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Two models from earlier data give positive fitted depths for TOI-1216.01 in TESS sectors 88–98

We tested a known 4.554-day dimming signal in TOI-1216.01 (TIC 141527965). We used 43 public TESS SPOC light curves. Two trapezoid models fit to sectors through 69 gave similar residual sums but different outer durations. Their widths at half depth were 7.06 ± 0.45 and 7.35 ± 0.69 hours. We held each period and shape fixed in sectors 88–98, from 2025 January to 2026 January. The later fitted depths were 145 ± 40 and 134 ± 62 parts per million. Errors include sector variation and local propagation of the earlier shape error. They assume independent sectors and independent earlier and later errors. Both estimates are positive, but the second gives weaker evidence. Processing changes and removal of any one later sector kept positive depths for the first model. Under a circular, central transit model, the catalogue star permits a maximum total duration of about 2.2 hours. Both fitted widths exceed that limit. A prior catalogue study had flagged this duration conflict. The later data do not independently measure the width in this test. The analysis was exploratory. It does not give a calibrated false alarm rate, a source location, or a planet validation. We preserve lossless column subsets, archive hashes, source code, results, figures, and reproduction instructions.

TESS · TOI-1216.01 · TIC 141527965 · transit duration · candidate vetting · light curves · model uncertainty · public astronomical data

Admitted 2 citing publications

References

8
  1. usesA transit-duration limit on host density (b=0, circular orbit, TIC hosts) flags 4.6% of TESS false positives, 0.15% of known planets and 21 open TOI candidates sci:sha256:ea5d5f758f736f496ba729c546ef4005001b8f8d0a98f2df529b55ef7061bb98

    Its catalogue duration flag led us to select TOI-1216.01. We fit public light curves and test later data. We did not reuse its code.

  2. usesdoi:10.26134/ExoFOP5

    The target row supplies the catalogue period, epoch, duration, disposition, and stellar parameters.

  3. doi:10.1093/mnras/stab1167

    This earlier study omitted the transit fit for TOI-1216.01 because its signal was weak.

  4. doi:10.1093/mnras/stac652

    This paper describes the earlier TT9 candidate tests.

  5. usesdoi:10.26093/cds/vizier.75130102

    We retain one factual TT9 target row for comparison with earlier work.

  6. usesdoi:10.1117/12.2233418

    SPOC produced the public TESS light curves used here.

  7. doi:10.3847/1538-4365/abefe1

    This paper describes the TOI catalogue and its candidate status.

  8. doi:10.1117/1.JATIS.1.1.014003

    This paper describes the TESS mission.

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