M. Taiuti - Universita di Genoa

M. Taiuti
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Name
M. Taiuti
Affiliation
Universita di Genoa
City
Genova
Country
Italy

Pubs By Year

Pub Categories

 
High Energy Astrophysical Phenomena (26)
 
Nuclear Experiment (17)
 
High Energy Physics - Experiment (15)
 
Instrumentation and Methods for Astrophysics (10)
 
Physics - Instrumentation and Detectors (9)
 
High Energy Physics - Phenomenology (9)
 
Cosmology and Nongalactic Astrophysics (2)
 
Nuclear Theory (1)
 
Astrophysics of Galaxies (1)

Publications Authored By M. Taiuti

2017Mar
Authors: CLAS Collaboration, I. Bedlinskiy, V. Kubarovsky, P. Stoler, K. P. Adhikari, Z. Akbar, S. Anefalos Pereira, H. Avakian, J. Ball, N. A. Baltzell, M. Battaglieri, V. Batourine, A. S. Biselli, S. Boiarinov, W. J. Briscoe, V. D. Burkert, T. Cao, D. S. Carman, A. Celentano, S. Chandavar, G. Charles, G. Ciullo, L. Clark, L. Colaneri, P. L. Cole, M. Contalbrigo, V. Crede, A. D'Angelo, N. Dashyan, R. De Vita, E. De Sanctis, A. Deur, C. Djalali, R. Dupre, A. El Alaoui, L. El Fassi, L. Elouadrhiri, P. Eugenio, E. Fanchini, G. Fedotov, R. Fersch, A. Filippi, J. A. Fleming, T. A. Forest, M. Garçon, N. Gevorgyan, Y. Ghandilyan, G. P. Gilfoyle, K. L. Giovanetti, F. X. Girod, C. Gleason, E. Golovatch, R. W. Gothe, K. A. Griffioen, M. Guidal, L. Guo, K. Hafidi, H. Hakobyan, C. Hanretty, N. Harrison, M. Hattawy, K. Hicks, S. M. Hughes, C. E. Hyde, Y. Ilieva, D. G. Ireland, B. S. Ishkhanov, E. L. Isupov, D. Jenkins, H. Jiang, H. S. Jo, K. Joo, S. Joosten, D. Keller, G. Khachatryan, M. Khachatryan, M. Khandaker, A. Kim, W. Kim, F. J. Klein, S. E. Kuhn, S. V. Kuleshov, L. Lanza, P. Lenisa, K. Livingston, I. J. D. MacGregor, N. Markov, B. McKinnon, Z. E. Meziani, M. Mirazita, V. Mokeev, R. A. Montgomery, A. Movsisyan, C. Munoz Camacho, P. Nadel-Turonski, L. A. Net, A. Ni, S. Niccolai, G. Niculescu, M. Osipenko, A. I. Ostrovidov, M. Paolone, R. Paremuzyan, K. Park, E. Pasyuk, P. Peng, W. Phelps, S. Pisano, O. Pogorelko, J. W. Price, Y. Prok, D. Protopopescu, A. J. R. Puckett, B. A. Raue, M. Ripani, A. Rizzo, G. Rosner, P. Rossi, P. Roy, F. Sabatié, M. S. Saini, C. Salgado, R. A. Schumacher, Y. G. Sharabian, Iu. Skorodumina, G. D. Smith, D. Sokhan, N. Sparveris, S. Stepanyan, I. I. Strakovsky, S. Strauch, M. Taiuti, Ye Tian, B. Torayev, M. Turisini, M. Ungaro, H. Voskanyan, E. Voutier, N. K. Walford, D. P. Watts, X. Wei, L. B. Weinstein, M. H. Wood, M. Yurov, N. Zachariou, J. Zhang, I. Zonta

The cross section of the exclusive $\eta$ electroproduction reaction $ep\to e^\prime p^\prime \eta$ was measured at Jefferson Lab with a 5.75-GeV electron beam and the CLAS detector. Differential cross sections $d^4\sigma/dtdQ^2dx_Bd\phi_\eta$ and structure functions $\sigma_U = \sigma_T+\epsilon\sigma_L, \sigma_{TT}$ and $\sigma_{LT}$, as functions of $t$ were obtained over a wide range of $Q^2$ and $x_B$. Read More

The Extreme Energy Events Project is a synchronous sparse array of 52 tracking detectors for studying High Energy Cosmic Rays (HECR) and Cosmic Rays-related phenomena. The observatory is also meant to address Long Distance Correlation (LDC) phenomena: the network is deployed over a broad area covering 10 degrees in latitude and 11 in longitude. An overview of a set of preliminary results is given, extending from the study of local muon flux dependance on solar activity to the investigation of the upward-going component of muon flux traversing the EEE stations; from the search for anisotropies at the sub-TeV scale to the hints for observations of km-scale Extensive Air Shower (EAS). Read More

2017Mar
Authors: 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, 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

