Empirically Constraining the Spectra of Stellar Surface Features Using Time-resolved Spectroscopy

Transmission spectroscopy is currently the technique best suited to study a wide range of planetary atmospheres, leveraging the filtering of a star’s light by a planet’s atmosphere rather than its own emission. However, as both a planet and its star contribute to the information encoded in a transmi...

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Bibliographic Details

Published in:	The Astrophysical Journal Letters
Main Authors:	David Berardo, Julien de Wit, Benjamin V. Rackham
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Exoplanets Stellar surfaces Transmission spectroscopy Astronomical techniques
Online Access:	https://doi.org/10.3847/2041-8213/ad1b5b