We present the results of a weakly modeled burst search for gravitational waves from mergers of nonspinning intermediate mass black holes in the total mass range 100–450 M⊙ 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 intermediate mass black holes mergers as a function of the component masses. In the most efficiently detected bin centered on 88+88 M⊙, for nonspinning sources, the rate density upper limit is 0.13 per Mpc3 per Myr at the 90% confidence level. © 2012 The American Physical Societ
The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2...
We report results from a search for gravitational waves produced by perturbed intermediate mass blac...
The physical mechanisms responsible for pulsar timing glitches are thought to excite quasinormal mod...
We present the results of a weakly modeled burst search for gravitational waves from mergers of non-...
We report on a search for gravitational waves from coalescing compact binaries using LIGO and Virgo ...
We report on a search for gravitational waves from coalescing compact binaries using LIGO and Virgo ...
We present the first modeled search for gravitational waves using the complete binary black-hole gra...
We report on a search for gravitational waves from coalescing compact binaries using LIGO and Virgo ...
We report on an all-sky search for periodic gravitational waves in the frequency band 50–800 Hz and ...
We report a search for gravitational waves from the inspiral, merger and ringdown of binary black ho...
We present the results of a weakly modeled burst search for gravitational waves from mergers of nons...
We report a search for gravitational waves from the inspiral, merger and ringdown of binary black ho...
The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2...
The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2...
On September 14, 2015, at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-W...
The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2...
We report results from a search for gravitational waves produced by perturbed intermediate mass blac...
The physical mechanisms responsible for pulsar timing glitches are thought to excite quasinormal mod...
We present the results of a weakly modeled burst search for gravitational waves from mergers of non-...
We report on a search for gravitational waves from coalescing compact binaries using LIGO and Virgo ...
We report on a search for gravitational waves from coalescing compact binaries using LIGO and Virgo ...
We present the first modeled search for gravitational waves using the complete binary black-hole gra...
We report on a search for gravitational waves from coalescing compact binaries using LIGO and Virgo ...
We report on an all-sky search for periodic gravitational waves in the frequency band 50–800 Hz and ...
We report a search for gravitational waves from the inspiral, merger and ringdown of binary black ho...
We present the results of a weakly modeled burst search for gravitational waves from mergers of nons...
We report a search for gravitational waves from the inspiral, merger and ringdown of binary black ho...
The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2...
The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2...
On September 14, 2015, at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-W...
The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2...
We report results from a search for gravitational waves produced by perturbed intermediate mass blac...
The physical mechanisms responsible for pulsar timing glitches are thought to excite quasinormal mod...