- AuthorJ. Abadie et al. (오정근)
-
JournalPhys. Rev. D 85 (2012
- Classification of papersSCI
We present the results of a weakly modeled burst search for gravitational waves from mergers of non-spinning
intermediate mass black holes (IMBH) in the total mass range $100-450$ solar masses and with the component
mass ratios between $1:1$ and $4:1$. The search was conducted on data collected by the LIGO and Virgo detectors
between November of 2005 and October of 2007. No plausible signals were observed by the search which
constrains the astrophysical rates of the IMBH mergers as a function of the component masses. In the most
efficiently detected bin centered on $88+88$ solar masses, for non-spinning sources, the rate density upper limit
is 0.13 per $\text{Mpc}^3$ per Myr at the 90% confidence level.
We present the results of a weakly modeled burst search for gravitational waves from mergers of non-spinning
intermediate mass black holes (IMBH) in the total mass range $100-450$ solar masses and with the component
mass ratios between $1:1$ and $4:1$. The search was conducted on data collected by the LIGO and Virgo detectors
between November of 2005 and October of 2007. No plausible signals were observed by the search which
constrains the astrophysical rates of the IMBH mergers as a function of the component masses. In the most
efficiently detected bin centered on $88+88$ solar masses, for non-spinning sources, the rate density upper limit
is 0.13 per $\text{Mpc}^3$ per Myr at the 90% confidence level.