisation would be beneficial.
- Good communication skills and ability to present work to technical and scientific audiences.
- Interest in contributing to the development of data sharing techniques and practices for Open Science.
- English, spoken and written at level of C1.
- Doctorate in astrophysics or a degree from an engineering school (or equivalent experience).
Work Context:
The Strasbourg Astronomical Data Centre (CDS) is dedicated to the collection and dissemination of astronomical data and information, as well as to the development of innovative techniques for the scientific exploitation of very large data sets. The CDS provides the SIMBAD reference database, the VizieR service for astronomical catalogues and tables published in scientific astronomical journals, the Aladin interactive sky atlas and the CDS portal. The CDS also contributes to the development of the Astronomical Virtual Observatory. (For more information, see http://cds.unistra.fr)
The CDS is participating in the ESCAPE and EOSC Future projects funded by the European Commission. ESCAPE is the "European Science Cluster of Astronomy & Particle physics ESFRI research infrastructures?. ESCAPE addresses the open science challenges shared by ESFRI infrastructures in the fields of astronomy and particle physics (CTA, ELT, EST, FAIR, HL-LHC, KM3NeT, SKA) as well as other pan-European research infrastructures (CERN, ESO, JIVE, EGO-Virgo). (for more information, see - https://www.projectescape.eu)
EOSC Future is a European funded project to integrate, consolidate, and connect e-infrastructures, research communities, and initiatives in Open Science. EOSC Future project includes the support of science projects that will serve as show cases of the use of open science tools and services. The CDS goals in the project are to support the use of Virtual Observatory services in EOSC to serve the scientific needs of the ESCAPE communities, and to develop training materials for scientific use of the systems.
Renumeration and starting date:
Remuneration : 2487 to 3157 euros gross per month depending on experience
The position is for an initial 12 month contract as a Research Engineer. The position is available immediately, and the starting date should be before April 2022.
To apply - provide a CV and Letter of motivation through the CNRS Employment Portal (note that the advertisement is available in both French and English.
https://bit.ly/3m5S6Gk
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| 6-year Research Position in Dynamics of Planetary Systems | Closing date: 2022-02-15
Contact: Alexandre Correia |
| The Physics Department of the University of Coimbra, Portugal, invites applications for a research position in Dynamics of Planetary Systems under the CEEC FCT 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 applicants are expected to do research in one of the following topics: solar system dynamics, TNOs, planet formation and evolution, dynamics of multi-planetary systems. Computational experience is required and a background in celestial mechanics is a plus. 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: 15th February 2022
Expecting starting date: October 2022, to be agreed upon with the successful candidate.
Host institution: CFisUC, Department of Physics, University of Coimbra, PORTUGAL (EU).
Type of contract: 6 year Contract:
Salary: from 30.000 to 60.000 EUR / year (depending on experience).
Benefits include social security and 23 vacation days.
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APPLICATION PROCEDURE:
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Job Reference: CEEC-FCT
Language: English
Candidates should contact Prof. Alexandre Correia (acor @ uc.pt) before February 15th 2022, 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(s) will get the support from the University of Coimbra to apply to the CEEC program.
Contacts and further information:
Alexandre Correia:
http://faculty.uc.pt/uc44419
University of Coimbra:
https://www.uc.pt/fctuc/fisica/en/
FCT Program:
https://www.fct.pt/apoios/contratacaodoutorados/empregocientifico/ceec_ind_5.phtml.en
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| Post-doctoral position at Ecole Normale Supérieure on the energy budget of galaxies | Closing date: 2022-01-31
Contact: Edith Falgarone |
Applications are invited for a post-doctoral position funded by a European Research Council (ERC) project that focusses on several facets of the dissipative physics of baryonic matter in the local and high-redshift universe.
The proposed research project addresses the energy budget of a sample of galaxies and their environment, using existing data and the models of molecular emission of turbulent dissipation regions developed by the team in the perspective of forthcoming data collected by the JWST.
| | ▸ more | Scientific context and environment:
Applications are invited for a postdoctoral position in Paris in the field of star and galaxy formation. The fellowship is funded by the European Research Council (ERC). The MIST (Molecules, Magnetic fields and Intermittency in Cosmic Turbulence) project focusses on several facets of the dissipative physics of baryonic matter in the local and high-redshift universe.
The MIST project fosters strong interactions between three main research axes: (1) observations of the chemical and thermal markers of turbulent dissipation in the high-redshift and local universe, (2) statistical analyses of the magnetic and velocity fields in samples of unprecedented size and sensitivity to study the non-Gaussian signatures of turbulent dissipation, and (3) numerical experiments dedicated to the space-time structures of turbulent dissipation and the formation of molecules in their wake.
The post-doctoral research project addresses the energy budget of a sample of galaxies and their environment, using the models of molecular emission of turbulent dissipation regions developed by the team in the perspective of forthcoming data collected by the JWST.
The MIST team is part of the astrophysics group at the Physics Department of Ecole Normale Supérieure and has close ties with astrophysicists in the Paris area. The successful candidate will benefit from this broad and stimulating research environment.
Perspectives:
The interpretation of ancillary data will be followed by the analysis of data
collected by the JWST. The JWST will allow to observe the infrared ro-vibrational lines of H2 with a sensitivity and a spatial resolution 100 to 1000 times greater than Spitzer and VLT/SINFONI/KMOS, and will therefore open the possibility to spatially and spectrally resolve H2 line emission in the population of galaxies explored in this project.
Desired profile of the candidates:
Candidates should have a good background in physics and astrophysics along with computational skills in python and/or fortran. An observational or theoretical expertise of extragalactic environments would be an invaluable asset to the project.
Application procedure:
The appointment is for 2 years with a possible extension to 3 years. The offer includes French social security benefits and funding for travel.
Applicants should submit a CV (max. 2 pages), a letter of intent, a publication list, and two letters of recommendation.
Applications should be sent via email to benjamin.godard @ obspm.fr and to
edith.falgarone @ ens.fr
Applications will be accepted until the position is filled. The contract will have to start before 1 September 2022.
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| Post-doctoral position at Ecole Normale Supérieure on dissipation of cosmic turbulence | Closing date: 2022-01-31
Contact: Edith Falgarone |
Applications are invited for a post-doctoral position funded by a European Research Council (ERC) project that focusses on several facets of the dissipative physics of baryonic matter in the local and high-redshift universe.
The proposed research includes numerical simulations of magneto-hydrodynamical turbulence dedicated to dissipation scales, with openings towards the formation of molecules in the wake of dissipative structures.
| | ▸ more | Scientific context and environment:
Applications are invited for a postdoctoral position in Paris in the field of star and galaxy formation. The fellowship is funded by the European Research Council (ERC). The ERC MIST (Molecules, Magnetic fields and Intermittency in Cosmic Turbulence) project focusses on several facets of the dissipative physics of baryonic matter in the local and high-redshift universe.
The MIST project fosters strong interactions between three main research axes: (1) observations of the chemical and thermal markers of turbulent dissipation in the high-redshift and local universe, (2) statistical analyses of the magnetic and velocity fields in samples of unprecedented size and sensitivity to study the non-Gaussian signatures of turbulent dissipation, and (3) numerical experiments dedicated to the space-time structures of turbulent dissipation and the formation of molecules in their wake.
The post-doctoral research project builds up on our recent achievements and includes numerical simulations of magneto-hydrodynamical turbulence dedicated to dissipation scales, with openings towards the formation of molecules in the wake of dissipative structures (shocks and current sheets).
The team of the MIST project is part of the astrophysics group at the Physics Department of Ecole Normale Supérieure and has close ties with astrophysicists in the Paris area. The successful candidate will benefit from this broad and stimulating research environment.
Perspectives:
Beyond the interpretation of molecular line and magnetic fields observations, the study of coherent structures in turbulent media is a promising alley. It could lead to a significant step forward in understanding key issues in the way turbulence dissipates and transports. We expect our results will impact a range of modern questions in plasma physics from solar physics to the various phases of the interstellar medium.
Desired profile of the candidates:
We are looking for a numerically oriented physicist, well acquainted with fluid mechanics. Programming fluency in python and/or Fortran is wished. Prior experience in high performance simulation is not requested but will be an asset. The successful candidate will have access to the local cluster of the ERC, which is well suited for the needs of the project.
Application procedure:
The appointment is for 2 years with a possible extension to 3 years. The offer includes French social security benefits and funding for travel.
Applicants should submit a CV (max. 2 pages), a letter of intent, a publication list, and two letters of recommendation.
Applications should be sent via email to pierre.lesaffre @ ens.fr and to
edith.falgarone @ ens.fr
Applications will be accepted until the position is filled. The contract will have to start before 1 September 2022.
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| Post-doctoral position on space astrometry (to process resolved binaries within Gaia DPAC) | Closing date: 2022-01-31
Contact: Alain Jorissen |
| The Gaia Data Processing and Analysis Consortium (DPAC) is the consortium responsible for processing the data that arrives from ESA's Gaia satellite. A major problem to be solved for Gaia Data Release 4 relates to stellar images not correctly matched by a single point-spread function (PSF). These situations cause problems in the further astrometric and binary-star processing, handled by the so-called Coordination Units "Core Processing" (CU3) and "Object Processing" (CU4). The objective of the project is to solve this problem by adding the necessary processing to the existing architecture. | | ▸ more | Although based in Brussels (Université libre de Bruxelles), the successful candidate will
work in close collaboration with colleagues from CU3 and CU4, located at ESAC (Madrid), Observatoire de Paris and CNES (Toulouse).
The Brussels Gaia DPAC team consists of three researchers (A. Jorissen, C. Siopis, G. Sadowski) working in the framework of Gaia CU4-NSS ("Non-single stars") who will provide regular guidance as well.
Applicant's Profile:
- The candidate must have a PhD in physics, preferentially astrophysics.
- The candidate must have a strong interest in "big data" processing (knowledge of Java is an asset).
- Some knowledge about image processing, astrometry and the Gaia DPAC environment will be a strong asset.
- Working in such an international team requires capacity of teamwork and a very good level of English language.
