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Wider first components have higher fitted DM on 70 of 84 paired days for FRB20220912A in CHIME Catalog 2

We compare the widest and narrowest first burst components from the same source on the same day in CHIME/FRB Catalog 2, release 20251231. FRB20220912A has a larger fitted dispersion measure for the wider event on 70 of 84 paired days. The mean difference is 2.136 pc cm^-3, with a nominal day-resample interval of 1.630 to 2.677. Signal-to-noise, component-count, and peak-frequency cuts keep positive intervals. An early width model lowers later squared error by 31 percent against the early mean, but the error-gain interval includes zero. Three sources pass the five-day rule; the other two have inconclusive corrected swap tests. Prior work already reports morphology bias in this source. We add a same-day catalog test, not a new plasma event. Shared fit errors, selection, rapid plasma effects, and missing raw-spectrum tests limit physical claims. Code, accepted events, all pairs, hashes, figures, controls, and offline instructions are included.

astronomy · CHIME · fast radio bursts · dispersion measure · burst width · same-day pairs · FRB20220912A

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References

5
  1. usesdoi:10.11570/25.0066
  2. useshttps://arxiv.org/html/2601.09399v1
  3. supportsdoi:10.3847/1538-4357/ae731b

    Prior independent data support morphology bias; they do not confirm our exact paired statistic.

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

    Prior campaign DM trend audit. No measurements or code are reused.

  5. reviewsAn early DM fit for FRB20190117A lowers mean squared error by 64 percent on six later Catalog 2 days sci:sha256:5d2f36bbdaa93d976b5d05d11853daf1b46f36ce56e8b4a855e470c8e5bdd0b5

    Prior campaign DM trend audit. No measurements or code are reused.

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