A novel method to analyse the spatial distribution of neutrino candidates recorded with the ANTARES neutrino telescope is introduced, searching for an excess of neutrinos in a region of arbitrary size and shape from any direction in the sky. Techniques originating from the domains of machine learning, pattern recognition and image processing are used to purify the sample of neutrino candidates and for the analysis of the obtained skymap. In contrast to a dedicated search for a specific neutrino emission model, this approach is sensitive to a wide range of possible morphologies of potential sources of high-energy neutrino emission. Read More

2017Mar
Authors: ANTARES Collaboration, 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, A. Domi, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, I. El Bojaddaini, D. Elsässer, A. Enzenhöfer, I. Felis, F. Folger, L. A. Fusco, S. Galatà, P. Gay, V. Giordano, 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, 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, R. Mele, K. Melis, T. Michael, P. Migliozzi, A. Moussa, E. Nezri, M. Organokov, G. E. Păvălaş, C. Pellegrino, C. Perrina, P. Piattelli, V. Popa, T. Pradier, L. Quinn, C. Racca, G. Riccobene, A. Sánchez-Losa, M. Saldaña, I. Salvadori, D. F. E. Samtleben, M. Sanguineti, P. Sapienza, F. Schüssler, C. Sieger, M. Spurio, Th. Stolarczyk, M. Taiuti, Y. Tayalati, A. Trovato, D. Turpin, C. Tönnis, B. Vallage, V. Van Elewyck, F. Versari, D. Vivolo, A. Vizzoca, J. Wilms, J. D. Zornoza, J. Zúñiga

A novel algorithm to reconstruct neutrino-induced particle showers within the ANTARES neutrino telescope is presented. The method achieves a median angular resolution of $6^\circ$ for shower energies below 100 TeV. Applying this algorithm to 6 years of data taken with the ANTARES detector, 8 events with reconstructed shower energies above 10 TeV are observed. Read More

2017Mar
Authors: 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, A. Domi, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, I. El Bojaddaini, D. Elsässer, A. Enzenhöfer, I. Felis, L. A. Fusco, S. Galatà, P. Gay, V. Giordano, 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, 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, R. Mele, K. Melis, T. Michael, P. Migliozzi, A. Moussa, S. Navas, E. Nezri, M. Organokov, G. E. Păvălaş, C. Pellegrino, C. Perrina, P. Piattelli, V. Popa, T. Pradier, L. Quinn, C. Racca, G. Riccobene, A. Sánchez-Losa, M. Saldaña, I. Salvadori, D. F. E. Samtleben, M. Sanguineti, P. Sapienza, F. Schüssler, C. Sieger, M. Spurio, Th. Stolarczyk, M. Taiuti, Y. Tayalati, A. Trovato, D. Turpin, C. Tönnis, B. Vallage, V. Van Elewyck, F. Versari, D. Vivolo, A. Vizzoca, J. Wilms, J. D. Zornoza, J. Zúñiga

A search for magnetic monopoles using five years of data recorded with the ANTARES neutrino telescope from January 2008 to December 2012 with a total live time of 1121 days is presented. The analysis is carried out in the range $\beta$ $>$ $0.6$ of magnetic monopole velocities using a strategy based on run-by-run Monte Carlo simulations. Read More

2017Mar
Authors: P. Collins, B. G. Ritchie, M. Dugger, A. V. Anisovich, M. Döring, E. Klempt, V. A. Nikonov, D. Rönchen, D. Sadasivan, A. Sarantsev, K. P. Adhikaria, Z. Akbar, M. J. Amaryana, S. Anefalos Pereira, H. Avakiana, J. Ball, I. Balossino, M. Bashkanova, M. Battaglieri, I. Bedlinskiy, A. S. Bisellik, W. J. Briscoe, W. K. Brooks, V. D. Burkert, Frank Thanh Cao, D. S. Carman, A. Celentano, S. Chandavar, G. Charles, T. Chetry, G. Ciullo, L. Clark, L. Colaneri, P. L. Cole, N. Compton, M. Contalbrigo, O. Cortes, V. Crede, A. D'Angelo, N. Dashyan, R. De Vita, E. De Sanctis, A. Deur, C. Djalali, R. Dupre, H. Egiyan, A. El Alaoui, L. El Fassi, L. Elouadrhiri, P. Eugenio, E. Fanchini, G. Fedotov, A. Filippi, J. A. Fleming, Y. Ghandilyan, G. P. Gilfoyle, K. L. Giovanetti, F. X. Girod, D. I. Glazier, C. Gleason, E. Golovatch, R. W. Gothe, K. A. Griffioen, L. Guo, K. Hafidi, H. Hakobyan, C. Hanretty, N. Harrison, D. Heddle, K. Hicks, M. Holtrop, S. M. Hughes, Y. Ilieva, D. G. Ireland, B. S. Ishkhanov, E. L. Isupov, D. Jenkins, H. S. Jo, S. Joosten, D. Keller, G. Khachatryan, M. Khachatryan, M. Khandaker, A. Kim, W. Kim, A. Klein, F. J. Klein, V. Kubarovsky, L. Lanza, P. Lenisa, K. Livingston, I. J. D. MacGregor, N. Markov, B. McKinnon, C. A. Meyer, M. Mirazita, V. Mokeev, R. A. Montgomery, A Movsisyan, C. Munoz Camacho, G. Murdoch, P. Nadel-Turonski, S. Niccolai, G. Niculescu, I. Niculescu, M. Osipenko, A. I. Ostrovidov, M. Paolone, R. Paremuzyan, K. Park, E. Pasyuk, W. Phelps, S. Pisano, O. Pogorelko, J. W. Price, Y. Prok, D. Protopopescu, B. A. Raue, M. Ripani, A. Rizzo, G. Rosner, P. Roy, F. Sabatié, C. Salgado, R. A. Schumacher, Y. G. Sharabian, Iu. Skorodumina, G. D. Smith, D. Sokhan, N. Sparveris, S. Stepanyan, I. I. Strakovsky, S. Strauch, M. Taiuti, Ye Tian, B. Torayev, M. Ungaro, H. Voskanyan, E. Voutier, N. K. Walford, X. Wei, N. Zachariou, J. Zhang

