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Under one reference profile, fixed pixel sums give a larger HAT-P-70 b half-depth width in TESS Sector 98 than in Sector 32

We test a reported HAT-P-70 b transit width increase with new sums of public TESS target pixels. The main rule uses a fixed circular aperture of radius 2.5 pixels and a local residual background estimate. The background pixels are selected from images outside transit. The extraction tests use common samples and weights within each sector. Each event has its own fitted center, depth scale, and linear baseline. A common asymmetric reference gives half-depth widths of 182.40 minutes in Sector 32 and 187.38 minutes in Sector 98. These visits cover 2020 and 2025–2026. The increase is 4.97 minutes, or 2.73%. We resample nine and twelve whole transits and refit the reference in 400 trials. The conditional 95% interval for the increase is 2.99 to 6.73 minutes. All tested aperture and background choices give positive differences. Omitting the local subtraction gives 4.40 minutes. Adding the pipeline background model back before local subtraction gives an exact duplicate. The stored model has no spatial variation in each retained stamp. It is not an independent check. Noiseless input differences of 0 and plus or minus 5 minutes are recovered to within 0.0028 minute. The result retains the earlier light-curve signal under fixed pixel sums. It shares TESS pixel calibration and does not measure errors common to a sector. A half-depth width is not a contact duration. The study does not establish orbital precession. The package preserves exact selected pixels, source hashes, comparison light curves, code, all resample draws, results, and figures. A fresh run gives identical bytes for 13 result files.

HAT-P-70 b · TESS · target pixel files · transit photometry · half-depth width · aperture photometry · background subtraction · reproducible research

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References

5
  1. supportsSpline fits give larger HAT-P-70 b half-depth widths in TESS Sector 98 than in Sector 32 sci:sha256:84b2d7ea0656b6874fe262dad202d25f7486bb51dcda4d2423810ca8d2046b9c

    The new pixel sums retain the positive width difference reported from public light curves. The observations are the same.

  2. usesTwo TESS flux products give different fitted widths for one January 2026 HAT-P-70 b transit under a fixed profile sci:sha256:16c7def968f7683a7d5ef4ea3b067371c8694e8874431a8d712dd409ac370a67

    We copy its MIT profile code and group fit. We also use its verified public light curves and source records.

  3. usesdoi:10.3847/1538-3881/ab36b5

    The discovery study supplies the event locator and physical context for the known planet.

  4. doi:10.3847/1538-3881/ac478f

    This study explains how gravity darkening can change the transit shape.

  5. usesdoi:10.17909/T9-NMC8-F686

    This public TESS collection supplies the target pixel files and SPOC comparison light curves.

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