A transiting warm giant planet around the young active star TOI-201
arXiv:2103.02685 · doi:10.3847/1538-3881/abeaa1
Abstract
We present the confirmation of the eccentric warm giant planet TOI-201 b, first identified as a candidate in \textit{TESS} photometry (Sectors 1-8, 10-13, and 27-28) and confirmed using ground-based photometry from NGTS and radial velocities from FEROS, HARPS, CORALIE, and \textsc{Minerva}-Australis. TOI-201 b orbits a young () and bright(V=9.07 mag) F-type star with a period. The planet has a mass of , a radius of , and an orbital eccentricity of ; it appears to still be undergoing fairly rapid cooling, as expected given the youth of the host star. The star also shows long-term variability in both the radial velocities and several activity indicators, which we attribute to stellar activity. The discovery and characterization of warm giant planets such as TOI-201 b is important for constraining formation and evolution theories for giant planets.
arXiv comment21 pages, 11 figures, accepted to AJ
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