We present the results of a directed search for continuous gravitational waves from unknown, isolated neutron stars in the Galactic Center region, performed on two years of data from LIGO's fifth science run from two LIGO detectors. The search uses a semi-coherent approach, analyzing coherently 630 segments, each spanning 11.5 hours, and then incoherently combining the results of the single segments. It covers gravitational wave frequencies in a range from 78 to 496 Hz and a frequency-dependent range of first order spindown values down to -7.86 x 10^-8 Hz/s at the highest frequency. No gravitational waves were detected. We place 90% confidence upper limits on the gravitational wave amplitude of sources at the Galactic Center. Placing 90% co...
We employ gravitational-wave radiometry to map the stochastic gravitational wave background expected...
The gravitational-wave (GW) sky may include nearby pointlike sources as well as stochastic backgroun...
Spinning neutron stars asymmetric with respect to their rotation axis are potential sources of conti...
We present the results of a directed search for continuous gravitational waves from unknown, isolate...
We describe directed searches for continuous gravitational waves in data from the sixth LIGO science...
We present the first results of an all-sky search for continuous gravitational waves from unknown sp...
We present results of an all-sky search for continuous gravitational waves (CWs), which can be produ...
In this paper we present the results of a coherent narrow-band search for continuous gravitational-w...
We report results of a wideband search for periodic gravitational waves from isolated neutron stars...
We present the results of a search for long-duration gravitational wave transients in two sets of da...
We report on a comprehensive all-sky search for periodic gravitational waves in the frequency band 1...
We present the results of a semicoherent search for continuous gravitational waves from the low-mass...
We employ gravitational-wave radiometry to map the stochastic gravitational wave background expected...
This paper presents results of an all-sky search for periodic gravitational waves in the frequency r...
We employ gravitational-wave radiometry to map the stochastic gravitational wave background expected...
The gravitational-wave (GW) sky may include nearby pointlike sources as well as stochastic backgroun...
Spinning neutron stars asymmetric with respect to their rotation axis are potential sources of conti...
We present the results of a directed search for continuous gravitational waves from unknown, isolate...
We describe directed searches for continuous gravitational waves in data from the sixth LIGO science...
We present the first results of an all-sky search for continuous gravitational waves from unknown sp...
We present results of an all-sky search for continuous gravitational waves (CWs), which can be produ...
In this paper we present the results of a coherent narrow-band search for continuous gravitational-w...
We report results of a wideband search for periodic gravitational waves from isolated neutron stars...
We present the results of a search for long-duration gravitational wave transients in two sets of da...
We report on a comprehensive all-sky search for periodic gravitational waves in the frequency band 1...
We present the results of a semicoherent search for continuous gravitational waves from the low-mass...
We employ gravitational-wave radiometry to map the stochastic gravitational wave background expected...
This paper presents results of an all-sky search for periodic gravitational waves in the frequency r...
We employ gravitational-wave radiometry to map the stochastic gravitational wave background expected...
The gravitational-wave (GW) sky may include nearby pointlike sources as well as stochastic backgroun...
Spinning neutron stars asymmetric with respect to their rotation axis are potential sources of conti...