Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope

J. A. Aguilar; I. Al Samarai; A. Albert; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J. J. Aubert; R. Auer; B. Baret; S. Basa; M. Bazzotti; V. Bertin; S. Biagi; C. Bigongiari; M. Bou-Cabo; M. C. Bouwhuis; A. Brown; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Cârloganu; G. Carminati; J. Carr; E. Castorina; V. Cavasinni; S. Cecchini; Ph Charvis; T. Chiarusi; N. Chon Sen; M. Circella; R. Coniglione; H. Costantini; N. Cottini; P. Coyle; C. Curtil; G. De Bonis; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; D. Drouhin; T. Eberl; U. Emanuele; J. P. Ernenwein; S. Escoffier; F. Fehr; V. Flaminio; K. Fratini; U. Fritsch; J. L. Fuda; P. Gay; G. Giacomelli; J. P. Gómez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; M. de Jong; N. Kalantar-Nayestanaki; O. Kalekin; A. Kappes; U. Katz; P. Kooijman; C. Kopper; A. Kouchner; W. Kretschmer; R. Lahmann; P. Lamare; G. Lambard; G. Larosa; H. Laschinsky; D. Lefèvre; G. Lelaizant; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; F. Lucarelli; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martinez-Mora; A. Mazure; T. Montaruli; M. Morganti; L. Moscoso; H. Motz; C. Naumann; M. Neff; R. Ostasch; G. Palioselitis; G. E. Pǎvǎlaş; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; C. Picq; R. Pillet; V. Popa; T. Pradier; E. Presani; C. Racca; A. Radu; C. Reed; C. Richardt; M. Rujoiu; V. Russo; F. Salesa; P. Sapienza; F. Schoeck; J. P. Schuller; R. Shanidze; F. Simeone; M. Spurio; J. J.M. Steijger; Th Stolarczyk; C. Tamburini; L. Tasca; S. Toscano; B. Vallage; V. Van Elewyck; M. Vecchi; P. Vernin; G. Wijnker; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

doi:10.1016/j.astropartphys.2009.12.002

Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope

J. A. Aguilar, I. Al Samarai, A. Albert, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, A. C. Assis Jesus, T. Astraatmadja, J. J. Aubert, R. Auer, B. Baret, S. Basa, M. Bazzotti, V. Bertin, S. Biagi, C. Bigongiari, M. Bou-Cabo, M. C. Bouwhuis, A. BrownJ. Brunner, J. Busto, F. Camarena, A. Capone, C. Cârloganu, G. Carminati, J. Carr, E. Castorina, V. Cavasinni, S. Cecchini, Ph Charvis, T. Chiarusi, N. Chon Sen, M. Circella, R. Coniglione, H. Costantini, N. Cottini, P. Coyle, C. Curtil, G. De Bonis, M. P. Decowski, I. Dekeyser, A. Deschamps, C. Distefano, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, U. Emanuele, J. P. Ernenwein, S. Escoffier, F. Fehr, V. Flaminio, K. Fratini, U. Fritsch, J. L. Fuda, P. Gay, G. Giacomelli, J. P. Gómez-González, K. Graf, G. Guillard, G. Halladjian, G. Hallewell, H. van Haren, A. J. Heijboer, Y. Hello, J. J. Hernández-Rey, B. Herold, J. Hößl, M. de Jong, N. Kalantar-Nayestanaki, O. Kalekin, A. Kappes, U. Katz, P. Kooijman, C. Kopper, A. Kouchner, W. Kretschmer, R. Lahmann, P. Lamare, G. Lambard, G. Larosa, H. Laschinsky, D. Lefèvre, G. Lelaizant, G. Lim, D. Lo Presti, H. Loehner, S. Loucatos, F. Lucarelli, S. Mangano, M. Marcelin, A. Margiotta, J. A. Martinez-Mora, A. Mazure, T. Montaruli, M. Morganti, L. Moscoso, H. Motz, C. Naumann, M. Neff, R. Ostasch, G. Palioselitis, G. E. Pǎvǎlaş, P. Payre, J. Petrovic, P. Piattelli, N. Picot-Clemente, C. Picq, R. Pillet, V. Popa, T. Pradier, E. Presani, C. Racca, A. Radu, C. Reed, C. Richardt, M. Rujoiu, V. Russo, F. Salesa, P. Sapienza, F. Schoeck, J. P. Schuller, R. Shanidze, F. Simeone, M. Spurio, J. J.M. Steijger, Th Stolarczyk, C. Tamburini, L. Tasca, S. Toscano, B. Vallage, V. Van Elewyck, M. Vecchi, P. Vernin, G. Wijnker, 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

38 被引用数 (Scopus)

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A new method for the measurement of the muon flux in the deep-sea ANTARES neutrino telescope and its dependence on the depth is presented. The method is based on the observation of coincidence signals in adjacent storeys of the detector. This yields an energy threshold of about 4 GeV. The main sources of optical background are the decay of ⁴⁰K and the bioluminescence in the sea water. The ⁴⁰K background is used to calibrate the efficiency of the photo-multiplier tubes.

