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Results of the follow-up of ANTARES neutrino alerts

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Hauptverfasser: Albert, A., Alves, S., André, M., Ardid, M., Ardid, S., Aubert, J. -J., Aublin, J., Baret, B., Basa, S., Becherini, Y., Belhorma, B., Bendahman, M., Benfenati, F., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bouta, M., Bouwhuis, M. C., Brânzas, H., Bruijn, R., Brunner, J., Busto, J., Caiffi, B., Calvo, D., Campion, S., Capone, A., Caramete, L., Carenini, F., Carr, J., Carretero, V., Celli, S., Cerisy, L., Chabab, M., Moursli, R. Cherkaoui El, Chiarusi, T., Circella, M., Coelho, J. A. B., Coleiro, A., Coniglione, R., Coyle, P., Creusot, A., Cruz, A. S. M., Díaz, A. F., De Martino, B., Distefano, C., Di Palma, I., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., van Eeden, T., van Eijk, D., Hedri, S. El, Khayati, N. El, Enzenhöfer, A., Fermani, P., Ferrara, G., Filippini, F., Fusco, L., Gagliardini, S., García, J., Oliver, C. Gatius, Gay, P., Geißelbrecht, N., Glotin, H., Gozzini, R., Ruiz, R. Gracia, Graf, K., Guidi, C., Haegel, L., Hallmann, S., van Haren, H., Heijboer, A. J., Hello, Y., Hennig, L., Hernández-Rey, J. J., Hößl, J., Hofestädt, J., Huang, F., Illuminati, G., James, C. W., Jisse-Jung, B., de Jong, M., de Jong, P., Kadler, M., Kalekin, O., Katz, U., Kouchner, A., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Lamoureux, M., Lazo, A., Lefèvre, D., Leonora, E., Levi, G., Stum, S. Le, Loucatos, S., Maderer, L., Manczak, J., Marcelin, M., Margiotta, A., Marinelli, A., Martínez-Mora, J. A., Migliozzi, P., Moussa, A., Muller, R., Navas, S., Nezri, E., Fearraigh, B. Ó, Oukacha, E., Pāun, A., Pāvālas, G. E., Peña-Martínez, S., Perrin-Terrin, M., Piattelli, P., Popa, V., Pradier, T., Randazzo, N., Real, D., Riccobene, G., Romanov, A., Sánchez-Losa, A., Saina, A., Greus, F. Salesa, Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schnabel, J., Schumann, J., Schüssler, F., Seneca, J., Spurio, M., Stolarczyk, Th., Taiuti, M., Tayalati, Y., Tingay, S. J., Vallage, B., Vannoye, G., Van Elewyck, V., Viola, S., Vivolo, D., Wilms, J., Zavatarelli, S., Zegarelli, A., Zornoza, J. D., Zúñiga, J., Lipunov, V., Antipov, G., Balanutsa, P., Buckley, D., Budnev, N., Chasovnikov, A., Cheryasov, D., Francile, C., Gabovich, A., Gorbovskoy, E., Gorbunov, I., Gress, O., Kornilov, V., Kuznetsov, A., Iyudin, A., Podesta, R., Podesta, F., Lopez, R. Rebolo, Senik, V., Sierra-Rucart, M., Svertilov, S., Tiurina, N., Vlasenko, D., Yashin, I., Zhirkov, K., Croft, S., Kaplan, D. L., Anderson, G. E., Williams, A., Dobie, D., Bannister, K. W., Hancock, P. J., Evans, P. A., Kennea, J. A., Osborne, J. P., Cenko, S. B., Antier, S., Atteia, J. L., Boër, M., Klotz, A., Chaty, S., Hodapp, K., Savchenko, V.
Format: Preprint
Veröffentlicht: 2024
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High Energy Astrophysical Phenomena
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author Albert, A.
Alves, S.
André, M.
Ardid, M.
Ardid, S.
Aubert, J. -J.
Aublin, J.
Baret, B.
Basa, S.
Becherini, Y.
Belhorma, B.
Bendahman, M.
Benfenati, F.
Bertin, V.
Biagi, S.
Bissinger, M.
Boumaaza, J.
Bouta, M.
Bouwhuis, M. C.
Brânzas, H.
Bruijn, R.
Brunner, J.
Busto, J.
Caiffi, B.
Calvo, D.
Campion, S.
Capone, A.
Caramete, L.
Carenini, F.
Carr, J.
Carretero, V.
Celli, S.
Cerisy, L.
Chabab, M.
Moursli, R. Cherkaoui El
Chiarusi, T.
Circella, M.
Coelho, J. A. B.
Coleiro, A.
Coniglione, R.
Coyle, P.
Creusot, A.
Cruz, A. S. M.
Díaz, A. F.
De Martino, B.
Distefano, C.
Di Palma, I.
Donzaud, C.
