The Detection of KIC 1718360, A Rotating Variable with a Possible Companion, Using Machine Learning
<|reference_start|>The Detection of KIC 1718360, A Rotating Variable with a Possible Companion, Using Machine Learning: 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.<|reference_end|>
@article{roche2024the,
    title={The Detection of KIC 1718360, A Rotating Variable with a Possible
  Companion, Using Machine Learning},
    author={Jakob Roche},
    journal={arXiv preprint arXiv:2405.05282},
    year={2024},
    archivePrefix={arXiv},
    eprint={2405.05282},
    primaryClass={astro-ph.EP astro-ph.IM cs.LG}
}