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supervisor. Possible present or future connections to his research are appreciated. Structure of the Research Group The group usually consists of around two MSc students, two PhD students, and two
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radiative transfer codes that bridge observations, as well as cosmological N-body codes including neutrinos. The CompAS and CHARMS projects are devoted to in-house algorithm and code developments driven by
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that bridge observations, as well as cosmological N-body codes including neutrinos. The CompAS and CHARMS projects are devoted to in-house algorithm and code developments driven by leading-edge scientific
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group The group usually consists of around two MSc students, two PhD students, and two postdoctoral researchers. For effective supervision and to increase connectedness within the group, each graduate
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. Candidates are expected to have completed their PhD by the start of the appointment. The primary responsibilities for each position are listed below: Postdoctoral associate in cosmology: We invite applications
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to apply. Several postdoctoral positions for young mathematicians with strong research potential are available. Candidates must have received their PhD degrees before officially taking up the position