Interested candidates should send their CV with a motivation letter and request two referees to send their recommendation letter directly to A. Jorissen (Alain.Jorissen at ulb.be)
The contract is for one year, with possible extension depending on funding.
It is funded by Belspo - PRODEX (Belgian Science Policy Office).
Applications are open until January 31, 2022. The position should start as soon as possible.
Université Libre de Bruxelles is a complete university maintaining 40 bachelor and
150 master programs, for 30 000 students of 140 nationalities, and hiring 9000 employees.
More information on the Institut d'Astronomie et d'Astrophysique, belonging to the Physics Department of the Science Faculty, can be found at http://www.astro.ulb.ac.be
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| Accretion variability of young stellar objects | Closing date: 2022-01-31
Contact: Beate Stelzer |
| The Institute for Astronomy & Astrophysics of the University of Tübingen (Germany) has an opening for a PhD position in stellar astrophysics / star formation on the topic of accretion variability of young stellar objects. | | ▸ more | The project is based on optical spectroscopy and photometry of pre-main sequence stars. The aim is to determine stellar and accretion properties of YSOs from time-series data and constrain their variability on days, months, years and secular time-scales. The PhD position is part of YTTHACA (Young Stellar Objects at Tübingen, Tautenburg, Hamburg & ESO - A Coordinated Analysis), a national german collaboration that is embedded in the framework of the international ULLYSES and PENELLOPE projects (see here https://sites.bu.edu/odysseus/ for details). Locally the project is part of the research group Space Based Astrophysics of Eberhard Karls Universität Tübingen led by JProf. B. Stelzer which has its focus on multi-wavelength observations of the formation and evolution of low-mass stars and brown dwarfs.
The applicant must have a master or equivalent degree in physics or astrophysics. Expertise with photometric and/or spectroscopic data analysis, and a background in star formation studies are useful.
The position will be funded for a duration of 3 years (36 months). Salary will be according to 75% E13 of the TV-L of the German public services. The application is expected to consist of a CV (including personal data, formation, skills and expertises), copies of university degrees and a brief (1-2 page) statement of previous research experiences and motivation. The candidate should arrange for two letters of recommendation to be sent directly to Prof. B. Stelzer. The deadline for applications is Jan 31, 2022 with a starting date as soon as possible.
Eberhard Karls Universität Tübingen is committed to increasing the percentage of women in research.
In case of equal qualification preference will be given to applicants with disabilities.
Employment takes place via the Central Administration of the University.
Contact for application and further information:
Beate Stelzer (stelzer @ astro.uni-tuebingen.de)
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| PhD positions in Astrophysics and Astroinformatics | Closing date: 2022-01-15
Contact: Médéric Boquien |
| At the Center of Astronomy of Universidad de Antofagasta (CITEVA) we are seeking enthusiastic students with a passion for understanding the wonders of the Universe to join our new PhD program in Astrophysics and Astroinformatics. | | ▸ more | Antofagasta, where CITEVA is based, is a large and rapidly expanding coastal city in northern Chile on the edge of the spectacular Atacama desert. In this scenic setting, our doctoral students will join our eight Professors who are involved in cutting-edge investigations on a broad range of topics including stellar systems, galaxies from the Milky Way to the farthest reaches of the universe, and the booming field of Astroinformatics. They will have the much sought-after access to the 10% time on current and future international observatories built in Chile (ESO, Las Campanas, CTIO, Gemini, ALMA, E-ELT, GMT, CTA, etc.) along with SDSS-V and LSST, as well as access to local and national computing facilities.
Applicants must have an undergraduate or Master?s degree in Astronomy or a related field. The application form and additional information regarding the program are available on our website. All materials must be submitted to astro.doctorado @ uantof.cl by January 15.
Further information can be obtained from the director of the program, Prof. Médéric Boquien.
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| Research Position in data intense radio astronomy | Closing date: 2022-01-10
Contact: Dominik Schwarz |
Big Bang to Big Data (B3D) is an interdisciplinary cluster in Nordrhein-Westfalen (Germany) for research,
technology and education in the field of data-intense radio astronomy. It brings together radio astronomy
and astrophysics with data science and data technology. We are a group of eight universities and research
institutes in NRW. We are involved in the development, operation and exploitation of leading radio
observatories (incl. ALMA, APEX, Effelsberg, FYST/CCAT-prime, LOFAR, MeerKAT, SKA, SOFIA) and the
handling and analysis of their radio data, or bring in data science and data technology expertise. W | | ▸ more | At Bielefeld University we are engaged in the fields of radio cosmology and pulsar astronomy, as well as the
data storage and management aspects of larges radio astronomy infrastructures like LOFAR, MeerKAT and
the SKA. In the context of B3D we will lead the work package on graduate education.
Your Tasks / research tasks (100 %):
- curriculum development for an integrated astronomy and data science graduate education
- development of new research questions by identifying synergies between LOFAR, MeerKAT and other radio astronomy instruments
- support of fund raising, especially application for a DFG reserach training group
- independent research
Your Profile
We expect:
- completed scientific degree
- completed doctorate in a field closely related to data-intensive radio astronomy, e. g. physics, astronomy, computer science, data science, etc.
- relevant research experience as evidenced by publications and conference presentations
- very good communication skills
- fluency in spoken and written English
Preferred experience and skills:
- experience in project management
- radio astronomical and astrophysical research experience
- knowledge in the field of IT
- knowledge or research experience in the field of data science
- experience in the acquisition of third-party funds
- proficiency in the German language, both spoken and written
We offer:
- salary according to Remuneration level 13 TV-L fixed-term (3 years) (§ 2 (1) sentence 2 of the WissZeitVG; in accordance with the provisions of the WissZeitVG and the Agreement on
Satisfactory Conditions of Employment, the length of contract may differ in individual cases)
- fulltime
- internal and external training opportunities
- wide range of health, consulting and prevention service
- reconcilability of family and working life
- flexible working hours
- job ticket for regional public transport network
- collegial working environment
- open and pleasant working atmosphere
- exciting, varied tasks
Application Procedure:
We are looking forward to receiving your application by January 10, 2022. Please include in your application names and contact of at least three persons that are willing to provide letters of reference for you. They will be contacted by us when required. For full consideration, your application should be received via email (a single PDF document is required) sent to reder @ physik.uni-bielefeld.de.
Please mark your application with the identification code:
Wiss22049.
The details can also be found on the University website:
https://uni-bielefeld.hr4you.org/job/view/1029/research-position-in-data-intense-radio-astronomy?page_lang=en
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| PhD position on distant star-forming galaxies | Closing date: 2022-03-01
Contact: Daniel Schaerer |
The research group on "Galaxies and the Universe" of the Geneva Observatory expects to recruit new PhD students to start in fall 2022.
| | ▸ more | The successful candidates will work on projects studying star-forming galaxies in the nearby and distant Universe, involving multi-wavelength observations and/or state-of-the-art modeling. The projects include in particular cycle 1 spectroscopic observations from the James Webb Space Telescope (the LyC22 survey with NIRSpec/JWST), and other studies of emission line galaxies, Lyman continuum emitters and related objects. A related project will focus on new, ambitious spectral models for star-forming galaxies. The candidates will work with the group of Prof. Daniel Schaerer in Geneva and within international collaborations.
The Geneva Observatory and the associated Laboratory of Astrophysics of the Swiss Federal Institute of Technology in Lausanne (EPFL) carry out observational, interpretative and theoretical research in the fields of extra-solar planets, stellar physics, high energy astrophysics, galaxy evolution, and observational cosmology.
The post-doc appointment will be for one to three years, renewable.
PhD appointments are for four years. Starting dates are in sept-oct 2022, negotiable.
Qualified candidates are encouraged to send the following material in a single pdf file
via email:
- post-docs (subject "post-doc Geneva-2022"): CV and publication list, description of
research experience and interests, and contact information of three references
- PhD students (subject "PhD Geneva-2022"): CV, motivation letter, list of MSc courses
and grades, and contact information of two or three references
Applications received by 1 march, 2022 will receive consideration.
Informal enquiries with Daniel Schaerer (daniel.schaerer @ unige.ch) are welcome.
For information on the research group visit https://www.unige.ch/sciences/astro/starbursts/en/
Included Benefits:
Standard Swiss Social Security, Accident Insurance and Pension contributions.
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| Postdoctoral research position on distant star-forming galaxies | Closing date: 2022-03-01
Contact: Daniel Schaerer |
| The research group on "Galaxies and the Universe" of the Geneva Observatory expects to recruit new PhD students and post-docs to start in fall 2022. | | ▸ more | The successful candidates will work on projects studying star-forming galaxies in the nearby and distant Universe, involving multi-wavelength observations and/or state-of-the-art modeling. The projects include in particular cycle 1 spectroscopic observations from the James Webb Space Telescope (the LyC22 survey with NIRSpec/JWST), and other studies of emission line galaxies, Lyman continuum emitters and related objects. A related project will focus on new, ambitious spectral models for star-forming galaxies. The candidates will work with the group of Prof. Daniel Schaerer in Geneva and within international collaborations.
The Geneva Observatory and the associated Laboratory of Astrophysics of the Swiss Federal Institute of Technology in Lausanne (EPFL) carry out observational, interpretative and theoretical research in the fields of extra-solar planets, stellar physics, high energy astrophysics, galaxy evolution, and observational cosmology.
The post-doc appointment will be for one to three years, renewable.
PhD appointments are for four years. Starting dates are in sept-oct 2022, negotiable.
Qualified candidates are encouraged to send the following material in a *single* pdf file
via email:
- post-docs (subject "post-doc Geneva-2022"): CV and publication list, description of
research experience and interests, and contact information of three references
- PhD students (subject "PhD Geneva-2022"): CV, motivation letter, list of MSc courses
and grades, and contact information of two or three references
Applications received by 1 march, 2022 will receive consideration.
Informal enquiries with Daniel Schaerer (daniel.schaerer @ unige.ch) are welcome.
For information on the research group visit https://www.unige.ch/sciences/astro/starbursts/en/
Included Benefits:
Standard Swiss Social Security, Accident Insurance and Pension contributions.
