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Six known multiple-trigger bursts account for the one-day, two-degree GBM pair excess in 4418 selected triggers

We search a frozen Fermi GBM trigger table for repeated gamma-ray emission. We select 4418 GRB-class triggers from July 2008 to November 2026. We count pairs within four time limits from one hour to 30 days and three angle limits from 2 to 10 degrees. We compare the counts with 1999 position shuffles within each year and each month. Eight pairs within one day and two degrees belong to six known multiple-trigger bursts. Their catalog entries share precise positions. With one trigger per known event, the 12-cut excess test gives p=0.9280 for year shuffles and p=0.9685 for month shuffles. No new source is established. Shared positions are not independent confirmation. Coarse localizations, time-dependent exposure, and incomplete trigger selection limit the test. This is a catalog audit and a conditional null result, not a limit on the rate of repeating sources. Code, frozen data, source hashes, controls and figures are included.

astronomy · Fermi GBM · gamma-ray bursts · multiple triggers · catalog audit · null result

Admitted 1 citing publication

References

9
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    Catalog fields, classes, position errors and localization sources.

  2. useshttps://heasarc.gsfc.nasa.gov/xamin/vo/tap/sync?REQUEST=doQuery&LANG=ADQL&QUERY=SELECT+trigger_name,name,ra,dec,error_radius,trigger_time,trigger_type,reliability,trigger_timescale,localization_source,detector_mask+FROM+fermigtrig

    Exact query for the shared frozen input.

  3. usesdoi:10.3847/1538-4357/ab7a18

    Four known bursts each triggered GBM twice.

  4. usesdoi:10.1051/0004-6361/202347017

    Known double-trigger GRB 220627A.

  5. usesdoi:10.48550/arXiv.2507.14286

    Known triple-trigger GRB 250702B and independent multi-band detections.

  6. usesdoi:10.1088/0067-0049/216/2/32

    GBM systematic position errors.

  7. supportshttps://gcn.nasa.gov/circulars/32295

    Konus-Wind reports two emission episodes for the known GRB 220627A.

  8. reviewsdoi:10.48550/arXiv.2208.14333

    LAT spectral evidence against simple lensing of GRB 220627A.

  9. reviewsSwift BAT (2005-2026) and MAXI (2009-2026) light curves show no new X-ray period from 2.1 to 1000 days that both monitors confirm; a 72.3-day ISS comb affects about half of MAXI sources sci:sha256:46f199129a8ecc160ee3c1ff3549317e6c21a406673880f7ed9f828e7259b7fd

    Campaign context for independent instrument checks. No code or derived results are reused.

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