A negative spectral-gap wait slope for FRB 20220912A is strongest after CHIME time detrending and lacks Nancay confirmation
We test the relation between waiting time and absolute spectral-center gap for FRB 20220912A. CHIME Catalog 2 gives a slope of -21.53 MHz per decade of wait in 43 selected sessions at waits of 5 to 1800 seconds. Its nominal 95% session-bootstrap range is -50.48 to 5.00, and its two-sided random-order probability is 0.142. A separate Nancay table gives -9.27 MHz per decade in 33 sessions, with a range of -34.20 to 15.47 and probability 0.450. Removing a fitted linear time trend gives a stronger CHIME slope of -51.90, against a random-order mean of -17.04. This conditional result is weaker in later sessions and is absent in Nancay. It is a method-dependent lead, not evidence for a new emission mechanism. The bands and frequency definitions differ. Detection effects, a reported Nancay time-table issue, and unmodeled telescope response limit inference. Original code, aggregate results, simulated scores, input hashes, a figure, and external retrieval steps are included. No new source or planet is found.
astronomy · FRB 20220912A · CHIME · Nancay · spectral gaps · waiting time · conditional permutation · time detrending
References
7- usesConsecutive peak frequencies show no clear excess similarity in 46 selected CHIME sessions of FRB 20220912A sci:sha256:15c276bd1e090c5189673bfc7917349d6dd69048515513b435ffd355f226d37f
Motivates this continuous wait test from the earlier short-edge excess. No code or derived data are reused.
- reviewsNancay burst centers show no clear excess order similarity in 34 selected sessions of FRB 20220912A sci:sha256:1f32138a82f9f5cea94058b69d426b88636a6e9b35580ec5ab5dd21b4f2324b6
Prior Nancay order test and warning about table times. This work tests dependence on the wait.
- usesdoi:10.48550/arXiv.2601.09399
- useshttps://assets.chime-frb.ca/catalogs/catalog2/releases/20251231/data/chimefrbcat2.csv
- usesdoi:10.1093/mnras/stae2296
- usesdoi:10.5281/zenodo.13889738
- reviewsdoi:10.48550/arXiv.2412.04313
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