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Zastosuj identyfikator do podlinkowania lub zacytowania tej pozycji: http://hdl.handle.net/20.500.12128/7195
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dc.contributor.authorAnkowski, A.-
dc.contributor.authorAntonello, M.-
dc.contributor.authorAprili, P.G.-
dc.contributor.authorArneodo, F.-
dc.contributor.authorBadertscher, A.-
dc.contributor.authorBaibussinov, B.-
dc.contributor.authorBaldo-Ceolin, M.-
dc.contributor.authorBattistoni, G.-
dc.contributor.authorBenetti, P.-
dc.contributor.authorBrunetti, R.-
dc.contributor.authorBueno, A.-
dc.contributor.authorCalligarich, E.-
dc.contributor.authorCambiagh, M.-
dc.contributor.authorCanci, N.-
dc.contributor.authorCarbonara, F.-
dc.contributor.authorCarmona, M.C.-
dc.contributor.authorCavanna, F.-
dc.contributor.authorCennini, P.-
dc.contributor.authorCentro, S.-
dc.contributor.authorCesana, A.-
dc.contributor.authorCieślik, K.-
dc.contributor.authorCline, D.-
dc.contributor.authorCocco, A.G.-
dc.contributor.authorDąbrowska, A.-
dc.contributor.authorDolfini, R.-
dc.contributor.authorFarnese, C.-
dc.contributor.authorFava, A.-
dc.contributor.authorFerrari, A.-
dc.contributor.authorFiorillo, G.-
dc.contributor.authorGalli, S.-
dc.contributor.authorGallo, V.-
dc.contributor.authorGarcia-Gamez, D.-
dc.contributor.authorGibin, D.-
dc.contributor.authorGigli Berzolari, A.-
dc.contributor.authorGraczyk, Konrad-
dc.contributor.authorGuglielmi, A.-
dc.contributor.authorHoleczek, Jacek-
dc.contributor.authorKiełczewska, D.-
dc.contributor.authorKisiel, Jan-
dc.contributor.authorKozłowski, T.-
dc.contributor.authorŁagoda, J.-
dc.contributor.authorLantz, M.-
dc.contributor.authorLozano, J.-
dc.contributor.authorMannocchi, G.-
dc.contributor.authorMarkiewicz, M.-
dc.contributor.authorDe La Ossa, A. Martinez-
dc.contributor.authorMauri, F.-
dc.contributor.authorMelgarejo, A.J.-
dc.contributor.authorMenegolli, A.-
dc.contributor.authorMeng, G.-
dc.contributor.authorMijakowski, P.-
dc.contributor.authorMontanari, C.-
dc.contributor.authorMuraro, S.-
dc.contributor.authorNavas, S.-
dc.contributor.authorOtwinowski, S.-
dc.contributor.authorPalamara, O.-
dc.contributor.authorPalczewski, T.J.-
dc.contributor.authorPeriale, L.-
dc.contributor.authorPiano Mortari, G.-
dc.contributor.authorPiazzoli, A.-
dc.contributor.authorPicchi, P.-
dc.contributor.authorPietropaolo, F.-
dc.contributor.authorPółchłopek, W.-
dc.contributor.authorPosiadała, M.-
dc.contributor.authorPrata, M.-
dc.contributor.authorPrzewłocki, P.-
dc.contributor.authorRappoldi, A.-
dc.contributor.authorRaselli, G.L.-
dc.contributor.authorRondio, E.-
dc.contributor.authorRossella, M.-
dc.contributor.authorRubbia, A.-
dc.contributor.authorRubbia, C.-
dc.contributor.authorSala, P.-
dc.contributor.authorScannicchio, D.-
dc.contributor.authorScaramelli, A.-
dc.contributor.authorSegreto, E.-
dc.contributor.authorSergiampietri, F.-
dc.contributor.authorSobczyk, J.-
dc.contributor.authorStefan, D.-
dc.contributor.authorStepaniak, J.-
dc.contributor.authorSulej, R.-
dc.contributor.authorSzarska, M.-
dc.contributor.authorSzeglowski, Tomasz-
dc.contributor.authorSzeptycka, M.-
dc.contributor.authorTerrani, M.-
dc.contributor.authorVaranini, F.-
dc.contributor.authorVentura, S.-
dc.contributor.authorVignoli, C.-
dc.contributor.authorWąchała, T.-
dc.contributor.authorWang, H.-
dc.contributor.authorZalewska, A.-
dc.date.accessioned2018-11-22T13:15:06Z-
dc.date.available2018-11-22T13:15:06Z-
dc.date.issued2010-
dc.identifier.citationActa Physica Polonica B, Vol. 41, no. 1 (2010), s. 103-125pl_PL
dc.identifier.issn0587-4254-
dc.identifier.urihttp://hdl.handle.net/20.500.12128/7195-
dc.description.abstractWe discuss the ICARUS T600 detector capabilities in electromagnetic shower reconstruction through the analysis of a sample of 212 events, coming from the 2001 Pavia surface test run, of hadronic interactions leading to the production of 0 mesons. Methods of shower energy and shower direction measurements were developed and the invariant mass of the photon pairs was reconstructed. The ( ) invariant mass was found to be consistent with the value of the 0 mass. The resolution of the reconstructed 0 mass was found to be equal to 27.3%. An improved analysis, carried out in order to clean the full event sample from the events measured in the crowded environment, mostly due to the trigger conditions, gave a 0 mass resolution of 16.1%, significantly better than the one evaluated for the full event sample. The trigger requirement of the coincidence of at least four photo-multiplier signals favored the selection of events with a strong pile up of cosmic ray tracks and interactions. Hence a number of candidate 0 events were heavily contaminated by other tracks and had to be rejected. Monte Carlo simulations of events with 0 production in hadronic and neutrino interactions confirmed the validity of the shower energy and shower direction reconstruction methods applied to the real data.pl_PL
dc.language.isoenpl_PL
dc.rightsUznanie autorstwa 3.0 Polska*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/pl/*
dc.subjectmetoda Monte Carlopl_PL
dc.subjectrozpady mezonówpl_PL
dc.subjectkalorymetrypl_PL
dc.subjectenergia elektromagnetycznapl_PL
dc.titleEnergy reconstruction of electromagnetic showers from [Pi 0] decays with the ICARUS T600 liquid argon TPCpl_PL
dc.typeinfo:eu-repo/semantics/articlepl_PL
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