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EAS Job Directory
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| Postdoctoral Position in the Astronomical Institute of the Czech Academy of Sciences | Closing date: 2021-07-31
Contact: Michal Dovciak |
| Astronomical Institute (http://www.asu.cas.cz/en/about/about-the-institute) of the Academy of Sciences of the Czech Republic announces a 2-year postdoctoral position, starting in October this year, in the Relativistic Astrophysics group (https://astro.cas.cz/) in the project "Accreting black holes in the new era of X-ray polarimetry missions" (https://astro.cas.cz/expro). | | ▸ more | The postdoc will model the emission of the X-ray corona in Galactic black holes in X-ray binary sources, i.e. study the spectral, timing, and polarimetric properties of the X-ray corona emission. To this aim he/she will use, modify and create numerical codes developed in our group. Thus experience with C++ and Python computer languages is needed. Some experience with astronomical data analysis in X-ray domain (using XSPEC or similar software) and knowledge of relativistic astrophysics (especially in the field of accretion theory, radiative processes, ray-tracing in curved space-time) will be appreciated. High motivation and ability to work independently as well as in the team collaboration are expected.
The position is opened for 1 year, after which it can be prolonged for another year based on applicant's successful performance. The salary will be based on the domestic level and it includes full health insurance. Commencement is expected on the 1st of October 2021.
Applications containing a Cover Letter, a Curriculum Vitae, a List of Publications, and a Summary of Research Plans should be submitted in a single pdf
to: dovciak (at) asu.cas.cz
subject: EXPRO-ABH postdoc 2021 - Prague
Two recommendation letters have to be sent to the same email addresses with the same subject.
The successful candidate must hold a PhD degree in the field and present a certificate of that by the date of employment. Preferences will be given to early-stage researchers. A necessary condition for the appointment is to satisfy the legal requirements for being employed in the Czech Republic.
To receive full consideration please submit your application and arrange your recommendation letters to be sent by the 31st of July 2021. Applications will be acknowledged by email. Once the selection process is completed, the successful applicant will be notified.
Further information:
http://www.asu.cas.cz for details on our Institute
http://www.euraxess.cz for details about the research employment and work
conditions in Czech Republic.
https://www.numbeo.com/cost-of-living/comparison.jsp to compare cost of living.
Note: Please understand that the COVID-19 challenge may prevent us from admitting applicants from some regions because of legal or travel restrictions related to the current medical situation in the world.
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| Senior Analyst - Her Majesty?s Nautical Almanac Office | Closing date: 2021-07-04
Contact: Adam Gray |
| A unique opportunity to combine your strong analytical skills with a passion for astronomy/navigation. We are seeking a Senior Analyst to support the delivery of Her Majesty's Nautical Office (HMNAO) product portfolio, spanning astronomical and celestial navigation and astronomical data. | | ▸ more | A unique opportunity to combine your strong analytical skills with a passion for astronomy/navigation. We are seeking a Senior Analyst to support the delivery of Her Majesty's Nautical Office (HMNAO) product portfolio, spanning astronomical and celestial navigation and astronomical data.
About UKHO
UKHO is an executive agency, sponsored by the Ministry of Defence. We work with a wide range of data partners to chart the world's oceans in order to develop and serve world leading software and data solutions to commercial shipping companies, navies and maritime organisations. Our products ensure safe navigation and global trade efficiency and support other marine activities including economic development, environmental protection, resource exploration and utilisation, scientific research and security and defence.
Her Majesty?s Nautical Almanac Office (HMNAO) ? sits within UKHO?s Operations Division?s Scientific Analysis Group. HMNAO is a specialist team whose purpose is to provide solutions to astronomical and celestial navigation problems and to provide astronomical data to a wide variety of customers, both military and civil, including the public.
The role
The purpose of this post is to support the delivery of the HMNAO product portfolio schedule. You will be responsible for:
? Analysing astronomical data and producing almanacs and other publications/web content/software in support of customers of HMNAO products and services.
? Supporting Technical Leads, in software development and documentation for HMNAO products and services (e.g. Publication software, NavPac)
? Developing and maintaining close working relationship with the United States Naval Observatory (USNO)
? Participating in the work of the IAU (International Astronomical Union).
What we are looking for
If you have a passion for astronomy/navigation and thrive on working in a small, close-knit technical team, then this could be the role for you.
We are looking for candidates who have the tenacity to analyse large volumes of numerical data and the ability to work with a high level of attention to detail to ensure a consistent and accurate output. You will have a degree/postgraduate qualification level, or equivalent experience, in mathematics (e.g. numerical analysis, vector/matrix manipulation) or physics related discipline and will be computer literate with experience of programming languages (e.g. Fortran, Python etc.).
And in return?
UKHO is a great place in which to explore your career potential and offers a wealth of training and development opportunities. While our projects are career-defining, the work/life balance that we can offer you is equally exceptional. From flexitime, flexible working, an award-winning office environment, wellbeing schemes, a generous annual leave allowance, and access to MOD and Civil service discounts, the opportunities open to you here are hard to beat.
For a full job description, including the competencies you will be assessed on in your application, please visit: https://www.civilservicejobs.service.gov.uk/csr/jobs.cgi?jcode=1727061 .
Closing date: 23:55 4 July 2021.
Selection for appointment to the Civil Service is on merit, on the basis of fair and open competition, as outlined in the Civil Service Commission?s Recruitment Principles.
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| Industry-Academic PhD position in data fusion | Closing date: 2021-06-28
Contact: Nick Cox |
Joint PhD position with ACRI-ST (Grasse, France) and the Institute d'Astrophysique Spatiale (Paris, France).
The objective of this PhD research is to develop, optimize, and implement state-of-the-art machine learning data fusion tools for the Sentinel 2 and 3 missions of the European Copernicus programme and the James Webb Space Telescope. | | ▸ more | Space missions for astronomical or Earth observations now carry multiple spectro-imaging instruments. A main challenge for their exploitation is the combination of data sets from different instruments to produce quality images and spectra. The focus of this project is to develop data fusion tools for the Sentinels 2 and 3 missions from the EU Copernicus program. This will then also be applied to the JWST Mid-InfraRed Instrument (MIRI).
- The European Copernicus programme is the most ambitious Earth observation program in the world, providing satellite data to improve environmental management, understand and mitigate the effects of climate change, and ensure civil security. To achieve this ESA is developing and operating the Sentinels satellites, which are equipped with a wide range of instruments for monitoring the Earth, oceans and atmosphere.
- The James Webb Space Telescope (launch 2021) will be the major space observatory of the next decade accessible to the world community and will enable considerable progress to be made on the biggest questions in astrophysics: the first lights of the Universe, the birth of stars and planets, the origins of life, etc.
The goal of this project is to use neural networks or similar techniques to reconstruct spectral images from incomplete spatial and/or spectral data, especially for observations where each pixel contains information from different sources. For instance, be able to reproduce the high spatial resolution of Sentinel 2 using Sentinel 3 images, as well as to reconstruct the high spectral information from Sentinel 3 for Sentinel 2 images. Similarly, for JWST the goal is to reconstruct the high spectral information, from the MIRI spectrograph using the MIRI imager.
Context and Supervision
The project is part of an ANR LabCom project that combines the expertise in imagery+spectroscopy and A.I.+inverse problem solutions of ACRI-ST and the Institut d'Astrophysique Spatiale (IAS). This project includes about 20 people from both institutions and started in May 2021.
The PhD is framed in the context of a French CIFRE agreement (convention industrielle de formation par la recherche) between ACRI-ST and the IAS and will follow CIFRE remuneration guidelines. The candidate will be based at ACRI-ST and obtain a PhD from the Université Paris-Saclay to which the IAS belongs. The student will be located in the recently inaugurated site at CERGA (Grasse, south of France) which hosts the activities in astrophysics and New Space of ACRI-ST, and it is close to its headquarters in Sophia-Antipolis. It is expected that the student will interact actively with the IAS.
Sentinel 2 and 3 data is readily available thanks to ACRI-ST participation to the ground-segment of these missions. Both ACRI-ST and the IAS are part of an awarded JWST Early Release Program, which data will be used for the project.
Profile PhD candidate
The applicant should have an MSc related to computer/data science or physical sciences and be familiar with some of the following:
- Coding (python)
- Machine Learning / Deep Learning
- Remote sensing (space) observations (either Earth Observations or astrophysics)
Desired skills
- Inquisitive, analytical, and critical thinker
- Independent mindset
- Strong communication skills
- Good level of English (oral and written)
How to Apply?
Send a CV, a letter of motivation, and arrange a reference/s to be sent to Dr. Jeronimo Bernard-Salas
(jeronimo.bernard-salas @ acri-st.fr) and do not hesitate in contacting him for more information on the
position.
Applications received by June 28th will be fully considered. Position is open until filled. Expected start is
in fall 2021 (September/October).
For more details on this position please visit https://astro.acri-st.fr/?page_id=116
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| POSTDOCTORAL RESEARCH FELLOW IN OPTICAL ASTRONOMY | Closing date: 2021-07-31
Contact: Manuel Linares |
We welcome applications for one postdoctoral research fellow position at the Department of Physics of the Norwegian University of Science and Technology (NTNU).