本文言語	English
ページ（範囲）	86-90
ページ数	5
ジャーナル	Astroparticle Physics
巻	33
号	2
DOI	https://doi.org/10.1016/j.astropartphys.2009.12.002
出版ステータス	Published - 2010 3月
外部発表	はい

ASJC Scopus subject areas

天文学と天体物理学

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10.1016/j.astropartphys.2009.12.002

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Aguilar, J. A., Al Samarai, I., Albert, A., Anghinolfi, M., Anton, G., Anvar, S., Ardid, M., Assis Jesus, A. C., Astraatmadja, T., Aubert, J. J., Auer, R., Baret, B., Basa, S., Bazzotti, M., Bertin, V., Biagi, S., Bigongiari, C., Bou-Cabo, M., Bouwhuis, M. C., ... Zúñiga, J. (2010). Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope. Astroparticle Physics, 33(2), 86-90. https://doi.org/10.1016/j.astropartphys.2009.12.002

Aguilar, JA, Al Samarai, I, Albert, A, Anghinolfi, M, Anton, G, Anvar, S, Ardid, M, Assis Jesus, AC, Astraatmadja, T, Aubert, JJ, Auer, R, Baret, B, Basa, S, Bazzotti, M, Bertin, V, Biagi, S, Bigongiari, C, Bou-Cabo, M, Bouwhuis, MC, Brown, A, Brunner, J, Busto, J, Camarena, F, Capone, A, Cârloganu, C, Carminati, G, Carr, J, Castorina, E, Cavasinni, V, Cecchini, S, Charvis, P, Chiarusi, T, Chon Sen, N, Circella, M, Coniglione, R, Costantini, H, Cottini, N, Coyle, P, Curtil, C, De Bonis, G, Decowski, MP, Dekeyser, I, Deschamps, A, Distefano, C, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Emanuele, U, Ernenwein, JP, Escoffier, S, Fehr, F, Flaminio, V, Fratini, K, Fritsch, U, Fuda, JL, Gay, P, Giacomelli, G, Gómez-González, JP, Graf, K, Guillard, G, Halladjian, G, Hallewell, G, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Herold, B, Hößl, J, de Jong, M, Kalantar-Nayestanaki, N, Kalekin, O, Kappes, A, Katz, U, Kooijman, P, Kopper, C, Kouchner, A, Kretschmer, W, Lahmann, R, Lamare, P, Lambard, G, Larosa, G, Laschinsky, H, Lefèvre, D, Lelaizant, G, Lim, G, Lo Presti, D, Loehner, H, Loucatos, S, Lucarelli, F, Mangano, S, Marcelin, M, Margiotta, A, Martinez-Mora, JA, Mazure, A, Montaruli, T, Morganti, M, Moscoso, L, Motz, H, Naumann, C, Neff, M, Ostasch, R, Palioselitis, G, Pǎvǎlaş, GE, Payre, P, Petrovic, J, Piattelli, P, Picot-Clemente, N, Picq, C, Pillet, R, Popa, V, Pradier, T, Presani, E, Racca, C, Radu, A, Reed, C, Richardt, C, Rujoiu, M, Russo, V, Salesa, F, Sapienza, P, Schoeck, F, Schuller, JP, Shanidze, R, Simeone, F, Spurio, M, Steijger, JJM, Stolarczyk, T, Tamburini, C, Tasca, L, Toscano, S, Vallage, B, Van Elewyck, V, Vecchi, M, Vernin, P, Wijnker, G, de Wolf, E, Yepes, H, Zaborov, D, Zornoza, JD & Zúñiga, J 2010, 'Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope', Astroparticle Physics, vol. 33, no. 2, pp. 86-90. https://doi.org/10.1016/j.astropartphys.2009.12.002

