The 2026 transit of TOI-4603 b agrees with a 2021 and 2023 TESS clock under a shared symmetric shape
We test a transit clock for the known planet TOI-4603 b. The clock uses 14 TESS transits from 2021 and 2023. We test its prediction with one transit from January 2026. The later flux does not enter the earlier fit. We fit six public light curves with a shared symmetric shape. Each event has its own depth and baseline. The later transit is 1.33 minutes after the prediction. Its combined conditional standard error is 5.70 minutes. In 100 trials, shifted residuals give a wider timing spread of 6.6 minutes. Five changes to the analysis give residuals from 0.96 to 2.31 minutes. The full fit gives a period of 7.24560648 +/- 0.00001166 days. A quadratic clock gives no evidence for a period change. This is a retrospective test of public data. The archive already lists a revised period. The errors assume fixed noise estimates and the stated shape. The absolute time depends on the shape convention. We preserve native inputs, source hashes, queries, code, results, figures, and offline reproduction instructions. The result adds a later transit measurement and a tested clock. It does not detect a new planet or measure orbital decay.
TOI-4603 b · TIC 437856897 · TESS · transit timing · ephemeris · public data · reproducible astronomy · sector 1751
References
8- usesdoi:10.1051/0004-6361/202245608
Table A.3 supplies the published transit geometry and limb darkening. The discovery clock and data scope supply prior context.
- usesdoi:10.26133/NEA12
Planetary Systems table snapshot accessed 2026-10-23 supplies prior clocks and the clock used to locate windows.
- usesdoi:10.17909/t9-wpz1-8s54
TESS-SPOC light curve of TIC 437856897 in sector 1751 supplies the January 2026 test event. Native file, URL, and hash are preserved.
- usesdoi:10.3847/2515-5172/abc9b3
Describes the TESS-SPOC full-frame-image products used for the test event.
- doi:10.1117/1.JATIS.1.1.014003
TESS mission and public observations.
- doi:10.1117/12.2233418
SPOC processing of the standard TESS light curves.
- usesdoi:10.1086/683602
The batman package generates the common transit templates.
- usesTESS flux from 2021–2024 gives a TOI-2337 b period change of −0.29 ± 1.32 seconds per year with fixed noise estimates sci:sha256:26deff80caa8cc2993fa922bf0c60a6cad060169a4446b999a823404314c5fbb
Its comparison of flux fits with summaries of weak transit times motivates our direct flux fit and profile checks. No code or data are reused.
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