The position has a duration of two years, with a possible extension to a third year contingent on the performance of the selected candidate (a fourth year may also be possible, depending on the availability of funds). Longer extensions might be possible if the researcher succeeds at securing independent funds/positions, through competitive national/international calls.
The expected start date is January 2022. | | ▸ more | The selected candidate will join a growing and multifaceted research team funded by the H2020 ERC Consolidator Grant LOVE-NEST (PI: M. Linares). The main focus of the ERC team is the study of compact binary millisecond pulsars, which has an impact on a broad range of science topics (including super-massive neutron stars, nuclear physics, gravitational wave astronomy, cosmic rays, accretion flows and pulsar winds).
The position is based in Trondheim: a vibrant multicultural city surrounded by beautiful landscapes and the third largest municipality in Norway (renowned as its technological capital). NTNU is the largest University in the country and provides excellent working conditions.
About the group:
The Astrophysics and Particle Physics (APP) Group carries out research in high-energy astrophysics, astroparticle physics and multi-wavelength astronomy, as well as particle physics. Its current scientific interests include compact objects, cosmic ray production, transport and detection, astrophysical neutrinos, active galactic nuclei and quantum chromodynamics.
The APP Group is part of the Department of Physics, which currently employs about 160 people. On average some 2000 NTNU students follow courses at the Department of Physics every year.
Duties of the position:
The postdoctoral research fellow will work on topics related to compact binary millisecond pulsars (aka 'spiders') within the LOVE-NEST team. She or he is expected to carry out an independent research program, and to contribute to the design, analysis and interpretation of ground-based optical observations of spiders and related systems.
Required selection criteria:
-A PhD in Astronomy or Astrophysics (by the start date of the position)
-Published experience in observational optical astronomy (photometry and/or spectroscopy)
-A strong publication record in high-impact journals
-Fluent English communication, written and oral.
Preferred selection criteria:
-Demonstrated hands-on experience in ground-based astronomical observations
-Demonstrated experience in student supervision (at the MSc and/or PhD level)
-Proven knowledge of astronomical software for optical data analysis (IRAF/PyRAF, Astropy, SIMBAD, Starlink)
Personal characteristics:
-Enthusiasm for science
-Independent
-Social and collaborative skills (ability to work in a team and contribute to its success)
-Systematic
We offer:
-Exciting and stimulating tasks in a strong international?academic environment
-An open and?inclusive work environment with dedicated colleagues
-Favourable terms in the Norwegian Public Service Pension Fund
-Employee benefits
-Ample budget for travel, computing equipment and other work expenses
-Access to the computer cluster at the Department of Physics
-Access to telescope time through dedicated ERC funds and the Nordic Optical Telescope
-Possibility to officially co-supervise PhD theses
Salary and conditions:
As a Postdoctoral Fellow (code 1352) you are normally paid from gross NOK 545?300 per annum before tax. From the salary, 2% is deducted as a contribution to the Norwegian Public Service Pension Fund.
The position has a duration of two years, with a possible extension to a third year contingent on the performance of the selected candidate (a fourth year may also be possible, depending on the availability of funds).
About the application:
The application and supporting documentation to be used as the basis for the assessment must be in English.
Publications and other scientific work must follow the application. Please note that applications are only evaluated based on the information available on the application deadline. You should ensure that your application shows clearly how your skills and experience meet the criteria which are set out above.?
If, for any reason, you have taken a career break or have had an atypical career and wish to disclose this in your application, the selection committee will take this into account, recognizing that the quantity of your research may be reduced as a result.
The application must include:
-Cover letter (summarize your background and motivation to apply; max. 1p)
-CV (max. 4p; and the most important certificates/diplomas, with English translation when necessary)
-List of publications (briefly describe your contribution in the case of large collaborations; max. 4p)
-Two reference letters sent directly by the academic references to Manuel.Linares @ ntnu.no
If you have any questions about the position, please contact Professor Manuel Linares (Manuel.Linares @ ntnu.no). If you have any questions about the recruitment process, please contact Magnus Gautvik (Magnus.Gautvik @ ntnu.no).
Application deadline: 31.07.21
For full details and application see:
https://www.jobbnorge.no/en/available-jobs/job/207138/postdoctoral-research-fellow-in-optical-astronomy
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| PhD POSITION IN OPTICAL STUDIES OF BINARY MILLISECOND PULSARS | Closing date: 2021-07-31
Contact: Manuel Linares |
We welcome applications for one PhD position at the Department of Physics of the Norwegian University of Science and Technology (NTNU).
The position has a duration of three years, with a possible extension to a fourth year contingent on availability and optional teaching duties. The expected start date is January 2022.
| | ▸ more | The selected candidate will join a growing and multifaceted research team funded by the H2020 ERC Consolidator Grant LOVE-NEST (PI: M. Linares). The main focus of the ERC team is the study of compact binary millisecond pulsars, which has an impact on a broad range of science topics (including super-massive neutron stars, nuclear physics, gravitational wave astronomy, cosmic rays, accretion flows and pulsar winds).
The position is based in Trondheim: a vibrant multicultural city surrounded by beautiful landscapes and the third largest municipality in Norway (renowned as its technological capital). NTNU is the largest University in the country and provides excellent working conditions.
About the group:
The Astrophysics and Particle Physics (APP) Group carries out research in high-energy astrophysics, astroparticle physics and multi-wavelength astronomy, as well as particle physics. Its current scientific interests include compact objects, cosmic ray production, transport and detection, astrophysical neutrinos, active galactic nuclei and quantum chromodynamics.
The APP Group is part of the Department of Physics, which currently employs about 160 people. On average some 2000 NTNU students follow courses at the Department of Physics every year.
Duties of the position:
The PhD candidate will work on topics related to compact binary millisecond pulsars (aka 'spiders') within the LOVE-NEST team. She or he is expected to implement, analyze and capitalize a large ground-based optical survey of spiders and related systems.
Required selection criteria:
-A MSc in Astronomy or Astrophysics (by the start date of the position)
-Experience in observational optical astronomy (photometry)
-Your education must correspond to a five-year Norwegian degree programme, where 120 credits are obtained at master's level
-You must have a strong academic background from your previous studies and an average grade from the master's degree program, or equivalent education, which is equal to B or better compared with NTNU's grading scale. If you do not have letter grades from previous studies, you must have an equally good academic basis. If you have a weaker grade background, you may be assessed if you can document that you are particularly suitable for a PhD education.
-You must meet the requirements for admission to the faculty's doctoral program (https://www.ntnu.edu/studies/phfy)
-Fluent English communication,written and oral.
Preferred selection criteria:
-Hands-on experience in ground-based astronomical observations
-Published experience in optical surveys and photometry
-Knowledge of astronomical software for optical data analysis (IRAF/PyRAF, Astropy, SIMBAD, Starlink)
Personal characteristics:
-Enthusiasm for science
-Independent
-Social and collaborative skills (ability to work in a team and contribute to its success)
-Systematic
We offer:
-Exciting and stimulating tasks in a strong international academic environment
-An open and inclusive work environment with dedicated colleagues
-Favourable terms in the Norwegian Public Service Pension Fund
-Employee benefits
-Ample budget for travel, computing equipment and other work expenses
-Access to the computer cluster at the Department of Physics
-Access to telescope time through dedicated ERC funds and the Nordic Optical Telescope
Salary and conditions:
PhD candidates are remunerated in code 1017, and are normally remunerated at gross from NOK 482 200 per annum before tax. From the salary, 2% is deducted as a contribution to the Norwegian Public Service Pension Fund.
The period of employment is 3 years with a possible extension to a fourth year contingent on availability and optional teaching duties.
About the application:
The application and supporting documentation to be used as the basis for the assessment must be in English.
Publications and other scientific work must follow the application. Please note that applications are only evaluated based on the information available on the application deadline. You should ensure that your application shows clearly how your skills and experience meet the criteria which are set out above.
The application must include:
-Cover letter (summarize your background and motivation to apply; max. 1p)
-CV (max. 4p; and the most important certificates/diplomas, with English translation when necessary)
-List of publications (briefly describe your contribution in the case of large collaborations; max. 4p)
-Two reference letters sent directly by the academic references to Manuel.Linares @ ntnu.no
If you have any questions about the position, please contact Professor Manuel Linares (Manuel.Linares @ ntnu.no). If you have any questions about the recruitment process, please contact Magnus Gautvik (Magnus.Gautvik @ ntnu.no).
Application deadline: 31.07.2021
For full details and application see:
https://www.jobbnorge.no/en/available-jobs/job/207154/phd-position-in-optical-studies-of-binary-millisecond-pulsars
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| SCIENCE SOFTWARE ENGINEER | Closing date: 2021-07-31
Contact: Manuel Linares |
We welcome applications for one science software engineer (senior engineer) position at the Department of Physics of the Norwegian University of Science and Technology (NTNU).
The selected candidate will join a growing and multifaceted research team funded by the H2020 ERC Consolidator Grant LOVE-NEST (PI: M. Linares). The main focus of the ERC team is the study of compact binary millisecond pulsars.
The position is permanent, with the first four years funded by the ERC Consolidator Grant and the following years funded by the Department of Physics.
The expected start date is December 2021. | | ▸ more | About the group and department:
The Astrophysics and Particle Physics (APP) Group carries out research in high-energy astrophysics, astroparticle physics and multi-wavelength astronomy, as well as particle physics. Its current scientific interests include compact objects, cosmic ray production, transport and detection, astrophysical neutrinos, active galactic nuclei and quantum chromodynamics.
