This should generate insight into the powerful celestial objects where acceleration mechanisms can bring up to 1 0 20 10^{20} 1020 eV. We describe the ...

Jun 10, 2003 · Title:Recent Results from the AMANDA Experiment. Authors:Peter Niessen (for the AMANDA collaboration). View a PDF of the paper titled Recent ...

The main aim of the AMANDA-Experiment at the South Pole is the detection of High Energy (> TeV) Neutrinos of galactic or extra-galactic origin.

Oct 22, 2024 · AMANDA B10: · Larger effective area/volume (~ 4x). ; Better acceptance at horizon · Lower background from misreconstructions near horizontal.

Once AMANDA is incorporated into the 1 km3 detector IceCube, only the TWR system will be kept. We report results from a first atmospheric neutrino analysis on ...

We report results from a first atmospheric neutrino analysis on data collected in 2003 with TWR. Good agreement in event rate and angular distribution verify ...

AMANDA-II is an operating neutrino telescope located at the South Pole. Recent results of AMANDA are presented, including the examination of the diffuse ...

Oct 1, 2001 · The talk highlights the detection of high energy atmospheric neutrinos, the search for extraterrestrial neutrinos, neutrinos from WIMP ...

Abstract. We present new data taken with the AMANDA-II neutrino telescope array. The AMANDA-II upgrade was completed at the beginning of 2000.

We report results from a first atmospheric neutrino analysis on data collected in 2003 with TWR. Good agreement in event rate and angular distribution verify ...