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29 results on '"ANTARES NEUTRINO TELESCOPE"'

1. Calibration of the ANTARES neutrino telescope.

Author: Fritsch, Ulf
Subjects: NEUTRINOS, TELESCOPES, MUONS, PHOTOMULTIPLIERS, ELECTRONICS
Published: 2010

2. ANTARES and IceCube Combined Search for Neutrino Point-like and Extended Sources in the Southern Sky

Author: Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, A*Midex Foundation, Junta de Andalucía, Region Ile-de-France, GENERALITAT VALENCIANA, Conseil régional du Grand Est, AGENCIA ESTATAL DE INVESTIGACION, Institut Universitaire de France, Université Sorbonne Paris Cité, Agencia Estatal de Investigación, European Regional Development Fund, Instituto Nazionale di Fisica Nucleare, Agence Nationale de la Recherche, Francia, Conseil Régional Provence-Alpes-Côte d'Azur, Netherlands Organization for Scientific Research, Centre National de la Recherche Scientifique, Francia, Bundesministerium für Bildung und Forschung, Alemania, Council on grants of the President of the Russian Federation, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, Laboratoire d'Excellence OCEVU (Origines, Constituants & ÉVolution de l'Univers), Ministère de l'Enseignement Supérieur, de la Recherche Scientifique et de la Formation des Cadres, Executive Agency for Higher Education, Scientific Research, Development and Innovation Funding, Rumanía, Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Aubert, J-J, Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bourret, S., Martínez Mora, Juan Antonio, Poirè, Chiara, Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, A*Midex Foundation, Junta de Andalucía, Region Ile-de-France, GENERALITAT VALENCIANA, Conseil régional du Grand Est, AGENCIA ESTATAL DE INVESTIGACION, Institut Universitaire de France, Université Sorbonne Paris Cité, Agencia Estatal de Investigación, European Regional Development Fund, Instituto Nazionale di Fisica Nucleare, Agence Nationale de la Recherche, Francia, Conseil Régional Provence-Alpes-Côte d'Azur, Netherlands Organization for Scientific Research, Centre National de la Recherche Scientifique, Francia, Bundesministerium für Bildung und Forschung, Alemania, Council on grants of the President of the Russian Federation, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, Laboratoire d'Excellence OCEVU (Origines, Constituants & ÉVolution de l'Univers), Ministère de l'Enseignement Supérieur, de la Recherche Scientifique et de la Formation des Cadres, Executive Agency for Higher Education, Scientific Research, Development and Innovation Funding, Rumanía, Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Aubert, J-J, Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bourret, S., Martínez Mora, Juan Antonio, and Poirè, Chiara
Abstract: [EN] A search for point-like and extended sources of cosmic neutrinos using data collected by the ANTARES and IceCube neutrino telescopes is presented. The data set consists of all the track-like and shower-like events pointing in the direction of the Southern Sky included in the nine-year ANTARES point-source analysis, combined with the throughgoing track-like events used in the seven-year IceCube point-source search. The advantageous ¿eld of view of ANTARES and the large size of IceCube are exploited to improve the sensitivity in the Southern Sky by a factor of ~2 compared to both individual analyses. In this work, the Southern Sky is scanned for possible excesses of spatial clustering, and the positions of preselected candidate sources are investigated. In addition, special focus is given to the region around the Galactic Center, whereby a dedicated search at the location of SgrA* is performed, and to the location of the supernova remnant RXJ 1713.7-3946. No signi¿cant evidence for cosmic neutrino sources is found, and upper limits on the ¿ux from the various searches are presented.
Published: 2020

3. Combined search for neutrinos from dark matter self-annihilation in the Galactic Center with ANTARES and IceCube

Author: Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, A*Midex Foundation, Junta de Andalucía, Region Ile-de-France, GENERALITAT VALENCIANA, Conseil régional du Grand Est, AGENCIA ESTATAL DE INVESTIGACION, Institut Universitaire de France, Université Sorbonne Paris Cité, Agencia Estatal de Investigación, European Regional Development Fund, Instituto Nazionale di Fisica Nucleare, Conseil Régional Provence-Alpes-Côte d'Azur, Netherlands Organization for Scientific Research, Centre National de la Recherche Scientifique, Francia, Bundesministerium für Bildung und Forschung, Alemania, Council on grants of the President of the Russian Federation, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, Laboratoire d'Excellence OCEVU (Origines, Constituants & ÉVolution de l'Univers), Ministère de l'Enseignement Supérieur, de la Recherche Scientifique et de la Formation des Cadres, Executive Agency for Higher Education, Scientific Research, Development and Innovation Funding, Rumanía, Albert, A., Andre, M., Anghinolfi, M., Ardid Ramírez, Miguel, Aubert, J-J., Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bouta, M., Bouwheis, M. C., Martínez Mora, Juan Antonio, Poirè, Chiara, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, A*Midex Foundation, Junta de Andalucía, Region Ile-de-France, GENERALITAT VALENCIANA, Conseil régional du Grand Est, AGENCIA ESTATAL DE INVESTIGACION, Institut Universitaire de France, Université Sorbonne Paris Cité, Agencia Estatal de Investigación, European Regional Development Fund, Instituto Nazionale di Fisica Nucleare, Conseil Régional Provence-Alpes-Côte d'Azur, Netherlands Organization for Scientific Research, Centre National de la Recherche Scientifique, Francia, Bundesministerium für Bildung und Forschung, Alemania, Council on grants of the President of the Russian Federation, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, Laboratoire d'Excellence OCEVU (Origines, Constituants & ÉVolution de l'Univers), Ministère de l'Enseignement Supérieur, de la Recherche Scientifique et de la Formation des Cadres, Executive Agency for Higher Education, Scientific Research, Development and Innovation Funding, Rumanía, Albert, A., Andre, M., Anghinolfi, M., Ardid Ramírez, Miguel, Aubert, J-J., Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bouta, M., Bouwheis, M. C., Martínez Mora, Juan Antonio, and Poirè, Chiara
Abstract: [EN] We present the results of the first combined dark matter search targeting the Galactic Center using the ANTARES and IceCube neutrino telescopes. For dark matter particles with masses from 50 to 1000 GeV, the sensitivities on the self-annihilation cross section set by ANTARES and IceCube are comparable, making this mass range particularly interesting for a joint analysis. Dark matter self-annihilation through the ¿+¿¿, ¿+¿¿, b¯b, and W+W¿ channels is considered for both the Navarro-Frenk-White and Burkert halo profiles. In the combination of 2101.6 days of ANTARES data and 1007 days of IceCube data, no excess over the expected background is observed. Limits on the thermally averaged dark matter annihilation cross section h¿A¿i are set. These limits present an improvement of up to a factor of 2 in the studied dark matter mass range with respect to the individual limits published by both collaborations. When considering dark matter particles with a mass of 200 GeV annihilating through the ¿þ¿¿ channel, the value obtained for the limit is 7.44 × 10¿24 cm3 s¿1 for the Navarro-Frenk-White halo profile. For the purpose of this joint analysis, the model parameters and the likelihood are unified, providing a benchmark for forthcoming dark matter searches performed by neutrino telescopes.
Published: 2020

4. Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope

Author: Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, Junta de Andalucía, GENERALITAT VALENCIANA, AGENCIA ESTATAL DE INVESTIGACION, Université Sorbonne Paris Cité, Agencia Estatal de Investigación, Agence Nationale de la Recherche, Francia, Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Aubert, J-J, Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., J. Boumaaza, Bouta, M., Martínez Mora, Juan Antonio, Poirè, Chiara, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, Junta de Andalucía, GENERALITAT VALENCIANA, AGENCIA ESTATAL DE INVESTIGACION, Université Sorbonne Paris Cité, Agencia Estatal de Investigación, Agence Nationale de la Recherche, Francia, Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Aubert, J-J, Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., J. Boumaaza, Bouta, M., Martínez Mora, Juan Antonio, and Poirè, Chiara
Abstract: [EN] An of¿ine search for a neutrino counterpart to gravitational-wave (GW) events detected during the second observation run (O2) of Advanced-LIGO and Advanced-Virgo performed with ANTARES data is presented. In addi-tion to the search for long tracks induced by ¿¿ (¿¿ bar) charged current interactions, a search for showering events induced by interactions of neutrinos of any ¿avour is conducted. The severe spatial and time coincidence provided by the gravitational-wave alert allows regions above the detector horizon to be probed, extending the ANTARES sensitivity over the entire sky. The results of this all-neutrino-¿avour and all-sky time dependent analysis are presented. The search for prompt neutrino emission within ±500 s around the time of six GW events yields no neutrino counterparts. Upper lim-its on the neutrino spectral ¿uence and constraints on the isotropic energy radiated via high-energy neutrinos (from a few TeV to a few tens of PeV) are set for each GW event analysed.
Published: 2020

5. Observation of the cosmic ray shadow of the Sun with the ANTARES neutrino telescope

Author: Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, GENERALITAT VALENCIANA, AGENCIA ESTATAL DE INVESTIGACION, Agencia Estatal de Investigación, European Regional Development Fund, Agence Nationale de la Recherche, Francia, Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Aubert, J-J, Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bouta, M., Martínez Mora, Juan Antonio, Poirè, Chiara, Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, GENERALITAT VALENCIANA, AGENCIA ESTATAL DE INVESTIGACION, Agencia Estatal de Investigación, European Regional Development Fund, Agence Nationale de la Recherche, Francia, Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Aubert, J-J, Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bouta, M., Martínez Mora, Juan Antonio, and Poirè, Chiara
Abstract: [EN] The ANTARES detector is an undersea neutrino telescope in the Mediterranean Sea. The search for pointlike neutrino sources is one of the main goals of the ANTARES telescope, requiring a reliable method to evaluate the detector angular resolution and pointing accuracy. This work describes the study of the Sun ¿shadow¿ effect with the ANTARES detector. The shadow is the deficit in the atmospheric muon flux in the direction of the Sun caused by the absorption of the primary cosmic rays. This analysis is based on the data collected between 2008 and 2017 by the ANTARES telescope. The observed statistical significance of the Sun shadow detection is 3.7¿, with an estimated angular resolution of 0.59° +- 0.10°for downward-going muons. The pointing accuracy is found to be consistent with the expectations and no evidence of systematic pointing shifts is observed.
Published: 2020

6. Acoustic and optical variations during rapid downward motion episodes in the deep north-western Mediterranean Sea

Author: van Haren, H., Taupier-Letage, I., Aguilar, J.A., 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., and Bouwhuis, M.C.
Subjects: *OCEANOGRAPHY, *WATER currents, *ACOUSTIC reflection, *TELESCOPES, *BIOLUMINESCENCE
Abstract: Abstract: An Acoustic Doppler Current Profiler (ADCP) was moored at the deep-sea site of the ANTARES neutrino telescope near Toulon, France, thus providing a unique opportunity to compare high-resolution acoustic and optical observations between 70 and 170m above the sea bed at 2475m. The ADCP measured downward vertical currents of magnitudes up to 0.03ms−1 in late winter and early spring 2006. In the same period, observations were made of enhanced levels of acoustic reflection, interpreted as suspended particles including zooplankton, by a factor of about 10 and of horizontal currents reaching 0.35ms−1. These observations coincided with high light levels detected by the telescope, interpreted as increased bioluminescence. During winter 2006 deep dense-water formation occurred in the Ligurian subbasin, thus providing a possible explanation for these observations. However, the 10–20 days quasi-periodic episodes of high levels of acoustic reflection, light and large vertical currents continuing into the summer are not direct evidence of this process. It is hypothesized that the main process allowing for suspended material to be moved vertically later in the year is local advection, linked with topographic boundary current instabilities along the rim of the ‘Northern Current’. [Copyright &y& Elsevier]
Published: 2011
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7. Luminous bacteria in the deep-sea waters near the ANTARES underwater neutrino telescope (Mediterranean Sea).

Author: Al Ali, Badr, Garel, Marc, Cuny, Philippe, Miquel, Juan-Carlos, Toubal, Tarik, Robert, Anne, and Tamburini, Christian
Subjects: *LUMINOUS bacteria, *NEUTRINOS, *PROKARYOTES, *BIOLUMINESCENCE, *HYDROSTATIC pressure
Abstract: Marine luminous deep-sea bacteria may represent a potential source of signal perturbation for the ANTARES neutrino telescope installed between 2000 and 2475 m depth in the Mediterranean Sea. Using the CARD-FISH method, we have estimated the relative abundances of total prokaryotes of Bacteria, γ -proteobacteria and Vibrinoceae (domain, class and family affiliation of marine luminous bacteria, respectively) through the water column close to the ANTARES site. At 2200 m depth, Vibrionaceae appeared to be far from negligible, representing 40% of γ -proteobacteria, 25% of Bacteria and 9% of the total DAPI-stained cells, while Bacteria and Archaea represented 35% each. Furthermore, during a high luminous background period detected by the neutrino telescope, we isolated, from a 2200 m depth sample, a piezophilic luminous bacterium, phylogenetically determined as Photobacterium phosphoreum strain ANT-2200. We have used this strain to investigate the effect of hydrostatic pressure on bioluminescence by developing a new high-pressure apparatus. First assays showed that the bioluminescence intensity of Photobacterium phosphoreum strain ANT-2200 was 5 times higher at 22 MPa than at 0.1 MPa (atmospheric pressure). [ABSTRACT FROM AUTHOR]
Published: 2010
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8. ANTARES: An Underwater Network of Sensors for Neutrino Astronomy and Deep-Sea Research.

Author: Ardid, Miguel
Subjects: NEUTRINOS, WIRELESS sensor networks, COSMIC ray muons, PHOTOMULTIPLIERS
Abstract: The detection of very high energy neutrinos is a technological challenge which requires a complex network of sensors performing as a huge detector, and a large shield of matter on top of it against the background of cosmic ray muons. ANTARES is at present the largest neutrino telescope in the northern hemisphere and the largest underwater neutrino telescope in the world. It has been installed at a depth of about 2500 m in the Mediterranean Sea, near the Southern French coast. A three-dimensional array of photomultipliers is used to detect the Cherenkov light emitted by neutrino-induced muons. The array consists of 12 lines, each covering a vertical length of about 450 m and equipped with 75 photomultipliers arranged in triplets, plus an additional instrumentation line. The readout electronics is connected to an on-shore laboratory through a 42 km long electro-optical cable. A promising science program is running nowadays by a large European collaboration. The detector design, which constitutes a complex network of underwater sensors, its performance, and the first technical results are presented. [ABSTRACT FROM AUTHOR]
Published: 2009

