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Towards a unified treatment of gravitational-wave data analysis

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arxiv 1305.2934 v2 pith:XEJTCIZP submitted 2013-05-13 gr-qc

Neil J.Cornish , Joseph D. Romano This is my paper · ORCID
classification gr-qc
keywords analysisgravitational-wavedatadetectsignalstemplate-basedunifiedused
verification ladder T0 review T1 audit T2 compute T3 formal
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We present a unified description of gravitational-wave data analysis that unites the template-based analysis used to detect deterministic signals from well-modeled sources, such as binary-black-hole mergers, with the cross-correlation analysis used to detect stochastic gravitational-wave backgrounds. We also discuss the connection between template-based analyses and those that target poorly-modeled bursts of gravitational waves, and suggest a new approach for detecting burst signals.

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Cited by 2 Pith papers

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

  1. Summary statistic for pulsar timing arrays

    astro-ph.CO 2026-08 conditional novelty 7.0 of 10

    A PTA likelihood expressed in terms of low-order spherical harmonics of the Earth term and pulsar-term variance retains roughly 95% of the information about a stochastic background, and ell_max=3 plus the pulsar-term ...

  2. Impact of numerical-relativity waveform calibration on parametrized post-Einsteinian tests

    gr-qc 2026-03 accept novelty 6.0 of 10

    NR late-inspiral calibration systematics in IMRPhenomD produce false ppE GR violations at O5 SNRs ≳60; an uncertainty-aware baseline restores consistency with GR up to SNR 330.

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