Non-transiting exoplanets as a means of understanding star–planet interactions in close-in systems

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Volume 699 (July 2025)

A&A, 699 (2025) A226

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Table A.1

Candidates with a contaminant located at least 10” away and less than 40” away from the considered star

KIC	Gaia ID	Contaminant Gaia ID	distance
3222610	2099534981005352576	2099535015365093120	17.88
5731359	2073820977455843200	2073821183614272256	16.51
5938531	2104466423796556160	2104466423796548992	19.02
6370174	2077612883814892160	2077614361283648128	20.54
7511885	2105555322564080384	2105555322564081664	18.85
7882472	2103046030870052224	2103046030870053760	18.29
10027247	2086316205543022336	2086316205543023104	14.29
10291936	2086348091380882688	2086348160100359808	13.29
11408355	2134998079291667968	2135001034229167232	11.04
11605209	2132673883508778880	2132673883508775168	18.45
…	…	…	…

Notes. Only the 10 closest contaminants are shown in this table. Gaia ID is the correponding Gaia ID of the Kepler star. The distance, measured as the angular separation between the star and the contaminant, is expressed in arcseconds.

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