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A Rule of Thumb for the Detectability of Gravitational-Wave Bursts

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arxiv 1304.0210 v1 pith:VRS2FIXM submitted 2013-03-31 gr-qc

classification gr-qc
keywords emissiongravitationalpolarizedwavesappropriateburstscasesconsider
verification ladder T0 review T1 audit T2 compute T3 formal
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We derive a simple relationship between the energy emitted in gravitational waves for a narrowband source and the distance to which that emission can be detected by a single detector. We consider linearly polarized, elliptically polarized, and unpolarized gravitational waves, and emission patterns appropriate for each of these cases. We ignore cosmological effects.

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Forward citations

Cited by 4 Pith papers

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

  1. All-sky search for long-duration gravitational-wave transients in the first part of the fourth LIGO-Virgo-KAGRA Observing run

    gr-qc 2025-07 accept novelty 6.0 of 10

    No long-duration gravitational-wave transients were found in O4a data; 50% efficiency amplitude limits improved by about 30% over O3, and eccentric CBC rate limits improved by factors of 2-7.

  2. Guiding interferometer improvements with the frequency-dependent inspiral range

    astro-ph.IM 2025-02 conditional novelty 6.0 of 10

    The cumulative normalized range and its two-curve difference make it easier to see which frequency bands actually limit a gravitational-wave detector's inspiral range.

  3. Search for gravitational waves associated with high-energy neutrinos detected by IceCube during the third observing run of LIGO-Virgo

    astro-ph.HE 2026-07 accept novelty 4.5 of 10

    An unmodeled targeted X-Pipeline search finds no significant GW counterparts to IceCat-1 neutrinos in O3 and reports 90% exclusion distances of tens to a few hundred Mpc depending on waveform model.

  4. All-sky search for short gravitational-wave bursts in the first part of the fourth LIGO-Virgo-KAGRA observing run

    astro-ph.HE 2025-07 conditional novelty 4.0 of 10

    An all-sky search of O4a LIGO data finds no new gravitational-wave bursts and improves burst sensitivity and rate limits by factors of 2 to 10 over the previous run.

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