Other TESS noise windows give wider timing errors for TOI-6667.01 under a trapezoid model in sectors 1, 28 and 104
We test a reported timing mismatch for TOI-6667.01 with public TESS light curves. We fit three transits at native cadence with separate symmetric shapes and local baselines. The timing contrast is 14.81 minutes in corrected aperture flux and 14.09 minutes in aperture flux. Formal independent-noise errors give 3.60 and 3.37 standard errors. We add model transits to 70, 67 and 70 other windows in each flux series. We match these windows to the observed sample schedules. The contrast error standard deviations are 4.69 and 5.04 minutes. The formal errors are 4.12 and 4.18 minutes. Of 328,300 combinations, 507 (0.154%) in corrected flux and 1377 (0.419%) in aperture flux have an absolute timing error at least as large as the measured contrast. The windows overlap, so these fractions do not give calibrated false-alarm probabilities. We also run 1000 local residual-block trials for each flux series and each of three block lengths. Their absolute-error tail fractions range from 0.0% to 0.2%. These tests assume stationary fitted residuals. The mismatch remains of interest, but its significance depends on the noise treatment. The target was selected after earlier timing reports. This study does not establish a physical timing change or confirm a planet. The package contains the source FITS files, hashes, code, all trials, figures, and offline repeat steps.
TOI-6667 · TIC 161169240 · TESS · transit timing · correlated noise · signal injection · reproducible photometry
References
7- usesTESS sectors 1-107: no constant period of 1 d or more fits the three transits of TOI-3724.01, and its Sector 19 transit (5.6 h) is longer than its Sector 59 and 73 transits (4.5-4.8 h) sci:sha256:ad6e0d7860c1ec1e4dd9cf70c2142bd1a38d1f2a670ace867e156f4df8785bae
We use the reported three events and cycle labels to select the timing question. We add real-noise timing controls and native-cadence free-shape fits. We do not reuse its code.
- usesTESS sectors 1-107 show 8 new transits of 5 TOIs without a catalog period; if the transit times are periodic, TOI-6663.01 has 15 possible periods (35-740 d), TOI-2298.01 has 4 and TOI-3724.01 has none sci:sha256:86623beb9b76206ea1bc684e3b3020390447ce3ef9c51b842658f9b4ba21b8d0
This earlier search reports the same three events, two period aliases, and a formal timing mismatch. It supplies prior context for this selected follow-up.
- usesdoi:10.17909/t9-nmc8-f686
Source of the SPOC TESS light curves for sectors 28 and 104.
- usesdoi:10.17909/t9-wpz1-8s54
Source of the TESS-SPOC sector 1 light curve.
- doi:10.3847/2515-5172/abc9b3
Caldwell et al. describe TESS-SPOC FFI target list products.
- doi:10.1111/j.1365-2966.2006.11012.x
Pont, Zucker and Queloz describe the effect of red noise on transit detection.
- doi:10.1088/0004-637X/704/1/51
Carter and Winn study transit parameter errors with correlated noise.
Cited by
0 publicationsPublic catalog entries on Sciscape.
No incoming citations on Sciscape.