Measurements of the linearly-polarized photon beam asymmetry $\Sigma$ for photoproduction from the proton of $\eta$ and $\eta^\prime$ mesons are reported. A linearly-polarized tagged photon beam produced by coherent bremsstrahlung was incident on a cryogenic hydrogen target within the CEBAF Large Acceptance Spectrometer. Results are presented for the $\gamma p \to \eta p$ reaction for incident photon energies from 1. Read More

2016Dec
Authors: 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, 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

Gamma-ray bursts are thought to be sites of hadronic acceleration, thus neutrinos are expected from the decay of charged particles, produced in p{\gamma} interactions. The methods and results of a search for muon neutrinos in the data of the ANTARES neutrino telescope from four bright GRBs (GRB 080916C, GRB 110918A, GRB 130427A and GRB 130505A) observed between 2008 and 2013 are presented. Two scenarios of the fireball model have been investigated: the internal shock scenario, leading to the production of neutrinos with energies mainly above 100 TeV, and the photospheric scenario, characterised by a low-energy component in neutrino spectra due to the assumption of neutrino production closer to the central engine. Read More

2016Dec
Authors: ANTARES Collaboration, 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, 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

A search for a neutrino signal from WIMP pair annihilations in the centre of the Earth has been performed with the data collected with the ANTARES neutrino telescope from 2007 to 2012. The event selection criteria have been developed and tuned to maximise the sensitivity of the experiment to such a neutrino signal. No significant excess of neutrinos over the expected background has been observed. Read More

2016Dec
Authors: 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 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, 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. Lefèver, 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

Using data recorded with the ANTARES telescope from 2007 to 2015, a new search for dark matter annihilation in the Milky Way has been performed. Three halo models and five annihilation channels, $\rm WIMP + WIMP \to b \bar b, W^+ W^-, \tau^+ \tau^-, \mu^{+} \mu^{-}$ and $\nu \bar{\nu}$, with WIMP masses ranging from 50 $\frac{\text{GeV}}{\text{c}^2}$ to 100 $\frac{\text{TeV}}{\text{c}^2}$, were considered. No excess over the expected background was found, and limits on the thermally averaged annihilation cross--section were set. Read More

