Posterior samples of the parameters of binary black holes from Advanced LIGO, Virgo’s second observing run
- Syracuse Univ., Syracuse, NY (United States)
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Max-Planck-Institut für Gravitationsphysik, Hannover (Germany); Leibniz Univ. Hannover, Hannover (Germany)
This paper presents a parameter estimation analysis of the seven binary black hole mergers—GW170104, GW170608, GW170729, GW170809, GW170814, GW170818, and GW170823—detected during the second observing run of the Advanced LIGO and Virgo observatories using the gravitational-wave open data. We describe the methodology for parameter estimation of compact binaries using gravitational-wave data, and we present the posterior distributions of the inferred astrophysical parameters. We release our samples of the posterior probability density function with tutorials on using and replicating our results presented in this paper.
- Research Organization:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Organization:
- National Science Foundation (NSF); USDOE
- Grant/Contract Number:
- 89233218CNA000001
- OSTI ID:
- 1532724
- Report Number(s):
- LA-UR-19-22468
- Journal Information:
- Scientific Data, Vol. 6, Issue 1; ISSN 2052-4463
- Publisher:
- Nature Publishing GroupCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Cited by: 6 works
Citation information provided by
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Web of Science
Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo
|
journal | January 2021 |
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