Status and Results from AMANDA/IceCube
Patrick Berghaus (for the IceCube Collaboration)

TL;DR
This paper reviews the progress and initial results of the IceCube neutrino telescope, including its predecessor AMANDA, highlighting the construction status, data collection, and scientific achievements in neutrino astronomy.
Contribution
It provides an overview of the development, current status, and early scientific results of the IceCube detector and its precursor AMANDA at the South Pole.
Findings
AMANDA operated successfully for 10 years producing scientific data.
IceCube has deployed 22 strings and is progressing towards full completion.
Initial physics results demonstrate the detector's capability for neutrino detection.
Abstract
IceCube is a cubic kilometer-scale neutrino telescope under construction at the South Pole since the austral summer 2004/2005. At the moment it is taking data with 22 deployed strings. The full detector is expected to be completed in 2011 with up to 80 strings each holding 60 digital optical modules. The progenitor detector AMANDA has been operating at the same site since 1997 and is still running as an integral part of IceCube. A summary of AMANDA science for its 10 years of standalone operations is presented, as well as the status and first physics results of the IceCube project.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae · Radio Astronomy Observations and Technology