Dornic, D.
Drouhin, D.
Eberl, T.
van Eeden, T.
van Eijk, D.
Hedri, S. El
Khayati, N. El
Enzenhöfer, A.
Fermani, P.
Ferrara, G.
Filippini, F.
Fusco, L.
Gagliardini, S.
García, J.
Oliver, C. Gatius
Gay, P.
Geißelbrecht, N.
Glotin, H.
Gozzini, R.
Ruiz, R. Gracia
Graf, K.
Guidi, C.
Haegel, L.
Hallmann, S.
van Haren, H.
Heijboer, A. J.
Hello, Y.
Hennig, L.
Hernández-Rey, J. J.
Hößl, J.
Hofestädt, J.
Huang, F.
Illuminati, G.
James, C. W.
Jisse-Jung, B.
de Jong, M.
de Jong, P.
Kadler, M.
Kalekin, O.
Katz, U.
Kouchner, A.
Kreykenbohm, I.
Kulikovskiy, V.
Lahmann, R.
Lamoureux, M.
Lazo, A.
Lefèvre, D.
Leonora, E.
Levi, G.
Stum, S. Le
Loucatos, S.
Maderer, L.
Manczak, J.
Marcelin, M.
Margiotta, A.
Marinelli, A.
Martínez-Mora, J. A.
Migliozzi, P.
Moussa, A.
Muller, R.
Navas, S.
Nezri, E.
Fearraigh, B. Ó
Oukacha, E.
Pāun, A.
Pāvālas, G. E.
Peña-Martínez, S.
Perrin-Terrin, M.
Piattelli, P.
Popa, V.
Pradier, T.
Randazzo, N.
Real, D.
Riccobene, G.
Romanov, A.
Sánchez-Losa, A.
Saina, A.
Greus, F. Salesa
Samtleben, D. F. E.
Sanguineti, M.
Sapienza, P.
Schnabel, J.
Schumann, J.
Schüssler, F.
Seneca, J.
Spurio, M.
Stolarczyk, Th.
Taiuti, M.
Tayalati, Y.
Tingay, S. J.
Vallage, B.
Vannoye, G.
Van Elewyck, V.
Viola, S.
Vivolo, D.
Wilms, J.
Zavatarelli, S.
Zegarelli, A.
Zornoza, J. D.
Zúñiga, J.
Lipunov, V.
Antipov, G.
Balanutsa, P.
Buckley, D.
Budnev, N.
Chasovnikov, A.
Cheryasov, D.
Francile, C.
Gabovich, A.
Gorbovskoy, E.
Gorbunov, I.
Gress, O.
Kornilov, V.
Kuznetsov, A.
Iyudin, A.
Podesta, R.
Podesta, F.
Lopez, R. Rebolo
Senik, V.
Sierra-Rucart, M.
Svertilov, S.
Tiurina, N.
Vlasenko, D.
Yashin, I.
Zhirkov, K.
Croft, S.
Kaplan, D. L.
Anderson, G. E.
Williams, A.
Dobie, D.
Bannister, K. W.
Hancock, P. J.
Evans, P. A.
Kennea, J. A.
Osborne, J. P.
Cenko, S. B.
Antier, S.
Atteia, J. L.
Boër, M.
Klotz, A.
Chaty, S.
Hodapp, K.
Savchenko, V.
author_facet Albert, A.
Alves, S.
André, M.
Ardid, M.
Ardid, S.
Aubert, J. -J.
Aublin, J.
Baret, B.
Basa, S.
Becherini, Y.
Belhorma, B.
Bendahman, M.
Benfenati, F.
Bertin, V.
Biagi, S.
Bissinger, M.
Boumaaza, J.
Bouta, M.
Bouwhuis, M. C.
Brânzas, H.
Bruijn, R.
Brunner, J.
Busto, J.
Caiffi, B.
Calvo, D.
Campion, S.
Capone, A.
Caramete, L.
Carenini, F.
Carr, J.
Carretero, V.
Celli, S.
Cerisy, L.
Chabab, M.
Moursli, R. Cherkaoui El
Chiarusi, T.
Circella, M.
Coelho, J. A. B.
Coleiro, A.
Coniglione, R.
Coyle, P.
Creusot, A.
Cruz, A. S. M.
Díaz, A. F.
De Martino, B.
Distefano, C.
Di Palma, I.
Donzaud, C.
Dornic, D.
Drouhin, D.
Eberl, T.
van Eeden, T.
van Eijk, D.
Hedri, S. El
Khayati, N. El
Enzenhöfer, A.
Fermani, P.
Ferrara, G.
Filippini, F.
Fusco, L.
Gagliardini, S.
García, J.
Oliver, C. Gatius
Gay, P.
Geißelbrecht, N.
Glotin, H.
Gozzini, R.
Ruiz, R. Gracia
Graf, K.