2016Nov
Authors: S. Adrián-Martínez, M. Ageron, S. Aiello, A. Albert, F. Ameli, E. G. Anassontzis, M. Andre, G. Androulakis, M. Anghinolfi, G. Anton, M. Ardid, T. Avgitas, G. Barbarino, E. Barbarito, B. Baret, J. Barrios-Martí, A. Belias, E. Berbee, A. van den Berg, V. Bertin, S. Beurthey, V. van Beveren, N. Beverini, S. Biagi, A. Biagioni, M. Billault, M. Bondì, R. Bormuth, B. Bouhadef, G. Bourlis, S. Bourret, C. Boutonnet, M. Bouwhuis, C. Bozza, R. Bruijn, J. Brunner, E. Buis, R. Buompane, J. Busto, G. Cacopardo, L. Caillat, M. Calamai, D. Calvo, A. Capone, L. Caramete, S. Cecchini, S. Celli, C. Champion, S. Cherubini, V. Chiarella, T. Chiarusi, M. Circella, L. Classen, D. Cobas, R. Cocimano, J. A. B. Coelho, A. Coleiro, S. Colonges, R. Coniglione, M. Cordelli, A. Cosquer, P. Coyle, A. Creusot, G. Cuttone, C. D'Amato, A. D'Amico, A. D'Onofrio, G. De Bonis, C. De Sio, I. Di Palma, A. F. Díaz, C. Distefano, C. Donzaud, D. Dornic, Q. Dorosti-Hasankiadeh, E. Drakopoulou, D. Drouhin, M. Durocher, T. Eberl, S. Eichie, D. van Eijk, I. El Bojaddaini, D. Elsaesser, A. Enzenhöfer, M. Favaro, P. Fermani, G. Ferrara, G. Frascadore, L. A. Fusco, T. Gal, S. Galatà, F. Garufi, P. Gay, M. Gebyehu, F. Giacomini, L. Gialanella, V. Giordano, N. Gizani, R. Gracia, K. Graf, T. Grégoire, G. Grella, A. Grmek, R. Habel, S. Hallmann, H. van Haren, S. Harissopulos, T. Heid, A. Heijboer, E. Heine, S. Henry, J. J. Hernández-Rey, M. Hevinga, J. Hofestädt, C. M. F. Hugon, G. Illuminati, C. W. James, P. Jansweijer, M. Jongen, M. de Jong, M. Kadler, O. Kalekin, A. Kappes, U. F. Katz, P. Keller, G. Kieft, D. Kießling, E. N. Koffeman, P. Kooijman, A. Kouchner, M. Kreter, V. Kulikovskiy, R. Lahmann, P. Lamare, G. Larosa, A. Leisos, F. Leone, E. Leonora, M. Lindsey Clark, A. Liolios, C. D. Llorens Alvarez, D. Lo Presti, H. Löhner, A. Lonardo, M. Lotze, S. Loucatos, E. Maccioni, K. Mannheim, M. Manzali, A. Margiotta, A. Marinelli, O. Mariş, C. Markou, J. A. Martínez-Mora, A. Martini, F. Marzaioli, R. Mele, K. W. Melis, T. Michael, P. Migliozzi, E. Migneco, P. Mijakowski, A. Miraglia, C. M. Mollo, M. Mongelli, M. Morganti, A. Moussa, P. Musico, M. Musumeci, S. Navas, C. A. Nicolau, I. Olcina, C. Olivetto, A. Orlando, A. Orzelli, A. Papaikonomou, R. Papaleo, G. E. Păvălaş, H. Peek, G. Pellegrini, C. Pellegrino, C. Perrina, M. Pfutzner, P. Piattelli, K. Pikounis, M. -O. Pleinert, G. E. Poma, V. Popa, T. Pradier, F. Pratolongo, G. Pühlhofer, S. Pulvirenti, L. Quinn, C. Racca, F. Raffaelli, N. Randazzo, T. Rauch, D. Real, L. Resvanis, J. Reubelt, G. Riccobene, C. Rossi, A. Rovelli, M. Saldaña, I. Salvadori, D. F. E. Samtleben, A. Sánchez García, A. Sánchez Losa, M. Sanguineti, A. Santangelo, D. Santonocito, P. Sapienza, F. Schimmel, J. Schmelling, J. Schnabel, V. Sciacca, M. Sedita, T. Seitz, I. Sgura, F. Simeone, V. Sipala, B. Spisso, M. Spurio, G. Stavropoulos, J. Steijger, S. M. Stellacci, D. Stransky, M. Taiuti, Y. Tayalati, F. Terrasi, D. Tézier, S. Theraube, P. Timmer, C. Tönnis, L. Trasatti, R. Travaglini, A. Trovato, A. Tsirigotis, S. Tzamarias, E. Tzamariudaki, B. Vallage, V. Van Elewyck, J. Vermeulen, P. Vicini, S. Viola, D. Vivolo, M. Volkert, L. Wiggers, J. Wilms, E. de Wolf, K. Zachariadou, J. D. Zornoza, J. Zúñiga

Studying atmospheric neutrino oscillations in the few-GeV range with a multimegaton detector promises to determine the neutrino mass hierarchy. This is the main science goal pursued by the future KM3NeT/ORCA water Cherenkov detector in the Mediterranean Sea. In this paper, the processes that limit the obtainable resolution in both energy and direction in charged-current neutrino events in the ORCA detector are investigated. Read More