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| Detection and characterization of planetary systems | Closing date: 2022-01-10
Contact: Pedro J. Amado |
The Instituto de Astrofísica de Andalucía (CSIC) in Granada, Spain, offers a postdoctoral position to work in exoplanets and stellar physics. Candidates are expected to carry out their activity in the research line of "Towards the understanding of the planetary systems" in the frame of the CARMENES collaboration.
| | ▸ more | This collaboration aims at detecting terrestrial temperate exoplanets around small red stars with the radial velocity technique to characterize the planetary system as a whole, including its star and circumstellar environment, as we are already doing with Proxima Cen and other benchmark systems. We also aim at understanding and characterizing the exoplanet atmospheres. Besides, our group contributes with our expertise in asteroseismology and stellar models.
The candidate will also have the opportunity to engage in the Phase B activities of HIRES/ELT and the preparation of the PLATO mission.
Tasks:
* Scientific exploitation of the CARMENES spectrograph (Calar Alto Observatory, Spain), with data obtained through guaranteed time observations, and of its extensions (CARMENES Legacy-Plus) or through open time.
* Exoplanet characterization through the analysis e interpretation of high-resolution spectra and the determination of high-precision radial velocities and orbital parameters.
* Depending on the complementary candidate expertise, the candidate will carry out any additional studies of dynamical stability of the planetary system, the circumstellar environment, planet formation, system evolution, influence and correction of the stellar activity on the planetary parameters or atmospheric characterization through the study of wavelength-dependent radial velocity curve amplitudes at transit time, to name a few possibilities.
Requirements:
* Degree in physics and PhD in astrophysics.
* Postdoc with a good scientific record of publications on planet detection and/or characterization.
* Knowledgeable in scientific programming and fluent in spoken and written English.
* Applications should be sent to Pedro J. Amado (pja @ iaa.csic.es) and include a cover letter, a curriculum vitae, a research statement, and a full list of publications. Candidates should arrange for at least two letters of recommendation to be emailed to the same address by the deadline.
Duration: The appointment will be for 2 years with possibilities for extensions. We estimate that the date of commencement will be during the first quarter of 2022.
Salary: 38 300 Euros/yr (taxes included)
Deadline: January 10, 2022, UT 23:59
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| Assistant Researchers in the Planetary and Space Sciences related to Astrobiology at the University of Hawai'i | Closing date: 2022-03-15
Contact: Eric Gaidos |
| The School of Ocean and Earth Sciences and Technology and the Institute for Astronomy at the University of Hawaii at Manoa have embarked on a NASA- and NSF-supported mission to understand the factors that govern the behavior of the light elements critical to habitability and life during planet formation, and the potential diversity of outcomes -- including Earth-like worlds -- around other stars. We are recruiting outstanding postdoctoral researchers to join our team of astronomers, cosmochemists, planetary scientists, and geophysicists in this pursuit. | | ▸ more | The School of Ocean and Earth Sciences and Technology and the Institute for Astronomy at the University of Hawaii at Manoa have embarked on a NASA- and NSF-supported mission to understand the factors that govern the behavior of the light elements critical to habitability and life during planet formation, and the potential diversity of outcomes -- including Earth-like worlds -- around other stars. We are recruiting outstanding postdoctoral researchers to join our team of astronomers, cosmochemists, planetary scientists, and geophysicists in this pursuit. We are especially interested in talking to prospective candidates in these areas:
* High-pressure mineral physics: experimental approaches to understand the behavior of light elements in the interiors of rocky planets during their accretion and early evolution, control by conditions at formation, and the effect on planetary outcomes.
* Cosmochemistry and meteoritics: investigation of meteorites and laboratory samples to understand the distribution, behavior, and transformation of key volatile elements in the primordial nebula and building blocks of the inner Solar System, especially Earth.
* Protoplanetary disks and planet formation: investigations of the inner planet-forming regions of disks related to disk chemistry, the distribution of biogenic elements, and the abundance of short-lived radionuclides using ground- and space-based observations.
* Exoplanet astronomy, confirmation and characterization of transiting planets, and studies of their host stars, including young planetary systems, to understand the composition, origins, evolution, and escape of their atmospheres.
Benefits include a competitive salary with full benefits, interaction with a team of experts in diverse fields of astronomy, planetary science, and Earth science, and access to all astronomical facilities on Maunakea and cutting-edge laboratory instruments for isotopic, chemical, and mineralogical investigation of planetary materials. Successful applications will become part of a multi-institutional, Interdisciplinary Consortium for Astrobiology Research. They will be granted PI status, have the ability to write grant proposals, and will receive structured mentoring on proposal writing, research organization, student supervision and instruction, and other aspects of research and teaching. They will also have the opportunity to participate in public engagement, education, and outreach events.
Qualifications: Applications must have received a PhD in astronomy/astrophysics, or planetary or Earth sciences. Appointments are initially for one year, with an additional two years based on satisfactory performance; additional years are possible depending on availability of funding.
Start date: negotiable, but before the end of 2022.
For all inquiries and application information, contact Eric Gaidos at gaidos @ hawaii.edu
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| Postdoc position at LERMA-LPENS on the statistical charaterization of the 21-cm signal from the Epoch of Reionization | Closing date: 2022-06-31
Contact: Benoit Semelin |
| The LERMA at Observatoire de Paris and the astrophysics group at LPENS are seeking candidates for a post-doctoral position funded by the ?Initiative Physique des Infinis? at Sorbonne Université on the development of novel statistical characterizations of the 21-cm signal from the Cosmic Dawn (CD) and Epoch of reionization (EoR). | | ▸ more | Context and project:
The LERMA at Observatoire de Paris and the astrophysics group at LPENS are seeking candidates for a post-doctoral position funded by the ?Initiative Physique des Infinis? at Sorbonne Université on the development of novel statistical characterizations of the 21-cm signal from the Cosmic Dawn (CD) and Epoch of reionization (EoR).
The team at LERMA has a strong expertise in the numerical modelling of the 21-cm signal from the CD-EoR while the team at LPENS has been developing novel statistical techniques based on Scattering Transforms for several years and applied them to astrophysical problems. Both teams are members of the Cosmic Dawn Key project on the NenuFAR radio-interferometer (https://nenufar.obs-nancay.fr).
The goal of the project is to explore the uses of the various flavors of scattering transforms to characterize the 21-cm signal, including non-gaussianity. Such novel summary statistics have potential in multiple applications such as in the foregrounds-signal separation or as a metric in the inference of the signal?s underlying model parameters. An application to the CD-EoR data from NenuFAR is intented.
Profile of the candidates:
The candidate will either be a cosmologist with expertise in statistical inference methods and some familiarity with the 21-cm signal science, or a data scientist with preferably previous experience in applying data science methods to astronomical data. He/she will play a federating role between the two teams.
Practical considerations:
The appointment is for 2 years with a possible extension to 3 years. The offer includes French social security benefits and funding for travel.
Applicants should submit a CV (max. 2 pages), a letter in intent, publication list, and two letters of recommendation. Applications should be sent via email to benoit.semelin @ obspm.fr and francois.boulanger @ phys.ens.fr . Applications will be accepted until the position is filled. The contract will have to start no later than 22 Dec 2022.
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| ALMA Regional Centre Astronomer | Closing date: 2022-02-06
Contact: Human Resources |
The ALMA Regional Centre (ARC) department at ESO provides the interface between the European ALMA Users Community and the ALMA observatory in Chile. Its mission is:
1. To achieve, promote, and provide high-caliber support to the ALMA user community and to ALMA observatory global operations, including coordinated delivery of software.
2. To provide quality-assured, high-quality data products for principal investigators and archive users, within target time-windows.
3. To facilitate ALMA science performed by expert and non-expert users alike via coordination of user support.
| | ▸ more | The ARC department is looking for an astronomer with a strong research profile in radio or millimetre astronomy. You should have a strong interest and demonstrated abilities to maximize ALMA?s science output through conducting expert user support and operations support tasks. As the ARC astronomer you will contribute to core ARC duties, in particular to those related to user-facing activities including project tracking, the phase 2 process and quality assurance. In addition, you should demonstrate scientific leadership and vision to conduct high-impact independent research.
Main Duties and Responsibilities:
*Play a key role in ALMA user-facing activities, including providing scientific guidance into tool development and Phase 2 support.
*Perform general ARC duties, including answering helpdesk tickets and undertaking astronomer-on-duty shifts in Chile.
*Proactively propose improvements of existing processes and documentation and suggest new methods to increase quality and efficiency of ARC services.
*Constructively work together with other ARC staff and ALMA operations staff around the globe
*Contribute to the development of training material for ALMA users.
*As an astronomer and 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. This includes the interaction and possible supervision of students and maintaining relations with other parts of the wider organisation. Up to 50% of your time will be available for research activities.
*The tasks are not limited to the above and a flexible approach and willingness 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 and experience in the use of large observing facilities and an understanding of their operations concepts.
*Excellent 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.
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 (tax free), comprehensive pension scheme and medical, educational and other social benefits, as well as financial help in relocating your family and the possibility 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 is a possibility of extension(s) subject to individual performance and organisational requirements as defined in the applicable policies and staff rules and regulations. For any further information, please visit https://www.eso.org/public/jobs/conditions/intstaff/. 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
Apply online at http://jobs.eso.org/. Applications must be completed in English and should include a motivation letter, CV containing a publication list and a research statement. You should also provide the names and contact details of three referees familiar with your work and willing to provide a reference letter. Referees will be automatically invited to submit their letter, however, applicants are strongly advised to trigger these invitations (using the web application form) well in advance of the application deadline.