Guidi, C.
Haegel, L.
Hallmann, S.
van Haren, H.
Heijboer, A. J.
Hello, Y.
Hennig, L.
Hernández-Rey, J. J.
Hößl, J.
Hofestädt, J.
Huang, F.
Illuminati, G.
James, C. W.
Jisse-Jung, B.
de Jong, M.
de Jong, P.
Kadler, M.
Kalekin, O.
Katz, U.
Kouchner, A.
Kreykenbohm, I.
Kulikovskiy, V.
Lahmann, R.
Lamoureux, M.
Lazo, A.
Lefèvre, D.
Leonora, E.
Levi, G.
Stum, S. Le
Loucatos, S.
Maderer, L.
Manczak, J.
Marcelin, M.
Margiotta, A.
Marinelli, A.
Martínez-Mora, J. A.
Migliozzi, P.
Moussa, A.
Muller, R.
Navas, S.
Nezri, E.
Fearraigh, B. Ó
Oukacha, E.
Pāun, A.
Pāvālas, G. E.
Peña-Martínez, S.
Perrin-Terrin, M.
Piattelli, P.
Popa, V.
Pradier, T.
Randazzo, N.
Real, D.
Riccobene, G.
Romanov, A.
Sánchez-Losa, A.
Saina, A.
Greus, F. Salesa
Samtleben, D. F. E.
Sanguineti, M.
Sapienza, P.
Schnabel, J.
Schumann, J.
Schüssler, F.
Seneca, J.
Spurio, M.
Stolarczyk, Th.
Taiuti, M.
Tayalati, Y.
Tingay, S. J.
Vallage, B.
Vannoye, G.
Van Elewyck, V.
Viola, S.
Vivolo, D.
Wilms, J.
Zavatarelli, S.
Zegarelli, A.
Zornoza, J. D.
Zúñiga, J.
Lipunov, V.
Antipov, G.
Balanutsa, P.
Buckley, D.
Budnev, N.
Chasovnikov, A.
Cheryasov, D.
Francile, C.
Gabovich, A.
Gorbovskoy, E.
Gorbunov, I.
Gress, O.
Kornilov, V.
Kuznetsov, A.
Iyudin, A.
Podesta, R.
Podesta, F.
Lopez, R. Rebolo
Senik, V.
Sierra-Rucart, M.
Svertilov, S.
Tiurina, N.
Vlasenko, D.
Yashin, I.
Zhirkov, K.
Croft, S.
Kaplan, D. L.
Anderson, G. E.
Williams, A.
Dobie, D.
Bannister, K. W.
Hancock, P. J.
Evans, P. A.
Kennea, J. A.
Osborne, J. P.
Cenko, S. B.
Antier, S.
Atteia, J. L.
Boër, M.
Klotz, A.
Chaty, S.
Hodapp, K.
Savchenko, V.
contents High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. To look for transient sources associated with neutrino emission, a follow-up program of neutrino alerts has been operating within the ANTARES Collaboration since 2009. This program, named TAToO, has triggered robotic optical telescopes (MASTER, TAROT, ROTSE and the SVOM ground based telescopes) immediately after the detection of any relevant neutrino candidate and scheduled several observations in the weeks following the detection. A subset of ANTARES events with highest probabilities of being of cosmic origin has also been followed by the Swift and the INTEGRAL satellites, the Murchison Widefield Array radio telescope and the H.E.S.S. high-energy gamma-ray telescope. The results of twelve years of observations are reported. No optical counterpart has been significantly associated with an ANTARES candidate neutrino signal during image analysis. Constraints on transient neutrino emission have been set. In September 2015, ANTARES issued a neutrino alert and during the follow-up, a potential transient counterpart was identified by Swift and MASTER. A multi-wavelength follow-up campaign has allowed to identify the nature of this source and has proven its fortuitous association with the neutrino. The return of experience is particularly important for the design of the alert system of KM3NeT, the next generation neutrino telescope in the Mediterranean Sea.
format Preprint
id arxiv_https___arxiv_org_abs_2402_16498
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Results of the follow-up of ANTARES neutrino alerts
Albert, A.
Alves, S.
André, M.
Ardid, M.
Ardid, S.
Aubert, J. -J.
Aublin, J.
Baret, B.
Basa, S.
Becherini, Y.
Belhorma, B.
Bendahman, M.
Benfenati, F.
Bertin, V.
Biagi, S.
Bissinger, M.
Boumaaza, J.
Bouta, M.
Bouwhuis, M. C.
Brânzas, H.
Bruijn, R.
Brunner, J.
Busto, J.
Caiffi, B.
Calvo, D.
Campion, S.
Capone, A.
Caramete, L.
Carenini, F.
Carr, J.
Carretero, V.
Celli, S.
Cerisy, L.
Chabab, M.
Moursli, R. Cherkaoui El
Chiarusi, T.