2016Nov
Authors: P. E. Bosted1, A. Kim2, K. P. Adhikari3, D. Adikaram4, Z. Akbar5, M. J. Amaryan6, S. Anefalos Pereira7, H. Avakian8, R. A. Badui9, J. Ball10, I. Balossino11, M. Battaglieri12, I. Bedlinskiy13, A. S. Biselli14, S. Boiarinov15, W. J. Briscoe16, W. K. Brooks17, S. Bültmann18, V. D. Burkert19, T. Cao20, D. S. Carman21, A. Celentano22, S. Chandavar23, G. Charles24, T. Chetry25, G. Ciullo26, L. Clark27, L. Colaneri28, P. L. Cole29, M. Contalbrigo30, O. Cortes31, V. Crede32, A. D'Angelo33, N. Dashyan34, R. De Vita35, E. De Sanctis36, A. Deur37, C. Djalali38, R. Dupre39, H. Egiyan40, A. El Alaoui41, L. El Fassi42, L. Elouadrhiri43, P. Eugenio44, E. Fanchini45, G. Fedotov46, S. Fegan47, R. Fersch48, A. Filippi49, J. A. Fleming50, T. A. Forest51, A. Fradi52, Y. Ghandilyan53, G. P. Gilfoyle54, F. X. Girod55, D. I. Glazier56, W. Gohn57, E. Golovatch58, R. W. Gothe59, K. A. Griffioen60, M. Guidal61, N. Guler62, H. Hakobyan63, L. Guo64, K. Hafidi65, H. Hakobyan66, C. Hanretty67, N. Harrison68, M. Hattawy69, D. Heddle70, K. Hicks71, G. Hollis72, M. Holtrop73, S. M. Hughes74, D. G. Ireland75, E. L. Isupov76, D. Jenkins77, H. Jiang78, H. S. Jo79, K. Joo80, D. Keller81, G. Khachatryan82, M. Khandaker83, W. Kim84, A. Klei85, F. J. Klein86, S. Koirala87, V. Kubarovsky88, S. E. Kuhn89, L. Lanza90, P. Lenisa91, K. Livingston92, H. Y. Lu93, I. J. D. MacGregor94, N. Markov95, M. Mayer96, M. E. McCracken97, B. McKinnon98, T. Mineeva99, M. Mirazita100, V. I. Mokeev101, R. A. Montgomery102, A Movsisyan103, C. Munoz Camacho104, G. Murdoch105, P. Nadel-Turonski106, A. Ni107, S. Niccolai108, G. Niculescu109, M. Osipenko110, A. I. Ostrovidov111, M. Paolone112, R. Paremuzyan113, K. Park114, E. Pasyuk115, W. Phelps116, S. Pisano117, O. Pogorelko118, J. W. Price119, Y. Prok120, D. Protopopescu121, A. J. R. Puckett122, B. A. Raue123, M. Ripani124, A. Rizzo125, G. Rosner126, P. Rossi127, P. Roy128, F. Sabatié129, M. S. Saini130, R. A. Schumacher131, E. Seder132, Y. G. Sharabian133, Iu. Skorodumina134, G. D. Smith135, D. Sokhan136, N. Sparveris137, I. Stankovic138, S. Stepanyan139, P. Stoler140, I. I. Strakovsky141, S. Strauch142, M. Taiuti143, Ye Tian144, B. Torayev145, M. Ungaro146, H. Voskanyan147, E. Voutier148, N. K. Walford149, D. P. Watts150, X. Wei151, L. B. Weinstein152, N. Zachariou153, J. Zhang154, Z. W. Zhao155, I. Zonta156
Affiliations: 1The CLAS Collaboration, 2The CLAS Collaboration, 3The CLAS Collaboration, 4The CLAS Collaboration, 5The CLAS Collaboration, 6The CLAS Collaboration, 7The CLAS Collaboration, 8The CLAS Collaboration, 9The CLAS Collaboration, 10The CLAS Collaboration, 11The CLAS Collaboration, 12The CLAS Collaboration, 13The CLAS Collaboration, 14The CLAS Collaboration, 15The CLAS Collaboration, 16The CLAS Collaboration, 17The CLAS Collaboration, 18The CLAS Collaboration, 19The CLAS Collaboration, 20The CLAS Collaboration, 21The CLAS Collaboration, 22The CLAS Collaboration, 23The CLAS Collaboration, 24The CLAS Collaboration, 25The CLAS Collaboration, 26The CLAS Collaboration, 27The CLAS Collaboration, 28The CLAS Collaboration, 29The CLAS Collaboration, 30The CLAS Collaboration, 31The CLAS Collaboration, 32The CLAS Collaboration, 33The CLAS Collaboration, 34The CLAS Collaboration, 35The CLAS Collaboration, 36The CLAS Collaboration, 37The CLAS Collaboration, 38The CLAS Collaboration, 39The CLAS Collaboration, 40The CLAS Collaboration, 41The CLAS Collaboration, 42The CLAS Collaboration, 43The CLAS Collaboration, 44The CLAS Collaboration, 45The CLAS Collaboration, 46The CLAS Collaboration, 47The CLAS Collaboration, 48The CLAS Collaboration, 49The CLAS Collaboration, 50The CLAS Collaboration, 51The CLAS Collaboration, 52The CLAS Collaboration, 53The CLAS Collaboration, 54The CLAS Collaboration, 55The CLAS Collaboration, 56The CLAS Collaboration, 57The CLAS Collaboration, 58The CLAS Collaboration, 59The CLAS Collaboration, 60The CLAS Collaboration, 61The CLAS Collaboration, 62The CLAS Collaboration, 63The CLAS Collaboration, 64The CLAS Collaboration, 65The CLAS Collaboration, 66The CLAS Collaboration, 67The CLAS Collaboration, 68The CLAS Collaboration, 69The CLAS Collaboration, 70The CLAS Collaboration, 71The CLAS Collaboration, 72The CLAS Collaboration, 73The CLAS Collaboration, 74The CLAS Collaboration, 75The CLAS Collaboration, 76The CLAS Collaboration, 77The CLAS Collaboration, 78The CLAS Collaboration, 79The CLAS Collaboration, 80The CLAS Collaboration, 81The CLAS Collaboration, 82The CLAS Collaboration, 83The CLAS Collaboration, 84The CLAS Collaboration, 85The CLAS Collaboration, 86The CLAS Collaboration, 87The CLAS Collaboration, 88The CLAS Collaboration, 89The CLAS Collaboration, 90The CLAS Collaboration, 91The CLAS Collaboration, 92The CLAS Collaboration, 93The CLAS Collaboration, 94The CLAS Collaboration, 95The CLAS Collaboration, 96The CLAS Collaboration, 97The CLAS Collaboration, 98The CLAS Collaboration, 99The CLAS Collaboration, 100The CLAS Collaboration, 101The CLAS Collaboration, 102The CLAS Collaboration, 103The CLAS Collaboration, 104The CLAS Collaboration, 105The CLAS Collaboration, 106The CLAS Collaboration, 107The CLAS Collaboration, 108The CLAS Collaboration, 109The CLAS Collaboration, 110The CLAS Collaboration, 111The CLAS Collaboration, 112The CLAS Collaboration, 113The CLAS Collaboration, 114The CLAS Collaboration, 115The CLAS Collaboration, 116The CLAS Collaboration, 117The CLAS Collaboration, 118The CLAS Collaboration, 119The CLAS Collaboration, 120The CLAS Collaboration, 121The CLAS Collaboration, 122The CLAS Collaboration, 123The CLAS Collaboration, 124The CLAS Collaboration, 125The CLAS Collaboration, 126The CLAS Collaboration, 127The CLAS Collaboration, 128The CLAS Collaboration, 129The CLAS Collaboration, 130The CLAS Collaboration, 131The CLAS Collaboration, 132The CLAS Collaboration, 133The CLAS Collaboration, 134The CLAS Collaboration, 135The CLAS Collaboration, 136The CLAS Collaboration, 137The CLAS Collaboration, 138The CLAS Collaboration, 139The CLAS Collaboration, 140The CLAS Collaboration, 141The CLAS Collaboration, 142The CLAS Collaboration, 143The CLAS Collaboration, 144The CLAS Collaboration, 145The CLAS Collaboration, 146The CLAS Collaboration, 147The CLAS Collaboration, 148The CLAS Collaboration, 149The CLAS Collaboration, 150The CLAS Collaboration, 151The CLAS Collaboration, 152The CLAS Collaboration, 153The CLAS Collaboration, 154The CLAS Collaboration, 155The CLAS Collaboration, 156The CLAS Collaboration

