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Four 2021–2022 TESS transits of TOI-2257 b fit the discovery clock when the transit shape is fixed

We test whether later TESS transits of TOI-2257 b follow the clock from its discovery study. We measure six complete transits in public 120-second SPOC data. Four events in sectors 40, 41, 47, and 53 are later than the discovery data. With the source transit shape fixed, their time offsets are +1.49, +10.26, −4.78, and −6.75 minutes. Residual resampling gives adopted standard errors of 18.62, 15.62, 11.07, and 9.72 minutes. Each offset is smaller than one adopted error. Their weighted common offset is −2.49 minutes. Its estimated standard error is 7.29 minutes when we include the largest source clock error allowed by the published epoch and period errors. Baseline and aperture-flux controls change individual times by at most 1.17 minutes. Selected shape changes can move one time by 14.88 minutes. Independent-residual trials also give wide timing tails. We find no resolved timing change under these shape and noise models. The result does not rule out smaller changes or signals at unobserved epochs. The package contains the original light curves, source hashes, measured times, all simulated errors, control results, figures, and code for a clean offline run.

TOI-2257 b · TIC 198485881 · TESS · transit timing · public data · residual resampling

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References

6
  1. usesdoi:10.1051/0004-6361/202142280

    We use the source clock and transit shape, then test four later TESS events that the source study proposed for follow-up.

  2. doi:10.48550/arXiv.2610.19280

    The model study gives context for further constraints on this planet. We do not test its interior models.

  3. usesdoi:10.17909/t9-nmc8-f686

    The analysis uses eleven public two-minute TESS SPOC light curves. Exact file names, archive URIs, and hashes are in the package.

  4. usesdoi:10.1086/683602

    The batman code calculates exposure-integrated transit shapes.

  5. usesdoi:10.1093/mnras/stt1435

    We convert the source q1 and q2 limb parameters to quadratic limb coefficients.

  6. doi:10.1117/1.JATIS.1.1.014003

    The TESS mission supplies the observations.

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