Premerger observation and characterization of massive black hole binaries

We demonstrate an end-to-end technique for observing and characterizing massive black hole binary signals before they merge with the LISA space-based gravitational-wave observatory. Our method uses a zero-latency whitening filter, originally designed for rapidly observing compact binary mergers in ground-based observatories, to be able to observe signals with no additional latency due to filter length. We show that with minimal computational cost, we are able to reliably observe signals as early as 14 days premerger as long as the signal has accrued a signal-to-noise ratio of at least 8 in the LISA data. We also demonstrate that this method can be used to characterize the source properties, providing early estimates of the source’s merger time, chirp mass, and sky localization. Early observation and characterization of massive black holes is crucial to enable the possibility of rapid multimessenger observations, and to ensure that LISA can enter a protected operating period when the merger signal arrives.

Authors

Institutions

Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-02-21
DOI
https://doi.org/10.1103/physrevd.111.043045
Citations
7
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
8.08

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Premerger observation and characterization of massive black hole binaries

Antoine Klein, G. Woan, G. Pratten, Leor Barack et al.
7 citations
Physical review. D/Physical review. D.
Pulsars and Gravitational Waves Research
8.08
article

Premerger observation and characterization of massive black hole binaries

Antoine Klein, G. Woan, G. Pratten, Leor Barack, Diganta Bandopadhyay, G. S. Davies, H. Middleton, C. G. Hoy, Jean-Baptiste Bayle, C. J. Moore, M. J. Williams, I. W. Harry, A. Vecchio, L. K. Nuttall
article en
7 citations

Abstract

We demonstrate an end-to-end technique for observing and characterizing massive black hole binary signals before they merge with the LISA space-based gravitational-wave observatory. Our method uses a zero-latency whitening filter, originally designed for rapidly observing compact binary mergers in ground-based observatories, to be able to observe signals with no additional latency due to filter length. We show that with minimal computational cost, we are able to reliably observe signals as early as 14 days premerger as long as the signal has accrued a signal-to-noise ratio of at least 8 in the LISA data. We also demonstrate that this method can be used to characterize the source properties, providing early estimates of the source’s merger time, chirp mass, and sky localization. Early observation and characterization of massive black holes is crucial to enable the possibility of rapid multimessenger observations, and to ensure that LISA can enter a protected operating period when the merger signal arrives.

Physical review. D/Physical review. D.Vol. 111(4)
University of Southampton (GB), University of Portsmouth (GB), University of Glasgow (GB), University of Birmingham (GB)
University of Portsmouth, UK Space Agency, UK Research and Innovation, Royal Society, South East Physics Network
Openalex Percentile: Top 3%
Pulsars and Gravitational Waves Research
8.08
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.