A method for detection of muon induced electromagnetic showers with the ANTARES detector

J. A. Aguilar; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J. J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; A. Bigi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; B. Bouhou; M. C. Bouwhuis; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Cârloganu; G. Carminati; J. Carr; S. Cecchini; Z. Charif; P. Charvis; T. Chiarusi; M. Circella; R. Coniglione; H. Costantini; P. Coyle; C. Curtil; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; A. Enzenhöfer; J. P. Ernenwein; S. Escoffier; P. Fermani; M. Ferri; V. Flaminio; F. Folger; U. Fritsch; J. L. Fuda; S. Galatà; P. Gay; G. Giacomelli; V. Giordano; J. P. Gómez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. Van Haren; J. Hartman; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; C. C. Hsu; M. De Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; O. Kavatsyuk; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; P. Lamare; G. Larosa; D. Lattuada; D. Lefèvre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martinez-Mora; A. Meli; T. Montaruli; L. Moscoso; H. Motz; M. Neff; E. Nezri; D. Palioselitis; G. E. Pvlaş; K. Payet; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; C. Richardt; R. Richter; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; J. Ruiz-Rivas; M. Rujoiu; G. V. Russo; F. Salesa; P. Sapienza; F. Schöck; J. P. Schuller; F. Schüssler; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. J.M. Steijger; T. Stolarczyk; A. Sánchez-Losa; M. Taiuti; C. Tamburini; S. Toscano; B. Vallage; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; G. Wijnker; J. Wilms; E. De Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

doi:10.1016/j.nima.2012.01.060

A method for detection of muon induced electromagnetic showers with the ANTARES detector

J. A. Aguilar, I. Al Samarai, A. Albert, M. André, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, A. C. Assis Jesus, T. Astraatmadja, J. J. Aubert, B. Baret, S. Basa, V. Bertin, S. Biagi, A. Bigi, C. Bigongiari, C. Bogazzi, M. Bou-Cabo, B. BouhouM. C. Bouwhuis, J. Brunner, J. Busto, F. Camarena, A. Capone, C. Cârloganu, G. Carminati, J. Carr, S. Cecchini, Z. Charif, P. Charvis, T. Chiarusi, M. Circella, R. Coniglione, H. Costantini, P. Coyle, C. Curtil, M. P. Decowski, I. Dekeyser, A. Deschamps, C. Distefano, C. Donzaud, D. Dornic, Q. Dorosti, D. Drouhin, T. Eberl, U. Emanuele, A. Enzenhöfer, J. P. Ernenwein, S. Escoffier, P. Fermani, M. Ferri, V. Flaminio, F. Folger, U. Fritsch, J. L. Fuda, S. Galatà, P. Gay, G. Giacomelli, V. Giordano, J. P. Gómez-González, K. Graf, G. Guillard, G. Halladjian, G. Hallewell, H. Van Haren, J. Hartman, A. J. Heijboer, Y. Hello, J. J. Hernández-Rey, B. Herold, J. Hößl, C. C. Hsu, M. De Jong, M. Kadler, O. Kalekin, A. Kappes, U. Katz, O. Kavatsyuk, P. Kooijman, C. Kopper, A. Kouchner, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, P. Lamare, G. Larosa, D. Lattuada, D. Lefèvre, G. Lim, D. Lo Presti, H. Loehner, S. Loucatos, S. Mangano^*, M. Marcelin, A. Margiotta, J. A. Martinez-Mora, A. Meli, T. Montaruli, L. Moscoso, H. Motz, M. Neff, E. Nezri, D. Palioselitis, G. E. Pvlaş, K. Payet, P. Payre, J. Petrovic, P. Piattelli, N. Picot-Clemente, V. Popa, T. Pradier, E. Presani, C. Racca, C. Reed, C. Richardt, R. Richter, C. Rivière, A. Robert, K. Roensch, A. Rostovtsev, J. Ruiz-Rivas, M. Rujoiu, G. V. Russo, F. Salesa, P. Sapienza, F. Schöck, J. P. Schuller, F. Schüssler, R. Shanidze, F. Simeone, A. Spies, M. Spurio, J. J.M. Steijger, T. Stolarczyk, A. Sánchez-Losa, M. Taiuti, C. Tamburini, S. Toscano, B. Vallage, V. Van Elewyck, G. Vannoni, M. Vecchi, P. Vernin, G. Wijnker, J. Wilms, E. De Wolf, H. Yepes, D. Zaborov, J. D. Zornoza, J. Zúñiga

^*この研究の対応する著者

研究成果: Article › 査読

4 被引用数 (Scopus)

抄録

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 Earths 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.

