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20032019
most citedLIGO: The Laser Interferometer Gravitational-Wave Observatory

1.2k citations · 3.9k across the 29 of their papers we have counts for

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astro-ph2008★ 414 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-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…

astro-ph2008★ 216 cited

Beating the spin-down limit on gravitational wave emission from the Crab pulsar

The LIGO Scientific Collaboration, B. Abbott, R. Abbott +440

We present direct upper limits on gravitational wave emission from the Crab pulsar using data from the first nine months of the fifth science run of the Laser Interferometer Gravit…

astro-ph2007★ 53 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…

astro-ph2003★ 46 cited

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…

astro-ph2003★ 1 cited

Catching NGC4051 in the low state with XMM-Newton

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

The Narrow Line Seyfert 1 galaxy NGC4051 shows unusual low flux states, lasting several months, when the 2-10 keV X-ray spectrum becomes unusually hard (photon index<1) while the s…