Beam-target double-spin asymmetries and target single-spin asymmetries were measured for the exclusive $\pi^0$ electroproduction reaction $\gamma^* p \to p \pi^0$, expanding an analysis of the $\gamma^* p \to n \pi^+$ reaction from the same experiment. The results were obtained from scattering of 6 GeV longitudinally polarized electrons off longitudinally polarized protons using the CEBAF Large Acceptance Spectrometer at Jefferson Lab. The kinematic range covered is $1. Read More

2016Sep
Authors: A. Albert, M. André, G. Anton, M. Ardid, J. -J. Aubert, T. Avgitas, B. Baret, J. Barrios-Martí, S. Basa, V. Bertin, S. Biagi, R. Bormuth, M. C. Bouwhuis, R. Bruijn, J. Brunner, J. Busto, A. Capone, L. Caramete, J. Carr, S. Celli, T. Chiarusi, M. Circella, 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. Geiÿelsöder, K. Geyer, V. Giordano, A. Gleixner, H. Glotin, R. Gracia-Ruiz, K. Graf, S. Hallmann, H. van Haren, A. J. Heijboer, Y. Hello, J. J. Hernández-Rey, J. Höÿl, J. Hofestädt, C. Hugon, G. Illuminati, C. W. James, M. de Jong, M. Jongen, M. Kadler, O. Kalekin, U. Katz, D. Kieÿling, A. Kouchner, M. Kreter, I. Kreykenbohm, V. Kulikovskiy, C. Lachaud, R. Lahmann, D. Lefèvre, E. Leonora, S. Loucatos, M. Marcelin, A. Margiotta, A. Marinelli, J. A. Martínez-Mora, A. Mathieu, K. Melis, T. Michael, P. Migliozzi, A. Moussa, C. Mueller, E. Nezri, G. E. Pavalas, C. Pellegrino, C. Perrina, P. Piattelli, V. Popa, T. Pradier, C. Racca, G. Riccobene, K. Roensch, M. Saldaña, D. F. E. Samtleben, A. Sánchez-Losa, M. Sanguineti, P. Sapienza, J. Schnabel, F. Schüssler, T. Seitz, C. Sieger, M. Spurio, Th. Stolarczyk, M. Taiuti, A. Trovato, M. Tselengidou, D. Turpin, C. Tönnis, B. Vallage, C. Vallée, V. Van Elewyck, D. Vivolo, S. Wagner, J. Wilms, J. D. Zornoza, J. Zúñiga

