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Public TESS data give 19 transit times for TOI-2525 b and c in 2023–2025

We measure 19 transit centers for the two known planets TOI-2525 b and c in public TESS data from 2023–2025. These 13 times for b and six times for c are absent from the two published timing tables checked in this study. We use all 27 public SPOC light curves at 120-second cadence returned for TIC 149601126. The median statistical errors are 4.9 minutes for b and 3.9 minutes for c. We require data across both transit edges and the nearby baseline. We also check older transits and insert 64 test transits into real flux. A two-planet model fits only 32 historical transit times. It fixes the published masses and orbit shapes, and adjusts four initial phase and period values. Its later residual RMS is 10.6 minutes for b and 11.0 minutes for c. The event search starts within 0.4 day of this model. These results apply to the accepted observed events. They do not test the full published orbit distribution or establish another planet. The package includes the source samples, file hashes, code, failed first-pass results, figures, and a separate repeat-run check.

TOI-2525 · TIC 149601126 · TESS · transit times · transit timing variations · public astronomical data · reproducible research

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References

6
  1. usesdoi:10.17909/T9-NMC8-F686

    We use 27 public TESS SPOC target light curves at 120-second cadence. The exact source URLs and file hashes are in the package.

  2. usesdoi:10.3847/1538-3881/acba9b

    We use the 32 historical times in Table A2, the rounded best orbit values in Table A3, and limb darkening in Table A1. We compare the older measured times with Table A2.

  3. usesdoi:10.48550/arXiv.2606.17218

    We compare the target times in Table 4 of arXiv version 1. All 19 later times reported here are absent from that table.

  4. usesdoi:10.1086/683602

    We use batman to compute finite-exposure transit shapes.

  5. usesdoi:10.1051/0004-6361/201118085

    We use REBOUND to integrate the two-planet model.

  6. usesdoi:10.1093/mnras/stu2164

    We use the IAS15 integrator and check the effect of a smaller integration tolerance.

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