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Trials recover transits of 1.8 Earth radii at all 240 grid points in TESS sectors 50–52 of GJ 3942 under a uniform star model

We test transit sensitivity near the 6.905 day period of GJ 3942 b. The data are TESS SPOC sectors 50–52. A box search from 6.785 to 7.025 days gives a maximum depth score of 9.44 at 6.9954 days. Of 200 shifted controls, 63 reach or exceed that score. This result does not support a transit detection. We then insert 1,440 trial transits before the study trend filter. Under a circular orbit and a uniform star model, all 240 trials at 1.8 Earth radii pass the timing check. Their scores also exceed every shifted control. The grid has three periods, 40 phases, and impact parameters of 0 and 0.8. The fixed star mass and radius are 0.63 solar masses and 0.61 solar radii. A separate test uses the original exposure times and assumed limb darkening. In that test, 119 of 120 trials exceed every control; all 120 pass the timing check. These tests measure sensitivity after mission processing. They do not give a general limit on the planet radius. The package includes original data, source queries, code, trial results, figures, and repeat instructions.

GJ 3942 · TESS · transit search · injection recovery · correlated noise · radial velocity planets · public astronomy data

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References

7
  1. usesdoi:10.1051/0004-6361/201731307

    This paper gives the planet period and the fixed star mass and radius. It also gives the trial radius examples.

  2. usesdoi:10.17909/t9-nmc8-f686

    The four original TESS SPOC light curves come from this public data collection.

  3. usesdoi:10.1117/12.2233418

    The SPOC pipeline produced the source light curves.

  4. usesdoi:10.1051/0004-6361:20020802

    We use box least squares through the Astropy implementation.

  5. usesdoi:10.3847/1538-4357/ac7c74

    Astropy reads the FITS data and runs the box search. The package version is fixed in the source files.

  6. doi:10.48550/arXiv.2411.05476

    This prior study uses these TESS data to examine star rotation.

  7. No transit template reaches a score of 8 near HD 48948 b's period in TESS sectors 20, 60, and 73 sci:sha256:7d32ac50b3d7e35d7c80710824f2a3fe901763d34276ef395ac7b376c6e3d785

    This related study tests transit sensitivity for another radial velocity planet. We use independent code and add shifted controls.

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