Early curvature marked 13 of 20 window failures in 711 selected Kepler planets with fixed durations and bounds of three reported timing errors
Can early transit timing curvature warn of later failures of a constant-period forecast? We tested a fixed rule on public timings for 711 selected confirmed Kepler planets at 623 stars. Early fits used expected days at or before BJD 2455700. A failure requires at least three selected later transits outside full windows twice the fixed transit duration. Each center can move favorably by three reported timing errors. A quadratic coefficient divided by its scatter-scaled standard error gave a warning at a score of at least 3. It marked 13 of 20 failures and 24 planets without this outcome. Failure rates were 35.1 percent with a warning and 1.04 percent without one. A quadratic forecast gave 77 failures, compared with 20 for the line. Using only timings with no source outlier flag left 14 failures among 665 planets; curvature marked 12. These are retrospective results conditional on catalog measurements, fixed event numbers, and fixed symmetric durations. The error bounds are not joint confidence levels. The package preserves source bytes, forecasts, selection ledgers, code, figures, and an offline repeat that reproduced all 22 numerical result files byte for byte. No new planet or physical timing signal is claimed.
Kepler · transit timing · observation windows · ephemeris · forecast validation · timing curvature · reproducible research
References
8- usesdoi:10.3847/0067-0049/225/1/9
Source transit timing measurements, total durations, error estimates, quality fields, and known long-term timing labels.
- usesdoi:10.26093/cds/vizier.22250009
CDS distribution of Holczer Tables 2, 3, and 5. Exact numeric source bytes are preserved.
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The frozen cumulative KOI query supplies confirmed status and names. It does not supply fitted periods.
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Prior analysis of period, epoch, and transit prediction errors under strict periodicity.
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Prior catalog work explains the limits from long timing changes on formal Kepler ephemeris errors.
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Related later-data tests of added timing waves. The present test uses a different diagnostic and window outcome.
- Constant period masks need widths above 1.5 durations for 23 of 1,096 selected Kepler planets with fixed event numbers and durations under bounds of three reported errors sci:sha256:a5dc6f3ef68eab01dafe0b170bb13daacb1fa4c21bbc73ebccda7148b2b8cf21
Related duration-relative width bounds for clocks optimized on full records. The present clock is frozen from early rows.
- usesLinear transit predictions with scaled errors had 98.06% mean coverage at three errors in a 70/30 test of 1229 Kepler objects sci:sha256:ccb7c433d9452451054515cecf761ee042fd0dc70d63bcb87e977a89dc05a891
We apply its fixed early adjacent-event correlation warning as a comparison. No code or prepared data is reused. The present outcome is a fixed window relative to transit duration.
Cited by
1 publicationPublic catalog entries on Sciscape.
- Early error medians gave 19.2% lower geometric mean transit interval width than later reported errors in 470 Kepler stars with quality cuts at a 90% target
This prior study of early curvature and Kepler line forecasts informed the original question.