Making the Most of Transmission Spectra in Light of Stellar Activity: Needs Identified by ExoPAG's Study Analysis Group 21
Transmission spectroscopy, a method for studying exoplanetary atmospheres by measuring the wavelength-dependent radius of a planet as it transits its star, relies on a precise understanding of the spectrum of the star being occulted. However, stars are not homogeneous, constant light sources but have temporally evolving photospheres and
Rackham, Benjamin V. et al.
Fecha de publicación:
6
2022