A companion depth correction with gain one increased the mean Q10–Q16 error ratio for 22 selected Kepler targets
We tested whether one planet can supply a transit depth correction for another planet at the same Kepler target. Fixed precision and coverage rules select 22 pairs with confirmed archive labels. Q2–Q9 sets each planet's constant and four season means. Q10–Q16 supplies 136 paired quarter measurements. The correction adds the companion's later depth residual with gain one. Against the recipient season baseline, the geometric mean RMSE ratio is 1.282. Its conditional 95% target bootstrap interval is 1.095–1.502. Only 6 of 22 targets have less error. The matched constant comparison gives 1.289, with an interval of 1.110–1.508. Every planned alternative rule gives a mean ratio above one, although some intervals include one. Simulations show that the same code removes a strong shared change and adds noise when that change is absent. An independent parser checks all 69,914 depth records against the original catalog. The package saves inputs, source hashes, the local plan, code, selection records, predictions, checks, and figures. The test uses full-mission catalog templates, flags, and current planet labels. It measures later catalog estimation error in a selected sample. It does not establish a physical cause or a new planet.
Kepler · transit depth · multiple planet systems · calibration · seasonal variation · reproducible benchmark
References
9- usesSeason offsets reduce Q10–Q17 depth errors for 15 of 19 Kepler signals selected from Q2–Q9 catalog data sci:sha256:40547a5271a3ab0a6a92cac20ab3e0b220a050bbeaade9c1c36335e4d4982411
We reuse the frozen Holczer depth extract, KOI metadata, NASA planet labels, and original source records. We test a new transfer of later residuals between planets at one target.
- usesSeason means reduce the aggregate depth forecast error for 193 selected Kepler signals in Q13–Q16 sci:sha256:123e4206ce4d16989815979de0abc7ddbf4fe0452852ea11143fe900a065ae42
We reuse the NASA FITS header prefixes, quarter limits, and source records. We recalculate the limits and retrieve three prefixes again.
- usesdoi:10.3847/0067-0049/225/1/9
Tables 2 and 3 supply the transit measurements and depth variation fields.
- usesdoi:10.26093/cds/vizier.22250009
The CDS catalog supplies the original tables and field definitions. Fresh downloads check the saved extract.
- usesdoi:10.26133/NEA4
The NASA Exoplanet Archive supplies target identifiers and confirmed planet labels in the frozen KOI table.
- doi:10.1088/2041-8205/774/2/L19
This study reports yearly transit depth changes at HAT-P-7 b. It supports the need for a season baseline.
- doi:10.3847/1538-3881/ad3807
This study reports four-quarter changes in several Kepler transit depths. It supplies prior context for instrumental depth variation.
- doi:10.1051/0004-6361/201425062
The saved literature review cites its quarter depth changes and crowding correction issues at Kepler-423 b. No measurements are reused.
- doi:10.3847/1538-4365/aab4f9
The saved literature review cites its use of seasonal depth differences in Kepler vetting. No measurements are reused.
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