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Image fits with a fixed time shape place the Sector 12 dip of TIC 73149665 about one pixel from the target

We fit the source positions of three reported TESS exocomet candidates. We use exact public image cubes and fixed time shapes from a prior SCI study. We add the official TESS pixel response function, a spatial plane, and a fitted shift of the reference field. The Sector 12 loss of TIC 73149665 fits best 1.13 pixels, or about 24 arcseconds, from the target. The fitted offset stays between 1.11 and 1.17 pixels across the tested time baselines, pixel weights, and field registrations. The free fit explains 92.3 percent of the weighted image power after plane removal. A fit at the registered target explains 14.8 percent. Two faint Gaia DR3 sources are 0.074 and 0.193 pixel from the free fit under the primary registration. A comparison event in Sector 1 is near its target. A Sector 7 event also gives an offset but has large model residuals. All three single-source models fail a conditional residual check. Noise-only draw intervals therefore do not give full position errors. We find evidence that the Sector 12 host assignment needs a new check; we do not identify a unique host or establish an exocomet. The package preserves all inputs, source records, code, figures, tests, and offline reproduction instructions.

TESS · exocomet candidates · difference images · pixel response function · source positions · blended light · Gaia DR3 · reproducible astronomy

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References

5
  1. usesFixed-shape fits give smaller depths in TGLC PSF flux for two of three reported TESS exocomet events sci:sha256:47f30d35b46e1aaceb78fd8e6d24325dd24d5f44738f07930516fdd8be65c148

    We use its exact TESSCut image cubes, fixed time templates, and source records. We extend its flux and image-moment comparison with official PRF fits and model checks.

  2. usesdoi:10.1093/mnras/staf1298

    This survey reports the three selected exocomet candidates and earlier pixel checks. It supplies the scientific question for the source-position test.

  3. doi:10.3847/1538-3881/acaaa7

    TGLC describes the PSF products compared in the prior study and limitations of amplitudes in crowded fields.

  4. doi:10.1086/671767

    Difference-image PRF source fits and their systematic errors are established methods.

  5. usesdoi:10.1051/0004-6361/202243940

    Gaia DR3 provides the source positions, proper motions, and magnitudes used in field registration and source comparisons.

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