The University of Bern seeks a PostDoc to analyze exoplanet atmospheres using JWST data and Bayesian methods, supporting a major research programme on sub-Neptunes.
This position supports the IN/AT-SYNC JWST large programme focused on studying the atmospheres of sub-Neptune planets within resonant systems. The successful candidate will contribute to obtaining and interpreting transmission spectra for these worlds.
Responsibilities
- Utilize Bayesian statistical techniques to analyze astronomical data.
- Simulate and model transits of exoplanets.
- Derive spectra from JWST time-series observations and determine chemical abundances.
- Investigate the relationship between sub-Neptune interiors and their atmospheres.
- Provide teaching assistance.
- Oversee Master's level student projects.
- Guide current PhD candidates.
Requirements
- Strong proficiency in applying Bayesian statistics to astronomical datasets.
- Hands-on experience with exoplanetary transit modeling.
- Comprehensive understanding of atmospheric physics, including chemistry and radiative transfer.
- Demonstrated history of independent research achievements.
Nice to have
- Further theoretical background in linking sub-Neptune interiors with atmospheric properties.
What the company offers
- Financial support for children and extended parental leave policies.
- Competitive salary rates aligned with international standards.
- A two-year contract with the option to extend for one additional year.
About the company
The University of Bern ranks among the top 200 global institutions and is situated in a highly liveable, international city. Its Physics institute fosters an inclusive and egalitarian research culture, hosting several groups dedicated to exoplanet and solar system astronomy.
- The Physics institute brings together multiple research groups focused on exoplanet and solar system studies.
- A welcoming and egalitarian environment is maintained for all researchers.
- The university is located in a city regularly ranked among the world's most liveable.
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