9. ANTARES and IceCube Combined Search for Neutrino Point-like and Extended Sources in the Southern Sky

Author: Antares, Collaboration, Albert, A., André, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J. -J., Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bourret, S., Bouta, M., Bouwhuis, M. C., Brânzaş, H., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Chabab, M., Chau, T. N., Cherkaoui El Moursli, R., Chiarusi, T., Circella, M., Coleiro, A., Colomer, M., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., Díaz, A. F., de Wasseige, G., Deschamps, A., Distefano, C., Di Palma, I., Domi, A., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., El Bojaddaini, I., El Khayati, N., Elsässer, D., Enzenhöfer, A., Ettahiri, A., Fassi, F., Fermani, P., Ferrara, G., Filippini, F., Fusco, L., Gay, P., Glotin, H., Gozzini, R., Gracia Ruiz, R., Graf, K., Guidi, C., Hallmann, S., van Haren, H., Heijboer, A. J., Hello, Y., Hernández-Rey, J. J., Hößl, J., Hofestädt, J., Illuminati, G., James, C. W., de Jong, M., de Jong, P., Jongen, M., Kadler, M., Kalekin, O., Katz, U., Khan-Chowdhury, N. R., Kouchner, A., Kreter, M., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Le Breton, R., Lefèvre, D., Leonora, E., Levi, G., Lincetto, M., Lopez-Coto, D., Loucatos, S., Maggi, G., Manczak, J., Marcelin, M., Margiotta, A., Marinelli, A., Martínez-Mora, J. A., Mele, R., Melis, K., Migliozzi, P., Moser, M., Moussa, A., Muller, R., Nauta, L., Navas, S., Nezri, E., Nielsen, C., Nuñez-Castiñeyra, A., O'Fearraigh, B., Organokov, M., Păvălaş, G. E., Pellegrino, C., Perrin-Terrin, M., Piattelli, P., Poirè, C., Popa, V., Pradier, T., Quinn, L., Randazzo, N., Riccobene, G., Sánchez-Losa, A., Salah-Eddine, A., Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schüssler, F., Spurio, M., Stolarczyk, Th., Strandberg, B., Taiuti, M., Tayalati, Y., Thakore, T., Tingay, S. J., Trovato, A., Vallage, B., Van Elewyck, V., Versari, F., Viola, S., Vivolo, D., Wilms, J., Zaborov, D., Zegarelli, A., Zornoza, J. D., Zúñiga, J., Icecube, Collaboration, Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Alispach, C., Andeen, K., Anderson, T., Ansseau, I., Argüelles, C., Auffenberg, J., Axani, S., Backes, P., Bagherpour, H., Bai, X., A. Balagopal V., Barbano, A., Barwick, S. W., Bastian, B., Baum, V., Baur, S., Bay, R., Beatty, J. J., Becker, K. -H., Becker Tjus, J., Benzvi, S., Berley, D., Bernardini, E., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bohm, C., Böser, S., Botner, O., Böttcher, J., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Bron, S., Brostean-Kaiser, J., Burgman, A., Buscher, J., Busse, R. S., Carver, T., Chen, C., Cheung, E., Chirkin, D., Choi, S., Clark, K., Classen, L., Coleman, A., Collin, G. H., Conrad, J. M., Coppin, P., Correa, P., Cowen, D. F., Cross, R., Dave, P., De Clercq, C., Delaunay, J. J., Dembinski, H., Deoskar, K., De Ridder, S., Desiati, P., de Vries, K. D., de With, M., Deyoung, T., Diaz, A., Díaz-Vélez, J. C., Dujmovic, H., Dunkman, M., Dvorak, E., Eberhardt, B., Ehrhardt, T., Eller, P., Engel, R., Evenson, P. A., Fahey, S., Fazely, A. R., Felde, J., Filimonov, K., Finley, C., Fox, D., Franckowiak, A., Friedman, E., Fritz, A., Gaisser, T. K., Gallagher, J., Ganster, E., Garrappa, S., Gerhardt, L., Ghorbani, K., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G., Grant, D., Grégoire, T., Griffith, Z., Griswold, S., Günder, M., Gündüz, M., Haack, C., Hallgren, A., Halliday, R., Halve, L., Halzen, F., Hanson, K., Haungs, A., Hebecker, D., Heereman, D., Heix, P., Helbing, K., Hellauer, R., Henningsen, F., Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Hoinka, T., Hokanson-Fasig, B., Hoshina, K., Huang, F., Huber, M., Huber, T., Hultqvist, K., Hünnefeld, M., Hussain, R., In, S., Iovine, N., Ishihara, A., Jansson, M., Japaridze, G. S., Jeong, M., Jero, K., Jones, B. J. P., Jonske, F., Joppe, R., Kang, D., Kang, W., Kappes, A., Kappesser, D., Karg, T., Karl, M., Karle, A., Kauer, M., Kelley, J. L., Kheirandish, A., Kim, J., Kintscher, T., Kiryluk, J., Kittler, T., Klein, S. R., Koirala, R., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krings, K., Krückl, G., Kulacz, N., Kurahashi, N., Kyriacou, A., Lanfranchi, J. L., Larson, M. J., Lauber, F., Lazar, J. P., Leonard, K., Leszczyńska, A., Leuermann, M., Liu, Q. R., Lohfink, E., Lozano Mariscal, C. J., Lu, L., Lucarelli, F., Lünemann, J., Luszczak, W., Lyu, Y., W. Y., Ma, Madsen, J., Mahn, K. B. M., Makino, Y., Mallik, P., Mallot, K., Mancina, S., Mariş, I. C., Maruyama, R., Mase, K., Maunu, R., Mcnally, F., Meagher, K., Medici, M., Medina, A., Meier, M., Meighen-Berger, S., Merino, G., Meures, T., Micallef, J., Mockler, D., Momenté, G., Montaruli, T., Moore, R. W., Morse, R., Moulai, M., Muth, P., Nagai, R., Naumann, U., Neer, G., Niederhausen, H., Nisa, M. U., Nowicki, S. C., Nygren, D. R., Obertacke Pollmann, A., Oehler, M., Olivas, A., O'Murchadha, A., O'Sullivan, E., Palczewski, T., Pandya, H., Pankova, D. V., Park, N., Peiffer, P., Pérez de los Heros, C., Philippen, S., Pieloth, D., Pieper, S., Pinat, E., Pizzuto, A., Plum, M., Porcelli, A., Price, P. B., Przybylski, G. T., Raab, C., Raissi, A., Rameez, M., Rauch, L., Rawlins, K., Rea, I. C., Reimann, R., Relethford, B., Renschler, M., Renzi, G., Resconi, E., Rhode, W., Richman, M., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk, D., Safa, I., Sanchez Herrera, S. E., Sandrock, A., Sandroos, J., Santander, M., Sarkar, S., Satalecka, K., Schaufel, M., Schieler, H., Schlunder, P., Schmidt, T., Schneider, A., Schneider, J., Schröder, F. G., Schumacher, L., Sclafani, S., Seckel, D., Seunarine, S., Shefali, S., Silva, M., Snihur, R., Soedingrekso, J., Soldin, D., Song, M., Spiczak, G. M., Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stein, R., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Strotjohann, N. L., Stürwald, T., Stuttard, T., Sullivan, G. W., Taboada, I., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Tilav, S., Tollefson, K., Tomankova, L., Tönnis, C., Toscano, S., Tosi, D., Trettin, A., Tselengidou, M., Tung, C. F., Turcati, A., Turcotte, R., Turley, C. F., Ty, B., Unger, E., Unland Elorrieta, M. A., Usner, M., Vandenbroucke, J., Van Driessche, W., van Eijk, D., van Eijndhoven, N., van Santen, J., Verpoest, S., Vraeghe, M., Walck, C., Wallace, A., Wallraff, M., Wandkowsky, N., Watson, T. B., Weaver, C., Weindl, A., Weiss, M. J., Weldert, J., Wendt, C., Werthebach, J., Whelan, B. J., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Wille, L., Williams, D. R., Wills, L., Wolf, M., Wood, J., Wood, T. R., Woschnagg, K., Wrede, G., D. L., Xu, X. W., Xu, Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., Yuan, T., Zöcklein, M., KM3NeT (IHEF, IoP, FNWI), ATLAS (IHEF, IoP, FNWI), IoP (FNWI), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Centre de Physique des Particules de Marseille (CPPM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 7329), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Informatique et Systèmes (LIS), Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Institut méditerranéen d'océanologie (MIO), Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN)-Aix Marseille Université (AMU)-Institut de Recherche pour le Développement (IRD), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, ANTARES, IceCube, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), Albert, A., André, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J.-J., Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bourret, S., Bouta, M., Bouwhuis, M. C., Brânzaş, H., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Chabab, M., Chau, T. N., El Moursli, R. Cherkaoui, Chiarusi, T., Circella, M., Coleiro, A., Colomer, M., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., Díaz, A. F., Wasseige, G. de, Deschamps, A., Distefano, C., Palma, I. Di, Domi, A., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., Bojaddaini, I. El, Khayati, N. El, Elsässer, D., Enzenhöfer, A., Ettahiri, A., Fassi, F., Fermani, P., Ferrara, G., Filippini, F., Fusco, L., Gay, P., Glotin, H., Gozzini, R., Ruiz, R. Gracia, Graf, K., Guidi, C., Hallmann, S., van Haren, H., Heijboer, A. J., Hello, Y., Hernández-Rey, J. J., Hößl, J., Hofestädt, J., Illuminati, G., James, C. W., Jong, M. de, Jong, P. de, Jongen, M., Kadler, M., Kalekin, O., Katz, U., Khan-Chowdhury, N. R., Kouchner, A., Kreter, M., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Breton, R. Le, Lefèvre, D., Leonora, E., Levi, G., Lincetto, M., Lopez-Coto, D., Loucatos, S., Maggi, G., Manczak, J., Marcelin, M., Margiotta, A., Marinelli, A., Martínez-Mora, J. A., Mele, R., Melis, K., Migliozzi, P., Moser, M., Moussa, A., Muller, R., Nauta, L., Navas, S., Nezri, E., Nielsen, C., Nuñez-Castiñeyra, A., O’Fearraigh, B., Organokov, M., Păvălaş, G. E., Pellegrino, C., Perrin-Terrin, M., Piattelli, P., Poirè, C., Popa, V., Pradier, T., Quinn, L., Randazzo, N., Riccobene, G., Sánchez-Losa, A., Salah-Eddine, A., Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schüssler, F., Spurio, M., Stolarczyk, Th., Strandberg, B., Taiuti, M., Tayalati, Y., Thakore, T., Tingay, S. J., Trovato, A., Vallage, B., Van Elewyck, V., Versari, F., Viola, S., Vivolo, D., Wilms, J., Zaborov, D., Zegarelli, A., Zornoza, J. D., Zúñiga, J., Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Alispach, C., Andeen, K., Anderson, T., Ansseau, I., Argüelles, C., Auffenberg, J., Axani, S., Backes, P., Bagherpour, H., Bai, X., V., A. Balagopal, Barbano, A., Barwick, S. W., Bastian, B., Baum, V., Baur, S., Bay, R., Beatty, J. J., Becker, K.-H., Tjus, J. Becker, BenZvi, S., Berley, D., Bernardini, E., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bohm, C., Böser, S., Botner, O., Böttcher, J., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Bron, S., Brostean-Kaiser, J., Burgman, A., Buscher, J., Busse, R. S., Carver, T., Chen, C., Cheung, E., Chirkin, D., Choi, S., Clark, K., Classen, L., Coleman, A., Collin, G. H., Conrad, J. M., Coppin, P., Correa, P., Cowen, D. F., Cross, R., Dave, P., Clercq, C. De, DeLaunay, J. J., Dembinski, H., Deoskar, K., Ridder, S. De, Desiati, P., Vries, K. D. de, With, M. de, DeYoung, T., Diaz, A., Díaz-Vélez, J. C., Dujmovic, H., Dunkman, M., Dvorak, E., Eberhardt, B., Ehrhardt, T., Eller, P., Engel, R., Evenson, P. A., Fahey, S., Fazely, A. R., Felde, J., Filimonov, K., Finley, C., Fox, D., Franckowiak, A., Friedman, E., Fritz, A., Gaisser, T. K., Gallagher, J., Ganster, E., Garrappa, S., Gerhardt, L., Ghorbani, K., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G., Grant, D., Grégoire, T., Griffith, Z., Griswold, S., Günder, M., Gündüz, M., Haack, C., Hallgren, A., Halliday, R., Halve, L., Halzen, F., Hanson, K., Haungs, A., Hebecker, D., Heereman, D., Heix, P., Helbing, K., Hellauer, R., Henningsen, F., Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Hoinka, T., Hokanson-Fasig, B., Hoshina, K., Huang, F., Huber, M., Huber, T., Hultqvist, K., Hünnefeld, M., Hussain, R., In, S., Iovine, N., Ishihara, A., Jansson, M., Japaridze, G. S., Jeong, M., Jero, K., Jones, B. J. P., Jonske, F., Joppe, R., Kang, D., Kang, W., Kappes, A., Kappesser, D., Karg, T., Karl, M., Karle, A., Kauer, M., Kelley, J. L., Kheirandish, A., Kim, J., Kintscher, T., Kiryluk, J., Kittler, T., Klein, S. R., Koirala, R., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krings, K., Krückl, G., Kulacz, N., Kurahashi, N., Kyriacou, A., Lanfranchi, J. L., Larson, M. J., Lauber, F., Lazar, J. P., Leonard, K., Leszczyńska, A., Leuermann, M., Liu, Q. R., Lohfink, E., Lozano Mariscal, C. J., Lu, L., Lucarelli, F., Lünemann, J., Luszczak, W., Lyu, Y., Ma, W. Y., Madsen, J., Mahn, K. B. M., Makino, Y., Mallik, P., Mallot, K., Mancina, S., Mariş, I. C., Maruyama, R., Mase, K., Maunu, R., McNally, F., Meagher, K., Medici, M., Medina, A., Meier, M., Meighen-Berger, S., Merino, G., Meures, T., Micallef, J., Mockler, D., Momenté, G., Montaruli, T., Moore, R. W., Morse, R., Moulai, M., Muth, P., Nagai, R., Naumann, U., Neer, G., Niederhausen, H., Nisa, M. U., Nowicki, S. C., Nygren, D. R., Obertacke Pollmann, A., Oehler, M., Olivas, A., O’Murchadha, A., O’Sullivan, E., Palczewski, T., Pandya, H., Pankova, D. V., Park, N., Peiffer, P., de los Heros, C. Pérez, Philippen, S., Pieloth, D., Pieper, S., Pinat, E., Pizzuto, A., Plum, M., Porcelli, A., Price, P. B., Przybylski, G. T., Raab, C., Raissi, A., Rameez, M., Rauch, L., Rawlins, K., Rea, I. C., Reimann, R., Relethford, B., Renschler, M., Renzi, G., Resconi, E., Rhode, W., Richman, M., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk, D., Safa, I., Sanchez Herrera, S. E., Sandrock, A., Sandroos, J., Santander, M., Sarkar, S., Satalecka, K., Schaufel, M., Schieler, H., Schlunder, P., Schmidt, T., Schneider, A., Schneider, J., Schröder, F. G., Schumacher, L., Sclafani, S., Seckel, D., Seunarine, S., Shefali, S., Silva, M., Snihur, R., Soedingrekso, J., Soldin, D., Song, M., Spiczak, G. M., Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stein, R., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Strotjohann, N. L., Stürwald, T., Stuttard, T., Sullivan, G. W., Taboada, I., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Tilav, S., Tollefson, K., Tomankova, L., Tönnis, C., Toscano, S., Tosi, D., Trettin, A., Tselengidou, M., Tung, C. F., Turcati, A., Turcotte, R., Turley, C. F., Ty, B., Unger, E., Elorrieta, M. A. Unland, Usner, M., Vandenbroucke, J., Van Driessche, W., van Eijk, D., van Eijndhoven, N., van Santen, J., Verpoest, S., Vraeghe, M., Walck, C., Wallace, A., Wallraff, M., Wandkowsky, N., Watson, T. B., Weaver, C., Weindl, A., Weiss, M. J., Weldert, J., Wendt, C., Werthebach, J., Whelan, B. J., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Wille, L., Williams, D. R., Wills, L., Wolf, M., Wood, J., Wood, T. R., Woschnagg, K., Wrede, G., Xu, D. L., Xu, X. W., Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., Yuan, T., Zöcklein, M., Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS)-Aix Marseille Université (AMU), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN), Albert, A, Andre, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, J-J, Aublin, J, Baret, B, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bissinger, M, Boumaaza, J, Bourret, S, Bouta, M, Bouwhuis, Mc, Branzas, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, Chau, Tn, El Moursli, Rc, Chiarusi, T, Circella, M, Coleiro, A, Colomer, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Diaz, Af, de Wasseige, G, Deschamps, A, Distefano, C, Palma, Id, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, El Bojaddaini, I, Khayati, Ne, Elsasser, D, Enzenhofer, A, Ettahiri, A, Fassi, F, Fermani, P, Ferrara, G, Filippini, F, Fusco, L, Gay, P, Glotin, H, Gozzini, R, Ruiz, Rg, Graf, K, Guidi, C, Hallmann, S, van Haren, H, Heijboer, Aj, Hello, Y, Hernandez-Rey, Jj, Hossl, J, Hofestadt, J, Illuminati, G, James, Cw, de Jong, M, de Jong, P, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, Nr, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Le Breton, R, Lefevre, D, Leonora, E, Levi, G, Lincetto, M, Lopez-Coto, D, Loucatos, S, Maggi, G, Manczak, J, Marcelin, M, Margiotta, A, Marinelli, A, Martinez-Mora, Ja, Mele, R, Melis, K, Migliozzi, P, Moser, M, Moussa, A, Muller, R, Nauta, L, Navas, S, Nezri, E, Nielsen, C, Nunez-Castineyra, A, O'Fearraigh, B, Organokov, M, Pavalas, Ge, Pellegrino, C, Perrin-Terrin, M, Piattelli, P, Poire, C, Popa, V, Pradier, T, Quinn, L, Randazzo, N, Riccobene, G, Sanchez-Losa, A, Salah-Eddine, A, Samtleben, Dfe, Sanguineti, M, Sapienza, P, Schussler, F, Spurio, M, Stolarczyk, T, Strandberg, B, Taiuti, M, Tayalati, Y, Thakore, T, Tingay, Sj, Trovato, A, Vallage, B, Van Elewyck, V, Versari, F, Viola, S, Vivolo, D, Wilms, J, Zaborov, D, Zegarelli, A, Zornoza, Jd, Zuniga, J, Aartsen, Mg, Ackermann, M, Adams, J, Aguilar, Ja, Ahlers, M, Ahrens, M, Alispach, C, Andeen, K, Anderson, T, Ansseau, I, Arguelles, C, Auffenberg, J, Axani, S, Backes, P, Bagherpour, H, Bai, X, Balagopal, Av, Barbano, A, Barwick, Sw, Bastian, B, Baum, V, Baur, S, Bay, R, Beatty, Jj, Becker, K-H, Tjus, Jb, Benzvi, S, Berley, D, Bernardini, E, Besson, Dz, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Boser, S, Botner, O, Bottcher, J, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Bron, S, Brostean-Kaiser, J, Burgman, A, Buscher, J, Busse, R, Carver, T, Chen, C, Cheung, E, Chirkin, D, Choi, S, Clark, K, Classen, L, Coleman, A, Collin, Gh, Conrad, Jm, Coppin, P, Correa, P, Cowen, Df, Cross, R, Dave, P, De Clercq, C, Delaunay, Jj, Dembinski, H, Deoskar, K, Ridder, Sd, Desiati, P, de Vries, Kd, With, M, Deyoung, T, Diaz, A, Diaz-Velez, Jc, Dujmovic, H, Dunkman, M, Dvorak, E, Eberhardt, B, Ehrhardt, T, Eller, P, Engel, R, Evenson, Pa, Fahey, S, Fazely, Ar, Felde, J, Filimonov, K, Finley, C, Fox, D, Franckowiak, A, Friedman, E, Fritz, A, Gaisser, Tk, Gallagher, J, Ganster, E, Garrappa, S, Gerhardt, L, Ghorbani, K, Glauch, T, Glusenkamp, T, Goldschmidt, A, Gonzalez, Jg, Grant, D, Gregoire, T, Griffith, Z, Griswold, S, Gunder, M, Gunduz, M, Haack, C, Hallgren, A, Halliday, R, Halve, L, Halzen, F, Hanson, K, Haungs, A, Hebecker, D, Heereman, D, Heix, P, Helbing, K, Hellauer, R, Henningsen, F, Hickford, S, Hignight, J, Hill, Gc, Hoffman, Kd, Hoffmann, R, Hoinka, T, Hokanson-Fasig, B, Hoshina, K, Huang, F, Huber, M, Huber, T, Hultqvist, K, Hunnefeld, M, Hussain, R, In, S, Iovine, N, Ishihara, A, Jansson, M, Japaridze, G, Jeong, M, Jero, K, Jones, Bjp, Jonske, F, Joppe, R, Kang, D, Kang, W, Kappes, A, Kappesser, D, Karg, T, Karl, M, Karle, A, Kauer, M, Kelley, Jl, Kheirandish, A, Kim, J, Kintscher, T, Kiryluk, J, Kittler, T, Klein, Sr, Koirala, R, Kolanoski, H, Kopke, L, Kopper, C, Kopper, S, Koskinen, Dj, Kowalski, M, Krings, K, Kruckl, G, Kulacz, N, Kurahashi, N, Kyriacou, A, Lanfranchi, Jl, Larson, Mj, Lauber, F, Lazar, Jp, Leonard, K, Leszczynska, A, Leuermann, M, Liu, Qr, Lohfink, E, Mariscal, Cjl, Lu, L, Lucarelli, F, Lunemann, J, Luszczak, W, Lyu, Y, Ma, Wy, Madsen, J, Mahn, Kbm, Makino, Y, Mallik, P, Mallot, K, Mancina, S, Maris, Ic, Maruyama, R, Mase, K, Maunu, R, Mcnally, F, Meagher, K, Medici, M, Medina, A, Meier, M, Meighen-Berger, S, Merino, G, Meures, T, Micallef, J, Mockler, D, Momente, G, Montaruli, T, Moore, Rw, Morse, R, Moulai, M, Muth, P, Nagai, R, Naumann, U, Neer, G, Niederhausen, H, Nisa, Mu, Nowicki, Sc, Nygren, Dr, Pollmann, Ao, Oehler, M, Olivas, A, O'Murchadha, A, O'Sullivan, E, Palczewski, T, Pandya, H, Pankova, Dv, Park, N, Peiffer, P, de los Heros, Cp, Philippen, S, Pieloth, D, Pieper, S, Pinat, E, Pizzuto, A, Plum, M, Porcelli, A, Price, Pb, Przybylski, Gt, Raab, C, Raissi, A, Rameez, M, Rauch, L, Rawlins, K, Rea, Ic, Reimann, R, Relethford, B, Renschler, M, Renzi, G, Resconi, E, Rhode, W, Richman, M, Robertson, S, Rongen, M, Rott, C, Ruhe, T, Ryckbosch, D, Rysewyk, D, Safa, I, Herrera, Se, Sandrock, A, Sandroos, J, Santander, M, Sarkar, S, Satalecka, K, Schaufel, M, Schieler, H, Schlunder, P, Schmidt, T, Schneider, A, Schneider, J, Schroder, Fg, Schumacher, L, Sclafani, S, Seckel, D, Seunarine, S, Shefali, S, Silva, M, Snihur, R, Soedingrekso, J, Soldin, D, Song, M, Spiczak, Gm, Spiering, C, Stachurska, J, Stamatikos, M, Stanev, T, Stein, R, Stettner, J, Steuer, A, Stezelberger, T, Stokstad, Rg, Stosssl, A, Strotjohann, Nl, Sturwald, T, Stuttard, T, Sullivan, Gw, Taboada, I, Tenholt, F, Ter-Antonyan, S, Terliuk, A, Tilav, S, Tollefson, K, Tomankova, L, Tonnis, C, Toscano, S, Tosi, D, Trettin, A, Tselengidou, M, Tung, Cf, Turcati, A, Turcotte, R, Turley, Cf, Ty, B, Unger, E, Elorrieta, Mau, Usner, M, Vandenbroucke, J, Van Driessche, W, van Eijk, D, van Eijndhoven, N, van Santen, J, Verpoest, S, Vraeghe, M, Walck, C, Wallace, A, Wallraff, M, Wandkowsky, N, Watson, Tb, Weaver, C, Weindl, A, Weiss, Mj, Weldert, J, Wendt, C, Werthebach, J, Whelan, Bj, Whitehorn, N, Wiebe, K, Wiebusch, Ch, Wille, L, Williams, Dr, Wills, L, Wolf, M, Wood, J, Wood, Tr, Woschnagg, K, Wrede, G, Xu, Dl, Xu, Xw, Xu, Y, Yanez, Jp, Yodh, G, Yoshida, S, Yuan, T, Zocklein, M, Centre Tecnològic de Vilanova i la Geltrú, Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques, Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Institut national des sciences de l'Univers (INSU - CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Physics, Faculty of Sciences and Bioengineering Sciences, Vriendenkring VUB, Elementary Particle Physics, Andre, M., Aubert, J. -J., Branzas, H., El Moursli, R. C., Diaz, A. F., Wasseige, G. D., Palma, I. D., Bojaddaini, I. E., Khayati, N. E., Elsasser, D., Enzenhofer, A., Ruiz, R. G., Van Haren, H., Hernandez-Rey, J. J., Hossl, J., Hofestadt, J., Jong, M. D., Jong, P. D., Breton, R. L., Lefevre, D., Martinez-Mora, J. A., Nuez-Castieyra, A., O'Fearraigh, B., Pavalas, G. E., Poire, C., Sanchez-Losa, A., Schussler, F., Stolarczyk, T., Zuiga, J., Arguelles, C., V. A., B., Becker, K. -H., Tjus, J. B., Benzvi, S., Boser, S., Bottcher, J., Clercq, C. D., Delaunay, J. J., Ridder, S. D., Vries, K. D. D., With, M. D., Deyoung, T., Diaz-Velez, J. C., Glusenkamp, T., Gregoire, T., Gunder, M., Gunduz, M., Hunnefeld, M., Kopke, L., Kruckl, G., Leszczynska, A., Lunemann, J., Maris, I. C., Mcnally, F., Momente, G., O'Murchadha, A., O'Sullivan, E., De Los Heros, C. P., Schroder, F. G., Stossl, A., Sturwald, T., Tonnis, C., Elorrieta, M. A. U., Van Eijk, D., Van Eijndhoven, N., Van Santen, J., and Zocklein, M.
Subjects: Astrofísica, 010504 meteorology & atmospheric sciences, Science and engineering, 01 natural sciences, Point like and extended sources, IceCube, particle source [neutrino], High-throughput computing, detector [neutrino], 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, Physics, Astrophysics::Instrumentation and Methods for Astrophysics, neutrinos, astrophysical neutrinos, neutrino telescopes, GAMMA RAY EMISSION, COSMIC RAYS, COSMIC-RAYS, neutrino: detector, Neutrino astronomy, Science policy, Engineering research, Astrophysics - High Energy Astrophysical Phenomena, Antares neutrino telescope, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Library science, 0103 physical sciences, supernova, Neutrins, Neutrinos, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Astroparticle physics, IceCube neutrino telescope, ANTARES, Telescopis, Astronomy and Astrophysics, DESY, neutrino: particle source, sensitivity, Neutrino astrophysics, Computing center, flux, Physics and Astronomy, 13. Climate action, Space and Planetary Science, Research council, FISICA APLICADA, Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], ddc:520, galaxy, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], GAMMA-RAY EMISSION, Telescopes
Abstract: [EN] A search for point-like and extended sources of cosmic neutrinos using data collected by the ANTARES and IceCube neutrino telescopes is presented. The data set consists of all the track-like and shower-like events pointing in the direction of the Southern Sky included in the nine-year ANTARES point-source analysis, combined with the throughgoing track-like events used in the seven-year IceCube point-source search. The advantageous ¿eld of view of ANTARES and the large size of IceCube are exploited to improve the sensitivity in the Southern Sky by a factor of ~2 compared to both individual analyses. In this work, the Southern Sky is scanned for possible excesses of spatial clustering, and the positions of preselected candidate sources are investigated. In addition, special focus is given to the region around the Galactic Center, whereby a dedicated search at the location of SgrA* is performed, and to the location of the supernova remnant RXJ 1713.7-3946. No signi¿cant evidence for cosmic neutrino sources is found, and upper limits on the ¿ux from the various searches are presented., The authors of the IceCube Collaboration acknowledge the support from the following agencies and institutions: USA-U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, Wisconsin Alumni Research Foundation, Center for High Throughput Computing (CHTC) at the University of Wisconsin-Madison, Open Science Grid (OSG), Extreme Science and Engineering Discovery Environment (XSEDE), U.S. Department of Energy-National Energy Research Scientific Computing Center, Particle astrophysics research computing center at the University of Maryland, Institute for Cyber-Enabled Research at Michigan State University, and Astroparticle physics computational facility at Marquette University; Belgium-Funds for Scientific Research (FRS-FNRS and FWO), FWO Odysseus and Big Science programmes, and Belgian Federal Science Policy Office (Belspo); Germany-Bundesministerium fur Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Initiative and Networking Fund of the Helmholtz Association, Deutsches Elektronen Synchrotron (DESY), and High Performance Computing Cluster of the RWTH Aachen; Sweden-Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation; Australia - Australian Research Council; Canada-Natural Sciences and Engineering Research Council of Canada, Calcul Quebec, Compute Ontario, Canada Foundation for Innovation, WestGrid, and Compute Canada; Denmark-Villum Fonden, Danish National Research Foundation (DNRF), Carlsberg Foundation; New Zealand-Marsden Fund; Japan-Japan Society for Promotion of Science (JSPS) and Institute for Global Prominent Research (IGPR) of Chiba University; Korea-National Research Foundation of Korea (NRF); Switzerland-Swiss National Science Foundation (SNSF); United Kingdom-Department of Physics, University of Oxford.
Published: 2020
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10. Observation of the cosmic ray shadow of the Sun with the ANTARES neutrino telescope

