The Enigmatic and Ephemeral M Dwarf System KOI 6705: Cheshire Cat or Wild Goose?
Eric Gaidos, Andrew W. Mann, Megan Ansdell

TL;DR
This paper investigates a mysterious periodic signal in Kepler data, ultimately suggesting it is a false positive caused by detector issues rather than a planet or dust disk around an M dwarf star.
Contribution
The study rules out planetary and dust disk explanations for KOI 6705.01 and identifies charge transfer inefficiency as the likely cause of the false positive signal.
Findings
The star is an older mid M-type dwarf with infrared excess suggesting a dust disk.
The transit-like signal's properties are inconsistent with a planetary origin.
Charge transfer inefficiency in the detector likely caused the false positive.
Abstract
We confirm a 0.995 d periodic planetary transit-like signal, KOI 6705.01, in the Kepler lightcurve of the star KIC 6423922. Optical and infrared spectra show that this star is a mid M-type dwarf with an effective temperature K, metallicity [Fe/H] , radius , and mass . The star is pc away and its space motion, rotation period, and lack of H emission indicate it is an older member of the "thin disk" population. On the other hand, the star exhibits excess infrared emission suggesting a dust disk more typical of a very young star. If the KOI 6705.01 signal is produced by a planet, the transit depth of 60 ppm means its radius is only , or about the size of the Moon. However, the duration (~hr) and time variation of KOI 6705.01 are…
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