Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA.
Data analysis
Electromagnetic counterparts
Gravitational waves
Gravitational-wave detectors
Journal
Living reviews in relativity
ISSN: 1433-8351
Titre abrégé: Living Rev Relativ
Pays: Switzerland
ID NLM: 101697608
Informations de publication
Date de publication:
2020
2020
Historique:
received:
01
10
2019
accepted:
27
05
2020
entrez:
5
10
2020
pubmed:
6
10
2020
medline:
6
10
2020
Statut:
ppublish
Résumé
We present our current best estimate of the plausible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next several years, with the intention of providing information to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals for the third (O3), fourth (O4) and fifth observing (O5) runs, including the planned upgrades of the Advanced LIGO and Advanced Virgo detectors. We study the capability of the network to determine the sky location of the source for gravitational-wave signals from the inspiral of binary systems of compact objects, that is binary neutron star, neutron star-black hole, and binary black hole systems. The ability to localize the sources is given as a sky-area probability, luminosity distance, and comoving volume. The median sky localization area (90% credible region) is expected to be a few hundreds of square degrees for all types of binary systems during O3 with the Advanced LIGO and Virgo (HLV) network. The median sky localization area will improve to a few tens of square degrees during O4 with the Advanced LIGO, Virgo, and KAGRA (HLVK) network. During O3, the median localization volume (90% credible region) is expected to be on the order of
Identifiants
pubmed: 33015351
doi: 10.1007/s41114-020-00026-9
pii: 26
pmc: PMC7520625
doi:
Types de publication
Journal Article
Review
Langues
eng
Pagination
3Informations de copyright
© The Author(s) 2020.
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