The occurrence rate of quiescent radio emission for ultracool dwarfs using a generalized semi-analytical Bayesian framework

ABSTRACT We present a generalized analytical Bayesian framework for calculating the occurrence rate of steady emission (or absorption) in astrophysical objects. As a proof-of-concept, we apply this framework to non-flaring quiescent radio emission in ultracool (≤M7) dwarfs. Using simulations, we sho...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2024-01, Vol.527 (3), p.6835-6866
Hauptverfasser:	Kao, Melodie M, Shkolnik, Evgenya L
Format:	Artikel
Sprache:	eng
Schlagworte:	Bayesian analysis Emission analysis Luminosity Radio emission Red dwarf stars
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