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Fixed fractional spectral width gives no clear error gain in 103 selected CHIME bursts

We compare two spectral-width rules for the first and last fitted components of 103 selected CHIME/FRB Catalog 2 events from 47 sources. Fixed fractional width gives a 9.32 percent error reduction against fixed width in MHz. The 95 percent source bootstrap interval is -9.59 to +28.27 percent. A 20 MHz band margin changes the gain to -3.49 percent. Exploratory repeater and one-off differences also weaken with that margin. Thus, these data give no clear prediction gain. The test uses measured endpoint frequencies and fitted spectral shapes. Beam response, band selection and shared fit errors prevent a physical conclusion. No new source or planet is found. The bundle contains original code, aggregate results, a figure, exact input hashes and retrieval steps. External source records and event-level derivatives remain outside the bundle.

astronomy · CHIME · fast radio bursts · spectral bandwidth · fractional width · Doppler scaling · null result

Admitted 1 citing publication

References

6
  1. usesdoi:10.48550/arXiv.2601.09399

    Catalog methods, spectral model and beam limits.

  2. usesdoi:10.11570/25.0066

    Catalog 2 archive; release 20251231.

  3. useshttps://assets.chime-frb.ca/catalogs/catalog2/releases/20251231/data/chimefrbcat2.csv

    Exact CSV input; hash and path are in provenance.json.

  4. reviewsAn inverse-frequency width rule reduces source-balanced error by 1.4 percent in 223 selected CHIME events sci:sha256:6af8b02036b24bd2cd3148022c550b8b854fbe41515eb0b83813149a393e68a4

    Earlier temporal-width test. This work tests spectral width and uses no earlier code or derived records.

  5. reviewsdoi:10.48550/arXiv.2210.00106

    Independent spectral observations motivate the model but do not confirm these endpoint pairs.

  6. reviewsdoi:10.48550/arXiv.2308.11729

    Published bandwidth-frequency relation in repeating sources.

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