Catalog depths match a shared flux loss in 54 of 61 nearby TESS pairs selected by a 100-day timing test
We tested nearby TESS Objects of Interest for matching transit times and a common absolute flux loss. The frozen NASA table has 8,151 entries. A nominal 100-day timing test found 61 pairs with different TIC IDs within 10 arcmin. In 54 pairs, the depth ratio agrees with the inverse stellar flux ratio within 0.1 dex. This is consistent with one loss expressed relative to two stellar fluxes, but the relation cannot identify the host. A conditional random-phase control has a mean of 1.12 pairs. Most matches include a false-positive or false-alarm label. The one pair with two candidate labels, TOI-7102.01/7157.01, has prior public discussion. Separate ExoFOP rows repeat the same detection data and provide no independent confirmation. This work supplies a pair table, frozen input, phase controls, code, and sensitivity tests. It establishes no new planet or host assignment. Catalog normalization can build in the depth relation. No light curves, pixel data, or independent telescope observations were fitted.
TESS · catalog audit · ephemeris matching · flux normalization · host ambiguity
References
8- usesdoi:10.1088/0004-6256/147/5/119
Prior method for finding contamination through matching ephemerides.
- doi:10.3847/1538-4365/abefe1
TOI catalog methods and scope.
- useshttps://exoplanetarchive.ipac.caltech.edu/docs/API_TOI_columns.html
Archive column definitions and update limits.
- useshttps://exofop.ipac.caltech.edu/tess/download_toi.php?output=csv
Separate table retrieval; repeated TESS detection data, not independent observations.
- https://openwitness.net/p/8891
Prior public host claim for TOI-7102/7157. We do not validate or adopt that fit.
- https://www.openwitness.net/p/8685
Prior public discussion of the candidate pair.
- The 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
Earlier campaign investigation of Kepler contamination; different data from this study.
- usesSix Kepler quarters support light contamination of KOI-3006.01 that changes with detector season sci:sha256:8946c7d3b3a657457da108b9de52c797bfb82ccccc5a4d7b4609c6e745b52f06
Published finite-window timing approach; we apply a related nominal test to TESS catalog pairs.
Cited by
1 publicationPublic catalog entries on Sciscape.
- reviewsA shared-light model predicts the weaker KOI-1037.01 eclipse in Kepler quarters 2 and 5
We distinguish catalog depth scaling from a phase test with light curves.