The APP Group is part of the Department of Physics, which currently employs about 160 people. Its central research areas are materials science, nanoscience, surface physics, modern optics, astrophysics, solar energy, biophysics, and medical technology. Research staff at the Department make a special effort to increase the awareness and understanding of the importance and impact of physics in our society. On average some 2000 NTNU students follow courses at the Department of Physics every year.
Duties of the position:
The science software engineer will actively support the research personnel in coding, setting up, running, debugging, optimizing and parallelizing scientific software.
During the first four years the engineer will spend most of the work time on topics related to compact binary millisecond pulsars (aka 'spiders'), within the LOVE-NEST team.The engineer is expected to contribute to the development of numerical simulations and computer models to tackle a number of scientific problems from a computational perspective.
Required selection criteria:
-MSc in Astronomy/Astrophysics, Physics, Mathematics or Computer Science.
-Proficient and documented knowledge of programming languages (C++, Fortran, Python, shell scripting)
-Proven Linux system management/administration skills
-Excellent oral and written communication skills in English
Preferred selection criteria:
-PhD in Astronomy/Astrophysics, Physics, Mathematics or Computer Science.
-A good publication record in Astronomy and Astrophysics
-Experience in use/development of numerical simulation codes (MHD, SPH)
-Experience in development of science visualization or Astronomical codes (AstroPy, IDL)
Personal characteristics:
-Enthusiasm for science
-Independent
-Social and collaborative skills (ability to work in a team and contribute to its success)
-Systematic
In the evaluation of which candidate is best qualified, emphasis will be placed on education, experience and personal suitability, as well as motivation, in terms of the qualification requirements specified in the advertisement
We offer:
-exciting and stimulating tasks in a strong international academic environment
-an open and inclusive work environment with dedicated colleagues
-favourable terms in the Norwegian Public Service Pension Fund
-employee benefits
-ample budget for travel, computing equipment and other work expenses
-access to the computer cluster at the Department of Physics
-possibility to take part in the scientific research of the Department of Physics
Salary and conditions:
The gross salary for the position of Senior Engineer code 1181 is remunerated according to the Norwegian State salary scale, depending on qualifications and seniority.From the salary, 2 % is deducted as a contribution to the Norwegian Public Service Pension Fund.
The engagement is to be made in accordance with the regulations in force concerning State Employees and Civil Servants, and the acts
relating to Control of the Export of Strategic Goods, Services and Technology. Candidates who by assessment of the application and
attachment are seen to conflict with the criteria's in the latter law will be prohibited from recruitment to NTNU. After the appointment you must assume that there may be changes in the area of work.
About the application:
Please note that the application will only be evaluated on the basis of the information available at the expiry of the application deadline. Therefore, make sure that your application clearly shows how your skills and experience meet the criteria described above.
The application must contain:
-CV, certificates and diplomas
-Name and adress of three references
-List of publications
If you have any questions about the position, please contact Professor Manuel Linares (Manuel.Linares @ ntnu.no). If you have any questions about the recruitment process, please contact Magnus Gautvik (Magnus.Gautvik @ ntnu.no).
Application deadline: 31.07.2021
For full details and application see:
https://www.jobbnorge.no/en/available-jobs/job/206784/science-software-engineer-position
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| Associate Professor in Radio Astronomy at Trinity College Dublin | Closing date: 2021-07-05
Contact: Colm Stephens |
The School of Physics at Trinity College Dublin invites applications for a position at the level of Associate Professor in Radio Astronomy. We seek motivated individuals with a strong potential to enhance astrophysics research and teaching at Trinity, in particular to fully exploit the opportunities arising from Ireland?s recent membership of the European Southern Observatory (ESO), continued membership of European Space Agency (ESA), and Trinity?s leading role in the Irish Low-Frequency Array (I-LOFAR).
| | ▸ more | Visit our website at https://www.tcd.ie/Physics/ for more information on the School of Physics and Trinity College Dublin.
More information on the position, including the detailed job description, as well as the application process can be found at https://my.corehr.com/pls/trrecruit/erq_jobspec_details_form.jobspec?p_id=035069
Informal queries about the post should be made to the Head of School, Prof. Jonathan Coleman. Please make contact via the School Manager, Dr. Colm Stephens, colm.stephens @ tcd.ie, who will coordinate these enquiries.
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| Assistant Professor in Astrophysics at Trinity College Dublin | Closing date: 2021-07-05
Contact: Colm Stephens |
The School of Physics at Trinity College Dublin invites applications for a position at the level of Assistant Professor in the field of observational or theoretical astrophysics. We seek motivated individuals with a strong potential to enhance astrophysics research and teaching at Trinity, in particular related to Ireland's recent membership of the European Southern Observatory (ESO), continued membership of the European Space Agency (ESA), and Trinity?s leading role in the Irish Low-Frequency Array (I-LOFAR) project.
| | ▸ more | Visit our website at https://www.tcd.ie/Physics/ for more information on the School of Physics and Trinity College Dublin.
More information on the position, including the detailed job description, as well as the application process, can be found at https://my.corehr.com/pls/trrecruit/erq_jobspec_details_form.jobspec?p_id=035068
Informal queries about the post should be made to the Head of School, Prof. Jonathan Coleman. Please make contact via the School Manager, Dr. Colm Stephens, colm.stephens @ tcd.ie, who will coordinate these enquiries.
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| H2020 SPACE NEMESIS postdoctoral position at Konkoly Observatory, Budapest | Closing date: 2021-06-30
Contact: Gabor Marton |
| We invite applications for a postdoctoral position at Konkoly Observatory as part of NEMESIS, a collaborative H2020 project between the University of Vienna, University of Geneva, and Konkoly Observatory. NEMESIS has the ambition to reshape our understanding on the formation of stars by employing artificial intelligence methods to compile and interpret the largest, panchromatic data collection of young stellar objects. | | ▸ more | The successful candidates should have a solid background in at least one of the following topics: star formation, classification of young stellar objects, application of machine learning techniques in large datasets.
Tasks will include processing of photometric and time domain data (mostly from the Herschel Space Observatory, but also from other IR and optical satellites/telescopes), collecting data, building training samples for supervised classification, regression, also unsupervised analysis of the available parameters of Young Stellar Objects. Programming skills in R and/or Python are advantageous.
The successful candidate will work with Dr. Gábor Marton at Konkoly Observatory (the Astronomical Institute of the Research Centre for Astronomy and Earth Sciences, which belongs to the Eötvös Loránd Research Network) in Budapest, Hungary, however candidates are expected to spend extended working visits at the other participating institutes. At Konkoly Observatory he/she will find a rich and vibrant research environment in the fields of extra-solar planets, solar and stellar physics, astrophysical and geochemical laboratory, nuclear and extragalactic astrophysics. Konkoly Observatory is Hungary's largest astronomical institute, located in a newly renovated building in a beautiful natural reserve area, half hour from the city center. The observatory has been dynamically expanding in recent years, including two ERC-funded projects and several international staff members. The observatory maintains telescopes at a Hungarian mountain station and astronomers regularly observe with international instrumentation as well.
The initial appointment will be for one year, renewable annually, contingent upon satisfactory performance, mutual agreement, and availability of funds. The appointments are expected to start as soon as possible but no later than end 2021, and require the completion of a PhD in Astronomy, or related field.
To apply, qualified candidates are encouraged to send an email with a single PDF file to marton.gabor @ csfk.org containing:
ˇ Cover letter
ˇ CV
ˇ Statement outlining any research experience so far
ˇ copy of PhD and a brief research statement
ˇ Candidates should also provide the names, addresses, phone numbers, and e-mail addresses of two or three reference persons.
Applications received by June 30, 2021, will receive full consideration, but the call will remain open until the position is filled.
The net salary of the postdoc will be around ~400K HUF/month. Apartments in Budapest are in the range of 100-150k HUF/month depending on needs.
Preliminary inquiries may be addressed via e-mail to marton.gabor @ csfk.org. For more information on Konkoly Observatory, please visit: https://konkoly.hu/ and on NEMESIS: https://nemesis.univie.ac.at/
Included Benefits:
The Eötvös Loránd Research Network is an Equal Opportunity Employer. The postdoc will be a state employee and will have access to the Hungarian public health system.
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| Visiting Research Fellow | Closing date: 2021-07-14
Contact: Jiri Svoboda |
| The Astronomical Institute of the Czech Academy of Sciences invites applications for an 8-month full-time Visiting Research Fellow program to study star-forming compact galaxies that exhibit possible signatures of active galactic nuclei. | | ▸ more | Our scientific goals are to better understand the role of star-forming galaxies in the Epoch of Re-Ionization and to characterize accretion processes around intermediate-mass black holes as possible precursors to super-massive black holes hosted in large galaxies.
We were recently awarded new observations of so-called ?Blueberry" and "Green Pea? galaxies with the VLA and XMM-Newton. Thus, we are looking for a candidate who is very experienced with radio interferometry, UV photometry/imaging and/or X-ray spectral analysis of faint targets. Our project provides a highly-competitive salary above the standards in Czechia for a postdoctoral researcher (about 48,000 CZK net salary). After this 8-month long project, it may be possible to prolong the stay of a postdoctoral researcher dependent upon the result of pre-submitted funding applications.
