We search for coincident gravitational wave signals from inspiralling neutron star binaries using LIGO and TAMA300 data taken during early 2003. Using a simple trigger exchange method, we perform an intercollaboration coincidence search during times when TAMA300 and only one of the LIGO sites were operational. We find no evidence of any gravitational wave signals. We place an observational upper limit on the rate of binary neutron star coalescence with component masses between 1 and 3Mסּ of 49 per year per Milky Way equivalent galaxy at a 90% confidence level. The methods developed during this search will find application in future network inspiral analyses
We report on a matched-filter search for gravitational wave bursts from cosmic string cusps using LI...
We report on a search for gravitational waves from coalescing compact binaries, of total mass betwee...
A search for periodic gravitational waves, from sources such as isolated rapidly spinning neutron st...
We search for coincident gravitational wave signals from inspiralling neutron star binaries using LI...
We search for coincident gravitational wave signals from inspiralling neutron star binaries using LI...
We use 373 hours (≈15 days) of data from the second science run of the LIGO gravitational-wave detec...
We report on the first joint search for gravitational waves by the TAMA and LIGO collaborations. We ...
We report on the methods and results of the first dedicated search for gravitational waves emitted d...
We report on a search for gravitational waves from the coalescence of compact binaries during the th...
We have searched for Gravitational Waves (GWs) associated with the SGR 1806-20 hyperflare of 27 Dece...
We report on a search for gravitational waves from coalescing compact binary systems in the Milky Wa...
We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequ...
This paper reports on an all-sky search for periodic gravitational waves from sources such as deform...
We have searched for gravitational waves from coalescing low mass compact binary systems with a tota...
We searched for an anisotropic background of gravitational waves using data from the LIGO S4 science...
We report on a matched-filter search for gravitational wave bursts from cosmic string cusps using LI...
We report on a search for gravitational waves from coalescing compact binaries, of total mass betwee...
A search for periodic gravitational waves, from sources such as isolated rapidly spinning neutron st...
We search for coincident gravitational wave signals from inspiralling neutron star binaries using LI...
We search for coincident gravitational wave signals from inspiralling neutron star binaries using LI...
We use 373 hours (≈15 days) of data from the second science run of the LIGO gravitational-wave detec...
We report on the first joint search for gravitational waves by the TAMA and LIGO collaborations. We ...
We report on the methods and results of the first dedicated search for gravitational waves emitted d...
We report on a search for gravitational waves from the coalescence of compact binaries during the th...
We have searched for Gravitational Waves (GWs) associated with the SGR 1806-20 hyperflare of 27 Dece...
We report on a search for gravitational waves from coalescing compact binary systems in the Milky Wa...
We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequ...
This paper reports on an all-sky search for periodic gravitational waves from sources such as deform...
We have searched for gravitational waves from coalescing low mass compact binary systems with a tota...
We searched for an anisotropic background of gravitational waves using data from the LIGO S4 science...
We report on a matched-filter search for gravitational wave bursts from cosmic string cusps using LI...
We report on a search for gravitational waves from coalescing compact binaries, of total mass betwee...
A search for periodic gravitational waves, from sources such as isolated rapidly spinning neutron st...