ANTARES is currently the largest neutrino telescope operating in the Northern Hemisphere, aiming at the detection of high-energy neutrinos from astrophysical sources. Neutrino telescopes constantly monitor at least one complete hemisphere of the sky, and are thus well-suited to detect neutrinos produced in transient astrophysical sources. A timedependent search has been applied to a list of 33 x-ray binaries undergoing high flaring activities in satellite data (RXTE/ASM, MAXI and Swift/BAT) and during hardness transition states in the 2008-2012 period. Read More

2016Aug
Authors: ANTARES Collaboration, S. Adrian-Martínez, A. Albert, M. André, M. Anghinolfi, G. Anton, M. Ardid, J. -J. Aubert, B. Baret, J. Barrios-Marti, S. Basa, V. Bertin, S. Biagi, R. Bormuth, M. C. Bouwhuis, R. Bruijn, J. Brunner, J. Busto, A. Capone, L. Caramete, J. Carr, T. Chiarusi, M. Circella, R. Coniglione, H. Costantini, P. Coyle, A. Creusot, I. Dekeyser, A. Deschamps, G. De Bonis, C. Distefano, C. Donzaud, D. Dornic, D. Drouhin, A. Dumas, T. Eberl, D. Elsasser, A. Enzenhofer, K. Fehn, I. Felis, P. Fermani, F. Folger, L. A. Fusco, S. Galatà, P. Gay, S. Geisselsoeder, K. Geyer, V. Giordano, A. Gleixner, R. Gracia-Ruiz, K. Graf, S. Hallmann, H. van Haren, A. J. Heijboer, Y. Hello, J. J. Hernàndez-Rey, J. Hoessl, J. Hofestadt, C. Hugon, C. W. James, M. de Jong, M. Kadler, M. Kadler, O. Kalekin, U. Katz, D. Kiessling, P. Kooijman, A. Kouchner, M. Kreter, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, D. Lefèvre, E. Leonora, S. Loucatos, M. Marcelin, A. Margiotta, A. Marinelli, J. A. Martínez-Mora, A. Mathieu, T. Michael, P. Migliozzi, A. Moussa, C. Muller, E. Nezri, G. E. Pavalas, C. Pellegrino, C. Perrina, P. Piattelli, V. Popa, T. Pradier, C. Racca, G. Riccobene, R. Richter, K. Roensch, M. Saldaña, D. F. E. Samtleben, A. Sánchez-Losa, M. Sanguineti, P. Sapienza, J. Schmid, J. Schnabel, F. Schussler, T. Seitz, C. Sieger, M. Spurio, J. J. M. Steijger, Th. Stolarczyk, M. Taiuti, C. Tamburini, A. Trovato, M. Tselengidou, C. Tonnis, B. Vallage, C. Vallée, V. Van Elewyck, E. Visser, D. Vivolo, S. Wagner, J. Wilms, J. D. Zornoza, J. Zúñiga

A search for high-energy neutrino emission correlated with gamma-ray bursts outside the electromagnetic prompt-emission time window is presented. Using a stacking approach of the time delays between reported gamma-ray burst alerts and spatially coincident muon-neutrino signatures, data from the Antares neutrino telescope recorded between 2007 and 2012 are analysed. One year of public data from the IceCube detector between 2008 and 2009 have been also investigated. Read More

