Numerical relativity injection analysis of signals from generically spinning intermediate mass black hole binaries in Advanced LIGO data (vol 102, 044035, 2020)

dc.contributor.author	CHANDRA, K
dc.contributor.author	GAYATHRI, V
dc.contributor.author	BUSTILLO, JC
dc.contributor.author	PAI, A
dc.date.accessioned	2021-03-10T08:19:19Z
dc.date.available	2021-03-10T08:19:19Z
dc.date.issued	2020
dc.identifier.citation	PHYSICAL REVIEW D 102(12)	en_US
dc.identifier.issn	2470-0010
dc.identifier.issn	2470-0029
dc.identifier.uri	https://doi.org/10.1103/PhysRevD.102.124014
dc.identifier.uri	http://localhost:8080/xmlui/handle/100/29397
dc.description.abstract	This article is an addendum to a recent publication by Chandra et al. [Phys. Rev. D 102, 044035 (2020)]. We present updated results on upper limits on the merger of intermediate-mass black holes (IMBHs) with total mass between 210 M-circle dot and 500 M-circle dot, mass ratio 1 to 7, and generic spins using data from the second Advanced LIGO observing run. Based on our analysis, we place the most stringent of our upper limits, of 0.28 Gpc(-3) yr(-1) on the merger rate density of precessing equal-mass intermediate-mass black holes with total masses of 210 M-circle dot.	en_US
dc.language.iso	English	en_US
dc.publisher	AMER PHYSICAL SOC	en_US
dc.title	Numerical relativity injection analysis of signals from generically spinning intermediate mass black hole binaries in Advanced LIGO data (vol 102, 044035, 2020)	en_US
dc.type	Correction	en_US