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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 Point Sources of High Energy Neutrinos with Final Data from AMANDA-II
The IceCube Collaboration
We present a search for point sources of high energy neutrinos using 3.8 years of data recorded by AMANDA-II during 2000-2006. After reconstructing muon tracks and applying selecti…
The Large Scale Cosmic-Ray Anisotropy as Observed with Milagro
A. A. Abdo, B. T. Allen, T. Aune +30
Results are presented of a harmonic analysis of the large scale cosmic-ray anisotropy as observed by the Milagro observatory. We show a two-dimensional display of the sidereal anis…
A Measurement of the Spatial Distribution of Diffuse TeV Gamma Ray Emission from the Galactic Plane with Milagro
A. A. Abdo, B. Allen, T. Aune +33
Diffuse -ray emission produced by the interaction of cosmic-ray particles with matter and radiation in the Galaxy can be used to probe the distribution of cosmic rays and their…
Discovery of Localized Regions of Excess 10-TeV Cosmic Rays
A. A. Abdo, B. Allen, T. Aune +30
An analysis of 7 years of Milagro data performed on a 10-degree angular scale has found two localized regions of excess of unknown origin with greater than 12 sigma significance. B…
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…
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…
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…
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…
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…
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…
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…
The ICECUBE prototype string in AMANDA
AMANDA Collaboration, M. Ackermann
The Antarctic Muon And Neutrino Detector Array (Amanda) is a high-energy neutrino telescope. It is a lattice of optical modules (OM) installed in the clear ice below the South Pole…
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
Studies of Air Showers above 10^18 eV with the CHICOS Array
T. W. Lynn, E. Brobeck, B. E. Carlson +10
CHICOS (California HIgh school Cosmic ray ObServatory) is presently an array of more than 140 detectors distributed over a large area (~400 km^2) of southern California, and will c…
Search for Correlated High Energy Cosmic Ray Events with CHICOS
R. D. McKeown, B. E. Carlson, E. Brobeck +8
We present the results of a search for time correlations in high energy cosmic ray data (primary E > 10^14 eV) collected by the California HIgh school Cosmic ray ObServatory (CHICO…
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…
Search for Correlated High Energy Cosmic Ray Events with CHICOS
B. E. Carlson, E. Brobeck, C. J. Jillings +8
We present the results of a search for time correlations in high energy cosmic ray data (primary E > 10^{14} eV) collected by the California HIgh school Cosmic ray ObServatory (CHI…
New results from the Antarctic Muon And Neutrino Detector Array
Kurt Woschnagg
We present recent results from the Antarctic Muon And Neutrino Detector Array (AMANDA) on searches for high-energy neutrinos of extraterrestrial origin. We have searched for a diff…
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…
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…
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…
Search for extraterrestrial point sources of neutrinos with AMANDA-II
AMANDA Collaboration, J. Ahrens
We present the results of a search for point sources of high energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits o…