The NEMO Collaboration installed art underwater detector including most of the critical elements of a possible km(3) neutrino telescope: a four-floor tower (called Mini-Tower) and a Junction Box, including the data transmission, the power distribution, the timing calibration and the acoustic positioning systems. These technical Solutions will be evaluated, among others proposed for the construction of the km(3) detector, within the KM3NeT Consortium. The main test of this test experiment was the validation of the proposed design solutions mentioned above. We present results of the analysis of data collected with the NEMO Mini-Tower. The position of PMTs is determined through the acoustic position system; signals detected with PMTs are used to reconstruct the tracks of atmospheric muons. The angular distribution of atmospheric muons was measured and results were compared with Monte Carlo simulations.
Status of NEMO: results from the NEMO Phase-1 detector / C., Distefano; Nemo, Collaboration; Capone, Antonio. - In: NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS. - ISSN 0920-5632. - STAMPA. - 190:(2009), pp. 109-114. (Intervento presentato al convegno Cosmic Ray International Seminar tenutosi a Malfa; Italy) [10.1016/j.nuclphysbps.2009.03.075].
Status of NEMO: results from the NEMO Phase-1 detector
CAPONE, Antonio
2009
Abstract
The NEMO Collaboration installed art underwater detector including most of the critical elements of a possible km(3) neutrino telescope: a four-floor tower (called Mini-Tower) and a Junction Box, including the data transmission, the power distribution, the timing calibration and the acoustic positioning systems. These technical Solutions will be evaluated, among others proposed for the construction of the km(3) detector, within the KM3NeT Consortium. The main test of this test experiment was the validation of the proposed design solutions mentioned above. We present results of the analysis of data collected with the NEMO Mini-Tower. The position of PMTs is determined through the acoustic position system; signals detected with PMTs are used to reconstruct the tracks of atmospheric muons. The angular distribution of atmospheric muons was measured and results were compared with Monte Carlo simulations.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