@article{b96709d7f64a4b97b916535c24a1b23a,

title = "Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope",

abstract = "A new method for the measurement of the muon flux in the deep-sea ANTARES neutrino telescope and its dependence on the depth is presented. The method is based on the observation of coincidence signals in adjacent storeys of the detector. This yields an energy threshold of about 4 GeV. The main sources of optical background are the decay of 40K and the bioluminescence in the sea water. The 40K background is used to calibrate the efficiency of the photo-multiplier tubes.",

keywords = "Atmospheric muons, Depth intensity relation, Potassium-40",

author = "Aguilar, {J. A.} and {Al Samarai}, I. and A. Albert 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 R. Auer and B. Baret and S. Basa and M. Bazzotti and V. Bertin and S. Biagi and C. Bigongiari and M. Bou-Cabo and Bouwhuis, {M. C.} and A. Brown and J. Brunner and J. Busto and F. Camarena and A. Capone and C. C{\^a}rloganu and G. Carminati and J. Carr and E. Castorina and V. Cavasinni and S. Cecchini and Ph Charvis and T. Chiarusi and {Chon Sen}, N. and M. Circella and R. Coniglione and H. Costantini and N. Cottini and P. Coyle and C. Curtil and {De Bonis}, G. and Decowski, {M. P.} and I. Dekeyser and A. Deschamps and C. Distefano and C. Donzaud and D. Dornic and D. Drouhin and T. Eberl and U. Emanuele and Ernenwein, {J. P.} and S. Escoffier and F. Fehr and V. Flaminio and K. Fratini and U. Fritsch and Fuda, {J. L.} and P. Gay and G. Giacomelli 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 Heijboer, {A. J.} and Y. Hello and Hern{\'a}ndez-Rey, {J. J.} and B. Herold and J. H{\"o}{\ss}l and {de Jong}, M. and N. Kalantar-Nayestanaki and O. Kalekin and A. Kappes and U. Katz and P. Kooijman and C. Kopper and A. Kouchner and W. Kretschmer and R. Lahmann and P. Lamare and G. Lambard and G. Larosa and H. Laschinsky and D. Lef{\`e}vre and G. Lelaizant and G. Lim and {Lo Presti}, D. and H. Loehner and S. Loucatos and F. Lucarelli and S. Mangano and M. Marcelin and A. Margiotta and Martinez-Mora, {J. A.} and A. Mazure and T. Montaruli and M. Morganti and L. Moscoso and H. Motz and C. Naumann and M. Neff and R. Ostasch and G. Palioselitis and Pǎvǎla{\c s}, {G. E.} and P. Payre and J. Petrovic and P. Piattelli and N. Picot-Clemente and C. Picq and R. Pillet and V. Popa and T. Pradier and E. Presani and C. Racca and A. Radu and C. Reed and C. Richardt and M. Rujoiu and V. Russo and F. Salesa and P. Sapienza and F. Schoeck and Schuller, {J. P.} and R. Shanidze and F. Simeone and M. Spurio and Steijger, {J. J.M.} and Th Stolarczyk and C. Tamburini and L. Tasca and S. Toscano and B. Vallage and {Van Elewyck}, V. and M. Vecchi and P. Vernin and G. Wijnker 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}Energie Atomique (CEA), 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{\textquoteright}Azur, D{\'e}partement du Var and Ville de La Seyne-sur-Mer, in France; Bundesministerium f{\"u}r Bildung und Forschung (BMBF), in Germany; Istituto Nazionale di Fisica Nucleare (INFN), in Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), in The Netherlands; Russian Foundation for Basic Research (RFBR), in Russia; National Authority for Scientific Research (ANCS) in Romania; Ministerio de Ciencia e Innovaci{\'o}n (MICINN) and Prometeo of Generalitat Valenciana, in 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 = "2010",

month = mar,

doi = "10.1016/j.astropartphys.2009.12.002",

language = "English",

volume = "33",

pages = "86--90",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier",

number = "2",

}

TY - JOUR

T1 - Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope

AU - Aguilar, J. A.

AU - Al Samarai, I.

AU - Albert, A.

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 - Auer, R.

AU - Baret, B.

AU - Basa, S.

AU - Bazzotti, M.

AU - Bertin, V.

AU - Biagi, S.

AU - Bigongiari, C.

AU - Bou-Cabo, M.

AU - Bouwhuis, M. C.

AU - Brown, A.

AU - Brunner, J.

AU - Busto, J.

AU - Camarena, F.

AU - Capone, A.

AU - Cârloganu, C.

AU - Carminati, G.

AU - Carr, J.

AU - Castorina, E.

AU - Cavasinni, V.

AU - Cecchini, S.

AU - Charvis, Ph

AU - Chiarusi, T.

AU - Chon Sen, N.

AU - Circella, M.

AU - Coniglione, R.

AU - Costantini, H.

AU - Cottini, N.

AU - Coyle, P.

AU - Curtil, C.

AU - De Bonis, G.

AU - Decowski, M. P.

