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Solar Energetic Particle Spectrum on 13 December 2006 Determined by IceTop
R. Abbasi
On 13 December 2006 the IceTop air shower array at the South Pole detected a major solar particle event. By numerically simulating the response of the IceTop tanks, which are thick…
Search for Ultra High-Energy Neutrinos with AMANDA-II
The IceCube Collaboration, M. Ackermann
A search for diffuse neutrinos with energies in excess of 10^5 GeV is conducted with AMANDA-II data recorded between 2000 and 2002. Above 10^7 GeV, the Earth is essentially opaque…
The Search for Muon Neutrinos from Northern Hemisphere Gamma-Ray Bursts with AMANDA
The IceCube Collaboration, A. Achterberg, the IPN Collaboration +2
We present the results of the analysis of neutrino observations by the Antarctic Muon and Neutrino Detector Array (AMANDA) correlated with photon observations of more than 400 gamm…
Search for neutrino-induced cascades from gamma-ray bursts with AMANDA
IceCube Collaboration, A. Achterberg
Using the neutrino telescope AMANDA-II, we have conducted two analyses searching for neutrino-induced cascades from gamma-ray bursts. No evidence of astrophysical neutrinos was fou…
Multi-Messenger Studies with AMANDA/IceCube: Observations and Strategies
Elisa Bernardini
Four years of AMANDA-II data have been searched for neutrinos from point sources. No statistically significant excess of events has been detected, neither integrated in the years 2…
The IceCube Collaboration: contributions to the 29th International Cosmic Ray Conference (ICRC 2005), Pune, India, Aug. 2005
The IceCube Collaboration
In this document we collect the 18 contributions of the IceCube Collaboration to the 29th International Cosmic Ray Conference (ICRC 2005), Pune, India, Aug. 2005
Search for very high energy gamma-rays from WIMP annihilations near the Sun with the Milagro Detector
Milagro Collaboration
The neutralino, the lightest stable supersymmetric particle, is a strong theoretical candidate for the missing astronomical ``dark matter''. A profusion of such neutralinos can acc…
The IceCube Project
Christian Spiering
This talk gives a brief description of goals, expected performance and status of the Icecube project.
TeV Gamma-Ray Survey of the Northern Hemisphere Sky Using the Milagro Observatory
The Milagro Collaboration
Milagro is a water Cherenkov extensive air shower array that continuously monitors the entire overhead sky in the TeV energy band. The results from an analysis of 3 years of…
Observation of TeV Gamma Rays from the Crab Nebula with Milagro Using a New Background Rejection Technique
The Milagro Collaboration
The recent advances in TeV gamma-ray astronomy are largely the result of the ability to differentiate between extensive air showers generated by gamma rays and hadronic cosmic rays…
The high-energy gamma-ray fluence and energy spectrum of GRB 970417a from observations with Milagrito
R. Atkins, W. Benbow, D. Berley +38
Evidence of TeV emission from GRB970417a has been previously reported using data from the Milagrito detector. Constraints on the TeV fluence and the energy spectrum are now derived…
A Survey of the Northern Sky for TeV Point Sources
K. Wang, R. Atkins, W. Benbow +4
A search for steady TeV point sources anywhere in the northern sky has been made with data from the Milagrito air-shower-particle detector. Over 3 x 10**9 events collected from 199…
Milagrito: a TeV air-shower array
The Milagro Collaboration, R. Atkins
Milagrito, a large, covered water-Cherenkov detector, was the world's first air-shower-particle detector sensitive to cosmic gamma rays below 1 TeV. It served as a prototype for th…
First Results of a Study of TeV Emission from GRBs in Milagrito
J. E. McEnery, R. Atkins, W. Benbow +36
Milagrito, a detector sensitive to gamma-rays at TeV energies, monitored the northern sky during the period February 1997 through May 1998. With a large field of view and high duty…
TeV Observations of Markarian 501 with the Milagrito Water Cherenkov Detector
R. Atkins
The Milagrito water Cherenkov detector near Los Alamos, New Mexico, operated as a sky monitor at energies of a few TeV between February 1997 and May 1998 including the period of th…
Detection of 6 November 1997 Ground Level Event by Milagrito
R. Atkins, W. Benbow, D. Berley +40
Solar Energetic Particles from the 6 November 1997 solar flare/CME(coronal mass ejection) with energies exceeding 10 GeV have been detected by Milagrito, a prototype of the Milagro…