To apply, please send a motivation letter and CV to jiri.svoboda @ asu.cas.cz before July 14, 2021. Please also ensure two letters of recommendation.
Expected start of the project: September 2021
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| Temporary senior scientist position, University of Vienna | Closing date: 2021-06-08
Contact: Manuel Guedel |
| The University of Vienna, Department of Astrophysics, offers a temporary senior scientist position; the position is vacant for the period of absence of a member of staff, until 26 February 2022. We seek an outstanding scientist working in the field of stellar activity with interest in star-planet interactions. Further activities include teaching. | | ▸ more |
Job Description:
The tasks conform to the collective agreement of the universities §26(2) and (5); they comprise as the main activities:
1) Scientific work within project participations in the framework of international co-operations, and/or direct scientific involvement in these projects (e.g., in working groups, science teams, access to observations). Space missions in which such participation is possible include PLATO, ARIEL, SMILE, and Athena.
2) Research within the research focus "planetary habitability" of the star and planet formation group of Univ.-Prof. Dr. Manuel Guedel, including topics related to stellar magnetic activity, flares, and radiation in the context of star-planet interactions. This also includes support for related organisational and administrative matters (budgets, organisation of meetings).
Further tasks include,
3) conducting independent teaching as defined by the collective agreement and organising exams
4) supervision/co-supervision of students
5) contributions to general organisational and administrative tasks as well as evaluation procedures
The specific tasks can be adjusted to ongoing and new projects.
Profile:
- doctoral degree in astronomy or astrophysics
- several years of experience in astrophysical research and in large astronomical projects - knowledge of programming languages, e.g. Fortran, C, C++, Python, etc.
- excellent command of written and spoken English
- good team-working ability
- excellent communication skills
- experience in student supervision
Applications should include a motivation letter, a CV, a publication list, a summary of past research (max. 1 page), and a description of proposed research (max. 1 page). They should be submitted via the Job Center to the University of Vienna (http://jobcenter.univie.ac.at) no later than 08 June 2021, mentioning reference number 12042.
For further information please contact Manuel Guedel, manuel.guedel @ univie.ac.at.
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.
Extent of Employment: 40 hours/week
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.
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| PhD position at CFT, Warsaw, Poland | Closing date: 2021-06-15
Contact: Bozena Czerny |
| We invite applications for PhD fellowship at the CFT PAN. We search for candidates interested in the research in the domain of astrophysics. Candidates with previous experience in AGN observational data analysis, and in programming are particularly welcome. The positionis financed from the project 'Constraints on the dark energy properties based on observations of active galaxies'. PI of the project is Prof. Bozena Czerny. Application should be submitted before June 15 2021. | | ▸ more | The Director of the Center for Theoretical Physics, Polish Academy of Sciences invites applications for PhD fellowship at the CTP PAS (CFT PAN in Polish), financed from the project 'Constraints on the dark energy properties based on observations of active galaxies', National Science Center (NCN), decision Nr DEC-2017/26/A/ST9/00756, project No. 2017/26/A/ST9/00756 (MAESTRO 9). PI of the project is Prof. Bo?ena Czerny.
At the time of application the candidates should either have a MSc degree in physics or astronomy, or will obtain it before signing the contract. We search for candidates interested in the research in the domain of astrophysics. Candidates with previous experience in AGN observational data analysis, and in programming are particularly welcome.
The topic of the student research will be focused on modeling continuum variability in active galaxies in different wavelength bands, including effects of the medium surrounding the accretion disk, predicting time delays between these bands, and finally using that to constrain the cosmological parameters. More information about the project is at http://old.cft.edu.pl/czerny2/en/project.html, or can be obtained directly from the project PI Bozena Czerny (bcz @ cft.edu.pl). The research will be done at the institute (CFT - Centrum Fizyki Teoretycznej PAN), but the PhD courses will be implemented as part of the "Geoplanet" Doctoral School (https://geoplanetschool.pl/home,2,en.html/). Recruitment to the School /project work is carried out by CFT.
Candidates should submit before June 15, 2021, the following documents to the Secretariat of the Center, at rekrutacja @ cft.edu.pl):
1. The scientific CV, including the list of major scientific achievements, list of publications, participation in research projects and conferences, and the document must contain a statement: ?I consent to the processing of my personal data for the needs of the recruitment process (in accordance with the Law dated 29.08.97 on the protection of personal data (Journal of Laws, No. 101, item 926)?.
2. Short motivation letter
3. Transcript of grades (Bachelor and Master degree courses)
4. Personal questionnaire form (should be downloaded from CTP web site)
5. At least one recommendation letter, including the letter from the MSc advisor
6. Certified copy of the MSc diploma or the letter from the supervisor about the prospects for completion of the Thesis before the beginning of the employment
The scholarship is awarded in accordance with the rules set out in the Regulations on granting scientific scholarships in research projects financed by the National Science Center, introduced by the resolution of the Council of the National Science Center no. 96/2016, dated 27/10/2016 r.). It will amount to PLN 4,500 gross per month (the amount may include a public law charge in accordance with applicable regulations, e.g. insurance).
Shortlisted candidates will be invited for an interview via video conferencing no later than 25 June 2021. The competition results will be announced by 5 July 2021. Candidates will be informed electronically about the results of the competition. Admission to the PhD School and work for the project are scheduled for 1 October 2021.
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| Postdoctoral position on modeling evolved massive stars | Closing date: 2021-06-10
Contact: Alceste Bonanos |
The National Observatory of Athens invites applications for 1 postdoctoral position on modeling evolved massive stars in nearby galaxies in the framework of the ERC consolidator grant titled ?Episodic Mass Loss in Massive Stars: Key to Understanding the Explosive Early Universe? (ASSESS). The aim of the program is to determine whether episodic mass loss is a dominant process in the evolution of the most massive stars. More details are available here:
https://www.astro.noa.gr/wp-content/uploads/2021/05/ERCadvert2021.pdf | | ▸ more | The National Observatory of Athens invites applications for 1 postdoctoral position on modeling evolved massive stars in nearby galaxies in the framework of the ERC consolidator grant titled ?Episodic Mass Loss in Massive Stars: Key to Understanding the Explosive Early Universe? (ASSESS). The aim of the program is to determine whether episodic mass loss is a dominant process in the evolution of the most massive stars.
Deadline: June 10, 2021
More details are available here:
https://www.astro.noa.gr/wp-content/uploads/2021/05/ERCadvert2021.pdf
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| Professor or Associate Professor in Physics | Closing date: 2021-06-23
Contact: Jan W. Thomsen |
| The Niels Bohr Institute announces the availability of a faculty position in physics. The position can be filled at the level of associate professor with tenure or professor with tenure depending on qualifications of the candidate. | | ▸ more | The Niels Bohr Institute announces the availability of a faculty position in physics. The position can be filled at the level of associate professor with tenure or professor with tenure depending on qualifications of the candidate.
- The candidate should have a research in profile in either computational methods in physics or in quantum information theory.
- Candidates within computational physics preferably have a research profile in one or more of the following areas, advanced statistical learning, algorithm development, numerical methods, or simulation-based inference.
- Candidates within quantum information theory preferably have experience with application and implementation of quantum information for quantum technology, quantum communication or quantum algorithms.
Relevant research activities at the Niels Bohr Institute can be found within Astrophysics (including Planetary Sciences and Cosmology); Biophysics and Biocomplexity; Condensed Matter and Quantum Physics, Geophysics (including Ice, Climate, and Earth Sciences); High Energy and Astro-particle Physics and in the Center for Quantum Devices (qdev.dk); quantum optics theory group (tqo.dk), the Quantum Photonics Center (hy-q.nbi.ku.dk), and the Quantum Optics Center (quantop.nbi.ku.dk). Related activities can further be found in the Center for the Mathematics of Quantum Theory (qmath.ku.dk/).
The successful candidate must be an outstanding scientist who has already had significant international impact on research and who has demonstrated: (1) the talent and vision to define an independent research program, (2) the scientific maturity to establish an independent research group, and (3) the ability to attract significant external funding in open competition at national and international levels. The successful candidate is expected to collaborate both internationally and within University of Copenhagen on research questions of broad-scale relevance and should preferably have experience from leading an internationally recognized research program.
The deadline for applications is June 23, 2021, 23:59 GMT +2.
<< Read more and apply the position here >>
Part of the International Alliance of Research Universities (IARU), and among Europe’s top-ranking universities, the University of Copenhagen promotes research and teaching of the highest international standard. Rich in tradition and modern in outlook, the University gives students and staff the opportunity to cultivate their talent in an ambitious and informal environment. An effective organisation – with good working conditions and a collaborative work culture – creates the ideal framework for a successful academic career.
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| Postdoctoral Researcher in Radio Astronomy Simulations | Closing date: 2021-08-31
Contact: Claire Taylor |
At the SKAO we are coordinating a global effort to deliver one fo the largest science facilities on the planet. The SKAO telescopes will be next-generation instruments that will help to answer key questions in astrophysics, drive technological innovation and support human capital development.
A unique opportunity for a Postdoctoral research position in Radio Astronomy Simulations.
