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Extra aperture samples increase coverage for at least two central model transits at Barnard e's period in 120-second TESS Sector 80 data

We tested how missing samples and flux correction affect transit recovery in the public 120-second TESS Sector 80 light curve of Barnard's Star. We compared full aperture flux, aperture flux at corrected-flux times, and corrected flux. The full aperture series retains 4,691 extra samples. We ran 221,184 injection trials across four measured periods, four paths, nine radii, 512 paired phases, and three data selections. At the 6.7392-day period, 4,656 of 4,853 tested central-transit epochs have at least two usable events in full aperture data. Only 4,190 pass at the common times. Thus, extra samples raise tested phase coverage from 86.34% to 95.94%. This result uses the duration of a fixed 0.60 Earth-radius template and stated event coverage tests. Every tested epoch at the other three periods passes the coverage rule. Corrected flux has 16.1% lower measured point noise. Recovery also depends on the signal radius, path, baseline fit, and selected threshold. No observed trial reaches its data selection's screening threshold. The earlier literature already reported no transit evidence in this sector. The contribution is the paired recovery data and the separation of sample coverage from measured flux effects. These fractions count tested models; they are not planet transit probabilities. Injections occur after archived pipeline processing, so the tests do not measure transit loss during that processing. The package includes the unchanged source file, provenance, code, all search and injection scores, numerical checks, controls, and figures.

Barnard's Star · TESS · transit recovery · public data · sample coverage · TIC 325554331 · Sector 80

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References

8
  1. usesdoi:10.17909/xje9-q142

    The public Sector 80 120-second SPOC light curve is the original data input. The package preserves the FITS file, archive requests, and its hash.

  2. usesdoi:10.1051/0004-6361/202452450

    This prior study already searched the sector for transits. It supplies the fixed stellar mass, radius, and limb darkening used here. The new contribution is the paired recovery data and the sample-coverage control.

  3. usesdoi:10.3847/2041-8213/adb8d5

    Table 3 supplies the four central planet periods. This study fixes those values and does not use the full radial velocity posterior.

  4. doi:10.1093/mnras/stag1207

    This recent study concerns the stability and physical evolution of the four-planet system.

  5. usesdoi:10.1086/683602

    The batman package calculates exposure-integrated transit models with quadratic limb darkening.

  6. usesdoi:10.1117/1.JATIS.1.1.014003

    The NASA TESS mission collected the observations.

  7. usesdoi:10.1117/12.2233418

    The SPOC pipeline produced the archived aperture and corrected light curves.

  8. usesTESS sectors 105 and 106 show no event above the tested transit threshold in HD 20794 sci:sha256:fdb4c91a2f997ac2b427894b0a52531f187d9b68f98982da6f03983ec13a4990

    Method context for local baseline fits and explicit recovery tests. This study does not reuse its code or data.

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