AU - Dekeyser, I.

AU - Deschamps, A.

AU - Distefano, C.

AU - Donzaud, C.

AU - Dornic, D.

AU - Drouhin, D.

AU - Eberl, T.

AU - Emanuele, U.

AU - Ernenwein, J. P.

AU - Escoffier, S.

AU - Fehr, F.

AU - Flaminio, V.

AU - Fratini, K.

AU - Fritsch, U.

AU - Fuda, J. L.

AU - Gay, P.

AU - Giacomelli, G.

AU - Gómez-González, J. P.

AU - Graf, K.

AU - Guillard, G.

AU - Halladjian, G.

AU - Hallewell, G.

AU - van Haren, H.

AU - Heijboer, A. J.

AU - Hello, Y.

AU - Hernández-Rey, J. J.

AU - Herold, B.

AU - Hößl, J.

AU - de Jong, M.

AU - Kalantar-Nayestanaki, N.

AU - Kalekin, O.

AU - Kappes, A.

AU - Katz, U.

AU - Kooijman, P.

AU - Kopper, C.

AU - Kouchner, A.

AU - Kretschmer, W.

AU - Lahmann, R.

AU - Lamare, P.

AU - Lambard, G.

AU - Larosa, G.

AU - Laschinsky, H.

AU - Lefèvre, D.

AU - Lelaizant, G.

AU - Lim, G.

AU - Lo Presti, D.

AU - Loehner, H.

AU - Loucatos, S.

AU - Lucarelli, F.

AU - Mangano, S.

AU - Marcelin, M.

AU - Margiotta, A.

AU - Martinez-Mora, J. A.

AU - Mazure, A.

AU - Montaruli, T.

AU - Morganti, M.

AU - Moscoso, L.

AU - Motz, H.

AU - Naumann, C.

AU - Neff, M.

AU - Ostasch, R.

AU - Palioselitis, G.

AU - Pǎvǎlaş, G. E.

AU - Payre, P.

AU - Petrovic, J.

AU - Piattelli, P.

AU - Picot-Clemente, N.

AU - Picq, C.

AU - Pillet, R.

AU - Popa, V.

AU - Pradier, T.

AU - Presani, E.

AU - Racca, C.

AU - Radu, A.

AU - Reed, C.

AU - Richardt, C.

AU - Rujoiu, M.

AU - Russo, V.

AU - Salesa, F.

AU - Sapienza, P.

AU - Schoeck, F.

AU - Schuller, J. P.

AU - Shanidze, R.

AU - Simeone, F.

AU - Spurio, M.

AU - Steijger, J. J.M.

AU - Stolarczyk, Th

AU - Tamburini, C.

AU - Tasca, L.

AU - Toscano, S.

AU - Vallage, B.

AU - Van Elewyck, V.

AU - Vecchi, M.

AU - Vernin, P.

AU - Wijnker, G.

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 à l’Energie Atomique (CEA), 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, in France; Bundesministerium für Bildung und Forschung (BMBF), in Germany; Istituto Nazionale di Fisica Nucleare (INFN), in Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), in The Netherlands; Russian Foundation for Basic Research (RFBR), in Russia; National Authority for Scientific Research (ANCS) in Romania; Ministerio de Ciencia e Innovación (MICINN) and Prometeo of Generalitat Valenciana, in 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 - 2010/3

Y1 - 2010/3

N2 - A new method for the measurement of the muon flux in the deep-sea ANTARES neutrino telescope and its dependence on the depth is presented. The method is based on the observation of coincidence signals in adjacent storeys of the detector. This yields an energy threshold of about 4 GeV. The main sources of optical background are the decay of 40K and the bioluminescence in the sea water. The 40K background is used to calibrate the efficiency of the photo-multiplier tubes.

AB - A new method for the measurement of the muon flux in the deep-sea ANTARES neutrino telescope and its dependence on the depth is presented. The method is based on the observation of coincidence signals in adjacent storeys of the detector. This yields an energy threshold of about 4 GeV. The main sources of optical background are the decay of 40K and the bioluminescence in the sea water. The 40K background is used to calibrate the efficiency of the photo-multiplier tubes.

KW - Atmospheric muons

KW - Depth intensity relation

KW - Potassium-40

UR - http://www.scopus.com/inward/record.url?scp=76549105416&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=76549105416&partnerID=8YFLogxK

U2 - 10.1016/j.astropartphys.2009.12.002

DO - 10.1016/j.astropartphys.2009.12.002

M3 - Article

AN - SCOPUS:76549105416

SN - 0927-6505

VL - 33

SP - 86

EP - 90

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 2

ER -

Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope

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