Zobrazeno 1 - 10
of 37
pro vyhledávání: '"the AMANDA Collaboration"'
Autor:
AMANDA Collaboration, Ackermann, M.
Publikováno v:
Nucl.Instrum.Meth.A556:169-181,2006
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 Station. Each OM contains a photomultiplier tube (PMT) that detects p
Externí odkaz:
http://arxiv.org/abs/astro-ph/0601397
Publikováno v:
Astropart.Phys.24:459-466,2006
A search for an excess of muon-neutrinos from neutralino annihilations in the Sun has been performed with the AMANDA-II neutrino detector using data collected in 143.7 days of live-time in 2001. No excess over the expected atmospheric neutrino backgr
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508518
Publikováno v:
Phys.Rev.D71:077102,2005
The results of a search for point sources of high energy neutrinos in the northern hemisphere using data collected by AMANDA-II in the years 2000, 2001 and 2002 are presented. In particular, a comparison with the single-year result previously publish
Externí odkaz:
http://arxiv.org/abs/astro-ph/0412347
Autor:
The AMANDA Collaboration, Ahrens, J.
Publikováno v:
Nucl.Instrum.Meth.A524:169-194,2004
The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope operating at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice between 1500m and 2000m. The primary goal of th
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407044
Publikováno v:
Astropart.Phys.22:127-138,2004
We report on a search for electro-magnetic and/or hadronic showers (cascades) induced by high energy neutrinos in the data collected with the AMANDA II detector during the year 2000. The observed event rates are consistent with the expectations for a
Externí odkaz:
http://arxiv.org/abs/astro-ph/0405218
Autor:
AMANDA Collaboration, Ahrens, J.
Publikováno v:
Phys.Rev.Lett.92:071102,2004
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 on several AGN blazars, microquasars, magnetars and other candidate neu
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309585
Observation of High Energy Atmospheric Neutrinos with the Antarctic Muon and Neutrino Detector Array
Autor:
AMANDA Collaboration, Ahrens, J.
Publikováno v:
Phys.Rev.D66:012005,2002
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 through the Earth from the Northern Hemisphere are identified by secondar
Externí odkaz:
http://arxiv.org/abs/astro-ph/0205109
Autor:
The AMANDA Collaboration, Ahrens, J.
Publikováno v:
Phys.Rev.D66:032006,2002
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 sample collected in 130.1 days of live-time in 1997, ~10^9 events, has be
Externí odkaz:
http://arxiv.org/abs/astro-ph/0202370
Autor:
AMANDA Collaboration, Ahrens, J.
Publikováno v:
in Proceedings of the EPS International Conference on High Energy Physics, Budapest, 2001 (D. Horvath, P. Levai, A. Patkos, eds.), JHEP Proceedings Section, PrHEP-hep2001/207
In the winter season of 2000, the AMANDA (Antarctic Muon And Neutrino Detector Array) detector was completed to its final state. We report on major physics results obtained from the AMANDA-B10 detector, as well as initial results of the full AMANDA-I
Externí odkaz:
http://arxiv.org/abs/hep-ph/0112083
Autor:
AMANDA collaboration
Publikováno v:
Astropart.Phys.16:345-359,2002
The core collapse of a massive star in the Milky Way will produce a neutrino burst, intense enough to be detected by existing underground detectors. The AMANDA neutrino telescope located deep in the South Pole ice can detect MeV neutrinos by a collec
Externí odkaz:
http://arxiv.org/abs/astro-ph/0105460