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| PhD position in high-resolution spectroscopy of exoplanetary atmospheres in Geneva | Closing date: 2022-01-31
Contact: David Ehrenreich |
| Applications are invited for a research assistant (PhD student) position at the University of Geneva (Department of Astronomy, aka the Geneva Observatory) working with Prof. David Ehrenreich on the characterisation of exoplanetary atmospheres. The successful applicant is expected to work on high-resolution spectra from the new Near-InfraRed Planet Searcher (NIRPS) at the European Southern Observatory 3.6m telescope in La Silla (Chile). | | ▸ more | Applications are invited for a research assistant (PhD student) position at the University of Geneva (Department of Astronomy, aka the Geneva Observatory) working with Prof. David Ehrenreich on the characterisation of exoplanetary atmospheres. The successful applicant is expected to work on high-resolution spectra from the new Near-InfraRed Planet Searcher (NIRPS) at the European Southern Observatory 3.6m telescope in La Silla (Chile). The Department of Astronomy is a member of the NIRPS Consortium, which involves partners in Canada, France, Spain, Portugal, Brazil, Switerzland and at ESO. The Consortium has access to 725 nights of Guaranteed Time Observations over 5 years, out of which a substantial part will be dedicated to study the atmospheres of exoplanets. The work will involve data reduction, analysis and interpretation, as well as a participation to the observations at the 3.6m telescope in La Silla (Chile). The scientific operations of NIRPS are expected to start in October 2022. The position is funded by PlanetS (see below) for 4 years.
Setting: The Geneva Observatory is at the origin of the exoplanet field with the discovery of the first exoplanet around a solar-type star by Michel Mayor and Didier Queloz (Nobel prize 2019). Today, it offers one of the most vibrant environment worldwide for exoplanet research. Nearly 60 people contributes to the exoplanet team (www.exoplanets.ch), currently including 11 faculty members, 16 postdoctoral researchers, 16 PhD students, and 16 project staff members. Research topics include exoplanet detection, exoplanet characterization (atmospheres, interiors), planetary system dynamics, and instrumentation. Team members are directly involved into a large number of projects, including photometric instruments (CHEOPS, TESS, PLATO, NGTS), high-resolution spectrographs (HARPS, HARPS-North, NIRPS and ESPRESSO) and direct imaging (SPHERE @ VLT). The exoplanet team is also part of PlanetS (www.nccr-planets.ch), a Swiss research network focused on exoplanetary science, which includes ~130 scientists from the Universities of Geneva, Bern, Zurich and the Zurich Institute of Technology. The successful applicant will be able to take advantage of this unique collaborative framework.
The University of Geneva is an equal opportunity employer committed to diversity in its workplace.
Start date is flexible; the position could start as early as June 2022.
Duration: This is a 4-year position.
Salary: ~45,000 CHF/year, according to rules of the University and Canton of Geneva.
Deadline: Candidates are encouraged to apply by January 31st, 2022, but later applications will be reviewed until the position is filled.
Requirements: A MSc degree in astronomy, astrophysics or related fields.
The successful applicant will be immersed in a team work environment, therefore good team playing abilities will be praised soft skills.
A curriculum vitae (2 pages max).
A cover letter (1 page max) listing the names and contact information for 2 reference persons.
The above application materials should be encapsulated within a single pdf and sent to david.ehrenreich @ unige.ch
Up to two letters of recommendation could be sent directly to Prof. Ehrenreich by the reference persons themselves. (Recommendation letters are welcome but not mandatory to apply to the position.)
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| PhD positions in Astronomy and Astrophysics at Warwick University | Closing date: 2022-01-14
Contact: Dr David Armstrong |
The University of Warwick Astronomy and Astrophysics group is seeking talented PhD applicants for our new Warwick Prize Scholarships in Astrophysics. Applications are due by January 14th 2022.
https://warwick.ac.uk/fac/sci/physics/research/astro/vacancies/prize/
| | ▸ more | The University of Warwick Astronomy and Astrophysics group is seeking talented PhD applicants for our new Warwick Prize Scholarships in Astrophysics. Applications are due by January 14th 2022.
The scholarships are open to national and international applicants and all are welcome to apply. We expect to offer around 10 funded PhD places in this round, including places funded via direct research grants, UK research agency support, and university allocations. All projects offered will provide a full stipend plus allocations for travel and computing.
Projects span a range of research areas including exoplanet discovery, characterisation and formation, transients and explosive astrophysical phenomena, white dwarfs and planetary remnants, and stellar populations. Details on potential projects and the application process can be found here: https://warwick.ac.uk/fac/sci/physics/research/astro/postgraduate/.
Applicants are encouraged to contact the project supervisors for further information on the projects -- this is especially important for international students seeking to be considered for additional scholarships.
Warwick is an internationally recognised centre of excellence in research. Our group is involved in many major ground and space-based projects, including the Sloan Digital Sky Survey, ESA's CHEOPS satellite and upcoming PLATO mission, the Next Generation Transit Survey (NGTS), and the Gravitational-wave Optical Transient Observer (GOTO).
Both the Physics Department and the University of Warwick hold Athena SWAN Silver awards, a national initiative to promote gender equality for all staff and students. Our Astronomy & Astrophysics group also hosts monthly equitea forums to break down barriers faced by all under-represented groups in science.
At the University of Warwick, we strongly value equity, diversity and inclusion, and encourage applications from all under-represented groups. More information on the Warwick Astronomy & Astrophysics Group can be found here: https://warwick.ac.uk/fac/sci/physics/research/astro/.
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| PhD positions in Astronomy and Astrophysics at Warwick University | Closing date: 2022-01-14
Contact: Dr David Armstrong |
The University of Warwick Astronomy and Astrophysics group is seeking talented PhD applicants for our new Warwick Prize Scholarships in Astrophysics. Applications are due by January 14th 2022.
https://warwick.ac.uk/fac/sci/physics/research/astro/vacancies/prize/
| | ▸ more | The University of Warwick Astronomy and Astrophysics group is seeking talented PhD applicants for our new Warwick Prize Scholarships in Astrophysics. Applications are due by January 14th 2022.
The scholarships are open to national and international applicants and all are welcome to apply. We expect to offer around 10 funded PhD places in this round, including places funded via direct research grants, UK research agency support, and university allocations. All projects offered will provide a full stipend plus allocations for travel and computing.
Projects span a range of research areas including exoplanet discovery, characterisation and formation, transients and explosive astrophysical phenomena, white dwarfs and planetary remnants, and stellar populations. Details on potential projects and the application process can be found here: https://warwick.ac.uk/fac/sci/physics/research/astro/postgraduate/.
Applicants are encouraged to contact the project supervisors for further information on the projects -- this is especially important for international students seeking to be considered for additional scholarships.
Warwick is an internationally recognised centre of excellence in research. Our group is involved in many major ground and space-based projects, including the Sloan Digital Sky Survey, ESA's CHEOPS satellite and upcoming PLATO mission, the Next Generation Transit Survey (NGTS), and the Gravitational-wave Optical Transient Observer (GOTO).
Both the Physics Department and the University of Warwick hold Athena SWAN Silver awards, a national initiative to promote gender equality for all staff and students. Our Astronomy & Astrophysics group also hosts monthly equitea forums to break down barriers faced by all under-represented groups in science.
At the University of Warwick, we strongly value equity, diversity and inclusion, and encourage applications from all under-represented groups. More information on the Warwick Astronomy & Astrophysics Group can be found here: https://warwick.ac.uk/fac/sci/physics/research/astro/.
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| Joint postdoctoral fellowship for AGN research in Bologna - JAB fellowship | Closing date: 2022-01-25
Contact: Roberto Gilli |
| The National Institute for Astrophysics - Observatory of Astrophysics and Space Science (INAF-OAS) and the University of Bologna, Department of Physics and Astronomy (UniBO-DIFA) are advertising their first Joint postdoctoral fellowship for AGN research in Bologna (JAB fellowship). | | ▸ more | The National Institute for Astrophysics - Observatory of Astrophysics and Space Science (INAF-OAS) and the University of Bologna, Department of Physics and Astronomy (UniBO-DIFA) are advertising their first Joint postdoctoral fellowship for AGN research in Bologna (JAB fellowship).
INAF-OAS is one of the main Departments of INAF, the main infrastructure in Italy for research in Astrophysics, made by a network of 17 Departments spread across the country. UniBO-DIFA is one Department of the Science School of UniBO, and one of the most scientifically productive Physics Departments of Italy, internationally well-known for its activities in a wide range of research fields.
Both institutes are located in the newly established Bologna Astrophysics campus, which also includes the INAF - Institute for Radio Astronomy hosting the Italian ALMA Regional Center, and the headquarters of the Cherenkov Telescope Array, all within walking distances and with shared facilities. This is the largest center for astrophysics in Italy, with a strong group at the forefront of European research in the field of galaxy formation, Active Galactic Nuclei (AGN), and AGN-galaxy co-evolution, and one of the largest astrophysics communities worldwide.
Applications are invited for an independent fellowship position to work on one or more AGN-related themes, such as the physics of accretion onto Supermassive Black Holes (SMBHs), the coevolution between SMBHs and their host galaxies, the small-to-large scale AGN feedback, the environment, demographics and cosmic evolution of AGN, the search for the most distant and hidden SMBHs. The prospective candidate is expected to develop an original research program, mainly of observational type, in collaboration with personnel at INAF-OAS and UniBO-DIFA.
Applicants should have a PhD in Physics or Astronomy obtained before January 25th, 2019. The position is expected to start by July 2022 and is for two years in the first instance and renewable afterwards, depending on fund availability and performance review. The yearly gross salary is 34,000 Euros. Generous funding will be allocated for publications, computing and travel expenses.
The applicant should prepare a CV, publication list, brief research project and fill all the application forms following the instructions of the official call: https://www.oas.inaf.it/en/opportunities/bando-191-2021-en/
All applications should be submitted via email to: inafoasbo @ postecert.it by January 25th, 2022. Up to three reference letters should be e-mailed separately to roberto.gilli @ inaf.it by the same deadline.
For inquiries, please contact any member of the search committee: Dr. Roberto Gilli (INAF-OAS; roberto.gilli @ inaf.it), Dr. Marcella Brusa (UniBO-DIFA; marcella.brusa3 @ unibo.it), Dr. Giorgio Lanzuisi (INAF-OAS; giorgio.lanzuisi @ inaf.it).
