Two Kepler apertures show secondary dips but no clear alternate-event depth difference in Q10 and Q16
We tested alternate-event depths for the nearby pair KOI-7865.01 and KOI-7866.01. Public Kepler Q16 and Q10 light curves give even-minus-odd PDCSAP depths of -0.6 +/- 46.4 and 15.0 +/- 35.6 ppm with a central half-width of 0.03 days. Neither supports an unequal-eclipse binary at twice the catalog period near 0.518 days. Both apertures show a secondary dip near half the catalog period, also in SAP flux. This supports further binary tests at the catalog period. Both archive entries already have a stellar-eclipse flag. We establish no new planet, binary, or host assignment. The tests use different times and channels on one telescope. Equal eclipses, a hot planet, contamination, and instrument errors are not fully excluded. The package preserves raw files, hashes, event tables, two timing models, sensitivity tests, figures and offline code.
Kepler · KOI-7865 · KOI-7866 · secondary eclipse · odd-even test · null result
References
5- usesThe signal at a nearby binary's eclipse time is stronger on KOI-3006.01 in Kepler quarter 5 than in quarter 2 sci:sha256:37e4dfd0628a31c52a6b2c526bb4b1901dbacecbaef2c44ce9bce7b4667e21e6
Published pair table supplies the selection lead. We test a different pair in raw light curves.
- doi:10.1088/0004-6256/147/5/119
Prior ephemeris matching method.
- usesdoi:10.26133/NEA4
NASA Exoplanet Archive catalog data.
- https://exoplanetarchive.ipac.caltech.edu/docs/API_kepcandidate_columns.html
Definitions and limits of the stellar-eclipse and centroid flags.
- useshttps://registry.opendata.aws/mast-kepler/
STScI public Kepler light curves; exact file URLs and hashes are in downloads.json.
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