The performance of the AMANDA-II 19 string array

Details The performance of the AMANDA-II 19 string array The performance of the AMANDA-II 19 string array

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....3.1105w&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

2

Scientific paper

The AMANDA-II High Energy Neutrino Detector at the South Pole consists of 19 strings with 677 optical modules, and started operation February, 2000. We describe the detector design with the different technologies used for signal transmission. The larger geometry of the AMANDA-II detector, compared to the AMANDA-B10 detector operated in 1997, yields an improved sensitivity to high energy neutrinos, in particular a more uniform angular response. We present MC results on νµ and νe event rates and first results on separation of atmospheric νµ events.

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