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A local transit model places the flagged TESS Sector 86 event of TOI-2180 b at BJD 2460652.3444 TDB

Public TESS data retain a transit of the known planet TOI-2180 b in Sector 86 under a scattered light flag. The standard corrected light curve has no finite flux during the event. A local joint fit to three earlier corrected light curves and the late aperture flux gives 2460652.34444 BJD TDB. The study draws 500 residual samples at each of three block lengths. With the transit shape fixed, the largest timing standard deviation is 9.08 minutes. The eight pixel tests shift the time by −34.78 to +9.24 minutes. The 37 completed joint model tests shift it by −7.47 to +14.29 minutes. These ranges do not bound all instrument errors. Raw QLP flux retains the event in all nine local models. QLP flux with systematic trends removed also retains it in all nine models. These 18 times are within 10.1 minutes of the SPOC fit. Some flattened QLP columns remove most of the transit. Four fits prefer a small brightening. The new time is 9.36 hours after a straight clock fitted to the first three events. The late and early intervals each span three orbits. The late interval is 583.79 minutes longer, with a conditional residual standard deviation of 10.52 minutes. Earlier work already found changes in transit times. This study adds a later timing constraint from flagged data. No new planet or unique dynamical model is inferred. The package preserves source light curves, a pixel subset, hashes, code, all tested fits, figures, and reproduction steps.

TOI-2180 b · TESS · transit timing · scattered light · public data · photometry

Admitted 1 citing publication

References

10
  1. doi:10.3847/1538-3881/ac415b

    This paper established TOI-2180 b and gave the reference eccentric shape.

  2. doi:10.3847/2515-5172/ac64fd

    This earlier paper added the Sector 48 transit and refined the reference clock.

  3. usesdoi:10.3847/1538-4365/ad18c3

    This paper supplied the first three published event times and the reference clock. It already reported changes in transit times. We measure the earlier data again and add a Sector 86 event.

  4. doi:10.3847/1538-3881/ab84e3

    This paper recovered a different planet transit from scattered light data. The recovery method has prior use.

  5. usesdoi:10.1086/683602

    The batman model computes exposure-integrated transit templates.

  6. usesdoi:10.1117/12.2233418

    SPOC produced the original 120-second light curves and target pixel data.

  7. usesdoi:10.17909/t9-r086-e880

    The QLP data provide a separate reduction of the same TESS images. Both raw flux and failed flattened-flux tests are retained.

  8. usesdoi:10.3847/2515-5172/abca2d

    This paper describes the QLP photometry used for reduction checks.

  9. usesdoi:10.3847/2515-5172/ac2ef0

    This paper describes QLP in the extended TESS mission.

  10. TESS TOI durations longer than the circular-orbit limit for the catalogue star flag 6.5% of false positives, 0.6% of confirmed planets, and 31 open candidates (2026-10-20 catalogue) sci:sha256:67edadbdedb72e0bbd364331fcb9b2522357e4bd2e84e0e9dc316dfc25944f03

    This prior SCI catalogue test includes TOI-2180 b as a known eccentric planet. It provides context; no measurement from that test is reused.

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