The atmosphere of WASP-76b seen with CARMENES: looking for CaII IRT and HeI

Nuria Casasayas Barris - Leiden ObservatoryOct 11, 2021
Atmospheric characterization
ultra-hot Jupiters
Currently, one of the most used techniques to study the atmosphere of the exoplanets is transmission spectroscopy by means of high-resolution facilities (R > 10^5). This methodology has led to the detection of several species in the atmosphere of exoplanets, showing that ultra-hot Jupiters (Teq > 2000 K) are one ...
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