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20032007
most citedTeV Gamma-Ray Sources from a Survey of the Galactic Plane with Milagro

285 citations · 578 across the 4 of their papers we have counts for

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astro-ph200736 cited

Milagro Constraints on Very High Energy Emission from Short Duration Gamma-Ray Bursts

A. A. Abdo, B. T. Allen, D. Berley +27

Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift and HETE satellites have led to the observation of the first afterglows and the measurement of the fi…

astro-ph2007285 cited

TeV Gamma-Ray Sources from a Survey of the Galactic Plane with Milagro

A. A. Abdo, B. Allen, D. Berley +31

A survey of Galactic gamma-ray sources at a median energy of ~20 TeV has been performed using the Milagro Gamma Ray Observatory. Eight candidate sources of TeV emission are detecte…

astro-ph2006213 cited

Discovery of TeV Gamma-Ray Emission from the Cygnus Region of the Galaxy

A. A. Abdo, B. Allen, D. Berley +36

The diffuse gamma radiation arising from the interaction of cosmic ray particles with matter and radiation in the Galaxy is one of the few probes available to study the origin of t…

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…

astro-ph2005

Constraints on Very High Energy gamma-ray emission from Gamma-Ray Bursts

R. Atkins, W. Benbow, D. Berley +31

The Milagro gamma-ray observatory employs a water Cherenkov detector to observe extensive air showers produced by high energy particles interacting in the Earth's atmosphere. Milag…

astro-ph2003

Limits on Very High Energy Emission from Gamma-Ray Bursts with the Milagro Observatory

The Milagro Collaboration, R. Atkins, W. Benbow +34

The Milagro telescope monitors the northern sky for 100 GeV to 100 TeV transient emission through continuous very high energy wide-field observations. The large effective area and…