The ANTARES telescope neutrino alert system

M. Ageron; 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; Ph 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. Martínez-Mora; A. Meli; T. Montaruli; L. Moscoso; H. Motz; M. Neff; E. Nezri; D. Palioselitis; G. E. Pǎvǎlaş; 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; Th 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.astropartphys.2011.11.011

The ANTARES telescope neutrino alert system

M. Ageron, 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-CaboB. Bouhou, M. C. Bouwhuis, J. Brunner, J. Busto, F. Camarena, A. Capone, C. Cârloganu, G. Carminati, J. Carr, S. Cecchini, Z. Charif, Ph 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. Martínez-Mora, A. Meli, T. Montaruli, L. Moscoso, H. Motz, M. Neff, E. Nezri, D. Palioselitis, G. E. Pǎvǎlaş, 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, Th 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

66 被引用数 (Scopus)

抄録

The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are generated for special events, such as two or more neutrinos, coincident in time and direction, or single neutrinos of very high energy.

本文言語	English
ページ（範囲）	530-536
ページ数	7
ジャーナル	Astroparticle Physics
巻	35
号	8
DOI	https://doi.org/10.1016/j.astropartphys.2011.11.011
出版ステータス	Published - 2012 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.2011.11.011

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Ageron, M., 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., ... Zúñiga, J. (2012). The ANTARES telescope neutrino alert system. Astroparticle Physics, 35(8), 530-536. https://doi.org/10.1016/j.astropartphys.2011.11.011

Ageron, M, 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, Martínez-Mora, JA, Meli, A, Montaruli, T, Moscoso, L, Motz, H, Neff, M, Nezri, E, Palioselitis, D, Pǎvǎlaş, 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, 'The ANTARES telescope neutrino alert system', Astroparticle Physics, vol. 35, no. 8, pp. 530-536. https://doi.org/10.1016/j.astropartphys.2011.11.011

@article{7e4d56dcc39c42b6a2ce06d85648e13b,

title = "The ANTARES telescope neutrino alert system",

abstract = "The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are generated for special events, such as two or more neutrinos, coincident in time and direction, or single neutrinos of very high energy.",

keywords = "ANTARES, Neutrino astronomy, Optical follow-up, Transient sources",

author = "M. Ageron and 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 Ph 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 Mart{\'i}nez-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 Pǎvǎla{\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 Th 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}nergie 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{\textquoteright}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. Funding Information: This work has been financially supported by the GdR PCHE in France. We want to thank M. Kowalski for discussions on the neutrino triggers and the organization of the optical follow-up.",

year = "2012",

month = mar,

doi = "10.1016/j.astropartphys.2011.11.011",

language = "English",

volume = "35",

pages = "530--536",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier",

number = "8",

}

TY - JOUR

T1 - The ANTARES telescope neutrino alert system

AU - Ageron, M.

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, Ph

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 - Martínez-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 - Pǎvǎlaş, 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, Th

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 à l’énergie 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. Funding Information: This work has been financially supported by the GdR PCHE in France. We want to thank M. Kowalski for discussions on the neutrino triggers and the organization of the optical follow-up.

PY - 2012/3

Y1 - 2012/3

N2 - The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are generated for special events, such as two or more neutrinos, coincident in time and direction, or single neutrinos of very high energy.

AB - The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are generated for special events, such as two or more neutrinos, coincident in time and direction, or single neutrinos of very high energy.

KW - ANTARES

KW - Neutrino astronomy

KW - Optical follow-up

KW - Transient sources

UR - http://www.scopus.com/inward/record.url?scp=84857556327&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84857556327&partnerID=8YFLogxK

U2 - 10.1016/j.astropartphys.2011.11.011

DO - 10.1016/j.astropartphys.2011.11.011

M3 - Article

AN - SCOPUS:84857556327

SN - 0927-6505

VL - 35

SP - 530

EP - 536

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 8

ER -

The ANTARES telescope neutrino alert system

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