activity
20062009
most citedLIGO: The Laser Interferometer Gravitational-Wave Observatory

1.2k citations · 2.2k across the 13 of their papers we have counts for

collaborators
Showing astro-phShow all

6 papers · 1 filter

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…

astro-ph2007184 cited

Implications for the Origin of GRB 070201 from LIGO Observations

LIGO Scientific Collaboration, K. Hurley

We analyzed the available LIGO data coincident with GRB 070201, a short duration hard spectrum gamma-ray burst whose electromagnetically determined sky position is coincident with…

astro-ph200773 cited

Detection of Atmospheric Muon Neutrinos with the IceCube 9-String Detector

The IceCube Collaboration, A. Achterberg

The IceCube neutrino detector is a cubic kilometer TeV to PeV neutrino detector under construction at the geographic South Pole. The dominant population of neutrinos detected in Ic…

astro-ph2007111 cited

Upper limit map of a background of gravitational waves

The LIGO Scientific Collaboration, B. Abbott

We searched for an anisotropic background of gravitational waves using data from the LIGO S4 science run and a method that is optimized for point sources. This is appropriate if, f…

astro-ph200666 cited

Five years of searches for point sources of astrophysical neutrinos with the AMANDA-II neutrino telescope

A. Achterberg

We report the results of a five-year survey of the northern sky to search for point sources of high energy neutrinos. The search was performed on the data collected with the AMANDA…

astro-ph200644 cited

On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes

A. Achterberg et al.

The sensitivity of a search for sources of TeV neutrinos can be improved by grouping potential sources together into generic classes in a procedure that is known as source stacking…