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A fit with a fixed shape places the 2024 TOI-4633 c transit within the errors of a forecast from two early events

We measure the 2024 TESS Sector 80 transit of TOI-4633 c and test a forecast from clean events in Sectors 20 and 40. The later time is BJD_TDB 2460496.46130. It is 22.4 minutes before the early forecast. With a fixed symmetric shape, residual block resampling gives standard deviations of 39.1 to 42.0 minutes for this difference. All four block settings have percentile ranges that contain zero. Their outer endpoints are -106.7 and +70.0 minutes. The test does not show a robust timing departure. Sector 50 has no valid corrected flux through the event and is excluded from the primary clock. Changes to the local background and window have small effects. Transit shape and flux correction have larger effects. A SAP test gives an offset of -121.6 minutes with a 64.7-minute standard deviation and a percentile range that contains zero. A conditional fit to the three clean times gives a period of 271.93904 days with a 0.00193-day standard deviation. These errors omit shared shape uncertainty and unknown calibration effects. The public archive already lists a revised period, so this is an independent timing and sensitivity record. It is not a new planet or a first report of the fourth event. We preserve four original FITS files, source queries, hashes, code, figures, trial draws, and repeat instructions.

TOI-4633 c · TIC 307958020 · TESS · transit timing · ephemeris · residual block bootstrap · data quality · public data

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References

8
  1. usesdoi:10.3847/1538-3881/ad1d5c

    This paper gives the planet discovery, the three early transit sectors, and the shape parameters used for our fixed template. It also describes the Sector 50 scattered-light problem.

  2. usesdoi:10.17909/t9-nmc8-f686

    We use four original public TESS SPOC light-curve files from MAST. The package gives their exact product records, URLs, and hashes.

  3. doi:10.1117/1.JATIS.1.1.014003

    This paper describes the TESS mission that collected the source data.

  4. doi:10.1117/12.2233418

    This paper describes the SPOC pipeline that produced the source light curves.

  5. usesdoi:10.1086/683602

    We use batman to compute the transit templates with exposure integration.

  6. usesdoi:10.1093/mnras/stt1435

    We use the conversion from q1 and q2 to quadratic limb coefficients.

  7. doi:10.48550/arXiv.2501.05506

    This later study gives binary-system stability work. It does not give a new Sector 80 transit time.

  8. doi:10.48550/arXiv.2608.29140

    This later study gives binary-system dynamics work. It does not give a new Sector 80 transit time.

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