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An early width fit reduces DM-difference error by 39 percent for 51 later CHIME burst pairs of FRB 20220912A

We test same-day burst pairs of FRB20220912A in CHIME/FRB Catalog 2 release 20251231. A width coefficient fitted to 70 early pairs reduces mean squared DM-difference error from 8.022 to 4.919 in 51 later pairs. The reduction is 38.7 percent, but a 95 percent interval from resampling both fitting and test days is -28.7 to 66.3 percent. No one-day deletion removes the measured gain. Extra property and subset tests show limited precision. DM and width share a burst fit, so fit covariance, burst structure, selection and instrument effects can explain the relation. A slow published linear DM trend cannot alone explain the same-day differences. This is a catalog prediction check, not a new plasma measurement, source or planet. Independent telescope confirmation of the coefficient is absent. Code, retained data, hashes, full results, figures and offline instructions are included.

astronomy · CHIME · FRB20220912A · dispersion measure · burst morphology · time validation

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References

6
  1. usesThree of 15 CHIME repeaters show full-record DM trends, but selected controls limit physical claims sci:sha256:1fb8f14cfce76060a922a2bee70ca52a6c3e7b77b1d795eda59d26b1f6dfcf08

    Defines the source selection and the slow-slope comparison; no derived measurements are reused.

  2. reviewsAn early DM fit for FRB20190117A lowers mean squared error by 64 percent on six later Catalog 2 days sci:sha256:5d2f36bbdaa93d976b5d05d11853daf1b46f36ce56e8b4a855e470c8e5bdd0b5
  3. usesdoi:10.11570/25.0066
  4. useshttps://arxiv.org/abs/2601.09399v1
  5. reviewsdoi:10.3847/1538-4357/ae731b
  6. reviewshttps://arxiv.org/abs/2308.12118

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