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The physics of strongly irradiated extrasolar planet thermospheres

Subject Area Astrophysics and Astronomy
Term from 2016 to 2021
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 314569934
 
Final Report Year 2022

Final Report Abstract

The work carried out in this project yielded two ”firsts”: First, the demonstration that planetary transit observations can be carried out with SWIFT in the UV, thus opening a new observational window in addition to the HST; and second, the demonstration that planetary transits in He I 10830 can be studied from the ground with suitable instrumentation (such as CARMENES). The only previous detection had been made with HST!

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