Aguilar JA, Al Samarai I, Albert A, Andre M, Anghinolfi M, Anton G, Anvar S, Ardid M, Jesus ACA, Astraatmadja T, Auberth JJ, Baret B, Basa S, Bertin V, Biagl S, Bigi A, Bigongiari C, Bogazzi C, Bou-Cabo M, Bouhou B, Bouwhuis MC, Brunner J, Busto J, Camarena F, Capone A, Carloganu C, Carminati G, Carr J, Cecchini S, Charif Z, Charvis P, Chiarusi T, Circella M, Coniglione R, Costantini H, Coyle P, Curtil C, Decowski MP, Dekeyser I, Deschamps A, Distefano C, Donzaud C, Dornic D, Dorosti Q, Drouhin D, Eberl T, Emanuele U, Enzenhöfer A, Ernenwein JP, Escoffier S, Fermani P, Ferri M, Flaminio V, Folger F, Fritsch U, Fuda JL, Galata S, Gay P, Giacomelli G, Giordano V, Gomez-Gonzalez JP, Graf K, Guillard G, Halladjian G, Hallewell G, Van Haren H, Hartman J, Heijboer AJ, Hello Y, Hernandez-Rey JJ, Herold B, Hößl J, Hsu CC, De Jong M, Kadler M, Kalekin O, Kappes A, Katz U, Kavatsyuk O, Kooijman P, Koppe C, Kouchner A, Kreykenbohm I, Kulikovskiy V, Lahmann R, Lamare P, Larosa G, Lattuada D, Lefevre D, Lim G, Lo Presti D, Loehner H, Loucatos S, Mangano S, Marcelin M, Margiotta A, Martinez-Mora JA, Meli A, Montaruli T, Moscoso L, Motz H, Neff M, Nezri E, Palioselitis D, Pavalas GE, Payet K, Payre P, Petrovic J, Piattelli P, Picot-Clemente N, Popa V, Pradier T, Presani E, Racca C, Reed C, Richardt C, Richter R, Riviere C, Robert A, Roensch K, Rostovtsev A, Ruiz-Rivas J, Rujoiu M, Russo GV, Salesa F, Sapienza P, Schoeck F, Schuller JP, Schuessler F, Shanidze R, Simeone F, Spies A, Spurio M, Steijger JJM, Stolarczyk T, Sanchez-Losa A, Taiuti M, Tamburini C, Toscano S, Vallage B, Van Elewyck V, Vannoni G, Vecchi M, Vernin P, Wijnker G, Wilms J, De Wolf E, Yepes H, Zaborov D, Zornoza JD, Zuniga J (2012)
Publication Status: Published
Publication Type: Journal article
Publication year: 2012
Publisher: ELSEVIER SCIENCE BV
Book Volume: 675
Pages Range: 56-62
DOI: 10.1016/j.nima.2012.01.060
The primary aim of ANTARES is neutrino astronomy with upward going muons created in charged current muon neutrino interactions in the detector and its surroundings. Downward going muons are background for neutrino searches. These muons are the decay products of cosmic-ray collisions in the Earth's atmosphere far above the detector. This paper presents a method to identify and count electromagnetic showers induced along atmospheric muon tracks with the ANTARES detector. The method is applied to both cosmic muon data and simulations and its applicability to the reconstruction of muon event energies is demonstrated. (C) 2012 Elsevier B.V. All rights reserved.
APA:
Aguilar, J.A., Al Samarai, I., Albert, A., Andre, M., Anghinolfi, M., Anton, G.,... Zuniga, J. (2012). A method for detection of muon induced electromagnetic showers with the ANTARES detector. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 675, 56-62. https://doi.org/10.1016/j.nima.2012.01.060
MLA:
Aguilar, J. A., et al. "A method for detection of muon induced electromagnetic showers with the ANTARES detector." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 675 (2012): 56-62.
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