activity
19962008
most citedUpper limits on gravitational wave emission from 78 radio pulsars

195 citations · 558 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2008★ 116 cited

Search for Gravitational Wave Bursts from Soft Gamma Repeaters

LIGO Scientific Collaboration, S. Barthelmy, N. Gehrels +2

We present the results of a LIGO search for short-duration gravitational waves (GWs) associated with Soft Gamma Repeater (SGR) bursts. This is the first search sensitive to neutron…

gr-qc2007★ 195 cited

Upper limits on gravitational wave emission from 78 radio pulsars

The LIGO Scientific Collaboration, B. Abbott, M. Kramer +1

We present upper limits on the gravitational wave emission from 78 radio pulsars based on data from the third and fourth science runs of the LIGO and GEO600 gravitational wave dete…

gr-qc2006★ 172 cited

Coherent searches for periodic gravitational waves from unknown isolated sources and Scorpius X-1: results from the second LIGO science run

The LIGO Scientific Collaboration

We carry out two searches for periodic gravitational waves using the most sensitive few hours of data from the second LIGO science run. The first search is targeted at isolated, pr…

gr-qc2003★ 5 cited

Upper limits on the strength of periodic gravitational waves from PSR J1939+2134

B. Allen, G. Woan

The first science run of the LIGO and GEO gravitational wave detectors presented the opportunity to test methods of searching for gravitational waves from known pulsars. Here we pr…

astro-ph2002

The GEO600 Gravitational Wave Detector -- Pulsar Prospects

G. Woan

The GEO600 laser-interferometric gravitational wave detector near Hannover, Germany, is one of six such interferometers now close to operation worldwide. The UK/German GEO collabor…

gr-qc1996★ 70 cited

Results of the First Coincident Observations by Two Laser-Interferometric Gravitational Wave Detectors

D. Nicholson

We report an upper bound on the strain amplitude of gravitational wave bursts in a waveband from around 800Hz to 1.25kHz. In an effective coincident observing period of 62 hours, t…