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Corrected and aperture TESS flux give dip change ranks of 0.27 and 1.00 for a sector 78 flare in LP 12-502

A sector 78 flare in LP 12-502 gives different dip change ranks in two TESS flux products. The event peaks at BTJD 3436.80991. Its rank among controls at the same rotation phase is 3/11 = 0.273 in corrected flux and 11/11 = 1.000 in aperture flux. This difference appears in a planned check of a flare and dip change test. It remains when both products use the same flare mask. We use 12 public 120-second light curves. The main sample has five sectors after the seven sectors in a 2024 study. We select the largest flare that passes fixed amplitude, partial equivalent duration, inspection, and coverage rules in each sector. Only sectors 78 and 79 supply events. We compare two-rotation median profiles before and after each flare, with a one-rotation guard. We remove two Fourier harmonics and measure the remaining change. The corrected-flux scores are 1.260 and 1.202 parts per thousand. Both are below their control medians. The mean rank is 0.215. An exact test gives an upper-tail probability of 551/608 = 0.90625 under independent uniform event-cycle assignments. In aperture flux the sector 79 rank is 0.000, and the two-event test also gives no evidence for an excess. Artificial dip removals show strong limits from phase and background changes. These data cannot identify the source of the flux-product difference or exclude a wider flare–dip relation. The package contains original FITS files, archive provenance, candidate decisions, code, figures, tables, and reproduction instructions.

LP 12-502 · TIC 402980664 · TESS · complex periodic variables · stellar flares · stellar rotation · periodic dips · conditional randomization · time series

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References

5
  1. usesdoi:10.3847/1538-3881/ad0c4c

    We use its rotation period and phase origin. Its reported flare and dip change coincidences motivate this test. Our event rule differs from its event analysis.

  2. doi:10.48550/arXiv.2609.00136

    This study gives spectra and optical colour tests of complex periodic variables. It describes the later dip profiles of LP 12-502.

  3. usesdoi:10.17909/t9-nmc8-f686

    We use twelve original public SPOC light curves from this TESS data collection. The package preserves archive identifiers and file hashes.

  4. usesdoi:10.1117/1.JATIS.1.1.014003

    The TESS mission supplies the optical data.

  5. Rotation alone does not explain CPV youth: M dwarfs (P < 2 d, d < 150 pc) in groups older than 60 Myr have 3 complex periodic variables where 30 are expected for their period, colour, T and sectors sci:sha256:46217c3d1ee4ed24dbcc3491a57bb8d00dfcf2ac03cfd790f950ada242274574

    This related SCI study tests CPV occurrence and age. Our test concerns flare times and dip changes within one star. We do not reuse its measurements or code.

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