Author: ANTARES Collaboration, Albert, A., André, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J. -J., Aublin, J., Baret, B., Basa, S., Belhorma1, B., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bouta, M., Bouwhuis, M. C., Brânzaş, H., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Chabab, M., Chau, T. N., Moursli, R. Cherkaoui El, Chiarusi, T., Circella, M., Coleiro, A., Colomer-Molla, M., Coniglione, R., Coyle, P., Creusot, A., Díaz, A. F., de Wasseige, G., Deschamps, A., Distefano, C., Di Palma, I., Domi, A., Donzaud, C., Dornic, D., Drouhin, D., Eber, T., Khayati, N. El, Enzenhöfer, A., Ettahiri, A., Fermani, P., Ferrara, G., Filippini, F., Fusco, L., Gay, P., Glotin, H., Gozzini, R., Graf, K., Guidi, C., Hallmann, S., van Haren, H., Heijboer, A. J., Hello, Y., Hernández-Rey, J. J., Hößl, J., Hofestädt, J., Huang, F., Illuminati, G., James, C. W., de Jong, M., de Jong, P., Jongen, M., Kadler, M., Kalekin, O., Katz, U., Khan-Chowdhury, N. R., Kouchner, A., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Breton, R. Le, Lefèvre, D., Leonora, E., Levi, G., Lincetto, M., Lopez-Coto, D., Loucatos, S., Maggi, G., Manczak, J., Marcelin, M., Margiotta, A., Marinelli, A., Martínez-Mora, J. A., Mele, R., Melis, K., Migliozzi, P., Moser, M., Moussa, A., Muller, R., Nauta, L., Navas, S., Nezri, E., Nielsen, C., Nuñez-Castiñeyra, A., O'Fearraigh, B., Organokov, M., Păvălaş, G. E., Pellegrino, C., Perrin-Terrin, M., Piattelli, P., Poirè, C., Popa, V., Pradier, T., Randazzo, N., Reck, S., Riccobene, G., Romanov, A., Sánchez-Losa, A., Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schnabe, J., Schüssler, F., Spurio, M., Stolarczyk, Th., Strandberg, B., Taiuti, M., Tayalati, Y., Thakore, T., Tingay, S. J., Vallage, B., Van Elewyck, V., Versari, F., Viola, S., Vivolo, D., Wilms, J., Zegarelli, A., Zornoza, J. D., Zúñiga, J., Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 7329), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Laboratoire d'Informatique et Systèmes (LIS), Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), Institut méditerranéen d'océanologie (MIO), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, ANTARES, ANR-18-IDEX-0001,Université de Paris,Université de Paris(2018), Albert A., Andre M., Anghinolfi M., Anton G., Ardid M., Aubert J.-J., Aublin J., Baret B., Basa S., Belhorma B., Bertin V., Biagi S., Bissinger M., Boumaaza J., Bouta M., Bouwhuis M.C., Branzas H., Bruijn R., Brunner J., Busto J., Capone A., Caramete L., Carr J., Celli S., Chabab M., Chau T.N., Cherkaoui El Moursli R., Chiarusi T., Circella M., Coleiro A., Colomer-Molla M., Coniglione R., Coyle P., Creusot A., Diaz A.F., De Wasseige G., Deschamps A., Distefano C., Di Palma I., Domi A., Donzaud C., Dornic D., Drouhin D., Eberl T., El Khayati N., Enzenhofer A., Ettahiri A., Fermani P., Ferrara G., Filippini F., Fusco L., Gay P., Glotin H., Gozzini R., Graf K., Guidi C., Hallmann S., Van Haren H., Heijboer A.J., Hello Y., Hernandez-Rey J.J., Hossl J., Hofestadt J., Huang F., Illuminati G., James C.W., De Jong M., De Jong P., Jongen M., Kadler M., Kalekin O., Katz U., Khan-Chowdhury N.R., Kouchner A., Kreykenbohm I., Kulikovskiy V., Lahmann R., Le Breton R., Lefevre D., Leonora E., Levi G., Lincetto M., Lopez-Coto D., Loucatos S., Maggi G., Manczak J., Marcelin M., Margiotta A., Marinelli A., Martinez-Mora J.A., Mele R., Melis K., Migliozzi P., Moser M., Moussa A., Muller R., Nauta L., Navas S., Nezri E., Nielsen C., Nunez-Castineyra A., O'Fearraigh B., Organokov M., Pavalas G.E., Pellegrino C., Perrin-Terrin M., Piattelli P., Poire C., Popa V., Pradier T., Randazzo N., Reck S., Riccobene G., Romanov A., Sanchez-Losa A., Samtleben D.F.E., Sanguineti M., Sapienza P., Schnabel J., Schussler F., Spurio M., Stolarczyk T., Strandberg B., Taiuti M., Tayalati Y., Thakore T., Tingay S.J., Vallage B., Van Elewyck V., Versari F., Viola S., Vivolo D., Wilms J., Zegarelli A., Zornoza J.D., Zuniga J., Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN), Centre Tecnològic de Vilanova i la Geltrú, Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS)-Aix Marseille Université (AMU), Ministerio de Ciencia, Innovación y Universidades (España), KM3NeT (IHEF, IoP, FNWI), ATLAS (IHEF, IoP, FNWI), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA), Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J. -J., Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bouta, M., Bouwhuis, M. C., Branzas, H., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Chabab, M., Chau, T. N., Cherkaoui El Moursli, R., Chiarusi, T., Circella, M., Coleiro, A., Colomer-Molla, M., Coniglione, R., Coyle, P., Creusot, A., Diaz, A. F., De Wasseige, G., Deschamps, A., Distefano, C., Di Palma, I., Domi, A., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., El Khayati, N., Enzenhofer, A., Ettahiri, A., Fermani, P., Ferrara, G., Filippini, F., Fusco, L., Gay, P., Glotin, H., Gozzini, R., Graf, K., Guidi, C., Hallmann, S., Van Haren, H., Heijboer, A. J., Hello, Y., Hernandez-Rey, J. J., Hossl, J., Hofestadt, J., Huang, F., Illuminati, G., James, C. W., De Jong, M., De Jong, P., Jongen, M., Kadler, M., Kalekin, O., Katz, U., Khan-Chowdhury, N. R., Kouchner, A., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Le Breton, R., Lefevre, D., Leonora, E., Levi, G., Lincetto, M., Lopez-Coto, D., Loucatos, S., Maggi, G., Manczak, J., Marcelin, M., Margiotta, A., Marinelli, Antonio, Martinez-Mora, J. A., Mele, Rosa, Melis, K., Migliozzi, P., Moser, M., Moussa, A., Muller, R., Nauta, L., Navas, S., Nezri, E., Nielsen, C., Nunez-Castineyra, A., O'Fearraigh, B., Organokov, M., Pavalas, G. E., Pellegrino, C., Perrin-Terrin, M., Piattelli, P., Poire, C., Popa, V., Pradier, T., Randazzo, N., Reck, S., Riccobene, G., Romanov, A., Sanchez-Losa, A., Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schnabel, J., Schussler, F., Spurio, M., Stolarczyk, T., Strandberg, B., Taiuti, M., Tayalati, Y., Thakore, T., Tingay, S. J., Vallage, B., Van Elewyck, V., Versari, F., Viola, S., Vivolo, Daniele, Wilms, J., Zegarelli, A., Zornoza, J. D., and Zuniga, J.
Subjects: Astrofísica, Physics::Instrumentation and Detectors, Raigs còsmics, Monte Carlo method, Astrophysics, 01 natural sciences, Cosmology, law.invention, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), law, Shadow, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Astrophysics::Solar and Stellar Astrophysics, Pointlike neutrinos, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, astro-ph.IM, Sun shadow effect, Astrophysics::Instrumentation and Methods for Astrophysics, solar, muon: atmosphere, Physique [physics]/Astrophysique [astro-ph], neutrino: detector, Neutrino detector, Sun shadow, ANTARES, Neutrino telescope, shadowing, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Antares neutrino telescope, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Cosmic Ray, Telescope, cosmic rays, hal-03171499, 0103 physical sciences, Experiments in gravity, Angular resolution, 14. Life underwater, Neutrins, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, muon: flux, Instrumentation and Methods for Astrophysics (astro-ph.IM), Muon, ANTARES, Telescopis, 010308 nuclear & particles physics, Astronomy, neutrino: particle source, Physique [physics]/Physique des Hautes Energies - Expérience [hep-ex], cosmic radiation: primary, angular resolution, FISICA APLICADA, Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], High Energy Physics::Experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], cosmology, statistical, absorption, Telescopes
Abstract: [EN] The ANTARES detector is an undersea neutrino telescope in the Mediterranean Sea. The search for pointlike neutrino sources is one of the main goals of the ANTARES telescope, requiring a reliable method to evaluate the detector angular resolution and pointing accuracy. This work describes the study of the Sun ¿shadow¿ effect with the ANTARES detector. The shadow is the deficit in the atmospheric muon flux in the direction of the Sun caused by the absorption of the primary cosmic rays. This analysis is based on the data collected between 2008 and 2017 by the ANTARES telescope. The observed statistical significance of the Sun shadow detection is 3.7¿, with an estimated angular resolution of 0.59° +- 0.10°for downward-going muons. The pointing accuracy is found to be consistent with the expectations and no evidence of systematic pointing shifts is observed., The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique, Commissariat `a l'' energie atomique et aux energies alternatives, Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France, LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), R ' egion Ile-de-France (DIM-ACAV), Region Alsace (contract CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung, Germany; Istituto Nazionale di Fisica Nucleare, Italy; Nederlandse organisatie voor Wetenschappelijk Onderzoek, the Netherlands; Council of the President of the Russian Federation for Young Scientists and Leading Scientific Schools supporting grants, Russia; Executive Unit for Financing Higher Education, Research, Development and Innovation (UEFISCDI), Romania; Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento (refs. PGC2018-096663-B-C41, -A-C42, -B-C43, -B-C44) (MCIU/FEDER), Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Junta de Andalucia (refs. SOMM17/6104/UGR and A-FQM-053-UGR18), Generalitat Valenciana: Grisolia (ref. GRISOLIA/2018/119), Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.
Published: 2020
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11. Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope

Author: ANTARES Collaboration, Albert, A., André, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J. J., Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bouta, M., Bouwhuis, M. C., Brânzaş, H., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Chabab, M., Chau, T. N., Moursli, R. Cherkaoui El, Chiarusi, T., Circella, M., Coleiro, A., Colomer-Molla, M., Coniglione, R., Coyle, P., Creusot, A., Díaz, A. F., de Wasseige, G., Deschamps, A., Distefano, C., Di Palma, I., Domi, A., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., Khayati, N. El, Enzenhöfer, A., Ettahiri, A., Fermani, P., Ferrara, G., Filippini, F., Fusco, L., Gay, P., Glotin, H., Gozzini, R., Ruiz, R. Gracia, Graf, K., Guidi, C., Hallmann, S., van Haren, H., Heijboer, A. J., Hello, Y., Hernández-Rey, J. J., Hößl, J., Hofestädt, J., Huang, F., Illuminati, G., James, C. W., de Jong, M., de Jong, P., Jongen, M., Kadler, M., Kalekin, O., Katz, U., Khan-Chowdhury, N. R., Kouchner, A., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Breton, R. Le, Lefèvre, D., Leonora, E., Levi, G., Lincetto, M., Lopez-Coto, D., Loucatos, S., Maggi, G., Manczak, J., Marcelin, M., Margiotta, A., Marinelli, A., Martínez-Mora, J. A., Mele, R., Melis, K., Migliozzi, P., Moser, M., Moussa, A., Muller, R., Nauta, L., Navas, S., Nezri, E., Nielsen, C., Nuñez-Castiñeyra, A., O'Fearraigh, B., Organokov, M., Păvălaş, G. E., Pellegrino, C., Perrin-Terrin, M., Piattelli, P., Poirè, C., Popa, V., Pradier, T., Randazzo, N., Reck, S., Riccobene, G., Sánchez-Losa, A., Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schüssler, F., Spurio, M., Stolarczyk, Th., Strandberg, B., Taiuti, M., Tayalati, Y., Thakore, T., Tingay, S. J., Trovato, A., Vallage, B., Van Elewyck, V., Versari, F., Viola, S., Vivolo, D., Wilms, J., Zaborov, D., Zegarelli, A., Zornoza, J. D., Zúñiga, J., Institut Pluridisciplinaire Hubert Curien (IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 7329), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Laboratoire d'Informatique et Systèmes (LIS), Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), Institut méditerranéen d'océanologie (MIO), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, ANTARES, Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS), ANR-18-IDEX-0001,Université de Paris,Université de Paris(2018), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS)-Aix Marseille Université (AMU), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN), Albert, A, Andre, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, Jj, Aublin, J, Baret, B, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bissinger, M, Boumaaza, J, Bouta, M, Bouwhuis, Mc, Branzas, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, Chau, Tn, El Moursli, Rc, Chiarusi, T, Circella, M, Coleiro, A, Colomer-Molla, M, Coniglione, R, Coyle, P, Creusot, A, Diaz, Af, de Wasseige, G, Deschamps, A, Distefano, C, Di Palma, I, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, El Khayati, N, Enzenhofer, A, Ettahiri, A, Fermani, P, Ferrara, G, Filippini, F, Fusco, L, Gay, P, Glotin, H, Gozzini, R, Ruiz, Rg, Graf, K, Guidi, C, Hallmann, S, van Haren, H, Heijboer, Aj, Hello, Y, Hernandez-Rey, Jj, Hoessl, J, Hofestadt, J, Huang, F, Illuminati, G, James, Cw, de Jong, M, de Jong, P, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, Nr, Kouchner, A, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Le Breton, R, Lefevre, D, Leonora, E, Levi, G, Lincetto, M, Lopez-Coto, D, Loucatos, S, Maggi, G, Manczak, J, Marcelin, M, Margiotta, A, Marinelli, A, Martinez-Mora, Ja, Mele, R, Melis, K, Migliozzi, P, Moser, M, Moussa, A, Muller, R, Nauta, L, Navas, S, Nezri, E, Nielsen, C, Nunez-Castineyra, A, O'Fearraigh, B, Organokov, M, Pavalas, Ge, Pellegrino, C, Perrin-Terrin, M, Piattelli, P, Poire, C, Popa, V, Pradier, T, Randazzo, N, Reck, S, Riccobene, G, Sanchez-Losa, A, Samtleben, Dfe, Sanguineti, M, Sapienza, P, Schussler, F, Spurio, M, Stolarczyk, T, Strandberg, B, Taiuti, M, Tayalati, Y, Thakore, T, Tingay, Sj, Trovato, A, Vallage, B, Van Elewyck, V, Versari, F, Viola, S, Vivolo, D, Wilms, J, Zaborov, D, Zegarelli, A, Zornoza, Jd, Zuniga, J, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Albert A., Andre M., Anghinolfi M., Anton G., Ardid M., Aubert J.-J., Aublin J., Baret B., Basa S., Belhorma B., Bertin V., Biagi S., Bissinger M., Boumaaza J., Bouta M., Bouwhuis M.C., Branzas H., Bruijn R., Brunner J., Busto J., Capone A., Caramete L., Carr J., Celli S., Chabab M., Chau T.N., Moursli R.C.E., Chiarusi T., Circella M., Coleiro A., Molla M.C., Coniglione R., Coyle P., Creusot A., Diaz A.F., de Wasseige G., Deschamps A., Distefano C., Palma I.D., Domi A., Donzaud C., Dornic D., Drouhin D., Eberl T., Khayati N.E., Enzenhofer A., Ettahiri A., Fermani P., Ferrara G., Filippini F., Fusco L., Gay P., Glotin H., Gozzini R., Ruiz R.G., Graf K., Guidi C., Hallmann S., van Haren H., Heijboer A.J., Hello Y., Hernandez-Rey J.J., Hossl J., Hofestadt J., Huang F., Illuminati G., James C.W., de Jong M., de Jong P., Jongen M., Kadler M., Kalekin O., Katz U., Khan-Chowdhury N.R., Kouchner A., Kreykenbohm I., Kulikovskiy V., Lahmann R., Le Breton R., Lefevre D., Leonora E., Levi G., Lincetto M., Lopez-Coto D., Loucatos S., Maggi G., Manczak J., Marcelin M., Margiotta A., Marinelli A., Martinez-Mora J.A., Mele R., Melis K., Migliozzi P., Moser M., Moussa A., Muller R., Nauta L., Navas S., Nezri E., Nielsen C., Nunez-Castineyra A., O'Fearraigh B., Organokov M., Pavalas G.E., Pellegrino C., Perrin-Terrin M., Piattelli P., Poire C., Popa V., Pradier T., Randazzo N., Reck S., Riccobene G., Sanchez-Losa A., Samtleben D.F.E., Sanguineti M., Sapienza P., Schussler F., Spurio M., Stolarczyk T., Strandberg B., Taiuti M., Tayalati Y., Thakore T., Tingay S.J., Trovato A., Vallage B., Van Elewyck V., Versari F., Viola S., Vivolo D., Wilms J., Zaborov D., Zegarelli A., Zornoza J.D., Zuniga J., Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), Centre Tecnològic de Vilanova i la Geltrú, Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA), KM3NeT (IHEF, IoP, FNWI), ATLAS (IHEF, IoP, FNWI), IoP (FNWI), Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J. -J., Aublin, J., Baret, B., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bouta, M., Bouwhuis, M. C., Branzas, H., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Chabab, M., Chau, T. N., Moursli, R. C. E., Chiarusi, T., Circella, M., Coleiro, A., Molla, M. C., Coniglione, R., Coyle, P., Creusot, A., Diaz, A. F., de Wasseige, G., Deschamps, A., Distefano, C., Palma, I. D., Domi, A., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., Khayati, N. E., Enzenhofer, A., Ettahiri, A., Fermani, P., Ferrara, G., Filippini, F., Fusco, L., Gay, P., Glotin, H., Gozzini, R., Ruiz, R. G., Graf, K., Guidi, C., Hallmann, S., van Haren, H., Heijboer, A. J., Hello, Y., Hernandez-Rey, J. J., Hossl, J., Hofestadt, J., Huang, F., Illuminati, G., James, C. W., de Jong, M., de Jong, P., Jongen, M., Kadler, M., Kalekin, O., Katz, U., Khan-Chowdhury, N. R., Kouchner, A., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Le Breton, R., Lefevre, D., Leonora, E., Levi, G., Lincetto, M., Lopez-Coto, D., Loucatos, S., Maggi, G., Manczak, J., Marcelin, M., Margiotta, A., Marinelli, A., Martinez-Mora, J. A., Mele, R., Melis, K., Migliozzi, P., Moser, M., Moussa, A., Muller, R., Nauta, L., Navas, S., Nezri, E., Nielsen, C., Nunez-Castineyra, A., O'Fearraigh, B., Organokov, M., Pavalas, G. E., Pellegrino, C., Perrin-Terrin, M., Piattelli, P., Poire, C., Popa, V., Pradier, T., Randazzo, N., Reck, S., Riccobene, G., Sanchez-Losa, A., Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schussler, F., Spurio, M., Stolarczyk, T., Strandberg, B., Taiuti, M., Tayalati, Y., Thakore, T., Tingay, S. J., Trovato, A., Vallage, B., Van Elewyck, V., Versari, F., Viola, S., Vivolo, D., Wilms, J., Zaborov, D., Zegarelli, A., Zornoza, J. D., and Zuniga, J.
Subjects: Astrofísica, Physics and Astronomy (miscellaneous), neutrino astronomy, ANATARES telescope, Physics::Instrumentation and Detectors, Astrophysics, 01 natural sciences, Coincidence, High Energy Physics - Experiment, law.invention, High Energy Physics - Experiment (hep-ex), neutrino, law, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], LIGO, 010303 astronomy & astrophysics, Charged current, media_common, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 4. Education, Astrophysics::Instrumentation and Methods for Astrophysics, neutrino telescopes, astroparticle physics, gravitational waves, Physique [physics]/Astrophysique [astro-ph], Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Antares neutrino telescope, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Run O2, FOS: Physical sciences, lcsh:Astrophysics, Gravitational waves, Telescope, Ones gravitacionals, lcsh:QB460-466, 0103 physical sciences, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, Neutrins, Engineering (miscellaneous), 010308 nuclear & particles physics, Gravitational wave, Horizon, High Energy Physics::Phenomenology, gravitational radiation, Electromagnetic fields, Physique [physics]/Physique des Hautes Energies - Expérience [hep-ex], Gravitational-wave, Neutrino, gravitational-wave, ANTARES, VIRGO, Sky, FISICA APLICADA, Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], lcsh:QC770-798, High Energy Physics::Experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: An offline search for a neutrino counterpart to gravitational-wave (GW) events detected during the second observation run (O2) of Advanced-LIGO and Advanced- Virgo performed with ANTARES data is presented. In addition to the search for long tracks induced by νμ (νμ) charged current interactions, a search for showering events induced by interactions of neutrinos of any flavour is conducted. The severe spatial and time coincidence provided by the gravitational-wave alert allows regions above the detector horizon to be probed, extending the ANTARES sensitivity over the entire sky. The results of this all-neutrino-flavour and all-sky time dependent analysis are presented. The search for prompt neutrino emission within ±500 s around the time of six GW events yields no neutrino counterparts. Upper limits on the neutrino spectral fluence and constraints on the isotropic energy radiated via high-energy neutrinos (from a few TeV to a few tens of PeV) are set for each GW event analysed., Centre National de la Recherche Scientifique (CNRS), French Atomic Energy Commission, Commission Europeenne (FEDER fund), France, European Union (EU), Institut Universitaire de France (IUF), France, LabEx UnivEarthS, France ANR-10-LABX-0023 ANR-18-IDEX-0001, Region Ile-de-France, Region Grand-Est, Region Provence-Alpes-Cote d'Azur, Ville de La Seyne-sur-Mer, France, Federal Ministry of Education & Research (BMBF), Istituto Nazionale di Fisica Nucleare (INFN), Netherlands Organization for Scientific Research (NWO) Netherlands Government, Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia, Executive Unit for Financing Higher Education, Research, Development and Innovation (UEFISCDI), Romania, Ministerio de Ciencia, Innovación, Investigación y Universidades (MCIU): Programa Estatal de Generación de Conocimiento, Spain PGC2018-096663-B-C41 PGC2018-096663-A-C42 PGC2018-096663-B-C43 PGC2018-096663-B-C44, Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Junta de Andalucía, Spain SOMM17/6104/UGR, Generalitat Valenciana: Grisolia, Spain GRISOLIA/2018/119, Ministry of Higher Education, Scientific Research and Professional Training, Morocco
Published: 2020
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12. Erratum to 'Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope' [Phys. Lett. B 769 (2017) 249–254]