To found out more and to apply : https://recruitment.skatelescope.org/vacancy/postdoctoral-researcher-in-radio-astronomy-simulations-440429.html
| | ▸ more | The Role
The successful candidate will play a major part in developing solutions for the SKA Science Data Challenge in collaboration with existing Science and Operations team members. This initiative aims to release with a regular cadence increasingly realistic simulated SKA datasets and data products to the international scientific user community, together with a specific data analysis exercise for them to solve (the “challenge”) and a set of tools and services to support the completion of the exercise and the evaluation of the results.
The post holder will report to the SKA Project Scientist and be responsible for the coordination of the SKA Science Data Challenges.
The role is a 3-year fixed term contract. Full-time hours will be 35 hours per week and flexible working may be considered compatible with reviews, milestones and office activities.
Key Responsibilities, Accountabilities and Duties
Development of radio astronomy simulations of SKA data products using existing packages and code as well as customised packages and code in collaboration with the SKAO Science and Operations teams;
Development of astrophysical sky models for use in radio astronomy simulations in consultation with the SKA user community;
Development and maintenance of tools to support the challenge progression (e.g. data challenge website, community forum, evaluation procedures);
Publication of data challenges outcomes in major astronomical journals;
Installation and maintenance of astronomy packages and software in a Linux cluster environment;
The role will provide the opportunity for 25 percent independent research.
Mandatory Knowledge, Skills and Experience
A PhD or equivalent in Astronomy, Physics or a closely related field;
Significant familiarity with the major calibration and imaging packages used in Radio Astronomy (AIPS, Miriad, CASA);
Significant familiarity with the underlying algorithms used in calibration and imaging in Radio Astronomy;
Experience with installation, maintenance and customisation of astronomical software packages in a Linux/Unix/MacOSX environment;
Experience with Python Scripting;
A flexible team player who is adaptable to change.
Desirable Knowledge, Skills and Experience
Knowledge of Software development including Version control/code collaboration tools (e.g. Git, Mercurial);
Knowledge of Open science and FAIR principles;
Knowledge of Code Optimization for multi-processor CPUs and/or GPUs.
Equality Diversity and Inclusion Statement
SKA Observatory recognises that our diversity is a strength. We aim to create a welcoming and inclusive environment where everyone feels they belong, and diverse perspectives and ideas thrive. As such, Equality, Diversity, and Inclusion are at the core of SKA Observatory?s agenda.
Our aim to is recruit and retain the most talented individuals, regardless of gender, race, disability, age, sexual orientation, marital status, religion, nationality or background.
Women have traditionally been under-represented in the fields of science and engineering; SKA Observatory welcomes and encourages female applicants.
Where applicants with a disability need facilities or adjustments to enable them to participate in the recruitment process, these will be provided.
SKA Observatory welcome all candidates, especially those from member countries.
The ?How to Apply? information contained within the SKA Observatory recruitment portal provides more detail regarding our application and selection approach.
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| Executive Director, Canada-France-Hawaii Telescope Corporation | Closing date: 2021-07-15
Contact: Tracy Yost |
Applications are invited for the position of Executive Director of the Canada-France-Hawaii Telescope (CFHT).
To obtain more information and apply online, please visit https://cfht.applicantpro.com/jobs/1792182.html | | ▸ more | Located on Maunakea, Hawaii, the 3.6m CFHT has historically been a world leader in wide-field optical and near infrared imaging and, with the recently commissioned instruments SPIRou and SITELLE, now also plays important roles in the search for exoplanets around low-mass stars and the study of emission line objects in the nearby and distant universe. We are seeking an innovative and creative leader who, while maximizing the scientific output of the current instrumentation suite, will usher CFHT into a new era of scientific discoveries by taking a proactive role in the advancement of the Maunakea Spectroscopic Explorer (MSE), endorsed by the CFHT Partners and Board of Directors as the most scientifically impactful future redevelopment of the site. The new CFHT Executive Director will also represent CFHT within the Maunakea Observatories in all negotiations regarding the renewal of the Maunakea Master Lease and CFHT sublease.
CFHT has a staff of approximately 50 and operates with a US$8M annual budget. The Executive Director is appointed by the Board of the CFHT Corporation, a non-profit organization incorporated in the State of Hawaii. Current members of the Corporation are the National Research Council of Canada, the Centre National de la Recherche Scientifique of France, and the University of Hawaii. The Executive Director is responsible to the Board for managing all aspects of the Corporation, including the operation of the telescope, the implementation of the observatory's scientific and technical program, the appointment of personnel, the preparation of budgets, the administration of financial affairs, communications, and the negotiations of international agreements. The Executive Director is also responsible for pursuing extramural funding and potential associate partners, as directed by the Board.
Applicants must hold a Ph.D. in Astronomy or a closely related field, or equivalent combination of education and experience. The successful applicant will be committed to promote, within the Observatory, a diverse, inclusive environment and a sense of belonging, and to foster a culture of understanding and reconciliation with the native Hawaiian community. In addition, the following qualifications are considered desirable:
- Strong scientific leadership and an established record of research achievement;
- Successful experience in administration and management, including overseeing the technical and/or scientific enterprise of an observatory or other astronomy institute;
- Proven skills in institutional and international relations;
- Excellent interpersonal, communication and listening skills, and a proven record of effective communications with governing bodies, staff, funding agencies, local community, and the astronomical community at large;
- Proven ability to work collaboratively with diverse teams;
- Successful experience in acting as an ambassador on behalf of their organization and/or of the community at large;
- Experience with the development, procurement or deployment of new instrumentation.
The Executive Director is expected to reside on Hawaii Island, and to take office in the CFHT Headquarters located in Waimea (Kamuela). A competitive salary will be offered and the Corporation provides a comprehensive benefit package. The starting date for the position is negotiable, and could be as early as September 2021. The Executive Director term is five years and can be extended upon review.
Post Offer/Employment conditions: To comply with the requirement to work occasionally at the observatory's altitude of 4200 meters, the applicant must pass a post-offer high altitude medical exam. Documentation to verify eligibility for employment in the United States will have to be furnished at the start of work.
How to apply: All applicants must submit their application through our confidential online portal at https://cfht.applicantpro.com/jobs/ . The full position description may also be downloaded at that site. Applications should include a Cover Letter, a Curriculum Vitae, a statement on Equity, Diversity and Inclusion, and the names of at least three references who may be contacted for confidential evaluations. Review of applications will begin on July 1, 2021, and the position will remain open until filled. All applications will be confidential to the CFHT Board of Directors and Search Committee. Potential applicants with questions about the position or the search are encouraged to contact the Chair of the Search Committee at employment @ cfht.hawaii.edu.
CFHT is committed to diversity and inclusion, and is proud to be an Equal Opportunity Employer.
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| Director of the Large Binocular Telescope | Closing date: 2021-06-30
Contact: Adriano Fontana |
A call is open to select the new Director of the Large Binocular Telescope, one of the largest and most advanced optical telescopes in the world.
To get more information and apply please visit the site https://www.lbtdirectorsearch.org/ or send an e-mail to LBTDirectorSearch@lbto.org | | ▸ more | Located atop Mt. Graham, Arizona, the LBT is one of the world's largest and most advanced optical/IR telescopes, with twin 8.4-m diameter primary mirrors spanning a 22.8-m baseline, each equipped with adaptive secondary mirrors. More information about the LBT is available at http://www.lbto.org/
The LBT governing organization is the LBT Corporation (LBTC), a non-profit organization based in Tucson, AZ, USA. Members are INAF (Italy), LBTB (a consortium of German Institutes), Ohio State University and Unioversity of Arizona.
The LBT Corporation is seearching for a new Director of the Observatory.
The Director is responsible for the operation and maintenance of the Observatory; prepares and implements the annual program plan and budget; and assigns observing time in accordance with the Partners? shares, the approved program plan and other guidelines as established by the Board.
The LBT Director will report to the LBTC Board of Directors and the Dean of the UA College of Science and will be formally employed through the University of Arizona.
The ideal candidate has:
- A PhD in astronomy or equivalent degree in a closely related field;
- A passion about reaching challenging scientific and technical goals;
- Demonstrated track record in leading complex scientific projects to success;
- Demonstrated skills in critical analysis, problem solving, and conflict resolution;
- Ability to manage multiple, potentially conflicting priorities;
- Demonstrated ability to build diverse, high-performing teams.
Experience in strategic planning, budgetary planning, and financial management, as well as specific experience in the field of AO and astronomical instrumentation, are considered strong assets.
The LBT Observatory Director is a full-time employee of the University of Arizona.
Applications received before June 30th, 2021 will receive full consideration.
Applications can be submitted and will be considered until the position is filled.
The LBTO Director will be hired as a Career Track Faculty, that is a non-tenured, non-continuing status position.
The Board intends to assign the Director a 5-year mandate, potentially renewable, and subject to annual performance reviews.
The new appointment can start as soon as the new Director is available to take the role. The ideal timing is January 2022, but earlier or later dates can also be considered.
For full information please visit the site http://www.LBTDirectorSearch.org/ or send an e-mail to LBTDirectorSearch @ lbto.org
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| Understanding the spectral evolution of hot hybrid white dwarfs | Closing date: 2021-06-30
Contact: Klaus Werner |
The Institute for Astronomy and Astrophysics at the University of Tübingen (IAAT) invites applications for the position of a PhD student of a DFG (German Research Foundation) funded project in stellar physics, entitled "Understanding the spectral evolution of hot hybrid white dwarfs".
| | ▸ more | The project focuses on the analysis of a large sample of optical and UV spectra of hot white dwarfs with state-of-the-art non-LTE model atmospheres. The starting date is negotiable but is expected to be in autumn 2021.
