The Detection of KIC 1718360, A Rotating Variable with a Possible Companion, Using Machine Learning

Jakob Roche
5/7/2024
astro-ph.EPastro-ph.IMcs.LG

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Abstract

This paper presents the detection of a periodic dimming event in the lightcurve of the G1.5IV-V type star KIC 1718360. This is based on visible-light observations conducted by both the TESS and Kepler space telescopes. Analysis of the data seems to point toward a high rotation rate in the star, with a rotational period of 2.938 days. The high variability seen within the star's lightcurve points toward classification as a rotating variable. The initial observation was made in Kepler Quarter 16 data using the One-Class SVM machine learning method. Subsequent observations by the TESS space telescope corroborated these findings. It appears that KIC 1718360 is a nearby rotating variable that appears in little to no major catalogs as such. A secondary, additional periodic dip is also present, indicating a possible exoplanetary companion.

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Cite this paper

@article{roche2024detection,
  title  = {The Detection of KIC 1718360, A Rotating Variable with a Possible Companion, Using Machine Learning},
  author = {Jakob Roche},
  year   = {2024},
  eprint = {2405.05282},
  archivePrefix = {arXiv},
  url    = {http://arxiv.org/abs/2405.05282v3}
}

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