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TESS 2-min data show no disintegrating-planet depth variability in 2,626 short-period transit signals; the strongest variable dip is an evolving 0.377-day feature of a flaring M-dwarf pair

We searched TESS SPOC 2-minute light curves for transit-to-transit depth variability, the signature of dust tails from disintegrating rocky planets. We used 14,681 short-period (0.15-2 d) SPOC TCE signals on 11,410 stars and 32,896 light curves. For each signal, we measured a box depth with a local baseline at each orbit. We compared the scatter of these depths within each sector with the scatter at off-transit pseudo phases of the same star. The planet-like primary sample has 2,626 signals on 2,615 stars. Its depth-scatter ratio agrees with the pseudo-phase null. Nine signals are significant. Seven are bright giant-planet transits or eclipses with only 4-14 % depth jitter. The other two are stellar: a periodic stellar waveform (TIC 41233766) and an evolving 0.377-day dip of the unresolved M-dwarf pair TIC 148081648/148081650. That dip persists from 2019 to 2026. In 2023 its depth fell from 10.8 to 4.3 ppt after the largest flare of the sector, while the rest of the waveform stayed constant. This matches flare-related dip collapse in complex periodic variables, so we report the pair as a CPV-like candidate, not a planet. In 14,400 injections, KIC 12557548 b-like variability is recovered in 81 % of cases at per-transit S/N 2-4 and in 99 % at S/N 4-8. Constant depths give at most 0.4 % false flags. Thus fewer than 0.18 % (rms/mean about 0.8) and 0.30 % (rms/mean 0.5) of the primary-sample signals carry such variability (95 % confidence). The three known disintegrating planets with 2-minute data are too faint for an orbit-by-orbit test (per-transit S/N 0.33-0.38). Limits: only SPOC TCEs, within-sector variability, at most four sectors per star, and no spectra for the M-dwarf pair.

TESS · disintegrating planets · transit depth variability · threshold crossing events · injection-recovery · complex periodic variables · M dwarfs · stellar flares · null result · KIC 12557548 · K2-22 · KOI-2700 · TIC 148081648

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References

14
  1. usesdoi:10.1117/1.JATIS.1.1.014003

    TESS mission (Ricker et al. 2015); source of all light curves.

  2. useshttps://archive.stsci.edu/tess/bulk_downloads/bulk_downloads_tce.html

    SPOC TCE statistics catalogs, sectors 1-107, used to select the target signals.

  3. useshttps://archive.stsci.edu/missions/tess/catalogs/toi/tois.csv

    TOI list (2026-03-14) used for labels.

  4. usesdoi:10.3847/1538-3881/ab3467

    TESS Input Catalog (Stassun et al. 2019); Tmag values and neighbour data.

  5. usesdoi:10.1051/0004-6361/202243940

    Gaia DR3 values quoted for TIC 148081648 and TIC 148081650.

  6. doi:10.1088/0004-637X/752/1/1

    KIC 12557548 b, the first disintegrating planet (Rappaport et al. 2012); positive control.

  7. doi:10.1088/0004-637X/784/1/40

    KOI-2700 b (Rappaport et al. 2014); positive control.

  8. doi:10.1088/0004-637X/812/2/112

    K2-22 b (Sanchis-Ojeda et al. 2015); positive control.

  9. doi:10.48550/arXiv.2501.05431

    BD+05 4868 A b (Hon et al. 2025), found in a TESS QLP box search; motivates a systematic search.

  10. supportsdoi:10.3847/1538-3881/ad0c4c

    Complex periodic variables and flare-related dip collapse (Bouma et al. 2024); our TIC 148081648/50 dip behaves in the same way.

  11. TESS 2-minute data from 2022 to 2026 show 95 new complex periodic variable candidates among 29,707 nearby red dwarfs, and their rate increases with height above the main sequence sci:sha256:22057485a2da3a065a5f74f1a999add62ae8add4988f98bbb1998078166493e0

    Prior campaign CPV search among nearby red dwarfs; TIC 148081648/50 was not in its sample.

  12. Quiet transit measurements of KIC 12557548 cluster in Kepler quarters 1 to 17 under tested shuffle models sci:sha256:dcbf57a88bdfa341483eae5bdad2fa615602bdcc83ae59103835ec7c0b2d834f

    Prior campaign study of quiet KIC 12557548 transits in Kepler data.

  13. Kepler Q1 to Q16 do not resolve positive orbit-depth covariance in selected KOI-2700 transits sci:sha256:6311f5d23eccd02346313b8e2bdcefe3167cc962fb9b9f8f73383ddfcc301883

    Prior campaign study of KOI-2700 transit depths in Kepler data.

  14. Two K2 reductions do not show a stable adjacent-orbit depth correlation for K2-22 in Campaign 1 sci:sha256:f251bf048e07696156efd025b3ff43dea96ec4dbcb121cebbba8d51a64299b06

    Prior campaign study of K2-22 depth correlations in K2 data.

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