Optimized localization for gravitational waves from merging binaries
Optimized localization for gravitational waves from merging binaries
The Advanced LIGO and Virgo gravitational-wave observatories have opened a new window with which to study the inspiral and mergers of binary compact objects. These observations are most powerful when coordinated with multimessenger observations. This was underlined by the first observation of a binary neutron star merger GW170817, coincident with a short gamma-ray burst, GRB170817A, and the identification of the host galaxy NGC 4993 from the optical counterpart AT2017gfo. Finding the fast-fading optical counterpart critically depends on the rapid production of a sky map based on LIGO/Virgo data. Currently, a rapid initial sky map is produced, followed by a more accurate, high-latency, ${\gtrsim}{12}\, {\rm h}$ sky map. We study optimization choices of the Bayesian prior and signal model, which can be used alongside other approaches such as reduced order quadrature. We find these yield up to a $60{{\ \rm per\ cent}}$ reduction in the time required to produce the high-latency localization for binary neutron star mergers.
gravitational waves, neutron star mergers
3957-3965
You, Zhi-Qiang
af0e4679-4f82-4164-9fb2-dc390cdd1fc8
Ashton, Gregory
a8cec4b1-3c98-4b28-af2a-1e37cb3b9f2a
Zhu, Xing-Jiang
e3acbe8f-e553-4118-b4f8-a49ef2808d40
Thrane, Eric
2bafe758-0f64-458f-9f9a-fede9abc343c
Zhu, Zong-Hong
a856211a-7ee2-463e-910e-761702235def
23 October 2021
You, Zhi-Qiang
af0e4679-4f82-4164-9fb2-dc390cdd1fc8
Ashton, Gregory
a8cec4b1-3c98-4b28-af2a-1e37cb3b9f2a
Zhu, Xing-Jiang
e3acbe8f-e553-4118-b4f8-a49ef2808d40
Thrane, Eric
2bafe758-0f64-458f-9f9a-fede9abc343c
Zhu, Zong-Hong
a856211a-7ee2-463e-910e-761702235def
You, Zhi-Qiang, Ashton, Gregory, Zhu, Xing-Jiang, Thrane, Eric and Zhu, Zong-Hong
(2021)
Optimized localization for gravitational waves from merging binaries.
Monthly Notices of the Royal Astronomical Society, 509 (3), .
(doi:10.1093/mnras/stab2977).
Abstract
The Advanced LIGO and Virgo gravitational-wave observatories have opened a new window with which to study the inspiral and mergers of binary compact objects. These observations are most powerful when coordinated with multimessenger observations. This was underlined by the first observation of a binary neutron star merger GW170817, coincident with a short gamma-ray burst, GRB170817A, and the identification of the host galaxy NGC 4993 from the optical counterpart AT2017gfo. Finding the fast-fading optical counterpart critically depends on the rapid production of a sky map based on LIGO/Virgo data. Currently, a rapid initial sky map is produced, followed by a more accurate, high-latency, ${\gtrsim}{12}\, {\rm h}$ sky map. We study optimization choices of the Bayesian prior and signal model, which can be used alongside other approaches such as reduced order quadrature. We find these yield up to a $60{{\ \rm per\ cent}}$ reduction in the time required to produce the high-latency localization for binary neutron star mergers.
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More information
Accepted/In Press date: 13 October 2021
Published date: 23 October 2021
Keywords:
gravitational waves, neutron star mergers
Identifiers
Local EPrints ID: 508308
URI: http://eprints.soton.ac.uk/id/eprint/508308
ISSN: 0035-8711
PURE UUID: 7bc7313d-a4c5-46aa-8d22-51534f058b1e
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Date deposited: 16 Jan 2026 17:41
Last modified: 17 Jan 2026 03:47
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Contributors
Author:
Zhi-Qiang You
Author:
Gregory Ashton
Author:
Xing-Jiang Zhu
Author:
Eric Thrane
Author:
Zong-Hong Zhu
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