Author: A. Albert, M. André, M. Anghinolfi, G. Anton, M. Ardid, J.-J. Aubert, T. Avgitas, B. Baret, J. Barrios-Martí, S. Basa, V. Bertin, S. Biagi, R. Bormuth, S. Bourret, M.C. Bouwhuis, R. Bruijn, J. Brunner, J. Busto, A. Capone, L. Caramete, J. Carr, S. Celli, T. Chiarusi, M. Circella, J.A.B. Coelho, A. Coleiro, R. Coniglione, H. Costantini, P. Coyle, A. Creusot, A. Deschamps, G. De Bonis, C. Distefano, I. Di Palma, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, I. El Bojaddaini, D. Elsässer, A. Enzenhöfer, I. Felis, L.A. Fusco, S. Galatà, P. Gay, S. Geißelsöder, K. Geyer, V. Giordano, A. Gleixner, H. Glotin, R. Gozzini, T. Grégoire, R. Gracia Ruiz, K. Graf, S. Hallmann, H. van Haren, A.J. Heijboer, Y. Hello, J.J. Hernández-Rey, J. Hößl, J. Hofestädt, C. Hugon, G. Illuminati, C.W. James, M. de Jong, M. Jongen, M. Kadler, O. Kalekin, U. Katz, D. Kießling, A. Kouchner, M. Kreter, I. Kreykenbohm, V. Kulikovskiy, C. Lachaud, R. Lahmann, D. Lefèvre, E. Leonora, M. Lotze, S. Loucatos, M. Marcelin, A. Margiotta, A. Marinelli, J.A. Martínez-Mora, A. Mathieu, R. Mele, K. Melis, T. Michael, P. Migliozzi, A. Moussa, C. Mueller, E. Nezri, G.E. Păvălaş, C. Pellegrino, C. Perrina, P. Piattelli, V. Popa, T. Pradier, L. Quinn, C. Racca, G. Riccobene, K. Roensch, A. Sánchez-Losa, M. Saldaña, I. Salvadori, D.F.E. Samtleben, M. Sanguineti, P. Sapienza, J. Schnabel, F. Schüssler, T. Seitz, C. Sieger, M. Spurio, Th. Stolarczyk, M. Taiuti, Y. Tayalati, A. Trovato, M. Tselengidou, D. Turpin, C. Tönnis, B. Vallage, C. Vallée, V. Van Elewyck, D. Vivolo, A. Vizzoca, S. Wagner, J. Wilms, J.D. Zornoza, J. Zúñiga, Centre de Physique des Particules de Marseille (CPPM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de Physique de Clermont (LPC), Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Albert, A, Andre, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, Jj, Avgitas, T, Baret, B, Barrios-Marti, J, Basa, S, Bertin, V, Biagi, S, Bormuth, R, Bourret, S, Bouwhuis, Mc, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chiarusi, T, Circella, M, Coelho, Jab, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Deschamps, A, Debonis, G, Distefano, C, Dipalma, I, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Elbojaddaini, I, Elsasser, D, Enzenhofer, A, Felis, I, Fusco, A, Galata, S, Gay, P, Geisselsoder, S, Geyer, K, Giordano, V, Gleixner, A, Glotin, H, Gozzini, R, Gregoire, T, Ruiz, Rg, Graf, K, Hallmann, S, van Haren, H, Heijboer, Aj, Hello, Y, Hernandez-Rey, Jj, Hossl, J, Hofestadt, J, Hugon, C, Illuminati, G, James, Cw, de Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Kiessling, D, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefevre, D, Leonora, E, Lotze, M, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martinez-Mora, Ja, Mathieu, A, Mele, R, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Mueller, C, Nezri, E, Pavalas, Ge, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Quinn, L, Racca, C, Riccobene, G, Roensch, K, Sanchez-Losa, A, Saldana, M, Salvadori, I, Samtleben, Dfe, Sanguineti, M, Sapienza, P, Schnabel, J, Schussler, F, Seitz, T, Sieger, C, Spurio, M, Stolarczyk, T, Taiuti, M, Tayalati, Y, Trovato, A, Tselengidou, M, Turpin, D, Tonnis, C, Vallage, B, Vallee, C, Van Elewyck, V, Vivolo, D, Vizzoca, A, Wagner, S, Wilms, J, Zornoza, Jd, and Zuniga, J
Subjects: Physics, [PHYS]Physics [physics], Nuclear and High Energy Physics, neutrino astronomy, dark matter, ANTARES neutrino telescope, 010308 nuclear & particles physics, Milky Way, Dark matter, Neutrino telescope, Astronomy, 01 natural sciences, 0103 physical sciences, 010306 general physics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS
Abstract: Erratum to “Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope” [Phys. Lett. B 769 (2017) 249–254]
Published: 2019
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13. The cosmic ray shadow of the Moon observed with the ANTARES neutrino telescope

Author: Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, A*Midex Foundation, Region Ile-de-France, Generalitat Valenciana, Ministerio de Economía y Empresa, Université Sorbonne Paris Cité, Institut Universitaire de France, European Regional Development Fund, Instituto Nazionale di Fisica Nucleare, Ministerio de Economía y Competitividad, Conseil Régional Provence-Alpes-Côte d'Azur, Netherlands Organization for Scientific Research, Département du Var and Ville de La Seyne-sur-Mer, Bundesministerium für Bildung und Forschung, Alemania, Centre National de la Recherche Scientifique, Francia, National Authority for Scientific Research, Rumanía, Council on grants of the President of the Russian Federation, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, Laboratoire d'Excellence OCEVU (Origines, Constituants & ÉVolution de l'Univers), Universidad Autónoma de Madrid, Ministère de l'Education Nationale, de la Formation professionnelle, de l'Enseignement Supérieur et de la Recherche Scientifique, Marruecos, Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Aubert, J. -J., Aublin, J., Avgitas, T., Baret, B., Barrios-Martit, J., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bormuth, R., Felis-Enguix, Iván, Martínez Mora, Juan Antonio, Saldaña-Coscollar, María, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, A*Midex Foundation, Region Ile-de-France, Generalitat Valenciana, Ministerio de Economía y Empresa, Université Sorbonne Paris Cité, Institut Universitaire de France, European Regional Development Fund, Instituto Nazionale di Fisica Nucleare, Ministerio de Economía y Competitividad, Conseil Régional Provence-Alpes-Côte d'Azur, Netherlands Organization for Scientific Research, Département du Var and Ville de La Seyne-sur-Mer, Bundesministerium für Bildung und Forschung, Alemania, Centre National de la Recherche Scientifique, Francia, National Authority for Scientific Research, Rumanía, Council on grants of the President of the Russian Federation, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, Laboratoire d'Excellence OCEVU (Origines, Constituants & ÉVolution de l'Univers), Universidad Autónoma de Madrid, Ministère de l'Education Nationale, de la Formation professionnelle, de l'Enseignement Supérieur et de la Recherche Scientifique, Marruecos, Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Aubert, J. -J., Aublin, J., Avgitas, T., Baret, B., Barrios-Martit, J., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bormuth, R., Felis-Enguix, Iván, Martínez Mora, Juan Antonio, and Saldaña-Coscollar, María
Abstract: [EN] One of the main objectives of the ANTARES telescope is the search for point-like neutrino sources. Both the pointing accuracy and the angular resolution of the detector are important in this context and a reliable way to evaluate this performance is needed. In order to measure the pointing accuracy of the detector, one possibility is to study the shadow of the Moon, i.e. the de¿cit of the atmospheric muon ¿ux from the direction of the Moon induced by the absorption of cosmic rays. Analysing the data taken between 2007 and 2016, the Moon shadow is observed with 3.5¿ statistical signi¿cance. The detector angular resolution for downward-going muons is 0.73¿ ±0.14¿. The resulting pointing performance is consistent with the expectations. An independent check of the telescope pointing accuracy is realised with the data collected by a shower array detector onboard of a ship temporarily moving around the ANTARES location.
Published: 2018

14. The cosmic ray shadow of the Moon observed with the ANTARES neutrino telescope

Author: A. Albert, M. André, M. Anghinolfi, G. Anton, M. Ardid, J. -J. Aubert, J. Aublin, T. Avgitas, B. Baret, J. Barrios-Martít, S. Basa, B. Belhorma, V. Bertin, S. Biagi, R. Bormuth, J. Boumaaza, S. Bourret, M. C. Bouwhuis, H. Brânzaş, R. Bruijn, J. Brunner, J. Busto, A. Capone, L. Caramete, J. Carr, S. Celli, M. Chabab, R. Cherkaoui El Moursli, T. Chiarusi, M. Circella, J. A. B. Coelho, A. Coleiro, M. Colomer, R. Coniglione, H. Costantini, P. Coyle, A. Creusot, A. F. Díaz, A. Deschamps, C. Distefano, I. Di Palma, A. Domi, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, I. El Bojaddaini, N. El Khayati, D. Elsässer, A. Enzenhöfer, A. Ettahiri, F. Fassi, I. Felis, P. Fermani, G. Ferrara, L. A. Fusco, P. Gay, H. Glotin, T. Grégoire, R. Gracia Ruiz, K. Graf, S. Hallmann, H. van Haren, A. J. Heijboer, Y. Hello, J. J. Hernández-Rey, J. Hößl, J. Hofestädt, G. Illuminati, M. de Jong, M. Jongen, M. Kadler, O. Kalekin, U. Katz, N. R. Khan-Chowdhury, A. Kouchner, M. Kreter, I. Kreykenbohm, V. Kulikovskiy, C. Lachaud, R. Lahmann, D. Lefèvre, E. Leonora, G. Levi, M. Lotze, S. Loucatos, M. Marcelin, A. Margiotta, A. Marinelli, J. A. Martínez-Mora, R. Mele, K. Melis, P. Migliozzi, A. Moussa, S. Navas, E. Nezri, A. Nuñez, M. Organokov, G. E. Păvălaş, C. Pellegrino, P. Piattelli, V. Popa, T. Pradier, L. Quinn, C. Racca, N. Randazzo, G. Riccobene, A. Sánchez-Losa, M. Saldaña, I. Salvadori, D. F. E. Samtleben, M. Sanguineti, P. Sapienza, F. Schüssler, M. Spurio, Th. Stolarczyk, M. Taiuti, Y. Tayalati, A. Trovato, B. Vallage, V. Van Elewyck, F. Versari, D. Vivolo, J. Wilms, D. Zaborov, J. D. Zornoza, J. Zúñiga, Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 7329), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Informatique et Systèmes (LIS), Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), Institut méditerranéen d'océanologie (MIO), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), ANTARES, Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Observatoire de la Côte d'Azur (OCA), Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN)-Aix Marseille Université (AMU)-Institut de Recherche pour le Développement (IRD), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS)-Aix Marseille Université (AMU), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN), KM3NeT (IHEF, IoP, FNWI), Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre Tecnològic de Vilanova i la Geltrú, Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques, Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J. -J., Aublin, J., Avgitas, T., Baret, B., Barrios-Martit, J., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bormuth, R., Boumaaza, J., Bourret, S., Bouwhuis, M. C., Branzas, H., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Chabab, M., Moursli, R. C. E., Chiarusi, T., Circella, M., Coelho, J. A. B., Coleiro, A., Colomer, M., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., Diaz, A. F., Deschamps, A., Distefano, C., Palma, I. D., Domi, A., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., Bojaddaini, I. E., Khayati, N. E., Elsasser, D., Enzenhofer, A., Ettahiri, A., Fassi, F., Felis, I., Fermani, P., Ferrara, G., Fusco, L. A., Gay, P., Glotin, H., Gregoire, T., Ruiz, R. G., Graf, K., Hallmann, S., van Haren, H., Heijboer, A. J., Hello, Y., Hernandez-Rey, J. J., Hossl, J., Hofestadt, J., Illuminati, G., de Jong, M., Jongen, M., Kadler, M., Kalekin, O., Katz, U., Khan-Chowdhury, N. R., Kouchner, A., Kreter, M., Kreykenbohm, I., Kulikovskiy, V., Lachaud, C., Lahmann, R., Lefevre, D., Leonora, E., Levi, G., Lotze, M., Loucatos, S., Marcelin, M., Margiotta, A., Marinelli, A., Martinez-Mora, J. A., Mele, R., Melis, K., Migliozzi, P., Moussa, A., Navas, S., Nezri, E., Nunez, A., Organokov, M., Pavalas, G. E., Pellegrino, C., Piattelli, P., Popa, V., Pradier, T., Quinn, L., Racca, C., Randazzo, N., Riccobene, G., Sanchez-Losa, A., Saldana, M., Salvadori, I., Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schussler, F., Spurio, M., Stolarczyk, T., Taiuti, M., Tayalati, Y., Trovato, A., Vallage, B., Van Elewyck, V., Versari, F., Vivolo, D., Wilms, J., Zaborov, D., Zornoza, J. D., Zuniga, J., Albert, A, Andre, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, Jj, Aublin, J, Avgitas, T, Baret, B, Barrios-Martit, J, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bormuth, R, Boumaaza, J, Bourret, S, Bouwhuis, Mc, Branzas, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, El Moursli, Rc, Chiarusi, T, Circella, M, Coelho, Jab, Coleiro, A, Colomer, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Diaz, Af, Deschamps, A, Distefano, C, Palma, I, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, I, Khayati, N, Elsaesser, D, Enzenhoefer, A, Ettahiri, A, Fassi, F, Felis, I, Fermani, P, Ferrara, G, Fusco, La, Gay, P, Glotin, H, Gregoire, T, Ruiz, Rg, Graf, K, Hallmann, S, Haren, H, Heijboer, Aj, Hello, Y, Hernandez-Rey, Jj, Hoessl, J, Hofestaedt, J, Illuminati, G, Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, Nr, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefevre, D, Leonora, E, Levi, G, Lotze, M, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martinez-Mora, Ja, Mele, R, Melis, K, Migliozzi, P, Moussa, A, Navas, S, Nezri, E, Nunez, A, Organokov, M, Pavalas, Ge, Pellegrino, C, Piattelli, P, Popa, V, Pradier, T, Quinn, L, Racca, C, Randazzo, N, Riccobene, G, Sanchez-Losa, A, Saldana, M, Salvadori, I, Samtleben, Dfe, Sanguineti, M, Sapienza, P, Schussler, F, Spurio, M, Stolarczyk, T, Taiuti, M, Tayalati, Y, Trovato, A, Vallage, B, Elewyck, V, Versari, F, Vivolo, D, Wilms, J, Zaborov, D, Zornoza, Jd, Zuniga, J, André, M., Aubert, J.-J., Barrios-Martít, J., Bouwhuis, M.C., Brânzaş, H., Moursli, R. Cherkaoui El, Coelho, J.A.B., Díaz, A.F., Palma, I. Di, Bojaddaini, I. El, Khayati, N. El, Elsässer, D., Enzenhöfer, A., Fusco, L.A., Grégoire, T., Ruiz, R. Gracia, Heijboer, A.J., Hernández-Rey, J.J., Hößl, J., Hofestädt, J., Khan-Chowdhury, N.R., Lefèvre, D., Martínez-Mora, J.A., Nuñez, A., Păvălaş, G.E., Sánchez-Losa, A., Saldaña, M., Samtleben, D.F.E., Schüssler, F., Stolarczyk, Th., Zornoza, J.D., and Zúñiga, J.
Subjects: Astrofísica, Physics and Astronomy (miscellaneous), Physics::Instrumentation and Detectors, Planets, Astrophysics, shadowing: lunar, 01 natural sciences, law.invention, Astronomical observatories, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), law, Shadow, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], cosmic ray, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, astro-ph.IM, Detector, Moon shadow, Astrophysics::Instrumentation and Methods for Astrophysics, muon: atmosphere, Physique [physics]/Astrophysique [astro-ph], neutrino: detector, Astrophysics::Earth and Planetary Astrophysics, Neutrino, Observatoris astronòmics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, performance, Regular Article - Experimental Physics, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Context (language use), Cosmic ray, lcsh:Astrophysics, Computer Science::Digital Libraries, Lluna, Telescope, neutrino astronomy, cosmic rays, 0103 physical sciences, lcsh:QB460-466, ANTARES, neutrino telescope, Angular resolution, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, Neutrins, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Neutrinos, Planetes, cosmic radiation: absorption, 010306 general physics, Engineering (miscellaneous), muon: flux, Instrumentation and Methods for Astrophysics (astro-ph.IM), Muon, Telescopis, Antares neutrino Telescope, 010308 nuclear & particles physics, Astronomy, showers, Physique [physics]/Physique des Hautes Energies - Expérience [hep-ex], Neutrino astrophysics, Point like neutrino sources, angular resolution, Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], FISICA APLICADA, lcsh:QC770-798, High Energy Physics::Experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], statistical, Telescopes
Abstract: [EN] One of the main objectives of the ANTARES telescope is the search for point-like neutrino sources. Both the pointing accuracy and the angular resolution of the detector are important in this context and a reliable way to evaluate this performance is needed. In order to measure the pointing accuracy of the detector, one possibility is to study the shadow of the Moon, i.e. the de¿cit of the atmospheric muon ¿ux from the direction of the Moon induced by the absorption of cosmic rays. Analysing the data taken between 2007 and 2016, the Moon shadow is observed with 3.5¿ statistical signi¿cance. The detector angular resolution for downward-going muons is 0.73¿ ±0.14¿. The resulting pointing performance is consistent with the expectations. An independent check of the telescope pointing accuracy is realised with the data collected by a shower array detector onboard of a ship temporarily moving around the ANTARES location., The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'energie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cite (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Labex OCEVU (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Region Provence-Allies-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fin Bildung and Forschung (BMBF), Germany; Istituto Naziona-le di Fisica Nucleare (INFN), Italy; 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 Economia y Competitividad (MINE-CO): Plan Estatal de Investigacion (refs. FPA2015-65150-C3-1-P, -2-P and -3-P, (MINECO/FEDER)), Severn Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolia programs (Generalitat Valencia-na), Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.
Published: 2018
Full Text: View/download PDF

