Occurrence Rates of Accreting Companions from a New Method for Computing Emission-line Survey Sensitivity: Application to the Hα Giant Accreting Protoplanet Survey

A key scientific goal of exoplanet surveys is to characterize the underlying population of planets in the local galaxy. In particular, the properties of accreting proto planets can inform the rates and physical processes of planet formation. We develop a novel method to compute sensitivity to protop...

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Auteurs principaux:	Cailin Plunkett, Katherine B. Follette, Gabriel-Dominique Marleau, Eric L. Nielsen
Format:	Artigo
Langue:	Inglês
Publié:	IOP Publishing 2025-01-01
Collection:	The Astronomical Journal
Sujets:	Accretion Brown dwarfs Direct imaging Exoplanet detection methods Astrometric exoplanet detection H alpha photometry
Accès en ligne:	https://doi.org/10.3847/1538-3881/adc09d
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