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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…
Feasibility of acoustic neutrino detection in ice: Design and performance of the South Pole Acoustic Test Setup (SPATS)
S. Boeser, C. Bohm, F. Descamps +11
The South Pole Acoustic Test Setup (SPATS) has been built to evaluate the acoustic characteristics of the South Pole ice in the 10 to 100 kHz frequency range so that the feasibilit…
Contributions to The 10th International Conference on Topics in Astroparticle and Underground Physics (TAUP) 2007, Sendai, Japan, Sep. 11-15, 2007
The IceCube Collaboration
This is the collection of the proceedings presented by the IceCube Collaboration at the TAUP2007 conference.
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…
Feasibility of acoustic neutrino detection in ice: First results from the South Pole Acoustic Test Setup (SPATS)
S. Böser, C. Bohm, F. Descamps +11
Astrophysical neutrinos in the EeV range (particularly those generated by the interaction of cosmic rays with the cosmic microwave background) promise to be a valuable tool to stud…
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…
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
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…
The IceCube Project
Christian Spiering
This talk gives a brief description of goals, expected performance and status of the Icecube project.
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…
Limits on diffuse fluxes of high energy extraterrestrial neutrinos with the AMANDA-B10 detector
J. Ahrens et al.
Data from the AMANDA-B10 detector taken during the austral winter of 1997 have been searched for a diffuse flux of high energy extraterrestrial muon-neutrinos, as predicted from, e…
Physics and Operation of the AMANDA-II High Energy Neutrino Telescope
Steven W. Barwick
This paper briefly describes the principle of operation and science goals of the AMANDA high energy neutrino telescope located at the South Pole, Antarctica. Results from an earlie…
Results from the Antarctic Muon and Neutrino Detector Array (AMANDA)
D. F. Cowen
We show new results from both the older and newer incarnations of AMANDA (AMANDA-B10 and AMANDA-II, respectively). These results demonstrate that AMANDA is a functioning, multipurp…
IceCube - the next generation neutrino telescope at the South Pole
A. Karle
IceCube is a large neutrino telescope of the next generation to be constructed in the Antarctic Ice Sheet near the South Pole. We present the conceptual design and the sensitivity…
Search for Point Sources of High Energy Neutrinos with AMANDA
J. Ahrens, X. Bai, G. Barouch +1
This paper describes the search for astronomical sources of high-energy neutrinos using the AMANDA-B10 detector, an array of 302 photomultiplier tubes, used for the detection of Ch…
Observation of High Energy Atmospheric Neutrinos with the Antarctic Muon and Neutrino Detector Array
AMANDA Collaboration, J. Ahrens
The Antarctic Muon and Neutrino Detector Array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming thr…
Physics Results from the AMANDA-B10 Neutrino Telescope
A. Hallgren
The data from the first year of operation of the 10-string, AMANDA-B10, high-energy neutrino detector array at the South Pole have been analyzed and searched for evidence of neutri…
Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector
The AMANDA Collaboration, J. Ahrens
A search for nearly vertical up-going muon-neutrinos from neutralino annihilations in the center of the Earth has been performed with the AMANDA-B10 neutrino detector. The data sam…
Results from AMANDA
Gary C. Hill
The AMANDA (Antarctic Muon And Neutrino Detector Array) detector, located at the South Pole station, Antarctica, was recently expanded with the addition of six new strings, complet…