15. All-sky Search for High-Energy Neutrinos from Gravitational Wave Event GW170104 with the ANTARES Neutrino Telescope

Author: Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Aubert , J.J., Avgitas, T., Baret, B., Barrios-Marti, J., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bormuth, R., Bourret, S., Felis-Enguix, Iván, Martínez Mora, Juan Antonio, and Saldaña-Coscollar, María
Subjects: FISICA APLICADA, High-energy neutrinos, Antares neutrino telescope, Gravitational event GW170104
Abstract: [EN] Advanced LIGO detected a significant gravitational wave signal (GW170104) originating from the coalescence of two black holes during the second observation run on January 4th, 2017. Anall-sky high-energy neutrino follow-up search has been made using data from the Antares neutrino telescope, including both upgoing and downgoing events in two separate analyses. No neutrino candidates were found within +/- 500 s around the GW event time nor any time clustering of events over an extended time window of +/- 3 months. The non-detection is used to constrain isotropic-equivalent high-energy neutrino emission from GW170104 to less than similar to 1.2 x 10(55) erg for a E-2 spectrum. This constraint is valid in the energy range corresponding to the 5-95% quantiles of the neutrino flux [3.2 TeV; 3.6 PeV], if the GW emitter was below the Antares horizon at the alert time., The ANTARES Collaboration is grateful to the LIGO Scientific Collaboration and the Virgo Collaboration for the setting up of an impressive follow-up observation program, and for sharing invaluable scientific information for the benefit of the emerging multi-messenger astronomy. The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'energie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cite (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Labex OCEVU (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; 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 Economia y Competitividad (MINECO): Plan Estatal de Investigacion (refs. FPA2015-65150-C3-1-P, -2-P and -3-P, (MINECO/FEDER)), Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolia programs (Generalitat Valenciana), Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco.
Published: 2017

16. Sperm whale long-range echolocation sounds revealed by ANTARES, a deep-sea neutrino telescope

Author: André, M., Caballé, A., van Der Schaar, M., Solsona, A., Houégnigan, L., Zaugg, S., Sánchez, M., Castell, J., Solé, M., Vila, F., Djokic, D., Adrián-Martínez, S., Albert, A., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J., Avgitas, T., Baret, B., Barrios-Martí, J., Basa, S., Bertin, V., Biagi, S., Bormuth, R., Bouwhuis, C., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Chiarusi, T., Circella, M., Coleiro, A., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., Deschamps, Anne, de Bonis, G., Distefano, C., Di Palma, I., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., El Bojaddaini, I., Elsässer, D., Enzenhöfer, A., Fehn, K., Felis, I., Fusco, A., Galatà, S., Gay, P., Geisselsöder, S., Geyer, K., Giordano, V., Gleixner, A., Glotin, Hervé, Gracia-Ruiz, R., Graf, K., Hallmann, S., van Haren, H., Heijboer, J., Hello, Y., Hernandez-Rey, J., Hössl, J., Hofestädt, J., Hugon, C., Illuminati, G., James, C., de Jong, M., Jongen, M., Kadler, M., Kalekin, O., Katz, U., Kiessling, D., Kouchner, A., Kreter, M., Kreykenbohm, I., Kulikovskiy, V., Lachaud, C., Lahmann, R., Lefèvre, Dominique, Leonora, E., Loucatos, S., Marcelin, M., Margiotta, A., Marinelli, A., Martínez-Mora, J., Mathieu, A., Melis, K., Michael, T., Migliozzi, P., Moussa, A., Mueller, C., Nezri, E., Păvălaş, G., Pellegrino, C., Perrina, C., Piattelli, P., Popa, V., Pradier, T., Racca, C., Riccobene, G., Roensch, K., Saldaña, M., Samtleben, D., Sanguineti, M., Sapienza, P., Schnabel, J., Schüssler, F., Seitz, T., Sieger, C., Spurio, M., Stolarczyk, Th., Sánchez-Losa, A., Taiuti, M., Trovato, A., Tselengidou, M., Turpin, D., Tönnis, C., Vallage, B., Vallée, Corentin, van Elewyck, V., Vivolo, D., Wagner, S., Wilms, J., Zornoza, J., Zuñiga, J., Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ANTARES, Andre, M, Caballe, A, Van der Schaar, M, Solsona, A, Houegnigan, L, Zaugg, S, Sanchez, Am, Castell, Jv, Sole, M, Vila, F, Djokic, D, Adrian-Martinez, S, Albert, A, Anghinolfi, M, Anton, G, Ardid, M, Aubert, Jj, Avgitas, T, Baret, B, Barrios-Marti, J, Basa, S, Bertin, V, Biagi, S, Bormuth, R, Bouwhuis, Mc, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chiarusi, T, Circella, M, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Deschamps, A, De Bonis, G, Distefano, C, Di Palma, I, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, El Bojaddaini, I, Elsasser, D, Enzenhofer, A, Fehn, K, Felis, I, Fusco, La, Galata, S, Gay, P, Geisselsoder, S, Geyer, K, Giordano, V, Gleixner, A, Glotin, H, Gracia-Ruiz, R, Graf, K, Hallmann, S, van Haren, H, Heijboer, Aj, Hello, Y, Hernandez-Rey, Jj, Hossl, J, Hofestadt, J, Hugon, C, Illuminati, G, James, Cw, de Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Kiessling, D, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefevre, D, Leonora, E, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martinez-Mora, Ja, Mathieu, A, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Mueller, C, Nezri, E, Pavalas, Ge, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Racca, C, Riccobene, G, Roensch, K, Saldana, M, Samtleben, Dfe, Sanguineti, M, Sapienza, P, Schnabel, J, Schussler, F, Seitz, T, Sieger, C, Spurio, M, Stolarczyk, T, Sanchez-Losa, A, Taiuti, M, Trovato, A, Tselengidou, M, Turpin, D, Tonnis, C, Vallage, B, Vallee, C, Van Elewyck, V, Vivolo, D, Wagner, S, Wilms, J, Zornoza, Jd, Zuniga, J, Centre de Physique des Particules de Marseille ( CPPM ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Aix Marseille Université ( AMU ), Andre, M., Caballe, A., Van Der Schaar, M., Solsona, A., Houegnigan, L., Zaugg, S., Sanchez, A. M., Castell, J. V., Sole, M., Vila, F., Djokic, D., Adrian-Martinez, S., Albert, A., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J. -J., Avgitas, T., Baret, B., Barrios-Marti, J., Basa, S., Bertin, V., Biagi, S., Bormuth, R., Bouwhuis, M. C., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Chiarusi, T., Circella, M., Coleiro, A., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., Deschamps, A., De Bonis, G., Distefano, C., Di Palma, I., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., El Bojaddaini, I., Elsasser, D., Enzenhofer, A., Fehn, K., Felis, I., Fusco, L. A., Galata, S., Gay, P., Geisselsoder, S., Geyer, K., Giordano, V., Gleixner, A., Glotin, H., Gracia-Ruiz, R., Graf, K., Hallmann, S., Van Haren, H., Heijboer, A. J., Hello, Y., Hernandez-Rey, J. J., Hossl, J., Hofestadt, J., Hugon, C., Illuminati, G., James, C. W., De Jong, M., Jongen, M., Kadler, M., Kalekin, O., Katz, U., Kiessling, D., Kouchner, A., Kreter, M., Kreykenbohm, I., Kulikovskiy, V., Lachaud, C., Lahmann, R., Lefevre, D., Leonora, E., Loucatos, S., Marcelin, M., Margiotta, A., Marinelli, A., Martinez-Mora, J. A., Mathieu, A., Melis, K., Michael, T., Migliozzi, P., Moussa, A., Mueller, C., Nezri, E., P Avalas, G. E., Pellegrino, C., Perrina, C., Piattelli, P., Popa, V., Pradier, T., Racca, C., Riccobene, G., Roensch, K., Saldana, M., Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schnabel, J., Schussler, F., Seitz, T., Sieger, C., Spurio, M., Stolarczyk, T., Sanchez-Losa, A., Taiuti, M., Trovato, A., Tselengidou, M., Turpin, D., Tonnis, C., Vallage, B., Vallee, C., Van Elewyck, V., Vivolo, D., Wagner, S., Wilms, J., Zornoza, J. D., Zuniga, J., André, M, Caballé, A., Houégnigan, L., Sánchez, A.M., Castell, J.V., Solé, M., Adrián-Martínez, S., Aubert, J.-J., Barrios-Martí, J., Bouwhuis, M.C., Elsässer, D., Enzenhöfer, A., Fusco, L.A., Galatà, S., Geißelsöder, S., Heijboer, A.J., Hernandez-Rey, J.J., Hößl, J., Hofestädt, J., James, C.W., Kießling, D., Lefèvre, D., Martínez-Mora, J.A., P Ǎvǎlaş, G.E., Saldaña, M., Samtleben, D.F.E., Schüssler, F., Stolarczyk, Th., Sánchez-Losa, A., Tönnis, C., Vallée, C., Zornoza, J.D., and Zuñiga, J.
Subjects: Sperm whale, Multidisciplinary, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], Echolocation, FISICA APLICADA, [ SDU.ASTR.IM ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Antares neutrino telescope, [ SDU.ASTR ] Sciences of the Universe [physics]/Astrophysics [astro-ph], Article, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
Abstract: [EN] Despite dedicated research has been carried out to adequately map the distribution of the sperm whale in the Mediterranean Sea, unlike other regions of the world, the species population status is still presently uncertain. The analysis of two years of continuous acoustic data provided by the ANTARES neutrino telescope revealed the year-round presence of sperm whales in the Ligurian Sea, probably associated with the availability of cephalopods in the region. The presence of the Ligurian Sea sperm whales was demonstrated through the real-time analysis of audio data streamed from a cabled-to- shore deep-sea observatory that allowed the hourly tracking of their long-range echolocation behaviour on the Internet. Interestingly, the same acoustic analysis indicated that the occurrence of surface shipping noise would apparently not condition the foraging behaviour of the sperm whale in the area, since shipping noise was almost always present when sperm whales were acoustically detected. The continuous presence of the sperm whale in the region confirms the ecological value of the Ligurian sea and the importance of ANTARES to help monitoring its ecosystems, The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a lenergie atomique et aux energies alternatives (CEA), la Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cite (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur 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 Economia y Competitividad (MINECO), Prometeo and Grisolia programs of Generalitat Valenciana and MultiDark, Spain; Agence de l'Oriental and CNRST, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities
Published: 2017
Full Text: View/download PDF

17. Sperm whale long-range echolocation sounds revealed by ANTARES, a deep-sea neutrino telescope

Author: Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, Region Ile-de-France, Generalitat Valenciana, Université Sorbonne Paris Cité, Institut Universitaire de France, European Regional Development Fund, Instituto Nazionale di Fisica Nucleare, Conseil Régional Provence-Alpes-Côte d'Azur, Netherlands Organization for Scientific Research, Ministerio de Economía, Industria y Competitividad, Bundesministerium für Bildung und Forschung, Alemania, Centre National de la Recherche Scientifique, Francia, National Authority for Scientific Research, Rumanía, Council on grants of the President of the Russian Federation, Centre National pour la Recherche Scientifique et Technique, Marruecos, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, Andre, M., Caballé, A., Van der Schaar, M., Solsona, A., Houégnigan, L., Zaugg, S., Sanchez, A. M., Castell, J. V., Solé, M., Vila, F., Djokic, D., Adrián Martínez, Silvia, Albert, A., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Felis-Enguix, Iván, Martínez Mora, Juan Antonio, Saldaña-Coscollar, María, Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, Region Ile-de-France, Generalitat Valenciana, Université Sorbonne Paris Cité, Institut Universitaire de France, European Regional Development Fund, Instituto Nazionale di Fisica Nucleare, Conseil Régional Provence-Alpes-Côte d'Azur, Netherlands Organization for Scientific Research, Ministerio de Economía, Industria y Competitividad, Bundesministerium für Bildung und Forschung, Alemania, Centre National de la Recherche Scientifique, Francia, National Authority for Scientific Research, Rumanía, Council on grants of the President of the Russian Federation, Centre National pour la Recherche Scientifique et Technique, Marruecos, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, Andre, M., Caballé, A., Van der Schaar, M., Solsona, A., Houégnigan, L., Zaugg, S., Sanchez, A. M., Castell, J. V., Solé, M., Vila, F., Djokic, D., Adrián Martínez, Silvia, Albert, A., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Felis-Enguix, Iván, Martínez Mora, Juan Antonio, and Saldaña-Coscollar, María
Abstract: [EN] Despite dedicated research has been carried out to adequately map the distribution of the sperm whale in the Mediterranean Sea, unlike other regions of the world, the species population status is still presently uncertain. The analysis of two years of continuous acoustic data provided by the ANTARES neutrino telescope revealed the year-round presence of sperm whales in the Ligurian Sea, probably associated with the availability of cephalopods in the region. The presence of the Ligurian Sea sperm whales was demonstrated through the real-time analysis of audio data streamed from a cabled-to- shore deep-sea observatory that allowed the hourly tracking of their long-range echolocation behaviour on the Internet. Interestingly, the same acoustic analysis indicated that the occurrence of surface shipping noise would apparently not condition the foraging behaviour of the sperm whale in the area, since shipping noise was almost always present when sperm whales were acoustically detected. The continuous presence of the sperm whale in the region confirms the ecological value of the Ligurian sea and the importance of ANTARES to help monitoring its ecosystems
Published: 2017

18. All-sky Search for High-Energy Neutrinos from Gravitational Wave Event GW170104 with the ANTARES Neutrino Telescope

Author: Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, A*Midex Foundation, Agence Nationale de la Recherche, Francia, European Commission, Region Ile-de-France, Generalitat Valenciana, Conseil Régional d'Alsace, Université Sorbonne Paris Cité, Institut Universitaire de France, European Regional Development Fund, Instituto Nazionale di Fisica Nucleare, Ministerio de Economía y Competitividad, Conseil Régional Provence-Alpes-Côte d'Azur, Netherlands Organization for Scientific Research, Département du Var and Ville de La Seyne-sur-Mer, National Authority for Scientific Research, Rumanía, Bundesministerium für Bildung und Forschung, Alemania, Centre National de la Recherche Scientifique, Francia, Council on grants of the President of the Russian Federation, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, Laboratoire d'Excellence OCEVU (Origines, Constituants & ÉVolution de l'Univers), Ministère de l'Education Nationale, de la Formation professionnelle, de l'Enseignement Supérieur et de la Recherche Scientifique, Marruecos, Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Aubert , J.J., Avgitas, T., Baret, B., Barrios-Marti, J., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bormuth, R., Bourret, S., Felis-Enguix, Iván, Martínez Mora, Juan Antonio, Saldaña-Coscollar, María, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, A*Midex Foundation, Agence Nationale de la Recherche, Francia, European Commission, Region Ile-de-France, Generalitat Valenciana, Conseil Régional d'Alsace, Université Sorbonne Paris Cité, Institut Universitaire de France, European Regional Development Fund, Instituto Nazionale di Fisica Nucleare, Ministerio de Economía y Competitividad, Conseil Régional Provence-Alpes-Côte d'Azur, Netherlands Organization for Scientific Research, Département du Var and Ville de La Seyne-sur-Mer, National Authority for Scientific Research, Rumanía, Bundesministerium für Bildung und Forschung, Alemania, Centre National de la Recherche Scientifique, Francia, Council on grants of the President of the Russian Federation, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, Laboratoire d'Excellence OCEVU (Origines, Constituants & ÉVolution de l'Univers), Ministère de l'Education Nationale, de la Formation professionnelle, de l'Enseignement Supérieur et de la Recherche Scientifique, Marruecos, Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid Ramírez, Miguel, Aubert , J.J., Avgitas, T., Baret, B., Barrios-Marti, J., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bormuth, R., Bourret, S., Felis-Enguix, Iván, Martínez Mora, Juan Antonio, and Saldaña-Coscollar, María
Abstract: [EN] Advanced LIGO detected a significant gravitational wave signal (GW170104) originating from the coalescence of two black holes during the second observation run on January 4th, 2017. Anall-sky high-energy neutrino follow-up search has been made using data from the Antares neutrino telescope, including both upgoing and downgoing events in two separate analyses. No neutrino candidates were found within +/- 500 s around the GW event time nor any time clustering of events over an extended time window of +/- 3 months. The non-detection is used to constrain isotropic-equivalent high-energy neutrino emission from GW170104 to less than similar to 1.2 x 10(55) erg for a E-2 spectrum. This constraint is valid in the energy range corresponding to the 5-95% quantiles of the neutrino flux [3.2 TeV; 3.6 PeV], if the GW emitter was below the Antares horizon at the alert time.
Published: 2017

19. Results from the ANTARES Neutrino Telescope with Six Years of Data

Author: Maurizio Spurio, Antonio Capone, and Spurio M.
Subjects: Physics, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Cosmic ray, Astrophysics, Physics and Astronomy(all), Solar neutrino problem, neutrino astrophysics, Physics::Geophysics, Neutrino detector, cosmic rays, neutrino physics, Measurements of neutrino speed, neutrino astrophysic, High Energy Physics::Experiment, Neutrino, Neutrino astronomy, Neutrino oscillation, ANTARES neutrino telescope, cosmic ray
Abstract: The ANTARES neutrino telescope, completed in 2008, is the largest neutrino telescope in the Northern hemisphere. Located at a depth of 2.5 km in the Mediterranean Sea, 40 km off the Toulon shore, its main goal is the search for high energy neutrinos of astrophysical origin. In this paper we review the main physics results, ranging from searches for steady point sources and diffuse fluxes of neutrinos, to multi-messenger analyses and particle physics.
Published: 2015

