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Comment on "Analysis of Ringdown Overtones in GW150914''

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arxiv 2310.13869 v1 pith:DOB7Q54X submitted 2023-10-21 astro-ph.HE astro-ph.IMgr-qc

Comment on "Analysis of Ringdown Overtones in GW150914''

classification astro-ph.HE astro-ph.IMgr-qc
keywords gw150914analysiscodecommentcotestadataovertonepresence
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Cotesta et al. (2022) reanalyze the GW150914 ringdown, arguing against the presence of an overtone and suggesting claims of its detection in Isi et al. (2019) were driven by noise. Here we point out a number of technical errors in that analysis, including a software bug, and show that features highlighted as problematic are in fact expected and encountered in simulated data. After fixes, the code in used in Cotesta et al. (2022) produces results consistent with the presence of the overtone. All code and data are available at https://github.com/maxisi/gw150914_rd_comment

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

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  3. Modeling the frequency-domain ringdown amplitude of comparable-mass mergers with greybody factors

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    A four-parameter greybody factor model reproduces the frequency-domain ringdown amplitude of comparable-mass aligned-spin mergers with mismatches of order 10^{-5}, improving existing models by two orders of magnitude.

  4. GW250114: testing Hawking's area law and the Kerr nature of black holes

    gr-qc 2025-09 accept novelty 5.0

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