Pith. sign in

REVIEW 5 cited by

Coherent WaveBurst, a pipeline for unmodeled gravitational-wave data analysis

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2006.12604 v2 pith:SAL42BHF submitted 2020-06-22 gr-qc

Coherent WaveBurst, a pipeline for unmodeled gravitational-wave data analysis

classification gr-qc
keywords beendatagravitational-waveanalysiscoherentdetectorspipelinesince
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

coherent WaveBurst (cWB) is a highly configurable pipeline designed to detect a broad range of gravitational-wave (GW) transients in the data of the worldwide network of GW detectors. The algorithmic core of cWB is a time-frequency analysis with the Wilson-Daubechies-Meyer wavelets aimed at the identification of GW events without prior knowledge of the signal waveform. cWB has been in active development since 2003 and it has been used to analyze all scientific data collected by the LIGO-Virgo detectors ever since. On September 14, 2015, the cWB low-latency search detected the first gravitational-wave event, GW150914, a merger of two black holes. In 2019, a public open-source version of cWB has been released with GPLv3 license.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 5 Pith papers

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

  1. GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors

    gr-qc 2026-05 unverdicted novelty 8.0

    The first informative astrophysical calibration of gravitational-wave detectors is reported using GW240925 and GW250207.

  2. Accelerated Time-domain Analysis for Gravitational Wave Astronomy

    gr-qc 2026-03 unverdicted novelty 7.0

    Presents a practical fully time-domain end-to-end likelihood for gravitational-wave inference with structured linear algebra and GPU acceleration.

  3. Toward claiming a detection of gravitational memory

    gr-qc 2026-01 unverdicted novelty 6.0

    A framework using scale separation in the Isaacson description defines observable gravitational memory rise for compact binary coalescences, providing a basis for hypothesis testing in LISA data.

  4. An explicit and differentiable Wilson-Daubechies-Meyer transform for gravitational-wave data analysis

    gr-qc 2026-06 conditional novelty 4.0

    An explicit, GPU-ready WDM wavelet-packet package reproduces frequency-domain LISA galactic-binary posteriors under stationary noise and documents the full discrete construction.

  5. An explicit and differentiable Wilson-Daubechies-Meyer transform for gravitational-wave data analysis

    gr-qc 2026-06 unverdicted novelty 3.0

    Open-source WDM transform package with JAX support and numerical validation of equivalence to frequency-domain likelihoods for a LISA binary under stationary noise.