activity
20022009
most citedMilagro Observations of Multi-TeV Emission from Galactic Sources in the Fermi Bright Source List

238 citations · 317 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.HE200914 cited

Neutrino Astronomy with IceCube

Tyce DeYoung

IceCube is a kilometer-scale high energy neutrino telescope under construction at the South Pole, a second-generation instrument expanding the capabilities of the AMANDA telescope.…

astro-ph.HE2009238 cited

Milagro Observations of Multi-TeV Emission from Galactic Sources in the Fermi Bright Source List

A. A. Abdo, B. T. Allen, T. Aune +27

We present the result of a search of the Milagro sky map for spatial correlations with sources from a subset of the recent Fermi Bright Source List (BSL). The BSL consists of the 2…

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-ph200621 cited

Astrophysical tau neutrino detection in kilometer-scale Cherenkov detectors via muonic tau decay

T. DeYoung, S. Razzaque, D. F. Cowen

Kilometer-scale deep under-ice or -water Cherenkov neutrino detectors may detect muon and electron neutrinos from astrophysical sources at energies of a TeV and above. Tau neutrino…

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…