20. A search for time dependent neutrino emission from microquasars with the ANTARES telescope

Author: C. Rivière, D. Elsässer, D. Lattuada, C. Racca, M. Saldaña, Oleg Kalekin, Z. Charif, G. De Rosa, P. Coyle, A. Gleixner, K. Geyer, Stephanie Escoffier, J-J. Aubert, F. Folger, Giorgio Riccobene, Thomas Eberl, Paolo Piattelli, J.D. Zornoza, S. Loucatos, Jörn Wilms, T. Pradier, A. Robert, B. Baret, Damien Dornic, Jos Steijger, R. Coniglione, Rainer Richter, Philippe Charvis, Daniele Vivolo, A. Mathieu, Yann Hello, M. Marcelin, D. Drouhin, Teresa Montaruli, Dominique Lefèvre, T. Seitz, Uli Katz, V. Kulikovskiy, Pasquale Migliozzi, Séverine Martini, L. A. Fusco, H. Loehner, E. A. De Wolf, R. Lahmann, J. Schmid, S. Schulte, A. Enzenhöfer, M. Neff, C. Vallée, J. P. Gómez-González, V. Giordano, B. Bouhou, Hugo Yepes, C. Perrina, E. Lambard, Tri L. Astraatmadja, Matthias Kadler, M. Anghinolfi, S. Galatà, C. Distefano, D. F. E. Samtleben, A. Creusot, M. Taiuti, Gisela Anton, S. Biagi, Q. Dorosti, Giuseppina Larosa, Th. Stolarczyk, Annarita Margiotta, P. Vernin, T. Michael, L. Core, S. Geißelsöder, U. Emanuele, A. Kouchner, P.M. Kooijman, Antonio Capone, S. Adrián-Martínez, Maurizio Spurio, V. Popa, A. Trovato, Marco Circella, Anne Deschamps, Ivan Dekeyser, Jose Busto, M. de Jong, J.-P. Ernenwein, K. Fehn, G.E. Păvălaş, Cornelia Müller, H. Costantini, Matteo Sanguineti, S. Mangano, Guillaume Lambard, S. Cecchini, Alexander Kappes, F. Schüssler, Yahya Tayalati, G. De Bonis, Juan José Hernández-Rey, H. van Haren, Ivan Felis, A. Heijboer, E. Visser, Miguel Ardid, L. Caramete, A. Rostovtsev, Arnauld Albert, J. Carr, Christian Tamburini, J. Zúñiga, Michel André, J. Hofestädt, J.A. Martínez-Mora, V. Bertin, C. Donzaud, B. Herold, K. Roensch, Tommaso Chiarusi, S. Basa, Stefan Wagner, Jutta Schnabel, A. Dumas, G. Guillard, Ciro Bigongiari, V. Van Elewyck, A. Sánchez-Losa, J. Barrios, Piera Sapienza, C. Cârloganu, C. W. James, B. Vallage, Jürgen Brunner, E. Leonora, C. Bogazzi, E. Nezri, K. Graf, K. Yatkin, Ingo Kreykenbohm, A. Spies, J. Hößl, M.C. Bouwhuis, C. Sieger, P. Fermani, D. Palioselitis, Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 7329), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Institut méditerranéen d'océanologie (MIO), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), ANTARES, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Sub Subatomic Physics (SAP), Subatomic Physics, Ecology and Biodiversity, Adrian-Martinez, S., Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid, M., Astraatmadja, T., Aubert, J. -J., Baret, B., Barrios, J., Basa, S., Bertin, V., Biagi, S., Bigongiari, C., Bogazzi, C., Bouhou, B., Bouwhuis, M. C., Brunner, J., Busto, J., Capone, A., Caramete, L., Carloganu, C., Carr, J., Cecchini, S., Charif, Z., Charvis, P., Chiarusi, T., Circella, M., Coniglione, R., Core, L., Costantini, H., Coyle, P., Creusot, A., De Rosa, G., Dekeyser, I., Deschamps, A., De Bonis, G., Distefano, C., Donzaud, C., Dornic, D., Dorosti, Q., Drouhin, D., Dumas, A., Eberl, T., Elsasser, D., Emanuele, U., Enzenhofer, A., Ernenwein, J. -P., Escoffier, S., Fehn, K., Felis, I., Fermani, P., Folger, F., Fusco, L. A., Galata, S., Gay, P., Geisselsoder, S., Geyer, K., Giordano, V., Gleixner, A., Gomez-Gonzalez, J. P., Graf, K., Guillard, G., van Haren, H., Heijboer, A. J., Hello, Y., Hernandez-Rey, J. J., Herold, B., Hossl, J., Hofestadt, J., James, C. W., de Jong, M., Kadler, M., Kalekin, O., Kappes, A., Katz, U., Kooijman, P., Kouchner, A., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Lambard, E., Lambard, G., Larosa, G., Lattuada, D., Lefevre, D., Leonora, E., Loehner, H., Loucatos, S., Mangano, S., Marcelin, M., Margiotta, A., Martinez-Mora, J. A., Martini, S., Mathieu, A., Michael, T., Migliozzi, P., Montaruli, T., Muller, C., Neff, M., Nezri, E., Palioselitis, D., Pavalas, G. E., Perrina, C., Piattelli, P., Popa, V., Pradier, T., Racca, C., Riccobene, G., Richter, R., Riviere, C., Robert, A., Roensch, K., Rostovtsev, A., Saldana, M., Samtleben, D. F. E., Sanchez-Losa, A., Sanguineti, M., Sapienza, P., Schmid, J., Schnabel, J., Schulte, S., Schussler, F., Seitz, T., Sieger, C., Spies, A., Spurio, M., Steijger, J. J. M., Stolarczyk, T., Taiuti, M., Tamburini, C., Tayalati, Y., Trovato, A., Vallage, B., Vallee, C., Van Elewyck, V., Vernin, P., Visser, E., Vivolo, D., Wagner, S., Wilms, J., de Wolf, E., Yatkin, K., Yepes, H., Zornoza, J. D., Zuniga, J., Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), S. Adrián-Martínez, A. Albert, M. André, M. Anghinolfi, G. Anton, M. Ardid, T. Astraatmadja, J.-J. Aubert, B. Baret, J. Barrio, S. Basa, V. Bertin, S. Biagi, C. Bigongiari, C. Bogazzi, B. Bouhou, M.C. Bouwhui, J. Brunner, J. Busto, A. Capone, L. Caramete, C. Cârloganu, J. Carr, S. Cecchini, Z. Charif, P. Charvi, T. Chiarusi, M. Circella, R. Coniglione, L. Core, H. Costantini, P. Coyle, A. Creusot, G. De Rosa, I. Dekeyser, A. Deschamp, G. De Boni, C. Distefano, C. Donzaud, D. Dornic, Q. Dorosti, D. Drouhin, A. Duma, T. Eberl, D. Elsässer, U. Emanuele, A. Enzenhöfer, J.-P. Ernenwein, S. Escoffier, K. Fehn, I. Feli, P. Fermani, F. Folger, L.A. Fusco, S. Galatà, P. Gay, S. Geißelsöder, K. Geyer, V. Giordano, A. Gleixner, J.P. Gómez-González, K. Graf, G. Guillard, H. van Haren, A.J. Heijboer, Y. Hello, J.J. Hernández-Rey, B. Herold, J. Hößl, J. Hofestädt, C.W. Jame, M. de Jong, M. Kadler, O. Kalekin, A. Kappe, U. Katz, P. Kooijman, A. Kouchner, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, E. Lambard, G. Lambard, G. Larosa, D. Lattuada, D. Lefèvre, E. Leonora, H. Loehner, S. Loucato, S. Mangano, M. Marcelin, A. Margiotta, J.A. Martínez-Mora, S. Martini, A. Mathieu, T. Michael, P. Migliozzi, T. Montaruli, C. Müller, M. Neff, E. Nezri, D. Palioseliti, G.E. Păvălaş, C. Perrina, P. Piattelli, V. Popa, T. Pradier, C. Racca, G. Riccobene, R. Richter, C. Rivière, A. Robert, K. Roensch, A. Rostovtsev, M. Saldaña, D.F.E. Samtleben, A. Sánchez-Losa, M. Sanguineti, P. Sapienza, J. Schmid, J. Schnabel, S. Schulte, F. Schüssler, T. Seitz, C. Sieger, A. Spie, M. Spurio, J.J.M. Steijger, T. Stolarczyk, M. Taiuti, C. Tamburini, Y. Tayalati, A. Trovato, B. Vallage, C. Vallée, V. Van Elewyck, P. Vernin, E. Visser, D. Vivolo, S. Wagner, J. Wilm, E. de Wolf, K. Yatkin, H. Yepe, J.D. Zornoza, J. Zúñiga, DE ROSA, Gianfranca, Vivolo, Daniele, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), and Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN)-Aix Marseille Université (AMU)-Institut de Recherche pour le Développement (IRD)
Subjects: Nuclear and High Energy Physics, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, 01 natural sciences, 7. Clean energy, Luminosity, law.invention, Telescope, neutrino, Astrophysical jet, law, Microquasars, 0103 physical sciences, microquasar, Neutrinos, 010303 astronomy & astrophysics, Astroparticle physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy, Física, Astronomy and Astrophysics, Solar neutrino problem, Neutrino detector, Space and Planetary Science, FISICA APLICADA, High Energy Physics::Experiment, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, ANTARES neutrino telescope, Fermi Gamma-ray Space Telescope
Abstract: [EN] Results are presented on a search for neutrino emission from a sample of six microquasars, based on the data collected by the ANTARES neutrino telescope between 2007 and 2010. By means of appropriate time cuts, the neutrino search has been restricted to the periods when the acceleration of relativistic jets was taking place at the microquasars under study. The time cuts have been chosen using the information from the X-ray telescopes RXTE/ASM and Swift/BAT, and, in one case, the gamma-ray telescope Fermi/LAT. No statistically significant excess has been observed, thus upper limits on the neutrino fluences have been derived and compared to the predictions by models. Constraints have been put on the ratio of proton to electron luminosity in the jets., 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 Nationale de la Recherche (ANR), Commission Européenne (FEDER fund and Marie Curie Program), Région Alsace (contract 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; Agence de l’Oriental and CNRST, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.
Published: 2014
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21. A search for neutrino emission from the Fermi bubbles with the ANTARES telescope

Author: The Antares Collaboration, Adrian Martinez, S., Albert, A., Al Samarai, I., Andre, M., Anghinolfi, M., Anton, G., Anvar, S., Ardid, M., Astraatmadja, T., Aubert, J. J., Baret, B., Barrios Marti, J., Basa, S., Bertin, V., Biagi, S., Bigongiari, C., Bogazzi, C., Bouhou, B., Bouwhuis, M. C., Brunner, J., Busto, J., Capone, Antonio, Caramete, L., Carloganu, C., Carr, J., Cecchini, S., Charif, Z., Charvis, Ph, Chiarusi, T., Circella, M., Classen, F., Coniglione, R., Core, L., Costantini, H., Coyle, P., Creusot, A., Curtil, C., DE BONIS, Giulia, Dekeyser, I., Deschamps, A., Decowski, M. P., Distefano, C., Donzaud, C., Dornic, D., Dorosti, Q., Drouhin, D., Dumas, A., Eberl, T., Emanuele, U., Enzenhofer, A., Ernenwein, J. P., Escoffier, S., Fehn, K., Fermani, Paolo, Ferry, S., Flaminio, V., Folger, F., Fritsch, U., Fuda, J. L., Fusco, L. A., Galata, S., Gay, P., Geisselsoder, S., Geyer, K., Giacomelli, G., Giordano, V., Gleixner, A., Gomez Gonzalez, J. P., Graf, K., Guillard, G., Hallewell, G., Hamal, M., Van Haren, H., Heijboer, A. J., Hello, Y., Hernandez Rey, J. J., Herold, B., Hossl, J., Hsu, C. C., Hugon, C., James, C. W., De Jong, M., Kadler, M., Kalekin, O., Kappes, A., Katz, U., Kooijman, P., Kopper, C., Kouchner, A., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Lambard, E., Lambard, G., Larosa, G., Lattuada, D., Lefevre, D., Leonora, E., Lo Presti, D., Loehner, H., Loucatos, S., Louis, F., Mangano, S., Marcelin, M., Margiotta, A., Martinez Mora, J. A., Martini, S., Michael, T., Montaruli, T., Morganti, M., Motz, H., Muller, C., Neff, M., Nezri, E., Palioselitis, D., Pavalas, G. E., Perrina, Chiara, Petrovic, J., Piattelli, P., Popa, V., Pradier, T., Racca, C., Reed, C., Riccobene, G., Richter, R., Riviere, C., Robert, A., Roensch, K., Rostovtsev, A., Rujoiu, M., Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schmid, J., Schnabel, J., Schulte, S., Schussler, F., Seitz, T., Shanidze, R., Sieger, C., Simeone, Francesco, Spies, A., Spurio, M., Steijger, J. J. M., Stolarczyk, Th, Sanchez Losa, A., Taiuti, M., Tamburini, C., Tayalati, Y., Trovato, A., Vallage, B., Vallee, C., Van Elewyck, V., Vecchi, M., Vernin, P., Visser, E., Wagner, S., Wijnker, G., Wilms, J., De Wolf, E., Yatkin, K., Yepes, H., Zaborov, D., Zornoza, J. D., Zuniga, J., ANTARES (IHEF, IoP, FNWI), Adrian-Martinez, S, Albert, A, Al Samarai, I, Andre, M, Anton, G, Anvar, S, Ardid, M, Astraatmadja, T, Aubert, Jj, Baret, B, Barrios-Marti, J, Basa, S, Bertin, V, Biagi, S, Bigongiari, C, Bogazzi, C, Bouhou, B, Bouwhuis, M, Brunner, J, Busto, J, Capone, A, Caramete, L, Carloganu, C, Carr, J, Cecchini, S, Charif, Z, Charvis, P, Chiarusi, T, Circella, M, Classen, F, Coniglione, R, Core, L, Costantini, H, Coyle, P, Creusot, A, Curtil, C, De Bonis, G, Dekeyser, I, Deschamps, A, Donzaud, C, Dornic, D, Dorosti, Q, Drouhin, D, Dumas, A, Eberl, T, Emanuele, U, Enzenhofer, A, Ernenwein, Jp, Escoffier, S, Fehn, K, Fermani, P, Flaminio, V, Folger, F, Fritsch, U, Fusco, L, Galata, S, Gay, P, Geisselsoder, S, Geyer, K, Giacomelli, G, Giordano, V, Gleixner, A, Gomez-Gonzalez, Jp, Graf, K, Guillard, G, van Haren, H, Heijboer, A, Hello, Y, Hernandez-Rey, J, Herold, B, Hossl, J, Hugon, C, James, C, de Jong, M, Kadler, M, Kalekin, O, Kappes, A, Katz, U, Kooijman, P, Kouchner, A, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Lambard, E, Lambard, G, Larosa, G, Lattuada, D, Lefevre, D, Leonora, E, Lo Presti, D, Loehner, H, Loucatos, S, Louis, F, Mangano, S, Marcelin, M, Margiotta, A, Martinez-Mora, J, Martini, S, Michael, T, Montaruli, T, Morganti, M, Muller, C, Neff, M, Nezri, E, Palioselitis, D, Pavalas, Ge, Perrina, C, Popa, V, Pradier, T, Racca, C, Riccobene, G, Richter, R, Riviere, C, Robert, A, Roensch, K, Rostovtsev, A, Samtleben, D, Sanguineti, M, Sapienza, P, Schmid, J, Schnabel, J, Schulte, S, Schussler, F, Seitz, T, Shanidze, R, Sieger, C, Simeone, F, Spies, A, Spurio, M, Steijger, J, Stolarczyk, T, Sanchez-Losa, A, Taiuti, M, Tamburini, C, Tayalati, Y, Trovato, A, Vallage, B, Vallee, C, Van Elewyck, V, Vecchi, M, Vernin, P, Visser, E, Wagner, S, Wilms, J, de Wolf, E, Yatkin, K, Yepes, H, Zornoza, J, Zuniga, J, Montaruli, Teresa, S. Adrián-Martínez, A. Albert, I. Al Samarai, M. André, G. Anton, S. Anvar, M. Ardid, T. Astraatmadja, J.-J. Aubert, B. Baret, J. Barrios-Martí, S. Basa, V. Bertin, S. Biagi, C. Bigongiari, C. Bogazzi, B. Bouhou, M. C. Bouwhui, J. Brunner, J. Busto, A. Capone, L. Caramete, C. Cârloganu, J. Carr, S. Cecchini, Z. Charif, Ph. Charvi, T. Chiarusi, M. Circella, F. Classen, R. Coniglione, L. Core, H. Costantini, P. Coyle, A. Creusot, C. Curtil, G. Boni, I. Dekeyser, A. Deschamp, C. Donzaud, D. Dornic, Q. Dorosti, D. Drouhin, A. Duma, T. Eberl, U. Emanuele, A. Enzenhöfer, J.-P. Ernenwein, S. Escoffier, K. Fehn, P. Fermani, V. Flaminio, F. Folger, U. Fritsch, L. A. Fusco, S. Galatà, P. Gay, S. Geißelsöder, K. Geyer, G. Giacomelli, V. Giordano, A. Gleixner, J. P. Gómez-González, K. Graf, G. Guillard, H. Haren, A. J. Heijboer, Y. Hello, J. J. Hernández-Rey, B. Herold, J. Hößl, C. Hugon, C. W. Jame, M. Jong, M. Kadler, O. Kalekin, A. Kappe, U. Katz, P. Kooijman, A. Kouchner, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, E. Lambard, G. Lambard, G. Larosa, D. Lattuada, D. Lefèvre, E. Leonora, D. Lo Presti, H. Loehner, S. Loucato, F. Loui, S. Mangano, M. Marcelin, A. Margiotta, J. A. Martínez-Mora, S. Martini, T. Michael, T. Montaruli, M. Morganti, C. Müller, M. Neff, E. Nezri, D. Palioseliti, G. E. Păvălaş, C. Perrina, V. Popa, T. Pradier, C. Racca, G. Riccobene, R. Richter, C. Rivière, A. Robert, K. Roensch, A. Rostovtsev, D. F. E. Samtleben, M. Sanguineti, P. Sapienza, J. Schmid, J. Schnabel, S. Schulte, F. Schüssler, T. Seitz, R. Shanidze, C. Sieger, F. Simeone, A. Spie, M. Spurio, J. J. M. Steijger, Th. Stolarczyk, A. Sánchez-Losa, M. Taiuti, C. Tamburini, Y. Tayalati, A. Trovato, B. Vallage, C. Vallée, V. Elewyck, M. Vecchi, P. Vernin, E. Visser, S. Wagner, J. Wilm, E. Wolf, K. Yatkin, H. Yepe, J. D. Zornoza, J. Zúñiga, Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 7329), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Université Paris-Sud - Paris 11 (UP11), Département de Physique des Particules (ex SPP) (DPhP), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ANTARES, SCOAP, Research unit Nuclear & Hadron Physics, Centre Tecnològic de Vilanova i la Geltrú, Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Département de Physique des Particules (ex SPP) (DPP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Astrofísica, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Physics and Astronomy (miscellaneous), Physics::Instrumentation and Detectors, Ray, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, antares, Astrophysics, ddc:500.2, Neutrino fluxes, Gamma ray bursts, Partícules (Física nuclear), law.invention, Telescope, neutrino, Raigs gamma, law, 14. Life underwater, Neutrins, Neutrinos, Engineering (miscellaneous), Cherenkov radiation, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, COSMIC cancer database, Muon, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], High Energy Physics::Phenomenology, Astrophysics::Instrumentation and Methods for Astrophysics, Gamma ray, fermi bubbles, Detector, Charged particle, Neutrino astrophysics, Fermi bubble, neutrino telecope, 13. Climate action, Fermi bubbles, Col·lisions (Física nuclear), Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], FISICA APLICADA, Física nuclear, High Energy Physics::Experiment, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Antares neutrino telescope, Fermi Gamma-ray Space Telescope
Abstract: Adrián-Martínez, S. et al., Analysis of the Fermi-LAT data has revealed two extended structures above and below the Galactic Centre emitting gamma rays with a hard spectrum, the so-called Fermi bubbles. Hadronic models attempting to explain the origin of the Fermi bubbles predict the emission of high-energy neutrinos and gamma rays with similar fluxes. The ANTARES detector, a neutrino telescope located in the Mediterranean Sea, has a good visibility to the Fermi bubble regions. Using data collected from 2008 to 2011 no statistically significant excess of events is observed and therefore upper limits on the neutrino flux in TeV range from the Fermi bubbles are derived for various assumed energy cutoffs of the source., The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat á 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; Ministerio de Ciencia e Innovación (MICINN), Prometeo of Generalitat Valenciana and MultiDark, Spain; Agence de l’Oriental, Morocco; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), The Netherlands;NationalAuthority for Scientific Research (ANCS-UEFISCDI), Romania; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia. Technical support of Ifremer, AIM and Foselev Marine for the sea operat.
Published: 2014
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22. Starlight beneath the waves: In search of TeV photon emission from Gamma-Ray Bursts with the ANTARES Neutrino Telescope