INAF and UniBo are equal opportunity employers. Members of underrepresented or disadvantaged groups are encouraged to apply.
Any personal data will be processed in accordance with the General Data Protection Regulation 679/2016 EU (GDPR) on the Protection of Individuals.
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| Post-doc position on "Physics of the ISM in galaxies through spec. surveys" at the Arcetri Obs. (Florence) | Closing date: 2022-01-15
Contact: Giovanni Cresci |
The Arcetri Astrophysical Observatory (INAF), in Florence, Italy, invites application for a two years post-doc position.
The fellow will focus on the study of the Interstellar Medium in galaxies (chemical abundances, dynamics and ionization conditions) using optical and near-IR spectroscopy, including data from GTO time on forthcoming new facilities such as MOONS and ERIS at the VLT. The activity will be carried out under the supervision of Dr. Giovanni Cresci, and in close collaboration with F. Mannucci, F. Belfiore and A. Marconi | | ▸ more | The official announcement can be found at https://www.arcetri.inaf.it/images/data/Concorsi/DD1272021/DD_127-2021_-Bando-MOONS_signed.pdf
A PhD in physics, astronomy or related discipline is required, or alternatively a Master degree and at least three years of documented experience in scientific activities. The position should start preferably before October 1st, 2022, and is tenable for two years after a review at the end of the first year. Applications must consist of:
- an application form consisting of Annex 1 & 2 (see the official announcement) and a certification form signed and dated by the applicant;
- A copy of a valid identity document (ID card for EU-citizens or passport for non-EU citizens);
- A CV, signed and dated by the applicant;
- A list of publications;
- a brief statement of research interests, up to three pages in length (12 pt Times New Roman);
- two reference letters to be sent before the deadline directly by the referees to the address: inafoaarcetri @ pcert.postecert.it, reporting in the subject line the indication of the related procedure: DD 127/2021 and the name of the candidate;
- A copy of the Masters and/or PhD certificate, and respective English translations (if the original is not in English);
Previous experience with optical and near-IR spectroscopy, chemical abundances in HII regions and galaxies, physics of the ISM and tools for data reduction and analysis of spectroscopic data will be considered as preferential qualifications.
All material shall be submitted in English. The deadline for applications is January 15th, 2022 1.00 p.m. (CET). The application must be submitted electronically at inafoaarcetri @ pcert.postecert.it .
Short-listed candidates will be contacted for interview likely in late January. The gross salary will be of 28000 euro/year. Employment conditions include social benefits granted according to applicable Italian regulations for public sector employment.
More information on the Extragalactic group of the Arcetri Observatory: https://www.arcetri.inaf.it/en/research/galaxies-and-cosmology
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| Senior Scientist at the Department of Astrophysics at the University of Vienna | Closing date: 2022-01-10
Contact: Werner Zeilinger |
We are looking for an outstanding candidate for a full-time senior scientist position to strengthen our instrumentation group of the Department of Astrophysics.The department is involved in the development of international astronomical instrumentation projects, both at the European Southern Observatory (ESO) and the European Space Agency (ESA).
Initially, this post is to be filled for 4 years. Afterwards, there is a possibility to extend the post to a permanent contract. | | ▸ more | Senior Scientist at the Department of Astrophysics at the University of Vienna
Reference number: 12495
Deadline for application: December 12, 2021
Applications should be submitted via the Job Center to the University of Vienna (http://jobcenter.univie.ac.at) mentioning reference number 12495.
Job grading in accordance with collective bargaining agreement: §48 VwGr. B1 lit. b (postdoc) with relevant work experience determining the assignment to a particular salary grade.
The successful candidate will have the opportunity to work within a dedicated team on forefront science while profiting from the international environment in the Department of Astrophysics within the lively city of Vienna. The department is involved in the development of international astronomical instrumentation projects, both at the European Southern Observatory (ESO) and the European Space Agency (ESA). We are looking for an outstanding candidate for a full-time position to strengthen our instrumentation group. Initially, this post is to be filled for 4 years. Afterwards, there is a possibility to extend the post to a permanent contract.
Job Description:
i) Coordination and implementation of astronomical projects connected with ESO, in particular, but not exclusively, instrumentation projects for the Extremely Large Telescope (ELT). Individual tasks include software development, (co-)organisation of and participation in international consortium and collaboration meetings, project administration and correspondence with funding agencies, and contributions to preparatory studies;
ii) Project management, (co-)supervision and (co-)organisation within the department's "laboratory for astronomical instrumentation" which comprises, apart from ESO and ESA related projects, also the university-owned Leopold Figl Observatory and a local student telescope for education.
iii) Conducting independent teaching of courses as defined by the collective agreement;
iv) (Co-)supervision of students;
v) Contributions to general organisational and administrative tasks.
Profile:
- PhD or doctoral degree in Astronomy/Astrophysics
- Experience in astronomical software development for data analysis of optical and infrared instrumentation
- Experiennce with programming languages (C, Python) and astronomical software tools (ESO data reduction pipelines)
- Ability to work in a team
- Excellent command of written and spoken English
- Excellent communication skills
- Experience in teaching and training
- Experience in (co-)supervising students
- Experience in (co-)organising events
The application should include a letter of motivation, a curriculum vitae (with a list of publications and presentations) and a statement of research interests (maximum of two pages). Please also give names and contact details of 3 persons that can provide on request a recommendation letter.
Link to the official job announcement: https://univis.univie.ac.at/ausschreibungstellensuche/flow/bew_ausschreibung-flow;jsessionid=581CEE5879FDE447D60EBBABC28A4CB9?_flowExecutionKey=_cBF576DE2-8239-F5BC-8781-D6D92E994A36_k2C530F0C-7A7D-F390-EC1F-064B097C416E&tid=88367.28&_language=en
For further information please contact:
Werner Zeilinger (werner.zeilinger @ univie.ac.at) +43-1-4277-51865
Bodo Ziegler (bodo.ziegler @ univie.ac.at) +43-1-4277-53825
The University pursues a non-discriminatory employment policy and values equal opportunities, as well as diversity (http://diversity.univie.ac.at/). The University lays special emphasis on increasing the number of women in senior and in academic positions. Given equal qualifications, preference will be given to female applicants.
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| Data Scientist in astronomical imaging and machine learning | Closing date: 2021-12-15
Contact: Daniel Schaerer |
| The Stochastic Information Processing Group (SIP) (http://sip.unige.ch) of Prof. Slava Voloshynovskiy and the Starbursts in the Universe group (https://www.unige.ch/sciences/astro/starbursts/en/) of Prof. Daniel Schaerer, University of Geneva, Switzerland, have an open data scientist in astronomical imaging and machine learning. | | ▸ more | The Stochastic Information Processing Group (SIP) (http://sip.unige.ch) of Prof. Slava Voloshynovskiy and the Starbursts in the Universe group (https://www.unige.ch/sciences/astro/starbursts/en/) of Prof. Daniel Schaerer, University of Geneva, Switzerland, have an open data scientist in astronomical imaging and machine learning.
Profile:
* PhD degree in one of the following domains: astronomy, astrophysics, computer science, data science or mathematics
* Proven record of achievements and previous experience with machine learning and imaging, knowledge of signal/image processing and astro-imaging
* Strong programming skills in Python with experience in TensorFlow, PyTorch or Keras that will be verified
* Knowledge of HPC and large-scale data processing
* Strong verbal and written communication skills in English
* Strong analytical abilities and problem solving/troubleshooting skills
We offer:
* Great multidisciplinary team
* Collaboration with the leading groups in machine learning and astronomy in Switzerland
* Great learning opportunities
* Competitive salary including Standard Swiss Social Security, Accident Insurance and Pension contributions
* The position is initially for 2 years with an option of extension for 2 additional years
The successful applicant will be involved in a project on the development of machine learning algorithms and innovative data analysis tools in the scope of the Swiss participation in the Square Kilometer Array observatory (SKA, https://www.skatelescope.org). The project concerns the development of new machine learning methods for the SKA that include imaging algorithms and classification techniques. The data scientist will be also engaged in the development and testing of scalable high-performance code on the data from SKA precursors and providing the technical support of developed code to other groups within a Swiss collaboration.
The hiring groups at the University of Geneva have a broad network of national and international collaboration and scientific exchange, visits and training.
STARTING DATE
The envisioned starting date is February-March, 2022 but it can be negotiated.
APPLICATION PROCEDURE
Qualified candidates are encouraged to send their applications including a CV and publication list, description of research experience and interests, contact information of three references in a single pdf by email. Applications received by 15 December, 2021 will receive consideration.
Pre-selected candidates will be invited for a skype/zoom interview.
CONTACT
Please, send your applications to the emails below:
E-mails: svolos @ unige.ch and daniel.schaerer @ unige.ch
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| Tenure-track Astrophysicist (m/f/d) position in the field of exoplanets | Closing date: 2021-12-31
Contact: Prof. Dr. Katja Poppenhaeger |
The Leibniz Institute for Astrophysics Potsdam (AIP) invites applications for a
Tenure-track astrophysicist
who will strengthen our research in the section Stellar Physics and Exoplanets, led by Prof. Dr. Katja Poppenhaeger. This section has a focus on investigating star-exoplanet systems through observations and simulations. The tenure-track researcher will enhance the section's profile through their expertise in the field of exoplanets, exoplanetary atmospheres, or stellar-planetary relations. | | ▸ more | This position gives the opportunity to pursue an independent research program within the section and contribute to the supervision of students at the undergraduate and graduate level. The AIP is a consortium member of the HIRES spectrograph for the ELT and has institutional access to several ground- and space-based observatories; candidates are encouraged to outline connections of their planned research to the relevant observational facilities of the current and next decade.
Qualifications
Applicants need to have a PhD in astrophysics, astronomy, or a closely related field. A convincing publication record in relevant topics and experience in acquiring external funding are expected. Experience in supervising students is welcome.
Salary and benefits
Salary and benefits are commensurate with those of public service organizations in Germany at the TV-L E14 level and include employer contributions to medical and dental insurance, parental leave, retirement benefits, and a subsidy for a public transportation ticket. The appointment will be for an initial period of five years, with tenure based on a successful performance review. For exceptional candidates with commensurate qualifications a directly tenured appointment may be considered. The position is anticipated to start in fall 2022, but this is subject to individual arrangements.
