Big flares from small stars: detecting flares from faint low-mass stars with NGTS full-frame images

ABSTRACT High-cadence observations of high-energy stellar flares from cool and ultracool dwarfs are often limited by the faint nature of their host stars. Many low-mass sources cannot be detected in quiescence by photometric surveys, meaning they are not targeted for high-cadence observations. This...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2023-08, Vol.525 (1), p.1588-1600
Hauptverfasser:	Jackman, James A G, Wheatley, Peter J, West, Richard G, Gill, Sam, Jenkins, James S
Format:	Artikel
Sprache:	eng
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