Author: Astraatmadja, Tri L. and de Jong, Maarten
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, gamma-ray burst, very-high-energy gamma-ray, High Energy Physics::Experiment, Astrophysics::Cosmology and Extragalactic Astrophysics, antares neutrino telescope, high-energy astrophysics
Abstract: At any given time, cosmic rays constantly shower the Earth from all direction. The origin of cosmic rays is still a mystery as their paths are deflected by magnetic fields to random directions. The most likely sources of cosmic rays are Gamma-Ray Bursts (GRB). As the most energetic events known in the universe, GRBs are the death throes of massive stars that end in the explosion of stellar materials into interstellar matters. The interactions between cosmic rays and materials surrounding the GRB can produce neutrinos and very-high energy gamma-rays. Studying these high-energy neutrinos and gamma-rays can enlighten us further on the origin of cosmic rays. Very-high energy gamma rays can be observed by very large volume neutrino telescopes such as ANTARES in the Mediterranean Sea and IceCube in the South Pole. This dissertation focuses on ANTARES telescope operated as a gamma-ray telescope, which is possible by searching for downgoing muons produced from the interaction of gamma-rays with the Earth's atmosphere. Analytical calculations necessary to estimate the rate of photon-induced muons from GRBs has been performed. The responses of the detector to downgoing muons have been understood by using Monte Carlo simulations. The findings also provide a discussion on the future prospect of this venture.
Published: 2013
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23. Deep-Sea Bioluminescence Blooms after Dense Water Formation at the Ocean Surface

Author: LO PRESTI, Domenico, Christian, Tamburini, Canals, M, Durrieu de Madron, X, Houpert, L, Lefe`vre, D, Se´verine, Martini1, 2, Fabrizio, D’Ortenzio5, Anne, Robert1, Pierre, Testor6, Juan Antonio Aguilar7, Imen Al Samarai8, Arnaud, Albert9, Michel Andre´ 10, Marco, Anghinolfi11, Gisela, Anton12, Shebli, Anvar13, Miguel, Ardid14, Ana Carolina Assis Jesus15, Astraatmadja15¤a, Tri L., Jean Jacques Aubert8, Bruny, Baret16, Ste´phane, Basa17, Vincent, Bertin8, Simone, Biagi18, Armando, Bigi20, Ciro, Bigongiari7, Claudio, Bogazzi15, Manuel Bou Cabo14, Boutayeb, Bouhou16, Bouwhuis15, Mieke C., Jurgen, Brunner8¤b, Jose´, Busto8, Francisco, Camarena14, Antonio, Capone21, Christina, Caˆrloganu23, Giada, Carminati18, 19¤c, John, Carr8, Stefano, Cecchini18, Ziad, Charif8, Philippe, Charvis25, Tommaso, Chiarusi18, Marco, Circella26, Rosa, Coniglione27, Heide, Costantini8, Paschal, Coyle8, Christian, Curtil8, Patrick, Decowski15, Ivan, Dekeyser1, Anne, Deschamps25, Corinne, Donzaud16, Damien, Dornic7, 8, Dorosti29, Hasankiadeh Q., Doriane, Drouhin9, Thomas, Eberl12, Umberto, Emanuele7, Jean Pierre Ernenwein8, Ste´phanie, Escoffier8, Paolo, Fermani21, Marcelino, Ferri14, Vincenzo, Flaminio20, Florian, Folger12, Ulf, Fritsch12, Jean Luc Fuda1, 2¤d, Salvatore Galata`, 8, Pascal, Gay23, Giorgio, Giacomelli18, Valentina, Giordano27, Juan Pablo Go´mez Gonza´ lez7, Kay, Graf12, Goulven, Guillard23, Garadeb, Halladjian8, Gregory, Hallewell8, Hans van Haren31, Joris, Hartman15, Heijboer15, Aart J., Yann, Hello25, Juan Jose Herna´ndez Rey7, Bjoern, Herold12, Jurgen Ho¨ ßl12, Ching Cheng Hsu15, Marteen de Jong15¤a, Matthias, Kadler32, Oleg, Kalekin12, Alexander, Kappes12, Uli, Katz12, Oksana, Kavatsyuk29, Paul, Kooijman15, 34, 33, Claudio, Kopper12, Antoine, Kouchner16, Ingo Kreykenbohm 32, Vladimir, Kulikovskiy11, Robert, Lahmann12, Patrick, Lamare13, Giuseppina, Larosa14, Dario, Lattuada27, Gordon, Lim15, Domenico Lo Presti36, Herbert, Loehner29, Sotiris, Loucatos38, Salvatore, Mangano7, Michel, Marcelin17, Annarita, Margiotta18, Juan Antonio Martinez Mora14, Athina, Meli12, Teresa, Montaruli26, Luciano, Moscoso16, 38{, Holger, Motz12, Max, Neff12, Emma nuel Nezri17, Dimitris, Palioselitis15, Pa˘va˘ las¸40, Gabriela E., Kevin, Payet38, Patrice, Payre8, Jelena, Petrovic15, Paolo, Piattelli27, Nicolas Picot Clemente8, Vlad, Popa40, Thierry, Pradier41, Eleonora, Presani15, Chantal, Racca9, Corey, Reed15, Giorgio, Riccobene27, Carsten, Richardt12, Roland, Richter12, Colas Rivie` re8, Kathrin, Roensch12, Andrei, Rostovtsev42, Joaquin Ruiz Rivas7, Marius, Rujoiu40, Russo36, Valerio G., Francisco, Salesa7, Augustin Sa´nchez Losa7, Piera, Sapienza27, Friederike Scho¨ ck12, Jean Pierre Schuller38, Fabian, Schussler38, Rezo, Shanidze12, Francesco, Simeone21, Andreas, Spies12, Maurizio, Spurio18, Steijger15, Jos J. M., Thierry, Stolarczyk38, Taiuti11, Mauro G. F., Simona, Toscano7, Bertrand, Vallage38, Ve´ronique Van Elewyck16, Giulia, Vannoni38, Manuela, Vecchi8, Pascal, Vernin38, Guus, Wijnker15, Jorn, Wilms32, Els de Wolf15, Harold, Yepes7, Dmitry, Zaborov42, Juan De Dios Zornoza7, Juan Zu´ n˜ iga7, Institut méditerranéen d'océanologie (MIO), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Centre de Formation et de Recherche sur les Environnements Méditérranéens (CEFREM), Université de Perpignan Via Domitia (UPVD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'océanographie de Villefranche (LOV), Observatoire océanologique de Villefranche-sur-mer (OOVM), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Couplage physique-biogéochimie-carbone (PHYBIOCAR), Laboratoire d'Océanographie et du Climat : Expérimentations et Approches Numériques (LOCEAN), Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Variabilité de l'Océan et de la Glace de mer (VOG), Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 7329), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Istituto Nazionale di Fisica Nucleare, Sezione di Catania (INFN), Università degli studi di Catania = University of Catania (Unict), Royal Netherlands Institute for Sea Research (NIOZ), Laboratori Nazionali del Sud (LNS), Istituto Nazionale di Fisica Nucleare (INFN), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ANTARES, ANR-05-BLAN-0161,POTES,Pressure effects On marine prokaryoTES(2005), European Project: 202955,EC:FP7:ENV,FP7-ENV-2007-1,EUROSITES(2008), Université de Perpignan Via Domitia (UPVD)-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut de la Mer de Villefranche (IMEV), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Muséum national d'Histoire naturelle (MNHN)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Muséum national d'Histoire naturelle (MNHN)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), Institut Pierre-Simon-Laplace (IPSL (FR_636)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Institut de Recherche pour le Développement (IRD)-Muséum national d'Histoire naturelle (MNHN)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Institut de Recherche pour le Développement (IRD)-Muséum national d'Histoire naturelle (MNHN)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Università degli studi di Catania [Catania], Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), KVI - Center for Advanced Radiation Technology, John Murray Robert, Christian Tamburini, Miquel Canal, Xavier Durrieu de Madron, Loïc Houpert, Dominique Lefèvre, Séverine Martini, Fabrizio D'Ortenzio, Anne Robert, Pierre Testor, Juan Antonio Aguilar, Imen Al Samarai, Arnaud Albert, Michel André, Marco Anghinolfi, Gisela Anton, Shebli Anvar, Miguel Ardid, Ana Carolina Assis Jesu, Tri L. Astraatmadja, Jean-Jacques Aubert, Bruny Baret, Stéphane Basa, Vincent Bertin, Simone Biagi, Armando Bigi, Ciro Bigongiari, Claudio Bogazzi, Manuel Bou-Cabo, Boutayeb Bouhou, Mieke C. Bouwhui, Jurgen Brunner, José Busto, Francisco Camarena, Antonio Capone, Christina Cârloganu, Giada Carminati, John Carr, Stefano Cecchini, Ziad Charif, Philippe Charvi, Tommaso Chiarusi, Marco Circella, Rosa Coniglione, Heide Costantini, Paschal Coyle, Christian Curtil, Patrick Decowski, Ivan Dekeyser, Anne Deschamp, Corinne Donzaud, Damien Dornic, Hasankiadeh Q. Dorosti, Doriane Drouhin, Thomas Eberl, Umberto Emanuele, Jean-Pierre Ernenwein, Stéphanie Escoffier, Paolo Fermani, Marcelino Ferri, Vincenzo Flaminio, Florian Folger, Ulf Fritsch, Jean-Luc Fuda, Salvatore Galatà, Pascal Gay, Giorgio Giacomelli, Valentina Giordano, Juan-Pablo Gómez-González, Kay Graf, Goulven Guillard, Garadeb Halladjian, Gregory Hallewell, Hans van Haren, Joris Hartman, Aart J. Heijboer, Yann Hello, Juan Jose Hernández-Rey, Bjoern Herold, Jurgen Hößl, Ching-Cheng Hsu, Marteen de Jong, Matthias Kadler, Oleg Kalekin, Alexander Kappe, Uli Katz, Oksana Kavatsyuk, Paul Kooijman, Claudio Kopper, Antoine Kouchner, Ingo Kreykenbohm, Vladimir Kulikovskiy, Robert Lahmann, Patrick Lamare, Giuseppina Larosa, Dario Lattuada, Gordon Lim, Domenico Lo Presti, Herbert Loehner, Sotiris Loucato, Salvatore Mangano, Michel Marcelin, Annarita Margiotta, Juan Antonio Martinez-Mora, Athina Meli, Teresa Montaruli, Luciano Moscoso, Holger Motz, Max Neff, Emma nuel Nezri, Dimitris Palioseliti, Gabriela E. Păvălaş, Kevin Payet, Patrice Payre, Jelena Petrovic, Paolo Piattelli, Nicolas Picot-Clemente, Vlad Popa, Thierry Pradier, Eleonora Presani, Chantal Racca, Corey Reed, Giorgio Riccobene, Carsten Richardt, Roland Richter, Colas Rivière, Kathrin Roensch, Andrei Rostovtsev, Joaquin Ruiz-Riva, Marius Rujoiu, Valerio G. Russo, Francisco Salesa, Augustin Sánchez-Losa, Piera Sapienza, Friederike Schöck, Jean-Pierre Schuller, Fabian Schussler, Rezo Shanidze, Francesco Simeone, Andreas Spie, Maurizio Spurio, Jos J. M. Steijger, Thierry Stolarczyk, Mauro G. F. Taiuti, Simona Toscano, Bertrand Vallage, Véronique Van Elewyck, Giulia Vannoni, Manuela Vecchi, Pascal Vernin, Guus Wijnker, Jorn Wilm, Els de Wolf, Harold Yepe, Dmitry Zaborov, Juan De Dios Zornoza, Juan Zúñiga, Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN)-Aix Marseille Université (AMU)-Institut de Recherche pour le Développement (IRD), Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Muséum national d'Histoire naturelle (MNHN), Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), National Institute for Nuclear Physics (INFN), Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA), ANR-05-BLAN-0161,POTES,Projet POTES - Pressure effects On marine prokaryoTES(2005), Universitat de Barcelona, Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre Tecnològic de Vilanova i la Geltrú, and Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
Subjects: Desenvolupament humà i sostenible::Medi ambient [Àrees temàtiques de la UPC], 0106 biological sciences, DYNAMICS, Salinity, ANTARES NEUTRINO TELESCOPE, 010504 meteorology & atmospheric sciences, Naturwissenschaftliche Fakultät -ohne weitere Spezifikation, IMPACT, Ocean Circulation, Psychologie appliquée, lcsh:Medicine, Cell Count, Astronomical Sciences, Oceanografia, Astrophysics, Oceanography, Ecologia marina, 01 natural sciences, Bathyal zone, NEUTRINO TELESCOPES, Mediterranean sea, Oceans, lcsh:Science, deep-sea bioluminescenceantares, Ecosistemes marins, Multidisciplinary, CLIMATE-CHANGE, Ecology, Mediterrània (Mar), Mediterranean Region, Marine Ecology, MEDITERRANEAN SEA, Eutrophication, Biogeochemistry, Sciences bio-médicales et agricoles, Deep sea, INTERANNUAL VARIABILITY, Light emission, Seasons, ddc:500, Bioluminescence, Biologie, Research Article, ATLANTIC, GULF, Oceans and Seas, [PHYS.PHYS.PHYS-BIO-PH]Physics [physics]/Physics [physics]/Biological Physics [physics.bio-ph], Marine Biology, Convection, Fluorescence, Microbial Ecology, Carbon Cycle, Marine ecology, Astroparticle Physics, Mediterranean Sea, Animals, Water Column, Ecosystem, Seawater, 14. Life underwater, Salinitat, Neutrinos, Biology, [SDU.STU.OC]Sciences of the Universe [physics]/Earth Sciences/Oceanography, 0105 earth and related environmental sciences, Marine plankton, BACKGROUND LIGHT, 010604 marine biology & hydrobiology, Biological Oceanography, lcsh:R, Plàncton, Pelagic zone, Marine and aquatic sciences, Earth sciences, Light intensity, Sea water, Geochemistry, 13. Climate action, CONVECTION, FISICA APLICADA, Luminescent Measurements, Aigua de mar, Environmental science, lcsh:Q, Physical Oceanography
Abstract: The deep ocean is the largest and least known ecosystem on Earth. It hosts numerous pelagic organisms, most of which are able to emit light. Here we present a unique data set consisting of a 2.5-year long record of light emission by deep-sea pelagic organisms, measured from December 2007 to June 2010 at the ANTARES underwater neutrino telescope in the deep NW Mediterranean Sea, jointly with synchronous hydrological records. This is the longest continuous time-series of deep-sea bioluminescence ever recorded. Our record reveals several weeks long, seasonal bioluminescence blooms with light intensity up to two orders of magnitude higher than background values, which correlate to changes in the properties of deep waters. Such changes are triggered by the winter cooling and evaporation experienced by the upper ocean layer in the Gulf of Lion that leads to the formation and subsequent sinking of dense water through a process known as "open-sea convection". It episodically renews the deep water of the study area and conveys fresh organic matter that fuels the deep ecosystems. Luminous bacteria most likely are the main contributors to the observed deep-sea bioluminescence blooms. Our observations demonstrate a consistent and rapid connection between deep open-sea convection and bathypelagic biological activity, as expressed by bioluminescence. In a setting where dense water formation events are likely to decline under global warming scenarios enhancing ocean stratification, in situ observatories become essential as environmental sentinels for the monitoring and understanding of deep-sea ecosystem shifts. © 2013 Tamburini et al., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2013
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24. The positioning system of the ANTARES Neutrino Telescope

Author: Adrian Martinez, S., Ageron, M., Aguilar, J. a., Al Samarai, I., Albert, A., Andre, 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., Bouhou, B., Bouwhuis, M. c., Brunner, J., Busto, J., Camarena, F., Capone, Antonio, Carloganu, C., Carminati, G., Carr, J., Cecchini, S., Charif, Z., Charvis, Ph, Chiarusi, T., Circella, M., Coniglione, R., Costantini, H., Coyle, P., Curtil, C., DE BONIS, Giulia, Decowski, M. p., Dekeyser, I., Deschamps, A., Distefano, C., Donzaud, C., Dornic, D., Dorosti, Q., Drouhin, D., Eberl, T., Emanuele, U., Enzenhofer, A., Ernenwein, J. P., Escoffier, S., Fermani, Paolo, Ferri, M., Flaminio, V., Folger, F., Fritsch, U., Fuda, J. L., Galata, S., Gay, P., Giacomelli, G., Giordano, V., Gomez Gonzalez, J. p., Graf, K., Guillard, G., Halladjian, G., Hallewell, G., Van Haren, H., Hartman, J., Heijboer, A. j., Hello, Y., Hernandez Rey, J. j., Herold, B., Hol, J., Hossl, J., Hsu, C. c., De Jong, M., Kadler, M., Kalekin, O., Kappes, A., Katz, U., Kavatsyuk, O., Keller, P., Kooijman, P., Kopper, C., Kouchner, A., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Lamare, P., Larosa, G., Lattuada, D., Lefevre, D., Le Van Suu, A., Lim, G., Lo Presti, D., Loehner, H., Loucatos, S., Mangano, S., Marcelin, M., Margiotta, A., Martinez Mora, J. a., Meli, A., Montaruli, T., Moscoso, L., Motz, H., Neff, M., Nezri, E., Niess, V., Palioselitis, D., Pavalas, G. e., Payet, K., Payre, P., Petrovic, J., Piattelli, P., Picot Clemente, N., Popa, V., Pradier, T., Presani, E., Racca, C., Real, D., Reed, C., Riccobene, G., Richardt, C., Richter, R., Riviere, C., Robert, A., Roensch, K., Rostovtsev, A., Ruiz Rivas, J., Rujoiu, M., Russo, G. v., Salesa, F., Samtleben, D. f. e., Schock, F., Schuller, J. P., Schussler, F., Seitz, T., Shanidze, R., Simeone, Francesco, Spies, A., Spurio, M., Steijger, J. j. m., Stolarczyk, Th, Sanchez Losa, A., Taiuti, M., Tamburini, C., Toscano, S., Vallage, B., Van Elewyck, V., Vannoni, G., Vecchi, M., Vernin, P., Wagner, S., Wijnker, G., Wilms, J., De Wolf, E., Yepes, H., Zaborov, D., Zornoza, J. d., Zuniga, J., Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Département d'Electronique, des Détecteurs et d'Informatique pour la Physique (ex SEDI) (DEDIP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'océanologie de Marseille (COM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de la Méditerranée - Aix-Marseille 2, Université Paris-Sud - Paris 11 (UP11), Département de Physique des Particules (ex SPP) (DPP), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ANTARES, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Département d'Electronique, des Détecteurs et d'Informatique (ex SEDI) (DEDI), APC - Astrophysique des Hautes Energies (APC - AHE), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), KVI - Center for Advanced Radiation Technology, Montaruli, Teresa, S Adrián-Martínez, M Ageron, J A Aguilar, I Al Samarai, A Albert, M André, M Anghinolfi, G Anton, S Anvar, M Ardid, A C Assis Jesu, 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 Bouwhui, J Brunner, J Busto, F Camarena, A Capone, C Cârloganu, G Carminati, J Carr, S Cecchini, Z Charif, Ph Charvi, T Chiarusi, M Circella, R Coniglione, H Costantini, P Coyle, C Curtil, G De Boni, M P Decowski, I Dekeyser, A Deschamp, 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 Kappe, U Katz, O Kavatsyuk, P Keller, P Kooijman, C Kopper, A Kouchner, I Kreykenbohm, V Kulikovskiy, R Lahmann, P Lamare, G Larosa, D Lattuada, D Lefèvre, A Le Van Suu, G Lim, D Lo Presti, H Loehner, S Loucato, S Mangano, M Marcelin, A Margiotta, J A Martínez-Mora, A Meli, T Montaruli, L Moscoso, H Motz, M Neff, E Nezri, V Nie, D Palioseliti, G E Păvălaş, K Payet, P Payre, J Petrovic, P Piattelli, N Picot-Clemente, V Popa, T Pradier, E Presani, C Racca, D Real, C Reed, G Riccobene, C Richardt, R Richter, C Rivière, A Robert, K Roensch, A Rostovtsev, J Ruiz-Riva, M Rujoiu, G V Russo, F Salesa, D F E Samtleben, F Schöck, J -P Schuller, F Schüssler, T Seitz, R Shanidze, F Simeone, A Spie, 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, S Wagner, G Wijnker, J Wilm, E de Wolf, H Yepe, D Zaborov, J D Zornoza, J Zúñiga, and ANTARES (IHEF, IoP, FNWI)
Subjects: Positioning system, Detector control systems (detector and experiment monitoring and slow-control systems, architecture, hardware, algorithms, databases), Detector modelling and simulations II (electric fields, Detector alignment and calibration methods (lasers, sources, particle-beams), 01 natural sciences, Timing detectors, hardware, Detector alignment and calibration methods, 010303 astronomy & astrophysics, Instrumentation, DETECTOR ALIGMENT, Mathematical Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, SOUND, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], Orientation (computer vision), [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Triangulation (computer vision), particle-beams), Geodesy, DETECTOR CONTROL SYSTEM, Detector modelling and simulations II (electric fields, charge transport, multiplication and induction, pulse formation, electron emission, etc), Física nuclear, Neutrino, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, databases), sources, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], pulse formation, architecture, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, ddc:500.2, DETECTOR MODELLING AND SIMULATIONS, Detector modelling and simulations II, algorithms, Physics::Geophysics, 0103 physical sciences, 14. Life underwater, Instrumentation and Methods for Astrophysics (astro-ph.IM), Cherenkov radiation, etc), multiplication and induction, Buoy, Detector control systems, 010308 nuclear & particles physics, Detector control systems (detector and experiment monitoring and slow-control systems, Mooring, charge transport, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Detector alignment and calibration methods (lasers, electron emission, FISICA APLICADA, detector modelling and simulations ii (electric fields, antares neutrino telescope, timing detectors, detector control systems (detector and experiment monitoring and slow-control systems, detector alignment, calibration, acoustic positioning, detector alignment and calibration methods (lasers
Abstract: The ANTARES neutrino telescope, located 40km off the coast of Toulon in the Mediterranean Sea at a mooring depth of about 2475m, consists of twelve detection lines equipped typically with 25 storeys. Every storey carries three optical modules that detect Cherenkov light induced by charged secondary particles (typically muons) coming from neutrino interactions. As these lines are flexible structures fixed to the sea bed and held taut by a buoy, sea currents cause the lines to move and the storeys to rotate. The knowledge of the position of the optical modules with a precision better than 10cm is essential for a good reconstruction of particle tracks. In this paper the ANTARES positioning system is described. It consists of an acoustic positioning system, for distance triangulation, and a compass-tiltmeter system, for the measurement of the orientation and inclination of the storeys. Necessary corrections are discussed and the results of the detector alignment procedure are described., The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'enegie atomique et aux energies alternatives (CEA), Agence National de la Recherche (ANR), Commission Europeenne (FEDER fund and Marie Curie Program), Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur 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 Innovacion (MICINN), Prometeo of Generalitat Valenciana and MultiDark, Spain. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation, the CC-IN2P3 for the computing facilities and the team of the former GENISEA company for their important contribution in the development of the acoustic positioning system.
Published: 2012
Full Text: View/download PDF