Circella, M.
Coelho, J. A. B.
Coleiro, A.
Coniglione, R.
Coyle, P.
Creusot, A.
Cruz, A. S. M.
Díaz, A. F.
De Martino, B.
Distefano, C.
Di Palma, I.
Donzaud, C.
Dornic, D.
Drouhin, D.
Eberl, T.
van Eeden, T.
van Eijk, D.
Hedri, S. El
Khayati, N. El
Enzenhöfer, A.
Fermani, P.
Ferrara, G.
Filippini, F.
Fusco, L.
Gagliardini, S.
García, J.
Oliver, C. Gatius
Gay, P.
Geißelbrecht, N.
Glotin, H.
Gozzini, R.
Ruiz, R. Gracia
Graf, K.
Guidi, C.
Haegel, L.
Hallmann, S.
van Haren, H.
Heijboer, A. J.
Hello, Y.
Hennig, L.
Hernández-Rey, J. J.
Hößl, J.
Hofestädt, J.
Huang, F.
Illuminati, G.
James, C. W.
Jisse-Jung, B.
de Jong, M.
de Jong, P.
Kadler, M.
Kalekin, O.
Katz, U.
Kouchner, A.
Kreykenbohm, I.
Kulikovskiy, V.
Lahmann, R.
Lamoureux, M.
Lazo, A.
Lefèvre, D.
Leonora, E.
Levi, G.
Stum, S. Le
Loucatos, S.
Maderer, L.
Manczak, J.
Marcelin, M.
Margiotta, A.
Marinelli, A.
Martínez-Mora, J. A.
Migliozzi, P.
Moussa, A.
Muller, R.
Navas, S.
Nezri, E.
Fearraigh, B. Ó
Oukacha, E.
Pāun, A.
Pāvālas, G. E.
Peña-Martínez, S.
Perrin-Terrin, M.
Piattelli, P.
Popa, V.
Pradier, T.
Randazzo, N.
Real, D.
Riccobene, G.
Romanov, A.
Sánchez-Losa, A.
Saina, A.
Greus, F. Salesa
Samtleben, D. F. E.
Sanguineti, M.
Sapienza, P.
Schnabel, J.
Schumann, J.
Schüssler, F.
Seneca, J.
Spurio, M.
Stolarczyk, Th.
Taiuti, M.
Tayalati, Y.
Tingay, S. J.
Vallage, B.
Vannoye, G.
Van Elewyck, V.
Viola, S.
Vivolo, D.
Wilms, J.
Zavatarelli, S.
Zegarelli, A.
Zornoza, J. D.
Zúñiga, J.
Lipunov, V.
Antipov, G.
Balanutsa, P.
Buckley, D.
Budnev, N.
Chasovnikov, A.
Cheryasov, D.
Francile, C.
Gabovich, A.
Gorbovskoy, E.
Gorbunov, I.
Gress, O.
Kornilov, V.
Kuznetsov, A.
Iyudin, A.
Podesta, R.
Podesta, F.
Lopez, R. Rebolo
Senik, V.
Sierra-Rucart, M.
Svertilov, S.
Tiurina, N.
Vlasenko, D.
Yashin, I.
Zhirkov, K.
Croft, S.
Kaplan, D. L.
Anderson, G. E.
Williams, A.
Dobie, D.
Bannister, K. W.
Hancock, P. J.
Evans, P. A.
Kennea, J. A.
Osborne, J. P.
Cenko, S. B.
Antier, S.
Atteia, J. L.
Boër, M.
Klotz, A.
Chaty, S.
Hodapp, K.
Savchenko, V.
High Energy Astrophysical Phenomena
High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. To look for transient sources associated with neutrino emission, a follow-up program of neutrino alerts has been operating within the ANTARES Collaboration since 2009. This program, named TAToO, has triggered robotic optical telescopes (MASTER, TAROT, ROTSE and the SVOM ground based telescopes) immediately after the detection of any relevant neutrino candidate and scheduled several observations in the weeks following the detection. A subset of ANTARES events with highest probabilities of being of cosmic origin has also been followed by the Swift and the INTEGRAL satellites, the Murchison Widefield Array radio telescope and the H.E.S.S. high-energy gamma-ray telescope. The results of twelve years of observations are reported. No optical counterpart has been significantly associated with an ANTARES candidate neutrino signal during image analysis. Constraints on transient neutrino emission have been set. In September 2015, ANTARES issued a neutrino alert and during the follow-up, a potential transient counterpart was identified by Swift and MASTER. A multi-wavelength follow-up campaign has allowed to identify the nature of this source and has proven its fortuitous association with the neutrino. The return of experience is particularly important for the design of the alert system of KM3NeT, the next generation neutrino telescope in the Mediterranean Sea.
title Results of the follow-up of ANTARES neutrino alerts
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2402.16498

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