Loose Ends for the Exomoon Candidate Host Kepler-1625b
Alex Teachey, David Kipping, Christopher J. Burke, Ruth Angus, and, Andrew W. Howard

TL;DR
This study critically examines the exomoon candidate in Kepler-1625b, exploring alternative explanations, data reduction differences, and the star's activity, ultimately questioning the original exomoon claim.
Contribution
It provides a detailed re-analysis of the Kepler-1625b data, highlighting the impact of data reduction methods and systematic effects on exomoon detection claims.
Findings
Flexible trend models can attenuate the exomoon signal.
The probability of a Neptune-sized planet causing the dip is less than 0.75%.
The star shows no significant stellar rotation period or false-positive signals.
Abstract
The claim of an exomoon candidate in the Kepler-1625b system has generated substantial discussion regarding possible alternative explanations for the purported signal. In this work we examine in detail these possibilities. First, the effect of more flexible trend models is explored and we show that sufficiently flexible models are capable of attenuating the signal, although this is an expected byproduct of invoking such models. We also explore trend models using X and Y centroid positions and show that there is no data-driven impetus to adopt such models over temporal ones. We quantify the probability that the 500 ppm moon-like dip could be caused by a Neptune-sized transiting planet to be < 0.75%. We show that neither autocorrelation, Gaussian processes nor a Lomb-Scargle periodogram are able to recover a stellar rotation period, demonstrating that K1625 is a quiet star with periodic…
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