本文言語	English
ページ（範囲）	56-62
ページ数	7
ジャーナル	Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
巻	675
DOI	https://doi.org/10.1016/j.nima.2012.01.060
出版ステータス	Published - 2012 5月 21
外部発表	はい

ASJC Scopus subject areas

核物理学および高エネルギー物理学
器械工学

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10.1016/j.nima.2012.01.060

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Aguilar, J. A., Al Samarai, I., Albert, A., André, M., Anghinolfi, M., Anton, G., Anvar, S., Ardid, M., Assis Jesus, A. C., Astraatmadja, T., Aubert, J. J., Baret, B., Basa, S., Bertin, V., Biagi, S., Bigi, A., Bigongiari, C., Bogazzi, C., Bou-Cabo, M., ... Zúñiga, 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

Aguilar, JA, Al Samarai, I, Albert, A, André, M, Anghinolfi, M, Anton, G, Anvar, S, Ardid, M, Assis Jesus, AC, Astraatmadja, T, Aubert, JJ, Baret, B, Basa, S, Bertin, V, Biagi, S, Bigi, A, Bigongiari, C, Bogazzi, C, Bou-Cabo, M, Bouhou, B, Bouwhuis, MC, Brunner, J, Busto, J, Camarena, F, Capone, A, Cârloganu, 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, Galatà, S, Gay, P, Giacomelli, G, Giordano, V, Gómez-González, JP, Graf, K, Guillard, G, Halladjian, G, Hallewell, G, Van Haren, H, Hartman, J, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Herold, B, Hößl, J, Hsu, CC, De Jong, M, Kadler, M, Kalekin, O, Kappes, A, Katz, U, Kavatsyuk, O, Kooijman, P, Kopper, C, Kouchner, A, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Lamare, P, Larosa, G, Lattuada, D, Lefèvre, 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, Pvlaş, 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, Rivière, C, Robert, A, Roensch, K, Rostovtsev, A, Ruiz-Rivas, J, Rujoiu, M, Russo, GV, Salesa, F, Sapienza, P, Schöck, F, Schuller, JP, Schüssler, F, Shanidze, R, Simeone, F, Spies, A, Spurio, M, Steijger, JJM, Stolarczyk, T, Sánchez-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 & Zúñiga, 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, vol. 675, pp. 56-62. https://doi.org/10.1016/j.nima.2012.01.060

@article{eae388ed60d5483ba380e743906f57ac,

title = "A method for detection of muon induced electromagnetic showers with the ANTARES detector",

abstract = "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 Earths 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.",

keywords = "Electromagnetic shower identification, Energy reconstruction, High energy muons, Neutrino telescope",

