Feb. 2, 2022, 2:11 a.m. | Matthew P. Battley, David J. Armstrong, Don Pollacco

cs.LG updates on arXiv.org arxiv.org

Young exoplanets and their corresponding host stars are fascinating
laboratories for constraining the timescale of planetary evolution and
planet-star interactions. However, because young stars are typically much more
active than the older population, in order to discover more young exoplanets,
greater knowledge of the wide array of young star variability is needed. Here
Kohonen Self Organising Maps (SOMs) are used to explore young star variability
present in the first year of observations from the Transiting Exoplanet Survey
Satellite (TESS), with …

arxiv data ii maps

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