2016Aug
Authors: Jim Alexander, Marco Battaglieri, Bertrand Echenard, Rouven Essig, Matthew Graham, Eder Izaguirre, John Jaros, Gordan Krnjaic, Jeremy Mardon, David Morrissey, Tim Nelson, Maxim Perelstein, Matt Pyle, Adam Ritz, Philip Schuster, Brian Shuve, Natalia Toro, Richard G Van De Water, Daniel Akerib, Haipeng An, Konrad Aniol, Isaac J. Arnquist, David M. Asner, Henning O. Back, Keith Baker, Nathan Baltzell, Dipanwita Banerjee, Brian Batell, Daniel Bauer, James Beacham, Jay Benesch, James Bjorken, Nikita Blinov, Celine Boehm, Mariangela Bondí, Walter Bonivento, Fabio Bossi, Stanley J. Brodsky, Ran Budnik, Stephen Bueltmann, Masroor H. Bukhari, Raymond Bunker, Massimo Carpinelli, Concetta Cartaro, David Cassel, Gianluca Cavoto, Andrea Celentano, Animesh Chaterjee, Saptarshi Chaudhuri, Gabriele Chiodini, Hsiao-Mei Sherry Cho, Eric D. Church, D. A. Cooke, Jodi Cooley, Robert Cooper, Ross Corliss, Paolo Crivelli, Francesca Curciarello, Annalisa D'Angelo, Hooman Davoudiasl, Marzio De Napoli, Raffaella De Vita, Achim Denig, Patrick deNiverville, Abhay Deshpande, Ranjan Dharmapalan, Bogdan Dobrescu, Sergey Donskov, Raphael Dupre, Juan Estrada, Stuart Fegan, Torben Ferber, Clive Field, Enectali Figueroa-Feliciano, Alessandra Filippi, Bartosz Fornal, Arne Freyberger, Alexander Friedland, Iftach Galon, Susan Gardner, Francois-Xavier Girod, Sergei Gninenko, Andrey Golutvin, Stefania Gori, Christoph Grab, Enrico Graziani, Keith Griffioen, Andrew Haas, Keisuke Harigaya, Christopher Hearty, Scott Hertel, JoAnne Hewett, Andrew Hime, David Hitlin, Yonit Hochberg, Roy J. Holt, Maurik Holtrop, Eric W. Hoppe, Todd W. Hossbach, Lauren Hsu, Phil Ilten, Joe Incandela, Gianluca Inguglia, Kent Irwin, Igal Jaegle, Robert P. Johnson, Yonatan Kahn, Grzegorz Kalicy, Zhong-Bo Kang, Vardan Khachatryan, Venelin Kozhuharov, N. V. Krasnikov, Valery Kubarovsky, Eric Kuflik, Noah Kurinsky, Ranjan Laha, Gaia Lanfranchi, Dale Li, Tongyan Lin, Mariangela Lisanti, Kun Liu, Ming Liu, Ben Loer, Dinesh Loomba, Valery E. Lyubovitskij, Aaron Manalaysay, Giuseppe Mandaglio, Jeremiah Mans, W. J. Marciano, Thomas Markiewicz, Luca Marsicano, Takashi Maruyama, Victor A. Matveev, David McKeen, Bryan McKinnon, Dan McKinsey, Harald Merkel, Jeremy Mock, Maria Elena Monzani, Omar Moreno, Corina Nantais, Sebouh Paul, Michael Peskin, Vladimir Poliakov, Antonio D Polosa, Maxim Pospelov, Igor Rachek, Balint Radics, Mauro Raggi, Nunzio Randazzo, Blair Ratcliff, Alessandro Rizzo, Thomas Rizzo, Alan Robinson, Andre Rubbia, David Rubin, Dylan Rueter, Tarek Saab, Elena Santopinto, Richard Schnee, Jessie Shelton, Gabriele Simi, Ani Simonyan, Valeria Sipala, Oren Slone, Elton Smith, Daniel Snowden-Ifft, Matthew Solt, Peter Sorensen, Yotam Soreq, Stefania Spagnolo, James Spencer, Stepan Stepanyan, Jan Strube, Michael Sullivan, Arun S. Tadepalli, Tim Tait, Mauro Taiuti, Philip Tanedo, Rex Tayloe, Jesse Thaler, Nhan V. Tran, Sean Tulin, Christopher G. Tully, Sho Uemura, Maurizio Ungaro, Paolo Valente, Holly Vance, Jerry Vavra, Tomer Volansky, Belina von Krosigk, Andrew Whitbeck, Mike Williams, Peter Wittich, Bogdan Wojtsekhowski, Wei Xue, Jong Min Yoon, Hai-Bo Yu, Jaehoon Yu, Tien-Tien Yu, Yue Zhang, Yue Zhao, Yiming Zhong, Kathryn Zurek

This report, based on the Dark Sectors workshop at SLAC in April 2016, summarizes the scientific importance of searches for dark sector dark matter and forces at masses beneath the weak-scale, the status of this broad international field, the important milestones motivating future exploration, and promising experimental opportunities to reach these milestones over the next 5-10 years. Read More

2016Jul
Authors: P. E. Bosted1, M. J. Amaryan2, S. Anefalos Pereira3, H. Avakian4, R. A. Badui5, J. Ball6, N. A. Baltzell7, M. Battaglieri8, V. Batourine9, I. Bedlinskiy10, A. S. Biselli11, W. J. Briscoe12, S. Bültmann13, V. D. Burkert14, D. S. Carman15, A. Celentano16, S. Chandavar17, G. Charles18, L. Clark19, L. Colaneri20, P. L. Cole21, M. Contalbrigo22, V. Crede23, A. D'Angelo24, R. De Vita25, A. Deur26, E. De Sanctis27, C. Djalali28, R. Dupre29, H. Egiyan30, A. El Alaoui31, L. El Fassi32, L. Elouadrhiri33, P. Eugenio34, E. Fanchini35, G. Fedotov36, A. Filippi37, J. A. Fleming38, T. Forest39, A. Fradi40, N. Gevorgyan41, G. P. Gilfoyle42, F. X. Girod43, C. Gleason44, W. Gohn45, E. Golovatch46, R. W. Gothe47, K. A. Griffioen48, M. Guidal49, H. Hakobyan50, M. Hattawy51, K. Hicks52, M. Holtrop53, S. M. Hughes54, