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Validating the Orbital Periods of the Coolest TESS Planet Candidates

When an exoplanet passes in front of its host star, the resulting eclipse causes an observable decrease in stellar flux, and when multiple such transits are detected, the orbital period of the exoplanet can be determined. Over the past seven years NASA’s Transiting Exoplanet Survey Satellite (TESS)...

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Bibliografiset tiedot
Päätekijät: Dillon J. Bass, Daniel C. Fabrycky
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: IOP Publishing 2025-01-01
Sarja:The Astronomical Journal
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Linkit:https://doi.org/10.3847/1538-3881/adcac6
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