Applicants are required to have a master's degree in astrophysics or physics. The salary is based upon the German public service scale (75% of E13 TV-L) with a temporary contract of 3 years. The university seeks to raise the number of women in research and teaching and therefore strongly encourages qualified women to apply. Disabled persons with equivalent aptitude will be given preference.
Interested students are invited to send by e-mail a single PDF file containing cover letter, curriculum vitae, master degree certificate, link to master thesis, and statement of previous reserach experience. Applicants should also provide the contact information for two reference letter writers. Applications received by June 30, 2021 will be given full consideration.
Prof. Klaus Werner
Kepler Center for Astro and Particle Physics
Institute for Astronomy and Astrophysics
Sand 1
72076 Tübingen
Germany
email: werner @ astro.uni-tuebingen.de
WWW: http://www.uni-tuebingen.de/en/39607
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| Postdoctoral position on Milky Way Models and Simulations in the Gaia Era | Closing date: 2021-06-15
Contact: Alejandra Recio-Blanco |
| Applications are invited for a postdoctoral position at the Observatoire de la Côte d'Azur (Nice, France) to work on Milky Way Models and Simulations in the Gaia era. The position is funded by the European Union's Horizon 2020 research and innovation programme, as part of the EXPLORE project. | | ▸ more | The host research team is strongly engaged in Gaia/DPAC activities for the Gaia DR3, many international ground based spectroscopic surveys like WEAVE, APOGEE, MOONS and 4MOST, as well as in cosmological simulations. In particular, we are responsible for the production of the stellar parameters and chemical abundances estimated from Gaia/RVS data that will be published with the next DR3 (first half of 2022). This new Gaia chemical dimension, available for millions of stars in one year from now, will pose strong constraints to our understanding of the Galaxy evolution, from the disc to the halo stellar populations.
We are seeking candidates with an expertise in Galaxy models and simulations, possibly including chemical evolution (although this is not a requisite) to work on the interpretation of Gaia EDR3 and DR3 data, as well as ground-based observations.
Position is for two years. Net annual salary will be in the range 27 600 to 42 000 euros, depending on experience, with included social security and public healthcare benefits, covering spouse and children. Position is expected to begin no later than the fall of 2021, although exceptions can be made.
Applications must be submitted by email to alejandra.recio-blanco @ oca.eu with the subject 'Explore-Gaia postdoc application'.
Required documents :
- Curriculum Vitae
- Research Description and Plan (6 pages max.)
- 3 letters of recommendation
- Complete list of publications
Our team promotes a diverse and inclusive environment and welcomes applicants regardless of age, disability, gender, nationality, race, religion or sexual orientation.
The EXPLORE EU H2020 project: https://www.explore-platform.eu
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| Ph.D. position in observational cosmology/photometric redshifts with Euclid | Closing date: 2021-06-15
Contact: Stéphane Paltani |
| We offer a Ph.D. position at the Department of Astronomy of the University of Geneva. The successful candidate will perform research activities to support the responsibilities of the Geneva group in the Euclid mission, a cosmology mission of the European Space Agency. They will be involved in the improvement of methods to compute photometric redshifts, with applications to scientific questions. They will become a member of the Euclid Consortium, and participate in meetings dedicated to this mission. | | ▸ more | Euclid is the second Medium mission of the Cosmic Vision program of the European Space Agency. Euclid will study the evolution of the large-scale structure of the Universe through the mapping of dark matter and galaxies, in order to constrain the properties of dark energy. It is currently in the final stage of the development phase with a planned launch in 2022-2023.
The Department of Astronomy of the University of Geneva offers a modern and vibrant work environment, with a wide range of activities including theory, numerical simulations, observations and instrumental developments in the domains of exoplanets, stellar physics, galaxy evolution, observational cosmology and high-energy astrophysics. The Department of Astronomy has a very active program in the development of scientific software and operations for space missions, which it built over more than 25 years with the creation of the INTEGRAL Science Data Centre; it is now involved in several other scientific missions in space, e.g., Gaia, CHEOPS, Euclid or Athena. The Department of Astronomy is in particular an important member of the Euclid collaboration; it is hosting the Swiss Euclid Science Data Center and holds the responsibility of producing the photometric redshifts for the Euclid mission.
The Ph.D. is proposed in the framework of this collaboration. The successful candidate will be in charge of understanding the origin of the defects in the photometric-redshift determination methods, namely bias and catastrophic failures, that are impeding the performance of the weak-lensing probe of the Euclid mission, and to devise methods to alleviate these issues. The Ph.D. will also focus on astrophysics applications of photometric redshifts.
The successful candidate must hold a Masters in physics or astrophysics; they will be enrolled in the astrophysics Ph.D. cursus of the University of Geneva. They need to demonstrate a good understanding of data analysis methods and ideally show good aptitudes with programming in Python or other programming languages. Candidates must send a motivation letter, a curriculum vitae, grades and a summary of their Master thesis (two pages) to the e-mail address below. In addition one reference letter must be sent separately to the same e-mail address.
The starting date, to be agreed with the candidate, is September 1st, 2021.
All correspondence should be sent by e-mail, with the subject line containing 'Euclid PhD'. Applications will be accepted until the position is filled. For applications or for further information, please contact:
Prof. Stéphane Paltani, Stephane.Paltani @ unige.ch
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| PhD study in astronomy, Krakow, Poland | Closing date: 2021-06-08
Contact: Elzbieta Danielkiewicz-Krosniak |
| PhD study in astronomy at Astronomical Observatory of the Jagiellonian University (Kraków, Poland) covers broad range of theoretical and observational research subjects, from analysis of optically variable objects (both stellar and active galactic nuclei), high energy astrophysics and accretion disks, radio astronomy, relativistic astrophysics and cosmology. Candidates eligible for admission to the Astronomy program of study are the holders of Master of Science (Magister, Magister engineer), or equivalent professional title awarded in the field of exact sciences. | | ▸ more | Doctoral School of Exact and Natural Sciences Astronomy at Jagiellonian University (city: Krakow, country: Poland)
PhD study in astronomy covers broad range of theoretical and observational research subjects, from analysis of optically variable objects (like accreting binary stars or active galactic nuclei), high energy astrophysics, multiwavelength astronomy, radio astronomy, relativistic astrophysics and cosmology. Astronomical Observatory of the Jagiellonian University participates in ESO, has access to the SALT optical telescope, collaborates in HESS and CTA projects (gamma-ray astrophysics) as well as in the network of LOFAR radio telescopes array, also participate in the VIRGO gravitational waves detector. Our researches use also several world class Earth bound radio (VLA, 100m Effelsberg) and space (Chandra, XMM, Fermi) observatories.
All interested candidates are welcome to register in our on-line system.
Accepted foreign students will obtain Ph.D. fellowships (equal to the ones provided to the Polish students i.e. approx. 2200* PLN per month, which is 26400 PLN per year), as well as, the health insurance (students from outside EU may be subject of another regulations in that matter).
Based on good progress in a PhD thesis preparation students can apply for support of travels and conference participation. They can also apply for research grants from the Polish Science Foundation.
There is NO tuition fee.
* Costs of living in Poland is significantly lower than in Western European countries.
Registration starts: 17.05.2021
Registration ends: 08.06.2021
Entrance exams: 14-18.06.2021
Start of studies: October 2021
http://www.oa.uj.edu.pl/Studia_Doktoranckie/stopien3.en.html
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| Post-doc position (4 years) on exoplanets in the Institute of Space Sciences, Barcelona (Spain) | Closing date: 2021-07-15
Contact: Daniele Viganň |
| The exoplanets group in the Institute of Space Sciences (Institut de Cičncies de l'Espai, ICE), Barcelona, Spain, www.ice.csic.es, invites applications for one post-doctoral position, to start between September and December 2021. The post-doc position will fit within the ERC Starting Grant IMAGINE, a new project aiming at considering the magnetic imprints on exoplanets from observational and theoretical perspectives. | | ▸ more | The post-doc is expected to contribute, together with the PI Daniele Viganň, to theoretical studies in long-term thermal and magnetic properties of gas and rocky exoplanets, as well as linking observational constraints to theory. Partial dedication to other topics of research will of course be possible upon agreement. Besides the PI, the growing exoplanet group at ICE currently includes, among others, the astronomers Guillem Anglada-Escudé and Ignasi Ribas, and there are active collaborations at ICE with groups working on the related subjects like magnetic fields or stellar formation.
Applicants with a good track record in the field of internal structure, cooling and evolution of planets will be positively evaluated. The position is preferentially (but not exclusively) oriented to a senior profile (3 years or more of post-doctoral experience), in which case the co-supervision of one PhD student working on the same subject will be offered. Moreover, the successful candidate, if interested to stay longer, will be able to receive support by the institute in applying to national and European calls (Ramón y Cajal Fellowship, Marie-Curie Fellowships, ERC Grants?).
