activity
20032008
most citedLIGO: The Laser Interferometer Gravitational-Wave Observatory

1.2k citations · 1.9k across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph2008414 cited

Science with ASKAP - the Australian Square Kilometre Array Pathfinder

S. Johnston, R. Taylor, M. Bailes +47

[ABRIDGED VERSION] The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries. The SKA will be…

astro-ph2008116 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-qc200830 cited

First joint search for gravitational-wave bursts in LIGO and GEO600 data

LIGO Scientific Collaboration, B. Abbott

We present the results of the first joint search for gravitational-wave bursts by the LIGO and GEO600 detectors. We search for bursts with characteristic central frequencies in the…

astro-ph200753 cited

The Arecibo Galaxy Environment Survey: II. A HI view of the Abell cluster 1367 and its outskirts

L. Cortese, R. F. Minchin, R. R. Auld +13

We present 21 cm HI line observations of 5x1 square degrees centered on the local Abell cluster 1367 obtained as part of the Arecibo Galaxy Environment Survey. One hundred sources…

gr-qc20071.2k cited

LIGO: The Laser Interferometer Gravitational-Wave Observatory

The LIGO Scientific Collaboration, B. Abbott

The goal of the Laser Interferometric Gravitational-Wave Observatory (LIGO) is to detect and study gravitational waves of astrophysical origin. Direct detection of gravitational wa…

astro-ph2003

Complex X-ray spectral behaviour of NGC 4051 in the low flux state

P. Uttley, R. D. Taylor, I. M. McHardy +4

The Narrow Line Seyfert 1 galaxy NGC 4051 was observed in one of its prolonged low-lux states by XMM-Newton in November 2002. Here we present the results of an analysis of EPIC-pn…