Application
To apply, please register at the AIP recruitment portal:
https://jobs.aip.de/rec119
and follow the instructions to upload the following documents, all in PDF format: A cover letter motivating your application, your curriculum vitae, a list of publications, a research plan (max. 3 pages), a summary of your past research (max. 2 pages), and the names of three individuals willing to provide reference letters upon request.
Applications received before 31.12.2021 will receive full consideration.
In case of questions please contact Prof. Poppenhaeger at the following email address:
bewerbung-2021-29 @ aip.de
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| INPhINIT Incoming PhD Fellowships at the Institute of Cosmos Sciences | Closing date: 2021-12-31
Contact: Esther Pallares |
The doctoral fellowship programme INPhINIT ?la Caixa? is devoted to attracting talented Early-Stage Researchers?of any nationality?who wish to pursue doctoral studies in Spanish or Portuguese territory. Sponsored by ?la Caixa? Foundation, it is aimed at supporting the best scientific talent and fostering innovative and high-quality research in Spain and Portugal by recruiting outstanding international students and offering them an attractive and competitive environment for conducting research of excellence.
| | ▸ more | The doctoral fellowship programme INPhINIT ?la Caixa? is devoted to attracting talented Early-Stage Researchers?of any nationality?who wish to pursue doctoral studies in Spanish or Portuguese territory. Sponsored by ?la Caixa? Foundation, it is aimed at supporting the best scientific talent and fostering innovative and high-quality research in Spain and Portugal by recruiting outstanding international students and offering them an attractive and competitive environment for conducting research of excellence.
The Institute of Cosmos Sciences of the University of Barcelona is a research centre accredited with the Spanish Seal of Excellence María de Maeztu in 2020, the perfect place to carry out your PhD project through an INPhINIT Incoming fellowship. The Institute is offering ten different projects:
-Axions as Dark Matter: experimental detection and dynamics in the Milky Way: https://finder.lacaixafellowships.org/finder?position=5360
-Constraining binary black hole mergers from star clusters: https://finder.lacaixafellowships.org/finder?position=5429
-High Performance Computing for Nuclear Physics in and beyond the Standard Model: https://finder.lacaixafellowships.org/finder?position=5362
-Holography in the Gravitational Wave era: https://finder.lacaixafellowships.org/finder?position=5382
-M dwarfs activity from a CubeSat (MACU): https://finder.lacaixafellowships.org/finder?position=5236
-Mining the Gaia catalogue: structure and kinematics of the Milky Way and the LMC: https://finder.lacaixafellowships.org/finder?position=5364
-Quantum machine learning to detect Dark Matter with atomic nuclei: https://finder.lacaixafellowships.org/finder?position=5361
-Solid state Entangled Photon Source for Earth and Space use: https://finder.lacaixafellowships.org/finder?position=5367
-The physics of flavour and its connection to dark matter searches: https://finder.lacaixafellowships.org/finder?position=5363
-Ultracold dipolar bosons trapped in quantum circuits: https://finder.lacaixafellowships.org/finder?position=5431
Employment conditions
The maximum total payment amount will be ?122,592, as broken down below:
-Three annual payments of ?34,800 each to the institution to cover the Fellow?s contract, who will receive a gross annual income of ?27.724,67. This amount might vary if there are modifications in the legal framework.
- ?3,564 per year, as an additional amount for conferences, courses, research stays, consumables, equipment, charges for the use of intellectual property, etc.
-The ?la Caixa? Foundation will award a prize of ?7,500, which will be paid to the fellows who deposit their thesis within 6 months after the third year of their fellowship has ended.
In addition to financial support, the fellowship includes a training programme on transversal skills, which has been specially designed by leading international institutions in the sector.
This programme includes aspects such as technology transfer, entrepreneurship, commercialisation of innovation, intellectual property, leadership, creativity, communication skills, teamwork, personal development, planning, assertiveness and networking.
For more information on the employment conditions, please refer to this document: https://fundacionlacaixa.org/documents/10280/1636133/programme-rules-inphinit-incoming-2022.pdf/fc7833bf-b9ee-6511-12bc-5b216173ba2f?t=1635950756692
Working at the Institute of Cosmos Sciences
The Institute of Cosmos Sciences is a research institute of the University of Barcelona. It is an interdisciplinary centre 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.
Moreover, the ICCUB participates in many key international scientific consortia and projects, such as the Large Hadron Collider, the Gaia astrometric space mission, the MAGIC / CTA high-energy astrophysics telescopes, and the Virgo gravitational wave detector, among others. Additional information about the Institute and the University of Barcelona can be found here.
You will be encouraged to contribute and interact with other researchers in the vibrant and international research environment as well as to participate in our outreach initiatives, more information at serviAstro and serviParticules.
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 in physical sciences 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 2021: one with near-perfect weather year-round, miles and miles of beaches, iconic parks, striking architecture and colourful neighbourhoods 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.
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| Atmospheres of temperate planets and their observability using RISTRETTO and HIRES | Closing date: 2021-12-15
Contact: Emeline Bolmont |
Applications are invited for a PhD student position at the University of Geneva (Geneva Observatory) working with Prof. Christophe Lovis and Prof. Emeline Bolmont on the modeling and future characterization of temperate/hot rocky planets around low-mass stars.
The successful applicant is expected to (1) work with a global climate model to study the atmosphere and habitability of planets and (2) link the outputs of the simulations of atmospheres to observables (like high-resolution spectroscopic diagnostics in reflected light) for future instruments, like RISTRETTO and HIRES. | | ▸ more | Applications are invited for a research assistant (PhD student) position at the University of Geneva (Geneva Observatory) working with Prof. Christophe Lovis and Prof. Emeline Bolmont on the modeling and future characterization of temperate/hot rocky planets around low-mass stars. The successful applicant is expected to work with a global climate model to study the effect of a variety of different parameters on the atmosphere and habitability of planets. The work will involve to run extensive simulations with the 3D Global Climate Model LMD-Generic and analyze the resulting outputs. The LMD-Generic (http://www-planets.lmd.jussieu.fr) is a generic version of the Earth global climate model used to study global warming. The student will work in close collaboration with Dr. Martin Turbet from the LMD.
The student will also work on the implementation of new physical processes in the model, in particular the heat flux due to tidal dissipation inside planets and the impact of volcanic gases and aerosols on the atmosphere. The student will also link the outputs of the simulations of atmospheres to observables for future instruments, in which Geneva has a leading role: RISTRETTO (VLT) and HIRES (ELT). A particular emphasis will be put on high-resolution spectroscopic diagnostics in reflected light. This PhD will therefore bring an important modeling effort for the preparation of these future atmospheric characterization instruments.
Setting: The Geneva Observatory offers one of the most vibrant environments worldwide for exoplanet research. Nearly 60 people contributes to the exoplanet team (www.exoplanets.ch), currently including 10 faculty members, 15 postdoctoral researchers, 17 PhD students, and 22 project staff members. Research topics include exoplanet detection, exoplanet characterization (atmospheres, interiors), planetary system dynamics, and instrumentation. Team members are directly involved into a large number of projects, including photometric instruments (CHEOPS, TESS, PLATO, NGTS), high-resolution spectrographs (HARPS, HARPS-North, NIRPS and ESPRESSO) and direct imaging (SPHERE @ VLT). The exoplanet team is also part of PlanetS (www.nccr-planets.ch), a Swiss research network focused on planetary science, which includes ~130 scientists from the Universities of Geneva, Bern, Zurich and ETH Zurich. The successful applicant will be able to take advantage of this unique collaborative framework and also participate to at least one observational run per year.
The University of Geneva is an equal opportunity employer committed to diversity in its workplace.
Start date: no later than June 2022.
Duration: This is a 4-year position.
Salary: ~48,000 CHF/year gross salary, according to rules of the University and Canton of Geneva.
Deadline: Candidates are encouraged to apply by December 15th, 2021, but later applications will be reviewed until the position is filled.
Requirements: A MSc degree in astronomy, astrophysics or related fields.
The successful applicant will be immersed in a team work environment, therefore good team playing abilities and focus will be praised soft skills.
The following application materials should be encapsulated within a single pdf and sent to emeline.bolmont @ unige.ch
- A curriculum vitae (2 pages).
- A cover letter (1 page) listing the names of 2 references/referees.
Up to two letters of recommendation should be sent directly to Prof. Bolmont by the referees themselves.
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| PhD student position in dwarf galaxies at Leibniz-Institute for Astrophysics, Potsdam | Closing date: 2021-12-31
Contact: Marcel Pawlowski |
| The Leibniz Institute for Astrophysics Potsdam (AIP) invites applications for a PhD student position in dwarf galaxies (m/f/d). The position is in the research group led by Dr Marcel S. Pawlowski, and part of the project "Cosmic Choreographies - Studying Systems of Satellite Galaxies and Their Phase-Space Correlations". The successful applicant will also become part of Prof. Maria-Rosa Cioni's Dwarf Galaxies section and collaborate with other researchers at the AIP. | | ▸ more | The PhD project studies satellite galaxy systems, with particular emphasis on the Milky Way system and signatures of the infall of dwarf galaxies in groups. It will involve analysing cosmological simulations, modelling orbital dynamics, and using observational data such as provided by the Gaia mission and other instruments.
We are looking for a new member of our internationally diverse team, who is interested in working and learning together while contributing to a culture of open debate. Applicants should hold a Master's degree (or equivalent) in astrophysics or a related discipline at the time of taking up the position. Any of the following skills would be advantageous: experience in scientific coding (preferentially Python), experience with running numerical simulations, analysing cosmological simulations, or observational studies of galaxies or proper motions. Advanced English skills (spoken and written) are a requirement.