author = "Aguilar, {J. A.} and {Al Samarai}, I. and A. Albert and M. Andr{\'e} and M. Anghinolfi and G. Anton and S. Anvar and M. Ardid and {Assis Jesus}, {A. C.} and T. Astraatmadja and Aubert, {J. J.} and B. Baret and S. Basa and V. Bertin and S. Biagi and A. Bigi and C. Bigongiari and C. Bogazzi and M. Bou-Cabo and B. Bouhou and Bouwhuis, {M. C.} and J. Brunner and J. Busto and F. Camarena and A. Capone and C. C{\^a}rloganu and G. Carminati and J. Carr and S. Cecchini and Z. Charif and P. Charvis and T. Chiarusi and M. Circella and R. Coniglione and H. Costantini and P. Coyle and C. Curtil and Decowski, {M. P.} and I. Dekeyser and A. Deschamps and C. Distefano and C. Donzaud and D. Dornic and Q. Dorosti and D. Drouhin and T. Eberl and U. Emanuele and A. Enzenh{\"o}fer and Ernenwein, {J. P.} and S. Escoffier and P. Fermani and M. Ferri and V. Flaminio and F. Folger and U. Fritsch and Fuda, {J. L.} and S. Galat{\`a} and P. Gay and G. Giacomelli and V. Giordano and G{\'o}mez-Gonz{\'a}lez, {J. P.} and K. Graf and G. Guillard and G. Halladjian and G. Hallewell and {Van Haren}, H. and J. Hartman and Heijboer, {A. J.} and Y. Hello and Hern{\'a}ndez-Rey, {J. J.} and B. Herold and J. H{\"o}{\ss}l and Hsu, {C. C.} and {De Jong}, M. and M. Kadler and O. Kalekin and A. Kappes and U. Katz and O. Kavatsyuk and P. Kooijman and C. Kopper and A. Kouchner and I. Kreykenbohm and V. Kulikovskiy and R. Lahmann and P. Lamare and G. Larosa and D. Lattuada and D. Lef{\`e}vre and G. Lim and {Lo Presti}, D. and H. Loehner and S. Loucatos and S. Mangano and M. Marcelin and A. Margiotta and Martinez-Mora, {J. A.} and A. Meli and T. Montaruli and L. Moscoso and H. Motz and M. Neff and E. Nezri and D. Palioselitis and Pvla{\c s}, {G. E.} and K. Payet and P. Payre and J. Petrovic and P. Piattelli and N. Picot-Clemente and V. Popa and T. Pradier and E. Presani and C. Racca and C. Reed and C. Richardt and R. Richter and C. Rivi{\`e}re and A. Robert and K. Roensch and A. Rostovtsev and J. Ruiz-Rivas and M. Rujoiu and Russo, {G. V.} and F. Salesa and P. Sapienza and F. Sch{\"o}ck and Schuller, {J. P.} and F. Sch{\"u}ssler and R. Shanidze and F. Simeone and A. Spies and M. Spurio and Steijger, {J. J.M.} and T. Stolarczyk and A. S{\'a}nchez-Losa and M. Taiuti and C. Tamburini and S. Toscano and B. Vallage and {Van Elewyck}, V. and G. Vannoni and M. Vecchi and P. Vernin and G. Wijnker and J. Wilms and {De Wolf}, E. and H. Yepes and D. Zaborov and Zornoza, {J. D.} and J. Z{\'u}{\~n}iga",

note = "Funding Information: The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS) , Commissariat {\'a} l{\textquoteright}{\'e}negie atomique et aux {\'e}nergies alternatives (CEA) , Agence National de la Recherche (ANR) , Commission Europ{\'e}enne (FEDER fund and Marie Curie Program) , R{\'e}gion Alsace (contrat CPER) , R{\'e}gion Provence-Alpes-C{\^o}te d'Azur, D{\'e}partement du Var and Ville de La Seyne-sur-Mer, France ; Bundesministerium f{\"u}r Bildung und Forschung (BMBF), Germany ; Istituto Nazionale di Fisica Nucleare (INFN), Italy ; Stichting voor Fundamenteel Onderzoek der Materie (FOM) , Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands ; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania ; Ministerio de Ciencia e Innovaci{\'o}n (MICINN) , Prometeo of Generalitat Valenciana and MultiDark, Spain . We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.",

year = "2012",

month = may,

day = "21",

doi = "10.1016/j.nima.2012.01.060",

language = "English",

volume = "675",

pages = "56--62",

journal = "Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment",

issn = "0168-9002",

publisher = "Elsevier",

}

TY - JOUR

T1 - A method for detection of muon induced electromagnetic showers with the ANTARES detector

AU - Aguilar, J. A.

AU - Al Samarai, I.

AU - Albert, A.

AU - André, M.

AU - Anghinolfi, M.

AU - Anton, G.

AU - Anvar, S.

AU - Ardid, M.

AU - Assis Jesus, A. C.

AU - Astraatmadja, T.

AU - Aubert, J. J.

AU - Baret, B.

AU - Basa, S.

AU - Bertin, V.

AU - Biagi, S.

AU - Bigi, A.

AU - Bigongiari, C.

AU - Bogazzi, C.

AU - Bou-Cabo, M.

AU - Bouhou, B.

AU - Bouwhuis, M. C.

AU - Brunner, J.

AU - Busto, J.

AU - Camarena, F.

AU - Capone, A.

AU - Cârloganu, C.

AU - Carminati, G.

AU - Carr, J.

AU - Cecchini, S.

AU - Charif, Z.

AU - Charvis, P.

AU - Chiarusi, T.

AU - Circella, M.

AU - Coniglione, R.

AU - Costantini, H.

AU - Coyle, P.

AU - Curtil, C.

AU - Decowski, M. P.

AU - Dekeyser, I.

AU - Deschamps, A.

AU - Distefano, C.

AU - Donzaud, C.

AU - Dornic, D.

AU - Dorosti, Q.

AU - Drouhin, D.

AU - Eberl, T.

AU - Emanuele, U.

AU - Enzenhöfer, A.

AU - Ernenwein, J. P.

AU - Escoffier, S.

