Estimation of the sensitive volume for gravitational-wave source populations using weighted Monte Carlo integration

The population analysis and estimation of merger rates of compact binaries is one of the important topics in gravitational wave astronomy. The primary ingredient in these analyses is the population-averaged sensitive volume. Typically, sensitive volume, of a given search to a given simulated source...

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Veröffentlicht in:	Classical and quantum gravity 2018-06, Vol.35 (14), p.145009
1. Verfasser:	Tiwari, Vaibhav
Format:	Artikel
Sprache:	eng
Schlagworte:	binary black hole coalescence rate sensitive volume weighted monte carlo
Online-Zugang:	Volltext
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