UniBE is prestigious. With us, you benefit from the excellent reputation of a long-standing institution all around the world.
Your profile The ideal candidate would have expertise in applying Bayesian statistical methods to astronomical datasets, experience modelling exoplanetary transits, deep knowledge of atmospheric physics (e.g. chemistry, radiative transfer, etc), and a proven track record as an independent researcher. Specifically, expertise extracting spectra from JWST timeseries data and the retrieval of abundances will be most useful. Additional theoretical expertise in connecting sub-Neptune interiors & atmospheres would also be beneficial. The fellow would have the opportunity to play a key role in the IN/AT-SYNC JWST large programme targeting the atmospheres of sub-Neptunes in resonant systems (Co-PI Osborn). The PostDoc is additionally expected to help obtain further JWST transmission spectra of sub-Neptunes.
PostDocs will be expected to assist with teaching, as well as the possibility to directly supervise Masters projects and to provide mentoring to existing PhD students.
We offer Bern's Physics institute hosts multiple groups studying both exoplanet (atmospheres, interiors, formation, direct imaging) and solar system (planetary imaging, remote sensing, etc) astronomy. This makes for a welcoming and egalitarian research environment. The university of Bern is a top-200 global university in a welcoming international city which is frequently found in the top-10 most liveable cities worldwide. PostDoc salaries are internationally competitive.
The position is funded for 2 years with a possible 1 year extension. We welcome candidates from diverse and minority groups & non-linear career paths.
The annual salary is determined by a matrix provided by the Swiss National Fund. Child allowance and maternity/paternity leave is offered.
Application and Contact Please send enquiries and application documents to hugh.osborn@unibe.ch. To be considered, send a cover letter (max 2 page), CV in months and years, publication list; max 4 page, PhD Diploma and contact details of two academic references before 23:39 CEST on August 31st 2026.
Online interviews will take place in October with an ideal start date in late 2026 or early 2027.
#J-18808-Ljbffr
Your profile The ideal candidate would have expertise in applying Bayesian statistical methods to astronomical datasets, experience modelling exoplanetary transits, deep knowledge of atmospheric physics (e.g. chemistry, radiative transfer, etc), and a proven track record as an independent researcher. Specifically, expertise extracting spectra from JWST timeseries data and the retrieval of abundances will be most useful. Additional theoretical expertise in connecting sub-Neptune interiors & atmospheres would also be beneficial. The fellow would have the opportunity to play a key role in the IN/AT-SYNC JWST large programme targeting the atmospheres of sub-Neptunes in resonant systems (Co-PI Osborn). The PostDoc is additionally expected to help obtain further JWST transmission spectra of sub-Neptunes.
PostDocs will be expected to assist with teaching, as well as the possibility to directly supervise Masters projects and to provide mentoring to existing PhD students.
We offer Bern's Physics institute hosts multiple groups studying both exoplanet (atmospheres, interiors, formation, direct imaging) and solar system (planetary imaging, remote sensing, etc) astronomy. This makes for a welcoming and egalitarian research environment. The university of Bern is a top-200 global university in a welcoming international city which is frequently found in the top-10 most liveable cities worldwide. PostDoc salaries are internationally competitive.
The position is funded for 2 years with a possible 1 year extension. We welcome candidates from diverse and minority groups & non-linear career paths.
The annual salary is determined by a matrix provided by the Swiss National Fund. Child allowance and maternity/paternity leave is offered.
Application and Contact Please send enquiries and application documents to hugh.osborn@unibe.ch. To be considered, send a cover letter (max 2 page), CV in months and years, publication list; max 4 page, PhD Diploma and contact details of two academic references before 23:39 CEST on August 31st 2026.
Online interviews will take place in October with an ideal start date in late 2026 or early 2027.
#J-18808-Ljbffr
PostDoc in exoplanet atmospheres at the University of Bern Arbeitgeber: University of Bern
Die University of Bern ist ein hervorragender Arbeitgeber, der eine inspirierende Arbeitsumgebung bietet, in der Vielfalt und Teamarbeit geschätzt werden. Als Leiter der Debitorenbuchhaltung profitieren Sie von umfangreichen Entwicklungsmöglichkeiten und einem unterstützenden Arbeitsklima, das Ihre berufliche Entfaltung fördert. Zudem genießen Sie die Vorzüge einer zentralen Lage in Bern, die sowohl kulturelle als auch Freizeitmöglichkeiten in unmittelbarer Nähe bietet.