25. A search for neutrino emission from the Fermi bubbles with ANTARES telescope

Author: Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, Conseil Régional d'Alsace, Foundation for Fundamental Research on Matter, Holanda, Conseil Régional Provence-Alpes-Côte d'Azur, Council on grants of the President of the Russian Federation, Executive Agency for Higher Education, Scientific Research, Development and Innovation Funding, Rumanía, Instituto Nazionale di Fisica Nucleare; Ministerio de Ciencia e Innovación, European Regional Development Fund, Agence Nationale de la Recherche, Francia, Netherlands Organization for Scientific Research, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, Agence de l'Oriental, Marruecos, Centre National de la Recherche Scientifique, Francia, Bundesministerium für Bildung und Forschung, Alemania, Adrián Martínez, Silvia, Albert, A., Al Samarai, I., André, M., Anton, G., Anvar, S., Ardid Ramírez, Miguel, Astraatmadja, T., Aubert, J.-J., Baret, B., Barrios-Marti, J., Basa, S., Bertin, V., Larosa, Giuseppina, Martínez Mora, Juan Antonio, Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, Conseil Régional d'Alsace, Foundation for Fundamental Research on Matter, Holanda, Conseil Régional Provence-Alpes-Côte d'Azur, Council on grants of the President of the Russian Federation, Executive Agency for Higher Education, Scientific Research, Development and Innovation Funding, Rumanía, Instituto Nazionale di Fisica Nucleare; Ministerio de Ciencia e Innovación, European Regional Development Fund, Agence Nationale de la Recherche, Francia, Netherlands Organization for Scientific Research, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, Agence de l'Oriental, Marruecos, Centre National de la Recherche Scientifique, Francia, Bundesministerium für Bildung und Forschung, Alemania, Adrián Martínez, Silvia, Albert, A., Al Samarai, I., André, M., Anton, G., Anvar, S., Ardid Ramírez, Miguel, Astraatmadja, T., Aubert, J.-J., Baret, B., Barrios-Marti, J., Basa, S., Bertin, V., Larosa, Giuseppina, and Martínez Mora, Juan Antonio
Abstract: Analysis of the Fermi-LAT data has revealed two extended structures above and below the Galactic Centre emitting gamma rays with a hard spectrum, the so-called Fermi bubbles. Hadronic models attempting to explain the origin of the Fermi bubbles predict the emission of high energy neutrinos and gamma rays with similar fluxes. The ANTARES detector, a neutrino telescope located in the Mediterranean Sea, has a good visibility to the Fermi bubble regions. Using data collected from 2008 to 2011 no statistically significant excess of events is observed and therefore upper limits on the neutrino flux in TeV range from the Fermi bubbles are derived for various assumed energy cutoffs of the source.
Published: 2014

26. Measurement of the atmospheric muon flux with the NEMO Phase-1 detector

Author: A. Orlando, G. Raia, G. C. Barbarino, G. De Rosa, M. Cordelli, M. Imbesi, C.A. Nicolau, S. Russo, E. Falchini, R. De Vita, I. Amore, Mário Costa, Nicolo' Beverini, Enzo Gandolfi, Paolo Sapienza, L. Caponetto, Alberto Rovelli, G.V. Russo, L. Trasatti, G. Cacopardo, A. Martini, Federico M. Giorgi, G. De Bonis, S. Reito, M. Ruppi, Alessandro Lonardo, D. Lattuada, Sebastiano Aiello, M. Taiuti, S. Galatà, Alessandro Gabrielli, V. Pappalardo, R. Coniglione, S. Urso, Maurizio Spurio, M. Osipenko, Piero Vicini, M. Ripani, M. Circella, G. Ricco, D. Lo Presti, A. Grimaldi, Annarita Margiotta, Marco Brunoldi, A. Anzalone, D. Sciliberto, Valeria Sipala, E. Leonora, M. Bonori, B. Bouhadef, M. Anghinolfi, A. Marinelli, M. Sedita, R. Masullo, A. Bersani, Mario Musumeci, Nunzio Randazzo, Francesco Simeone, D. Piombo, G. De Ruvo, Riccardo Papaleo, M. Bazzotti, E. Migneco, V. Flaminio, R. Habel, Tommaso Chiarusi, A. D'Amico, K. Fratini, S. Minutoli, V. Kulikovsky, F. Lucarelli, G. Giacomelli, Paolo Musico, C. Distefano, M. Battaglieri, Rosanna Cocimano, C. De Marzo, Manuela Vecchi, S. Biagi, Gabriele Giovanetti, P. Piattelli, Fabrizio Ameli, G. Riccobene, E. Shirokov, M. Morganti, Ralf Wischnewski, Alessia Capone, G. Carminati, S. Aiello, F. Ameli, I. Amore, M. Anghinolfi, A. Anzalone, G. Barbarino, M. Battaglieri, M. Bazzotti, A. Bersani, N. Beverini, S. Biagi, M. Bonori, B. Bouhadef, M. Brunoldi, G. Cacopardo, A. Capone, L. Caponetto, G. Carminati, T. Chiarusi, M. Circella, R. Cocimano, R. Coniglione, M. Cordelli, M. Costa, A. D’Amico, G. De Boni, C. De Marzo, G. De Rosa, G. De Ruvo, R. De Vita, C. Distefano, E. Falchini, V. Flaminio, K. Fratini, A. Gabrielli, S. Galata, E. Gandolfi, G. Giacomelli, F. Giorgi, G. Giovanetti, A. Grimaldi, R. Habel, M. Imbesi, V. Kulikovsky, D. Lattuada, E. Leonora, A. Lonardo, D. Lo Presti, F. Lucarelli, A. Marinelli, A. Margiotta, A. Martini, R. Masullo, E. Migneco, S. Minutoli, M. Morganti, P. Musico, M. Musumeci, C.A. Nicolau, A. Orlando, M. Osipenko, R. Papaleo, V. Pappalardo, P. Piattelli, D. Piombo, G. Raia, N. Randazzo, S. Reito, G. Ricco, G. Riccobene, M. Ripani, A. Rovelli, M. Ruppi, G.V. Russo, S. Russo, P. Sapienza, D. Sciliberto, M. Sedita, E. Shirokov, F. Simeone, V. Sipala, M. Spurio, M. Taiuti, L. Trasatti, S. Urso, M. Vecchi, P. Vicini, R. Wischnewski, DE ROSA, Gianfranca, Barbarino, Giancarlo, Longo, Giuseppe, Russo, Stefano, Osteria, Giuseppe, and S., Aiello
Subjects: MODULE, Photomultiplier, ANTARES NEUTRINO TELESCOPE, Physics::Instrumentation and Detectors, Monte Carlo method, FOS: Physical sciences, LINE, atmospheric muons, nemo, neutrino telescopes, Nuclear physics, Optics, Data acquisition, DESIGN, OCEAN, Calibration, NEUTRINO TELESCOPE, Underwater, Junction box, Instrumentation and Methods for Astrophysics (astro-ph.IM), DEEP-SEA, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), ANTARES NEUTRINO TELESCOPE, DEEP-SEA, DATA-ACQUISITION, PERFORMANCE, PROJECT, SYSTEM, LINE, DESIGN, MODULE, OCEAN, business.industry, Detector, Astronomy and Astrophysics, DATA-ACQUISITION, COSMIC RAYS, PERFORMANCE, MUON FLUX, Neutrino detector, High Energy Physics::Experiment, UNDERWATER DETECTOR, business, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, PROJECT, SYSTEM
Abstract: The NEMO Collaboration installed and operated an underwater detector including prototypes of the critical elements of a possible underwater km3 neutrino telescope: a four-floor tower (called Mini-Tower) and a Junction Box. The detector was developed to test some of the main systems of the km3 detector, including the data transmission, the power distribution, the timing calibration and the acoustic positioning systems as well as to verify the capabilities of a single tridimensional detection structure to reconstruct muon tracks. We present results of the analysis of the data collected with the NEMO Mini-Tower. The position of photomultiplier tubes (PMTs) is determined through the acoustic position system. Signals detected with PMTs are used to reconstruct the tracks of atmospheric muons. The angular distribution of atmospheric muons was measured and results compared with Monte Carlo simulations., Astrop. Phys., accepted
Published: 2010

27. Positioning system of the ANTARES Neutrino Telescope

Author: Brown, Anthony M., Cristofol, Danielle, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and ANTARES
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, alignment, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [SDU.ASTR.IM] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, ANTARES neutrino telescope, [PHYS.ASTR.IM] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Instrumentation and Methods for Astrophysics (astro-ph.IM), acoustic positioning system
Abstract: Completed in May 2008, the ANTARES neutrino telescope is located 40 km off the coast of Toulon, at a depth of about 2500 m. The telescope consists of 12 detect or lines housing a total of 884 optical modules. Each line is anchored to the seabed and pulled taught by the buoyancy of the individual optical modules and a top buoy. Due to the fluid nature of the sea-water detecting medium and the flexible nature of the detector lines, the optical modules of the ANTARES telescope can suffer from deviations of up to several meters from the vertical and as such, real time positioning is needed. Real time positioning of the ANTARES telescope is achieved by a combination of an acoustic positioning system and a lattice of tiltmeters and compasses. These independent and complementary systems are used to compute a global fit to each individual detector line, allowing us to construct a 3 dimensional picture of the ANTARES neutrino telescope with an accuracy of less than 10 cm. In this paper we describe the positioning system of the ANTARES neutrino telescope and discuss its performance during the first year of 12 line data taking., Proceedings of 31st ICRC conference, Lodz 2009, 4 pages, 3 pictures
Published: 2009

28. Deep-Sea Bioluminescence Blooms after Dense Water Formation at the Ocean Surface

Author: Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, European Commission, Generalitat de Catalunya, Ministerio de Ciencia e Innovación, Generalitat Valenciana, Agence Nationale de la Recherche, Francia, Ministerio de Economía y Competitividad, Institut National des Sciences de l'Univers, Institut National de Physique Nucléaire et de Physique des Particules, Francia, Université de la Méditerranée - Aix-Marseille II, Ministère de l'Enseignement supérieur, de la Recherche et de l'Innovation, Francia, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, European Regional Development Fund, Conseil Régional d'Alsace, Conseil Régional Provence-Alpes-Côte d'Azur, Département du Var and Ville de La Seyne-sur-Mer, Bundesministerium für Bildung und Forschung, Alemania, Instituto Nazionale di Fisica Nucleare, Netherlands Organization for Scientific Research, Council on grants of the President of the Russian Federation, National Authority for Scientific Research, Rumanía, Ministerio de Educación y Ciencia, Tamburini, Christian, Canals, Miquel, de Madron, Xavier Durrieu, Houpert, Loic, Lefevre, Dominique, Martini, Verine, D'Ortenzio, Fabrizio, Robert, Anne, Testor, Pierre, Ardid Ramírez, Miguel, Bou Cabo, Manuel, Camarena Femenia, Francisco, Ferri García, Marcelino, Larosa, Giuseppina, Martínez Mora, Juan Antonio, Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada, Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres, European Commission, Generalitat de Catalunya, Ministerio de Ciencia e Innovación, Generalitat Valenciana, Agence Nationale de la Recherche, Francia, Ministerio de Economía y Competitividad, Institut National des Sciences de l'Univers, Institut National de Physique Nucléaire et de Physique des Particules, Francia, Université de la Méditerranée - Aix-Marseille II, Ministère de l'Enseignement supérieur, de la Recherche et de l'Innovation, Francia, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia, European Regional Development Fund, Conseil Régional d'Alsace, Conseil Régional Provence-Alpes-Côte d'Azur, Département du Var and Ville de La Seyne-sur-Mer, Bundesministerium für Bildung und Forschung, Alemania, Instituto Nazionale di Fisica Nucleare, Netherlands Organization for Scientific Research, Council on grants of the President of the Russian Federation, National Authority for Scientific Research, Rumanía, Ministerio de Educación y Ciencia, Tamburini, Christian, Canals, Miquel, de Madron, Xavier Durrieu, Houpert, Loic, Lefevre, Dominique, Martini, Verine, D'Ortenzio, Fabrizio, Robert, Anne, Testor, Pierre, Ardid Ramírez, Miguel, Bou Cabo, Manuel, Camarena Femenia, Francisco, Ferri García, Marcelino, Larosa, Giuseppina, and Martínez Mora, Juan Antonio
Abstract: [EN] The deep ocean is the largest and least known ecosystem on Earth. It hosts numerous pelagic organisms, most of which are able to emit light. Here we present a unique data set consisting of a 2.5-year long record of light emission by deep-sea pelagic organisms, measured from December 2007 to June 2010 at the ANTARES underwater neutrino telescope in the deep NW Mediterranean Sea, jointly with synchronous hydrological records. This is the longest continuous time-series of deep-sea bioluminescence ever recorded. Our record reveals several weeks long, seasonal bioluminescence blooms with light intensity up to two orders of magnitude higher than background values, which correlate to changes in the properties of deep waters. Such changes are triggered by the winter cooling and evaporation experienced by the upper ocean layer in the Gulf of Lion that leads to the formation and subsequent sinking of dense water through a process known as "open-sea convection". It episodically renews the deep water of the study area and conveys fresh organic matter that fuels the deep ecosystems. Luminous bacteria most likely are the main contributors to the observed deep-sea bioluminescence blooms. Our observations demonstrate a consistent and rapid connection between deep open-sea convection and bathypelagic biological activity, as expressed by bioluminescence. In a setting where dense water formation events are likely to decline under global warming scenarios enhancing ocean stratification, in situ observatories become essential as environmental sentinels for the monitoring and understanding of deep-sea ecosystem shifts.
Published: 2013

29. Acoustic and optical variations during rapid downward motion episodes in the deep north-western Mediterranean Sea

Author: Aguilar Sanchez, Juan Antonio, Toscano, Simona, Aguilar Sanchez, Juan Antonio, and Toscano, Simona
Abstract: An Acoustic Doppler Current Profiler (ADCP) was moored at the deep-sea site of the ANTARES neutrino telescope near Toulon, France, thus providing a unique opportunity to compare high-resolution acoustic and optical observations between 70 and 170m above the sea bed at 2475m. The ADCP measured downward vertical currents of magnitudes up to 0.03ms-1 in late winter and early spring 2006. In the same period, observations were made of enhanced levels of acoustic reflection, interpreted as suspended particles including zooplankton, by a factor of about 10 and of horizontal currents reaching 0.35ms-1. These observations coincided with high light levels detected by the telescope, interpreted as increased bioluminescence. During winter 2006 deep dense-water formation occurred in the Ligurian subbasin, thus providing a possible explanation for these observations. However, the 10-20 days quasi-periodic episodes of high levels of acoustic reflection, light and large vertical currents continuing into the summer are not direct evidence of this process. It is hypothesized that the main process allowing for suspended material to be moved vertically later in the year is local advection, linked with topographic boundary current instabilities along the rim of the 'Northern Current'. © 2011 Elsevier Ltd., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2011

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29 results on '"ANTARES NEUTRINO TELESCOPE"'

1. Calibration of the ANTARES neutrino telescope.

2. ANTARES and IceCube Combined Search for Neutrino Point-like and Extended Sources in the Southern Sky

3. Combined search for neutrinos from dark matter self-annihilation in the Galactic Center with ANTARES and IceCube

4. Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope

5. Observation of the cosmic ray shadow of the Sun with the ANTARES neutrino telescope

6. Acoustic and optical variations during rapid downward motion episodes in the deep north-western Mediterranean Sea

7. Luminous bacteria in the deep-sea waters near the ANTARES underwater neutrino telescope (Mediterranean Sea).

8. ANTARES: An Underwater Network of Sensors for Neutrino Astronomy and Deep-Sea Research.

9. ANTARES and IceCube Combined Search for Neutrino Point-like and Extended Sources in the Southern Sky

10. Observation of the cosmic ray shadow of the Sun with the ANTARES neutrino telescope

11. Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope

12. Erratum to 'Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope' [Phys. Lett. B 769 (2017) 249–254]

13. The cosmic ray shadow of the Moon observed with the ANTARES neutrino telescope

14. The cosmic ray shadow of the Moon observed with the ANTARES neutrino telescope

15. All-sky Search for High-Energy Neutrinos from Gravitational Wave Event GW170104 with the ANTARES Neutrino Telescope

16. Sperm whale long-range echolocation sounds revealed by ANTARES, a deep-sea neutrino telescope

17. Sperm whale long-range echolocation sounds revealed by ANTARES, a deep-sea neutrino telescope

18. All-sky Search for High-Energy Neutrinos from Gravitational Wave Event GW170104 with the ANTARES Neutrino Telescope

19. Results from the ANTARES Neutrino Telescope with Six Years of Data

20. A search for time dependent neutrino emission from microquasars with the ANTARES telescope

21. A search for neutrino emission from the Fermi bubbles with the ANTARES telescope

22. Starlight beneath the waves: In search of TeV photon emission from Gamma-Ray Bursts with the ANTARES Neutrino Telescope

23. Deep-Sea Bioluminescence Blooms after Dense Water Formation at the Ocean Surface

24. The positioning system of the ANTARES Neutrino Telescope

25. A search for neutrino emission from the Fermi bubbles with ANTARES telescope

26. Measurement of the atmospheric muon flux with the NEMO Phase-1 detector

27. Positioning system of the ANTARES Neutrino Telescope

28. Deep-Sea Bioluminescence Blooms after Dense Water Formation at the Ocean Surface

29. Acoustic and optical variations during rapid downward motion episodes in the deep north-western Mediterranean Sea

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29 results on '"ANTARES NEUTRINO TELESCOPE"'

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