The salary is based on the German public service scale (66% TV-L E13). Employer contributions to medical and dental insurance, parental leave, and retirement benefits are included. The position comes with funding for research travel as well as access to training opportunities within the graduate program of the University of Potsdam. The anticipated start date is June 1, 2022, but an earlier or later start can be negotiated. The AIP is an equal opportunity employer who values diversity and particularly encourages women and other underrepresented groups to apply. Inquiries about the position are welcome and should be sent to Dr Marcel S. Pawlowski (mpawlowski @ aip.de).
To apply, please send a cover letter motivating the application, a curriculum vitae, and a one-page statement of research interests and experiences to the address below. The application should contain your Master degree certificate or expected degree completion date, and a link to the Master thesis if already available. Please send all documents in a single pdf file to: bewerbung-2021-27 @ aip.de. Applications received by December 31, 2021 will be given full consideration. Applicants should also arrange for two letters of recommendation to be sent to the same address by this date.
Equal opportunities are an integral part of personnel and organizational development at the AIP, therefore applications from men and women are equally welcome. People with disabilities will be given preferential consideration if they are equally qualified and skilled.
Application documents will be kept for at least three months after completion of the recruitment process, even if your application is unsuccessful. As a rule, your documents will be made available to a selection committee and the committees and officials to be involved.
Link to pdf-version of this job ad: https://www.aip.de/documents/231/phd-student-position-in-dwarf-galaxies-mfd/
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| Professorship in Astrophysics | Closing date: 2021-12-17
Contact: Prof Paul Callanan |
The Department of Physics, University College Cork (UCC), Ireland invites applications for a permanent whole time senior professorship, with specialisation in astrophysics, gravitational physics or cosmology.
| | ▸ more | The Department of Physics, University College Cork (UCC), Ireland invites applications for a permanent whole time professorship, with specialisation in astrophysics, gravitational physics or cosmology.
UCC is one of Ireland?s foremost research universities, with ~18,000 students and 3,000 staff. The Department of Physics has a long established reputation for excellence in teaching and research. Current strengths include optics and photonics, condensed matter theory, experimental quantum topological matter, quantum information technology, laser spectroscopy and astrophysics. Cork is a dynamic and engaging city of ~200,000, recently rated by Lonely Planet as one of the top ten cities to visit in the world. Ireland has a thriving astronomy community and is a member of ESA, the LOFAR radio network, and ESO.
Applicants must hold a doctoral qualification in Physics or a closely related area, and a portfolio of significant research accomplishments and publications. The appointee will be required to contribute teaching to the range of BSc degrees offered by the Department of Physics, as well as at postgraduate level. Demonstrated teaching ability is essential, as is ability to generate research funding. Applicants should have research interests and accomplishments specific to astrophysics, gravitational physics or cosmology. Note that an additional position in UCC, with an emphasis on theoretical astrophysics, has also been advertised.
For further information on the Department of Physics, see http://physics.ucc.ie
UCC is committed to creating and fully embracing an inclusive environment where diversity is celebrated. Appointments will be made on the Professor or Professor (Scale 2) Salary Scale [new entrants 2021]: 99,097 - 150,712 euro.
Application forms must be completed and are available together with full details, from www.ucc.ie/en/hr/vacancies or the Department of Human Resources, University College Cork, Ireland. Email: recruitment @ per.ucc.ie / Tel: +353 21 4901814/ Fax: +353 21 4271568.
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| Astronomer / Project Scientist | Closing date: 2021-12-31
Contact: Human Resources |
| The European Organisation for Astronomical Research in the Southern Hemisphere (ESO) is the foremost intergovernmental astronomy organisation in Europe and the world?s most productive ground-based astronomical observatory. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. | | ▸ more | The Project Science Department, within the Directorate for Science at its Headquarters in Garching, near Munich, Germany, ESO is advertising the position of
ESO is engaged in the operation and construction of a number of state-of-the-art optical and infrared instruments for its observatories. The Instrument Project Scientist supports the development of science goals for new instruments, and monitors and nurtures those objectives during the full development, construction and commissioning phases. The Project Scientist thus ensures that the top-level requirements are fulfilled and that the operational scenarios are commensurate with the scientific needs and the constraints of the observatory. 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, as well as for the ESO scientific community at large when it comes to preparing for and advertising the science. The successful applicant will be assigned to follow one or more instruments at any given time.
We are looking for an enthusiastic and outstanding scientist, with the prime objective to support and follow the new generation multi-object optical and near-infrared spectrograph for the Very Large Telescope: MOONS. MOONS is a remarkable spectrograph, which will be positioned at one of the Nasmyth foci of the VLT, based on a fiber-positioner with superb multiplexing capabilities, and delivering thousands of low / high spectral resolution spectra. From surveys of nearby stars to remote high-redshift galaxies, MOONS will be a powerful machine to probe the physics of astronomical targets, and to reveal their formation and evolution histories, serving a broad range of science topics and a large community of scientists throughout the world. MOONS is in the final stages of its construction and integration life, with a potential sky commissioning at Paranal in 2024. We expect the successful candidate to acquire and/or develop unique competences and skills which will be further applied and developed beyond the early operations of MOONS for future ESO instrumentation projects.
ESO encourages junior-career scientists to apply for this position.
Main Duties and Responsibilities:
? Provides strong scientific leadership to the assigned instrument programmes within ESO;
? Acts as the principle scientific contact to the instrument building consortium;
? 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;
Astronomer / Project Scientist
? 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 the 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; and
? Coordinates the activities of the instrument Science Team.
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.
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:
? Active research programme and robust publication record;
? Expertise in optical and/or near-infrared spectroscopy;
? Understanding of the science requirements on instruments and strategies for their realisation;
? Experience with the planning, execution, analysis and publication of scientific research arising from said instrumentation;
? 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;
? Cooperative team player;
? Ability to work in a clear and structured manner producing meaningful reports to supervisors and presentations to 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; and
? Ability to negotiate with external scientists and instrument builders to achieve ESO's goals.
Desirable:
? Experience and involvement in the key phases of the development of an astronomical instrumentation project (initial/final design, system testing, or commissioning and early operations).
Qualifications
Essential educational level:
? PhD in Astronomy, Physics or equivalent
Qualifications which would be an asset:
? Expertise in multi-object spectroscopy; and
? Expertise in fiber-fed astronomical instrumentation.
Language skills:
Excellent command of the English language (written and oral) is essential.
For more details and to apply, please follow this link: https://recruitment.eso.org/jobs/2021_0047
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| Postdoctoral Research Fellowship in Cosmology (Euclid) at the University of Oslo | Closing date: 2021-12-15
Contact: Per Barth Lilje |
| The Institute of Theoretical Astrophysics, University of Oslo, has available a 3-year Postdoctoral Research Fellowship for research within the Euclid Consortium Science Working Groups. | | ▸ more | This position is dedicated to the Institute?s participation in the European space mission Euclid, and especially in Euclid?s Cosmological Simulations and Cosmological Theory Science Working Groups (SWGs). Possible projects for the postdoctoral research fellow include, in coordination with the mentioned SWGs, to perform theoretical predictions for weak lensing observables, to do post-processing of simulations performed within the SWGs and to perform data preparation for the galaxy mock production in theories beyond General Relativity. Candidates that are already involved in Euclid on similar projects critical for the success of the mission will also be considered.
Previous experience with cosmological simulations, especially for cosmological models beyond the Lambda-Cold-Dark-Matter paradigm, is considered highly beneficial for this position, as are strong computing and programming skills. The Institute has access to world-class computing facilities, both in-house, on-campus and nationally, that are directly available to the candidate.
For further information and application portal, see https://www.jobbnorge.no/en/available-jobs/job/214136/postdoctoral-research-fellow-in-cosmology-euclid
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| Postdoctoral Research Fellowship in Astrophysics at the University of Oslo | Closing date: 2021-12-15
Contact: Per Barth Lilje |
| We are seeking an enthusiastic and collaborative postdoctoral researcher to join the extragalactic astrophysics group led by Drs. Sijing Shen and Claudia Cicone. | | ▸ more | The extragalactic astrophysics group studies the formation and evolution of galaxies, observationally as well as through numerical simulations, with a focus on both the local and the high-redshift Universe. Special scientific interests are the interstellar and circumgalactic media of galaxies and the baryon cycle. In the selection, the academic quality and promise of the candidates will be of primary importance, as well as their ability to work within the extragalactic astrophysics group.
For further information, and application portal, see: https://www.jobbnorge.no/en/available-jobs/job/214124/postdoctoral-research-fellow-in-extragalactic-astrophysics
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| Trottier Postdoctoral Fellowship in Exoplanetary Science (iREx) | Closing date: 2021-12-15
Contact: Nathalie Ouellette |
| The Institute for Research on Exoplanets (iREx), affiliated with the physics department of the University of Montreal (UdeM), invites applications for a postdoctoral fellowship in experimental, observational or theoretical astrophysics applied to the study of exoplanets. A number of iREx projects are described below for reference. | | ▸ more | The Institute for Research on Exoplanets (iREx), affiliated with the physics department of the University of Montreal (UdeM), invites applications for a postdoctoral fellowship in experimental, observational or theoretical astrophysics applied to the study of exoplanets. A number of iREx projects are described below for reference.
Applicants should submit 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. Applicants may also include a cover letter, but this is not mandatory. All application materials including letters of reference must be received electronically at the following address: irex @ astro.umontreal.ca, by December 15th 2021 for full consideration.
A PhD in physics, astronomy or related discipline is required at the time when the position starts. Preference will be given to applicants within 3 years of obtaining their PhD. Applicants with career interruptions resulting from parental, medical or family leaves, or other causes are invited to mention these in their cover letter, if so desired. The successful applicant is expected to start between May and September 2022. The position is for two years, renewable for a third year subject to performance and availability of funds.
The iREx consists of a growing team of over 60 people (professors, postdocs, research assistants and students) mostly from UdeM and McGill University all working on various research programs focused on the study of exoplanets and related fields of stellar astrophysics. Members of iREx are actively involved in large international projects related to the detection and characterisation of exoplanets such as the JWST, SPIRou and NIRPS. More information on iREx research programs can be found on our website.
