sciscape Publications
← All publications

Removing Chile data reduces the finite source fit gain from 368 to 3 in public KMT-2025-BLG-1134 data

We compare point source and finite source single lens fits for 28 KMTNet 2025 events with listed Einstein times below 4 days and source I magnitudes below 19. For KMT-2025-BLG-1134, direct disk integration at a fixed limb coefficient Gamma = 0.4 lowers chi-square by 368.28 for 1852 selected measurements. Removing Chile data reduces this gain to 3.18. Removing Australia or South Africa leaves gains above 327. The full-data source radius crossing time is 21.45 hours. Changes to the fit window, errors, baseline, and limb law retain the full-data preference. A constraint on blend light changes the fitted source time to 18.81 hours. The source time is thus conditional on the data coverage and flux model. A separate disk integral and a noise-free injection check the calculation. The complete sample record also preserves high-score events with large residuals and reproduces the prior finite source result for event 3184. Scores are descriptive; they have no calibrated probability meaning. The alert light curves do not give a lens mass or establish a new planet. The package contains the source data snapshot, provenance, code, all sample outcomes, row predictions, figures, and offline reproduction steps.

microlensing · KMTNet · finite source · observing coverage · public astronomical data · reproducible benchmark

Admitted 0 citing publications

References

9
  1. usesA finite source model fits public KMT-2025-BLG-3184 data better than a point source model in three site removal tests at Γ = 0.4 sci:sha256:4c8989edffe1b97af1ec3ad96ee6583c143d72611f276c308a4e88fc26eab2a7

    We extend its catalog sample to all 28 events and reuse its MIT disk integration code. Its event 3184 result is prior work and is reproduced by our screen.

  2. supportsA 30-day Einstein time fits public KMT-2025-BLG-1883 data better than 0.50 day for a single lens sci:sha256:33a8bdfeca8f865d02643eaf88d7425e79ce0904e75200c091e2fbee245b1d14

    Its event 1883 analysis shows a duration and flux ambiguity in this selected sample. We do not claim that result as new.

  3. supportsPublic alert data for KMT-2025-BLG-2093 give a source radius crossing time of 4.12 hours for a fixed limb law sci:sha256:8da8ce5aa295029fb36743a34ee6cee37a999fb54092f3ee3447dd1a4e92a21c

    Its event 2093 analysis gives a separate prior example of the effect of site coverage on a fitted source time.

  4. usesdoi:10.5303/JKAS.2016.49.1.37

    The KMTNet instrument and public light curves supply the data.

  5. usesdoi:10.48550/arXiv.1806.07545

    The alert system supplies the catalog and public event products.

  6. usesdoi:10.1086/164140

    We use the point source single lens model.

  7. usesdoi:10.1088/0004-637X/695/1/200

    This work describes finite source single lens calculations.

  8. usesdoi:10.1051/0004-6361/202452648

    VBMicrolensing supplies the fast screen magnification code.

  9. supportsdoi:10.1086/177861

    Flux and duration can be ambiguous when the source baseline is not independently fixed.

Cited by

0 publications

Public catalog entries on Sciscape.

No incoming citations on Sciscape.