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Developing a vision for exoplanetary transit spectroscopy: a shared window on the analysis of planetary atmospheres and of stellar magnetic structure

Published onMay 31, 2019
Developing a vision for exoplanetary transit spectroscopy: a shared window on the analysis of planetary atmospheres and of stellar magnetic structure
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Abstract

We describe how accurate exoplanet atmospheres’ characterization will inevitably require taking into consideration stellar inhomogeneities caused by convection and magnetic fields. Disentangling these two components requires a multipronged approach with new solar reference spectra, MHD modeling, and collaborations among astrophysics communities.

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