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Archival searches for stellar-mass binary black holes in LISA

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arxiv 2011.03036 v1 pith:7BZWIHZL submitted 2020-11-05 gr-qc astro-ph.HE

Becca Ewing , Surabhi Sachdev , Ssohrab Borhanian , B.S. Sathyaprakash This is my paper · ORCID
classification gr-qcastro-ph.HE
keywords lisadetectorsground-basedwillarchivalbinaryblackgravitational-wave
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abstract

Stellar-mass binary black holes will sweep through the frequency band of the Laser Interferometer Space Antenna (LISA) for months to years before appearing in the audio-band of ground-based gravitational-wave detectors. One can expect several tens of these events up to a distance of $500 \,\mathrm{Mpc}$ each year. The LISA signal-to-noise ratio for such sources even at these close distances will be too small for a blind search to confidently detect them. However, next generation ground-based gravitational-wave detectors, expected to be operational at the time of LISA, will observe them with signal-to-noise ratios of several thousands and measure their parameters very accurately. We show that such high fidelity observations of these sources by ground-based detectors help in archival searches to dig tens of signals out of LISA data each year.

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Cited by 3 Pith papers

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

  1. Multiband parameter estimation with phase coherence and extrinsic marginalization: Extracting more information from low-SNR CBC signals in LISA data

    gr-qc 2025-06 conditional novelty 8.0 of 10

    A coherent multiband Bayesian parameter estimation method with extrinsic-parameter marginalization extracts useful information from LISA observations of stellar-mass binary black holes down to LISA SNR 3, nearly doubl...

  2. Constraining Dipole Radiation with Multiband Gravitational Waves from Eccentric Binary Black Holes

    gr-qc 2026-04 unverdicted novelty 7.0 of 10

    Multiband observations of eccentric binary black holes can constrain dipole-radiation deviations from general relativity to |b| ≲ 10^{-7} for a GW231123-like event when combining one year of space-based data with grou...

  3. Searching for stellar-origin binary black holes in LISA Data Challenge 1b: Yorsh

    gr-qc 2024-12 conditional novelty 5.0 of 10

    An existing semi-coherent hierarchical search recovers the five loudest injected stellar-origin binary black holes in LISA Data Challenge 1b Yorsh, with SNR as low as 12.94.

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