The expressions of interest for this position have to be sent to vigano (at) ice.csic.es , providing the following:
- CV (maximum 4 pages)
- Two reference providers (name, affiliation, relation with the candidate and e-mail), who will be contacted if the candidate is shortlisted
- Research statement (maximum 2 pages)
The 4 year contract will cover the costs of National Social Security with a gross salary in the range 37.000-42.000 Euros per year ("Doctor FC2" or "Doctor FC3" in the CSIC salary scheme), depending on the applicant's experience. Budget for material and attendance to conferences and visits will be granted by the project. Given the current situation, substantial remote working and high flexibility will be allowed until at least end of 2021, if requested. Once selected, the ICE administration will assist the candidate, within their possibilities, with the required bureaucratic steps, like title equivalence, work permit and visa application, if applicable.
The expressions of interest will be reviewed after July, 15th 2021. However, later applications may also be considered if the position remains open. Inquiries can be sent to the above e-mail.
About the institution:
Currently, ICE counts over 20 faculty members, about 20 engineers, about 20 post-doc fellows and a dozen of PhD students. The areas of research vary, from engineering applied to several space missions to fundamental physics, from high-energy astronomy to theoretical astrophysics. ICE pertains to the "Consejo Superior de Investigaciones Científicas" (CSIC, the Spanish National Research Council). CSIC is the largest public institution dedicated to research in Spain and the third largest in Europe. ICE is also part of the Catalan Institute of Space Studies (Institut d'Estudis Espacials de Catalunya). Our institute is committed to building a culturally diverse community of researchers, dedicated to contributing to an inclusive environment.
ICE is located in the campus of the Autonomous University of Barcelona in Bellaterra, just outside Barcelona. The campus is well served by public transportation (railways and buses), and a variety of temporary and long-term accommodation options can be found both in Barcelona city and in the smaller towns close to the campus.
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| PhD position on magnetic exoplanets in the Institute of Space Sciences, Barcelona (Spain) | Closing date: 2021-06-15
Contact: Daniele Viganň |
| The exoplanets group in the Institute of Space Sciences (Institut de Cičncies de l'Espai, ICE), Barcelona, Spain, www.ice.csic.es, invites applications for one PhD position, to start between September and December 2021. The PhD position will fit within the ERC Starting Grant IMAGINE, a new project aimed at considering the imprints of magnetic fields on exoplanets, from observational and theoretical perspectives. | | ▸ more | The successful candidate will be supervised by Daniele Viganň, PI of the grant. The tasks of the PhD student will include the theoretical and numerical modeling of cooling and magnetic field evolution in giants and rocky planets. A good numerical background and formation on planetary structure and evolution will be positively evaluated. As a part of the PhD program, the successful candidate will also join schools and conferences and visit international groups working in magnetism and exoplanets. Besides the PI, the growing exoplanet group at ICE currently includes, among others, the astronomers Guillem Anglada-Escudé and Ignasi Ribas, and there are active collaborations at ICE with groups working on the related subjects like magnetic fields or stellar formation.
Applicants are required to have a master degree (or an equivalent degree) in the branches of Theoretical Physics, Astrophysics or Geophysics. Students about to complete their master studies will also be considered.
The expressions of interest for this position have to be sent to Daniele Viganň, vigano (at) ice.csic.es , providing the following:
- CV (maximum 2 pages)
- Academic Certificate of Bachelor and Master Degree
- Two reference providers (name, affiliation, relation with the candidate and e-mail), who will be contacted if the candidate is shortlisted
- Research statement (maximum 1 page)
The contract will last for the entire PhD program, up to 4 years. The contract covers the costs of National Social Security and the gross salary is about 21.700 Euros per year ("Contrato predoctoral fuera de convenio" in the CSIC salary scheme). Budget for material and attendance to schools, conferences and visits will be granted as well. Given the current situation, substantial remote working and high flexibility will be allowed until at least end of 2021, if requested. Once selected, the ICE administration will assist the candidate, within their possibilities, with the required bureaucratic steps, like title equivalence, work permit and visa application, if applicable.
The expressions of interest will be reviewed after June, 15th 2021. However, later applications may also be considered if the position remains open. Inquiries can be sent to the above e-mail.
About the institution:
Currently, ICE counts over 20 faculty members, about 20 engineers, about 20 post-doc fellows and a dozen of PhD students. The areas of research vary, from engineering applied to several space missions to fundamental physics, from high-energy astronomy to theoretical astrophysics. ICE pertains to the "Consejo Superior de Investigaciones Científicas" (CSIC, the Spanish National Research Council). CSIC is the largest public institution dedicated to research in Spain and the third largest in Europe. ICE is also part of the Catalan Institute of Space Studies (Institut d'Estudis Espacials de Catalunya). Our institute is committed to building a culturally diverse community of researchers, dedicated to contributing to an inclusive environment.
ICE is located in the campus of the Autonomous Univerisity of Barcelona in Bellaterra, just outside Barcelona. The campus is well served by public transportation (railways and buses), and a variety of temporary and long-term accommodation options can be found both in Barcelona city and in the smaller towns close to the campus.
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| Postdoctoral position in theoretical astrophysics | Closing date: 2021-06-15
Contact: Agnieszka Janiuk |
Center for Theoretical Physics in Warsaw, Poland, invites applications for the postdoctoral fellowship, financed from the project "Origin of Gamma Ray Bursts and their multimessenger appearance" from Polish National Science Center. PI of the project is prof. dr.hab. Agnieszka Janiuk.
We are looking for a candidate with a PhD and experience in theoretical and computational astrophysics. The research involves study of stellar evolution and collapse in the context of long gamma ray bursts. We are also studying r-process nucleosynthesis in the outflows from accretion disks in GRB engines. | | ▸ more | The position will be available for initially two years, with a possible extension for the third year, subject to satisfactory performance.
The application should include: 1. The scientific CV, including publication list, participation in research projects and conferences (with the clause "I agree to the processing of my personal data contained in the application documents?) 2. Motivation letter, with a brief description of the Candidate scientific interests and future research plans. 3. A copy of the PhD diploma, or statement from the PhD Advisor on the planned date of defense (the PhD should be awarded before the post-doc contract starting date). 4. Applicants should also arrange to have two letters of reference separately sent to the email address given below.
The documents should be sent electronically to rekrutacja @ cft.edu.pl, by 15 June 2021. All further questions should be addressed by e-mail to agnes @ cft.edu.pl.
The competition will be settled by 15 July, 2021. Candidates will be informed electronically about the results of the competition. Applications submitted by the mid of June, 2021 will receive full consideration. Candidates might be asked to present an on-line seminar talk. The position will remain open until filled. The prospective starting date of the contract is October 1st 2021, but it can be negotiated.
More information about the project and astrophysics group activities at CTP PAS can be found on our website, http://www.cft.edu.pl/astrofizyka.
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| H2020 NEMESIS postdoctoral/PhD positions in star formation using machine learning techniques | Closing date: 2021-06-30
Contact: Marc Audard |
| We invite applications for postdoctoral and PhD student positions in star formation using machine learning techniques. The successful candidate(s) will work with members of the recently established project NEMESIS, and in particular with Odysseas Dionatos (U. Vienna), Marc Audard (U. Geneva) and Gabor Marton (Konkoly Obs.), however, candidates will have the opportunity to spend extended working visits at the other participating institutes. | | ▸ more | NEMESIS is a H2020 funded project (grant agreement 101004141; https://nemesis.univie.ac.at/) that has the ambition to reshape our understanding on the formation of stars by employing artificial intelligence methods to compile and interpret the largest, panchromatic data collection of young stellar objects.
The successful candidates should have a solid background (experience) in at least one of the following topics: star formation, classification of young stellar objects, application of machine learning techniques in large datasets. Candidates for the postdoc positions must hold PhD in astrophysics or in a closely related discipline, or have completed their MSc studies (or equivalent) for the PhD positions. Starting date can be as early as June 1st but no later than December 1st, 2021.
Applicants should send to nemesis @ unige.ch
• Cover letter
• CV and Publication list if applicable
• 5-page (maximum) statement of research, outlining any research experience so far
•For PhD student applicants: copy of Bachelor and master academic records (exams, grades).
•Candidates should also provide the names and contact details for at least two references.
Applications received by June 30, 2021, will receive full consideration, but the call will remain open until the position is filled. For further inquiries please write to nemesis? @ ?unige.ch
Further details on the NEMESIS project can be found at https://nemesis.univie.ac.at/
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| WaterStars, from observation to experiments on water in space | Closing date: 2021-10-01
Contact: Fabrice Herpin |
| Understanding the excitation of water in evolved stars implies knowing the collision rates for pure rotational transitions within the first four excited vibrational states (v1=1, v2=1, 2 and v3=1) as well as the rotational transitions between the ground state and these excited states. The first objective is therefore to obtain these collision rates. The second is to include these in an advanced radiative transfer code to reproduce the ALMA observations (ATOMIUM consortium). | | ▸ more | Scientific subject: Water is the third most abundant molecule in the interstellar medium. It has been observed in various objects, but it is only in the extended atmosphere of the envelope of O-rich evolved stars that the very rich spectrum of rotational, vibrational and ro-vibrational transitions of water is observed, and sometimes in surprisingly excited energy states. To understand the excitation of water in these environments, it is necessary to model the excitation of water not only by the radiation from the central star and by radiative coupling with the background radiation, but also by collisions with its most abundant partners (H2, He, H, e-). This implies knowing the collision rates for pure rotational transitions within the first four excited vibrational states (v1=1, v2=1, 2 and v3=1) as well as the rotational transitions between the ground state and these excited states. The first objective is therefore to obtain these collision rates. The second is to include these in an advanced radiative transfer code to reproduce the ALMA observations (ATOMIUM consortium, (https://fys.kuleuven.be/ster/research-projects/aerosol/atomium/atomium) and interpret them. The crossed molecular beam experiment in Bordeaux allows the study of inelastic collisions down to very low collision energies, where quantum effects may be observed. The experimental studies will be used to validate theoretical methods in order to provide reliable data to astrophysicists. The first objective of the thesis will be to extend our first experimental studies on H2O and D2O + H2 to vibrationally excited water molecules. To model the emission of water lines from highly excited levels we will use a radiative transfer code published by Gray, Baudry et al (2016). The next step will be to include the results of the experimental or theoretical work done at the ISM, i.e. to incorporate the new collision rates, and to extend the code to the first four vibrational levels of water in an attempt to model all the lines observed in ATOMIUM.
