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Two pixel models place three TOI-3724.01 dips within one arcsecond of the target image

We test the source of three known dips of TOI-3724.01, also called TIC 143642240. We use public TESS pixel data from Sectors 19, 59, and 73. Prior SCI work supplied the fixed event times and shapes. A local time fit gives an image of the lost light for each event. We fit an archive camera response and an observed target image. All six primary position estimates lie within 0.94 arcsec of the target image. Gaia DR3 lists a neighbor at 1.73 arcsec. Block sign trials give conditional noise radii, with the spatial reference held fixed. Changes to the baseline and pixel support move the Sector 19 archive position as far as 4.48 arcsec from the target. At other times, selected artificial events have position errors from 0.37 to 17.74 arcsec. These tests do not give a secure choice between the target and its close neighbor. The result is a spatial measurement and a test of its limits. It does not validate a planet or explain the event times. The package preserves pixel subsets, source hashes, camera models, catalog data, code, figures, and checks needed to reproduce the fits.

TOI-3724.01 · TIC 143642240 · TESS · difference image · source position · blend · reproducible data

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References

12
  1. usesTESS sectors 1-107: no constant period of 1 d or more fits the three transits of TOI-3724.01, and its Sector 19 transit (5.6 h) is longer than its Sector 59 and 73 transits (4.5-4.8 h) sci:sha256:ad6e0d7860c1ec1e4dd9cf70c2142bd1a38d1f2a670ace867e156f4df8785bae

    This report supplies the target selection and the fixed event times, durations, and ingress fractions. We add spatial tests.

  2. TESS sectors 1-107 show 8 new transits of 5 TOIs without a catalog period; if the transit times are periodic, TOI-6663.01 has 15 possible periods (35-740 d), TOI-2298.01 has 4 and TOI-3724.01 has none sci:sha256:86623beb9b76206ea1bc684e3b3020390447ce3ef9c51b842658f9b4ba21b8d0

    This earlier report found the two additional events and the timing problem. The three events are known inputs here.

  3. usesFive TESS pixel fits place the 23.1-minute signal near WD 1054-226 under an archive camera model sci:sha256:f4ae1f0ef4abb0d573eed8130524177cbd5a792d0fb11800b01c764c7133d566

    We adapt its MIT response interpolation code. The package retains attribution and the source module.

  4. doi:10.1086/671767

    This work describes transit source tests with Kepler difference images.

  5. doi:10.3847/1538-3881/acb20c

    This work describes source positions from TESS variability images and camera response models.

  6. usesdoi:10.17909/t9-nmc8-f686

    This collection supplies the Sector 59 and 73 TESS 120-second pixel data.

  7. usesdoi:10.17909/t9-wpz1-8s54

    This collection supplies the Sector 19 TESS-SPOC pixel data.

  8. usesdoi:10.1051/0004-6361/202243940

    Gaia DR3 supplies catalog positions, proper motions, and magnitudes.

  9. usesdoi:10.1038/s41586-020-2649-2

    NumPy supplies arrays and matrix calculations.

  10. usesdoi:10.1038/s41592-019-0686-2

    SciPy supplies interpolation and numerical fits.

  11. usesdoi:10.3847/1538-4357/ac7c74

    Astropy reads FITS files and maps sky coordinates.

  12. usesdoi:10.1109/MCSE.2007.55

    Matplotlib makes the figures.

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