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Five TESS visits leave 5.41% of phases unobserved for a circular central GJ 357 d model at 55.661 days and 1.5 Earth radii

We test transit coverage for GJ 357 d with five public TESS visits. We use 75,104 selected 120-second samples from sectors 8, 35, 62, 89, and 99. The planet model is circular and central. Its radius is 1.5 Earth radii. Its period is 55.661 days. Five visits leave 5.41% of midpoint phases without selected exposure overlap. The first three visits leave 17.12% unobserved. Four visits leave 5.54% unobserved. Gaps remain at all 901 tested periods from 55.4 to 55.85 days. We also add 512 signals for each of three impact parameters at 55.661 days. Five visits recover 477 central signals, 392 at impact parameter 0.8, and none at impact parameter 1.0. Recovery requires a matched phase and a scaled box-search score of at least 8. A separate post hoc check uses the quoted 2019 marginal period and epoch ranges as a coordinate box. Five visits overlap every central-model epoch at all 221 tested periods in this box. At its nominal period, all 256 added central signals are recovered. The quoted 2026 box still has observation gaps. The primary real-data search has maximum score 6.01, below the fixed threshold. We hold stellar parameters fixed and add circular signals to delivered SPOC flux. These tests do not measure a joint orbit probability or signal loss before the delivered product. The package contains original FITS files, input hashes, full trial tables, code, and figures.

GJ 357 d · TESS · transit search · observation windows · signal injection · grazing transit · public data

Admitted 1 citing publication

References

11
  1. usesTESS sectors 21 and 48 recover added circular 3-Earth-radius HD 86728 b transits at all 256 tested phases for impact parameters 0, 0.5, and 0.8 sci:sha256:1414559d98e85edf44f9fd7d7c735642e676553bdb28e47f61c75d96ec04c091

    We adapt the local linear filter, noise scaling, search, and signal injection code. We keep its MIT notice.

  2. usesFive TESS sectors leave 6.3% of phases unobserved for a circular central GJ 887 d transit model at 50.77 days and 2.29 Earth radii sci:sha256:a1add1aa4b929c55e8d7e1fb161f6b7e693d94b0841bcfd079f26bfdfdfdeca7

    We use its exposure interval method and its separate treatment of coverage and signal recovery.

  3. usesdoi:10.17909/t9-nmc8-f686

    We use five public TESS SPOC 120-second light curves. The input manifest identifies each file and data release.

  4. usesdoi:10.1051/0004-6361/201935801

    We use the 2019 period and conjunction epoch as one orbit reference.

  5. usesdoi:10.3847/1538-3881/acff5a

    This prior transit test uses sectors 8, 35, and 62. We add phase coverage and signal recovery maps.

  6. usesdoi:10.48550/arXiv.2609.30552

    This preprint uses sectors 8, 35, 62, and 89. We use its fixed star and limb parameters, planet b mask, and second orbit reference.

  7. usesdoi:10.1086/683602

    We calculate exposure-integrated quadratic-limb transit models with batman.

  8. usesdoi:10.1051/0004-6361:20020802

    We use the box least-squares search method through Astropy.

  9. usesdoi:10.3847/1538-4357/ac7c74

    We use Astropy for FITS data and the box search.

  10. doi:10.1117/1.JATIS.1.1.014003

    This paper describes the TESS mission.

  11. doi:10.1117/12.2233418

    This paper describes the TESS science data pipeline.

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