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| M2FINDERS-3 - TWO POSTDOCTORAL POSITIONS (m/f/x) IN RADIO ASTRONOMY | Closing date: 2021-12-31
Contact: Eduardo Ros |
| The Max Planck Institute for Radio Astronomy (MPIfR) - the leading radio astronomical institute in Germany - is recruiting up to two postdoctoral researchers in Radio Astronomy to join the project M2FINDERS (Mapping Magnetic Fields with INterferometry Down to Event hoRizon Scales) led by Prof. J. A. Zensus (ERC grant No 101018682). | | ▸ more | MPIfR operates the 100-m radio telescope in Effelsberg (as a single telescope and as an element of the European VLBI Network - EVN and the Global Millimetre VLBI Array - GMVA), the LOFAR DE1 station, which is part of the International LOFAR Telescope, the APEX telescope in Chile (also an element of the Event Horizon Telescope - EHT), and a state-of-the-art VLBI (Very Long Baseline Interferometry) correlator. The department of Radio Astronomy/VLBI, led by Prof. Dr. J. A. Zensus, has a broad research portfolio, with a focus on compact extragalactic objects (AGN) and their broad-band emission, through very-high-resolution studies with mm- and space-VLBI imaging and blazar monitoring.
The MPIfR is recruiting up to two postdoctoral researchers in Radio Astronomy to join the project M2FINDERS (Mapping Magnetic Fields with INterferometry Down to Event hoRizon Scales). M2FINDERS is led by Prof. Zensus as the principal investigator, with funding from the European Research Council (grant agreement No 101018682). The project will measure and model the three-dimensional morphology of the magnetic field in the immediate vicinity of supermassive black holes. The primary goal is to use VLBI observations to measure the strength and distribution of the magnetic field within 10000 gravitational radii of the black hole and to use these measurements as a probe of physical conditions on the event horizon scale. The postdoctoral researchers will work on Magnetic field measurements in the vicinity of supermassive black holes. For this purpose, multifrequency polarimetric VLBI observations of a sample of radio-loud AGN with the available cm- and mm-wavelength VLBI arrays will be carried out, in order to obtain linear polarisation and Faraday rotation information. These observations will be used to map the structure of the magnetic field: Faraday rotation measure, core shift, and turnover frequency/flux density distribution.
There will also be opportunities to supervise and collaborate with PhD students and gain teaching experience in the International Max Planck Research School for Astronomy and Astrophysics (IMPRS).
We are looking for researchers with related scientific interests, qualifications and skills. Experience in polarimetric and/or astrometric radio interferometry techniques and VLBI is desirable.
Interested and qualified individuals are encouraged to apply by submitting their curriculum vitae, list of publications, and a research motivation letter. Applicants should also arrange for three letters of recommendation to be sent to the MPIfR application portal at the address given below by December 31, 2021.
The initial appointments are for two years with the possibility of extension after review. The anticipated starting date is February 2022, or later. The recruitment process will remain open until the positions are filled. Remuneration is within the framework of the German wage agreement for the public service (TVöD-Bund) in level 13.
The Max Planck Society is committed to increasing the number of individuals with disabilities in its workforce and therefore encourages applications from such qualified individuals. Furthermore, the Max Planck Society seeks to increase the number of women in areas where they are underrepresented and therefore explicitly encourages women to apply.
Please submit your application at
https://s-lotus.gwdg.de/mpg/mbra/perso/mpifr_bonn_sci_012.nsf/application
Contact information for inquiries:
Prof. Dr. Eduardo Ros
Tel. +49 228 525 125
ros @ mpifr.de
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| M2FINDERS-1 - TWO POSTDOCTORAL POSITIONS (m/f/x) IN RADIO ASTRONOMY | Closing date: 2021-12-31
Contact: Eduardo Ros |
| The Max Planck Institute for Radio Astronomy (MPIfR) - the leading radio astronomical institute in Germany - is recruiting up to two postdoctoral researchers in Radio Astronomy to join the project M2FINDERS (Mapping Magnetic Fields with INterferometry Down to Event hoRizon Scales) led by Prof. J A. Zensus (ERC Grant No 101018682). | | ▸ more | MPIfR operates the 100-m radio telescope in Effelsberg (as a single telescope and as an element of the European VLBI Network - EVN and the Global Millimetre VLBI Array - GMVA), the LOFAR DE1 station, which is part of the International LOFAR Telescope, the APEX telescope in Chile (also an element of the Event Horizon Telescope - EHT), and a state-of-the-art VLBI (Very Long Baseline Interferometry) correlator. The department of Radio Astronomy/VLBI, led by Prof. Dr. J. A. Zensus, has a broad research portfolio, with a focus on compact extragalactic objects (AGN) and their broad-band emission, through very-high-resolution studies with mm- and space-VLBI imaging and blazar monitoring.
The MPIfR is recruiting up to two postdoctoral researchers in Radio Astronomy to join the project M2FINDERS (Mapping Magnetic Fields with INterferometry Down to Event hoRizon Scales). M2FINDERS is led by Prof. Zensus as the principal investigator, with funding from the European Research Council (grant agreement No 101018682). The project will use multifrequency polarimetric, spectral, and astrometric measurements to measure and model the strength and the three-dimensional morphology of the magnetic field in the immediate vicinity of supermassive black holes in order to probe the physical conditions on the event horizon scale. The project will comprise a dedicated in depth study of prominent nearby AGN, using multifrequency VLBI observations with the VLBA and EVN at 15, 22, and 43 GHz, the GMVA at 86 GHz, and the EHT at 230 GHz. The successful candidates will work on reconstruction of the 3D structure of the magnetic field near supermassive black holes in these AGN. One of the two positions will be dedicated to development and application of methods for obtaining information about the magnetic field from polarisation mapping and Faraday rotation, turnover frequency imaging, and frequency dependent opacity (core shift). The other position will focus on developing and applying analytical and numerical modelling frameworks for estimating the strength and reconstructing the morphology of magnetic field from the observational measurements listed above. The two researchers will be working in close coordination with each other and with the entire M2FINDERS team.
There will also be opportunities to supervise and collaborate with PhD students and gain teaching experience in the International Max Planck Research School for Astronomy and Astrophysics (IMPRS).
Interested and qualified individuals are encouraged to apply by submitting their curriculum vitae, list of publications, and a research motivation letter. Applicants should also arrange for three letters of recommendation to be sent to the MPIfR application portal at the address given below by December 31, 2021.
The initial appointments are for two years with the possibility of extension after review. The anticipated starting date is February 2022, or later. The recruitment process will remain open until the positions are filled. Remuneration is within the framework of the German wage agreement for the public service (TVöD-Bund) in level 13.
The Max Planck Society is committed to increasing the number of individuals with disabilities in its workforce and therefore encourages applications from such qualified individuals. Furthermore, the Max Planck Society seeks to increase the number of women in areas where they are underrepresented and therefore explicitly encourages women to apply.
Please submit your application at
https://s-lotus.gwdg.de/mpg/mbra/perso/mpifr_bonn_sci_011.nsf/application
Contact information for inquiries:
Prof. Dr. Eduardo Ros
Tel. +49 228 525 125
ros @ mpifr.de
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| Long-term post-doctoral position in stellar spectroscopy of multiple systems | Closing date: 2021-12-15
Contact: Griet Van de Steene |
The Royal Observatory of Belgium and the Université Libre de Bruxelles are looking for a postdoc with some experience (between 3 and 12 years after the PhD) on a long-term position (5-10 years).
The candidate is to work on the BISTRO-project: 'The influence of binary stars on stellar and Galactic evolution, as revealed by current and large surveys' | | ▸ more | In the first two years the activities of the researcher will be dedicated to developing an automated spectral fitting package using machine-learning techniques relying on artificial neural networks for the study of single stars and multiple systems in current and future large spectral surveys.
For more details on the project and how to apply, see http://aa.oma.be/Jobs
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| Post-Doctoral Position in Radio Astronomy SAASST | Closing date: 2021-12-31
Contact: Prof. Ilias Fernini |
| We are looking for an individual to join our research laboratory as a postdoctoral researcher. Technical mastery of radio interferometry techniques is a must, as well as a good publication record. The candidate with complementary skills to our research portfolio are especially encouraged to apply. The appointee will be expected to help build a 1-km radio interferometer and collaborate closely with other researchers. SAASST and the Department for Applied Physics and Astronomy offer the opportunity for the candidate to supervise students in the MSc in Astronomy and Space Sciences. | | ▸ more | The Sharjah Academy for Astronomy, Space Sciences, and Technology (SAASST) is recruiting a qualified individual for a postdoctoral appointment in radio astronomy. This position is based in the Radio Astronomy Laboratory led by Prof. Ilias Fernini.
The research laboratory has a broad research portfolio. Key research topics focus on the investigation of AGN, GRS (Giant Radio Sources), Sun observations, Jupiter observation, and Hydrogen line observation. The SAASST Radio Astronomy Laboratory operates two main systems: (1) A Decametric Radio Array that works at 20 MHz, and (2) a 40-m Radio Interferometer that works at 1.4 GHz.
We are looking for an individual to join our research laboratory as a postdoctoral researcher. Technical mastery of radio interferometry techniques is a must, as well as a good publication record. The candidate with complementary skills to our research portfolio are especially encouraged to apply. The appointee will be expected to help build a 1-km radio interferometer and collaborate closely with other researchers. SAASST and the Department for Applied Physics and Astronomy offer the opportunity for the candidate to supervise students in the MSc in Astronomy and Space Sciences.
Interested and qualified individuals are encouraged to apply by submitting curriculum vitae, list of publications, research interests, and have three letters of recommendation sent to Prof. Ilias Fernini (ifernini @ sharjah.ac.ae).
Included Benefits:
The initial appointment is for one year, and renewed every year based on the performance. The incentives are within the bylaws of the University of Sharjah and are as follows: (1) a monthly salary of 16,000 AED, (2) an extra 2,000 AED per month for housing, (3) free medical insurance, and (4) a one time flight ticket. (1 USD ~ 3.67 AED)
For more information about SAASST, please check the following link: www.saasst.ae
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