Additional information: The Ph.D. student will work mainly at ISM, together with Fabrice Herpin (LAB) and Astrid Bergeat (ISM) and other WATERSTARS team members, in close collaboration with the ATOMIUM team. More information on the Laboratoire d?Astrophysique de Bordeaux and Institut des Sciences Moléculaires can be found at https://astrophy.u-bordeaux.fr and http://www.ism.u-bordeaux.fr, respectively. The 3-year paid thesis contract requires a Master's degree in Astronomy, Physics or Physical Chemistry (or equivalent), obtained before the start of the contract. The start date of the thesis will be between 1 October 2021 and 1 March 2022. Applications should include a brief description of research interests and a summary of previous experience relevant to the subject, a CV, copies of Master's and Bachelor's degrees, Master's certificates or transcripts and internships, as well as contact details of the Master's supervisor and internship supervisors. Applications are open until the vacancy is filled and should be sent to Fabrice Herpin (fabrice.herpin @ u-bordeaux.fr) or Astrid Bergeat (astrid.bergeat @ u-bordeaux.fr). A complete description of the position can be found at https://www.ism.u-bordeaux.fr/spip.php?article354
Skills required: Practical experience with spectroscopy, experimental kinetic techniques, use of lasers, programming language, radiative transfer calculations or analysis of observational data will be considered a merit.
Funding details: secured financing (ANR Ph-D fellowship)
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| A study of the winds of evolved cold stars | Closing date: 2021-06-01
Contact: Fabrice Herpin |
| This thesis aims to build a coherent and comprehensive description of the mass-loss mechanism. How are the winds launched and which physical processes determine their properties? How do the mass-loss rate and other wind properties depend on fundamental stellar parameters? What is the origin of the detected magnetic field on the stellar surface? What chemical processes dominate in the winds? Where does the interaction between dynamics and chemical phenomena lie? | | ▸ more | Applications are invited for a Ph.D. student position in Astrophysics at the Laboratoire d?Astrophysique de Bordeaux, Bordeaux University, France.
Project description: Evolved cool stars are major cosmic engines, providing strong mechanical, chemical, and radiative feedback to their host environments. Through strong stellar winds, still poorly understood, they enrich their environment with chemical elements, which are the building blocks of planets and life. A complete understanding of their evolution in the near and distant Universe can only be achieved with detailed knowledge of wind physics over the life cycle of these stars as well as in relation to their circumstellar environment. A complete picture of all the physical processes that simultaneously trigger and shape the strong winds of evolved cold stars is still missing. This thesis is part of Project PEPPER (https://lagrange.oca.eu/fr/welcome-to-anr-pepper), funded by the French Agence Nationale pour la Recherche, aiming to build a coherent and comprehensive description of the mass-loss mechanism, in close collaboration with the ATOMIUM project (https://fys.kuleuven.be/ster/research-projects/aerosol/atomium/atomium). The main questions we endeavour to tackle in this project are: How are the winds launched and which physical processes determine their properties? How do the mass-loss rate and other wind properties depend on fundamental stellar parameters? What is the origin of the detected magnetic field on the stellar surface? What chemical processes dominate in the winds? Where does the interaction between dynamics and chemical phenomena lie? The core of our approach is the synergy between theory and observation in order to obtain a global, coherent vision of the evolved cool stars, from the bottom of the atmosphere up to the circumstellar environment. We will use high-angular resolution observations with SPHERE and MATISSE and observations made quasi-simultaneously with ALMA (all already in hand). For the interpretation, the student will actively participate in the modeling using various codes.
The Ph.D. student will work together with Fabrice Herpin and other PEPPER team members, in close collaboration with the ATOMIUM team. More information on the Laboratoire d?Astrophysique de Bordeaux can be found at https://astrophy.u-bordeaux.fr
The position is a 3-year appointment and requires a University degree in Astronomy or Physics at an advanced level (e.g., a M.Sc. degree), completed by the time of employment. The earliest starting date is 1 October 2021. Applications should include a brief description of research interests and relevant experience, CV, copies of Master?s University grades, certificates and diplomas, B.Sc./M.Sc. thesis/internship (or draft thereof), and contact details for the Master director and internship supervisors. Practical experience with python, numerical simulations of gas dynamics, or with observational data on AGB and RSG stars, will be considered a merit.
The complete announcement is posted at https://lagrange.oca.eu/fr/welcome-to-anr-pepper and the application deadline is 1 June 2021. Applications should be sent to Fabrice Herpin (fabrice.herpin @ u-bordeaux.fr).
For further information, please contact Fabrice Herpin (fabrice.herpin @ u-bordeaux.fr).
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| Postdoctoral Research Position - Solar Radio Astronomy with LOFAR and MWA | Closing date: 2021-06-31
Contact: Kamen Kozarev |
| Applications are invited for a Post-doctoral researcher position to work on processing and analyzing advanced low-frequency radio imaging observations of solar coronal shocks and coronal mass ejections from the Low Frequency Array (LOFAR) and Murchison Widefield Array (MWA) low-frequency telescopes. The Institute of Astronomy and National Astronomical Observatory (IANAO) of the Bulgarian Academy of Sciences will host this three-year position with a preferable starting date in May or June 2021. | | ▸ more | The Institute of Astronomy and National Astronomical Observatory (IANAO) of the Bulgarian Academy of Sciences invites applications for a Post-doctoral researcher position to work on processing and analyzing advanced low-frequency radio imaging observations of solar coronal shocks and coronal mass ejections from the Low Frequency Array (LOFAR) and Murchison Widefield Array (MWA) low-frequency telescopes.
The postdoctoral researcher will join Dr. Kamen Kozarev and his research group to study the dynamic features of solar eruptions and time-dependent spectra of energetic electron beams in the corona. The researcher will help develop and employ processing pipelines for solar interferometric observations. These data can reveal the locations of charged particle acceleration with great spatial, temporal and frequency resolutions. While such observations have traditionally been challenging, new advanced approaches, together with improved computing technology and software, have made them more accessible for routine investigation of solar activity. Available synergistic EUV and in situ data (from Parker Solar Probe and Solar Orbiter) will also be analyzed.
Requirements:
- Applicants must hold a PhD in physics, astronomy, or astrophysics, with a focus in radio astronomy, heliophysics, or a closely related field. Previous experience in scientific programming in Python, CASA or similar, Linux/Unix environments, version control (svn, git), and work on building processing pipelines will be considered an advantage. The full-time position is available starting on May 1st 2021, or soon thereafter. A very competitive salary and ample conference travel funds are offered.
How to Apply:
- Interested candidates should contact Dr. Kamen Kozarev (kkozarev @ astro.bas.bg), arrange for three letters of recommendation to be sent to him, and provide a cover letter describing their experience and interests, as well as a curriculum vitae including a list of relevant publications.
Additional Information:
- The position is part of the 5-year CAREER-type project ?Modeling and ObServAtional Integrated Investigations of Coronal Solar Eruptions? (MOSAIICS), funded by the National Science Fund of Bulgaria. The project is led by Assoc. Prof. Kamen Kozarev.
- The overall goal of the MOSAIICS project is to adopt an integrated approach providing a deeper understanding of the plasma processes leading to charged particle acceleration by CMEs near the Sun. The project?s high level objectives are to (i) develop and integrate novel image processing and machine learning techniques to reliably analyze radio and EUV remote imaging observations of CMEs and their shocks; (ii) investigate the origins and evolution of radio emission from energetic electron beams in CMEs, comparing with in situ measurements; (iii) develop and apply advanced global data-driven models of particle acceleration and transport to test and improve our theoretical understanding of SEP production and transport. This postdoctoral position will focus on the second objective.
- The Institute of Astronomy is a leader in astrophysical research in Bulgaria and Southeast Europe. It hosts over 80 researchers working in several areas of astrophysics, namely solar activity and solar system small bodies, stars and stellar systems, galaxies and cosmology. Additionally, IANAO staff have strong expertise in operating and maintaining the National Observatory Rozhen - a dedicated facility in the Rhodopi mountains with a flagship 2-meter reflective optical telescope, as well as a number of smaller research-grade telescopes. IANAO is currently actively developing a radio astronomy research programme, including development of a LOFAR observing station. For more information, visit http://astro.bas.bg.
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