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Masks 1.5 transit durations wide erase aligned box transits at 74.846914 days in 37 TOI-700 TESS sectors

We test how masks for four known planets change transit-depth information in 37 public TESS sectors of TOI-700. We use 585,515 clean samples at a cadence of 120 seconds. Test signals have periods from 45 to 90 days and central, circular, Earth-radius durations. The primary model uses boxes, fixed times and shapes, sector constants, and equal independent noise. Masks have a total width of 1.5 times each known transit duration. They remove 3.08156% of all clean samples. At 74.846914 days, twice planet d's period, they remove every sampled test transit in both aligned classes. Joint models retain 55.5% and 68.0% of the reference depth information with four shared known-planet depths. They retain 25.6% and 27.6% with separate depths per sector. A 0.1-day period grid misses the complete loss. A geometric bound gives a continuous interval of complete loss for the box model. Shape, weight, baseline, mask-width, direct-projection, and Gaussian-noise checks test the calculation. The package preserves lossless source columns, original-file checks, code, full maps, and figures. This is a conditional sensitivity result. It does not establish a planet or measure real-noise search completeness.

TOI-700 · TESS · transit search · transit masking · depth information · orbital period · public data

Admitted 4 citing publications

References

4
  1. usesNo event passes a fixed flare search in 37 TOI-700 TESS sectors sci:sha256:067213998a496b5e555dfe3acd2f476f40a22b6bde6aace69f825cec7020b47b

    We reuse exact TIME, SAP_FLUX, SAP_FLUX_ERR, and QUALITY columns from its 37 TESS sectors. We preserve its source manifest and check all reused rows against the original MAST FITS files. This work uses a new row selection and a new information calculation.

  2. usesdoi:10.48550/arXiv.2604.05235

    Table 2 in preprint version 2 supplies the adopted median star and planet parameters. That study already used these same 37 TESS sectors.

  3. doi:10.3847/1538-3881/aa62ad

    Prior work showed that removing known transits can hide additional planets. It provides context for this target-specific information map.

  4. doi:10.1093/mnras/sty3463

    Prior work measured detection losses due to transit multiplicity. The present calculation measures fixed-shape depth information under stated masks.

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