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-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

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69 Scopus citations

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.

Original language	English
Pages (from-to)	530-536
Number of pages	7
Journal	Astroparticle Physics
Volume	35
Issue number	8
DOIs	https://doi.org/10.1016/j.astropartphys.2011.11.011
State	Published - Mar 2012

Keywords

ANTARES
Neutrino astronomy
Optical follow-up
Transient sources

Access to Document

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

@article{14a320d28acb4312a1257cb2cd7cf7e9,

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",

year = "2012",

month = mar,

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

language = "Ingl{\'e}s",

volume = "35",

pages = "530--536",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier",

number = "8",

}

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

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.

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 - https://www.scopus.com/pages/publications/84857556327

U2 - 10.1016/j.astropartphys.2011.11.011

DO - 10.1016/j.astropartphys.2011.11.011

M3 - Artículo

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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Keywords

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