AU - Fermani, P.

AU - Ferri, M.

AU - Flaminio, V.

AU - Folger, F.

AU - Fritsch, U.

AU - Fuda, J. L.

AU - Galatà, S.

AU - Gay, P.

AU - Giacomelli, G.

AU - Giordano, V.

AU - Gómez-González, J. P.

AU - Graf, K.

AU - Guillard, G.

AU - Halladjian, G.

AU - Hallewell, G.

AU - Van Haren, H.

AU - Hartman, J.

AU - Heijboer, A. J.

AU - Hello, Y.

AU - Hernández-Rey, J. J.

AU - Herold, B.

AU - Hößl, J.

AU - Hsu, C. C.

AU - De Jong, M.

AU - Kadler, M.

AU - Kalekin, O.

AU - Kappes, A.

AU - Katz, U.

AU - Kavatsyuk, O.

AU - Kooijman, P.

AU - Kopper, C.

AU - Kouchner, A.

AU - Kreykenbohm, I.

AU - Kulikovskiy, V.

AU - Lahmann, R.

AU - Lamare, P.

AU - Larosa, G.

AU - Lattuada, D.

AU - Lefèvre, D.

AU - Lim, G.

AU - Lo Presti, D.

AU - Loehner, H.

AU - Loucatos, S.

AU - Mangano, S.

AU - Marcelin, M.

AU - Margiotta, A.

AU - Martinez-Mora, J. A.

AU - Meli, A.

AU - Montaruli, T.

AU - Moscoso, L.

AU - Motz, H.

AU - Neff, M.

AU - Nezri, E.

AU - Palioselitis, D.

AU - Pvlaş, G. E.

AU - Payet, K.

AU - Payre, P.

AU - Petrovic, J.

AU - Piattelli, P.

AU - Picot-Clemente, N.

AU - Popa, V.

AU - Pradier, T.

AU - Presani, E.

AU - Racca, C.

AU - Reed, C.

AU - Richardt, C.

AU - Richter, R.

AU - Rivière, C.

AU - Robert, A.

AU - Roensch, K.

AU - Rostovtsev, A.

AU - Ruiz-Rivas, J.

AU - Rujoiu, M.

AU - Russo, G. V.

AU - Salesa, F.

AU - Sapienza, P.

AU - Schöck, F.

AU - Schuller, J. P.

AU - Schüssler, F.

AU - Shanidze, R.

AU - Simeone, F.

AU - Spies, A.

AU - Spurio, M.

AU - Steijger, J. J.M.

AU - Stolarczyk, T.

AU - Sánchez-Losa, A.

AU - Taiuti, M.

AU - Tamburini, C.

AU - Toscano, S.

AU - Vallage, B.

AU - Van Elewyck, V.

AU - Vannoni, G.

AU - Vecchi, M.

AU - Vernin, P.

AU - Wijnker, G.

AU - Wilms, J.

AU - De Wolf, E.

AU - Yepes, H.

AU - Zaborov, D.

AU - Zornoza, J. D.

AU - Zúñiga, J.

N1 - Funding Information: The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS) , Commissariat á l’énegie atomique et aux énergies alternatives (CEA) , Agence National de la Recherche (ANR) , Commission Européenne (FEDER fund and Marie Curie Program) , Région Alsace (contrat CPER) , Région Provence-Alpes-Côte d'Azur, Département du Var and Ville de La Seyne-sur-Mer, France ; Bundesministerium für Bildung und Forschung (BMBF), Germany ; Istituto Nazionale di Fisica Nucleare (INFN), Italy ; Stichting voor Fundamenteel Onderzoek der Materie (FOM) , Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands ; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania ; Ministerio de Ciencia e Innovación (MICINN) , Prometeo of Generalitat Valenciana and MultiDark, Spain . We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.

PY - 2012/5/21

Y1 - 2012/5/21

N2 - 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 Earths 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.

AB - 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 Earths 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.

KW - Electromagnetic shower identification

KW - Energy reconstruction

KW - High energy muons

KW - Neutrino telescope

UR - http://www.scopus.com/inward/record.url?scp=84858305729&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84858305729&partnerID=8YFLogxK

U2 - 10.1016/j.nima.2012.01.060

DO - 10.1016/j.nima.2012.01.060

M3 - Article

AN - SCOPUS:84858305729

SN - 0168-9002

VL - 675

SP - 56

EP - 62

JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

ER -

A method for detection of muon induced electromagnetic showers with the ANTARES detector

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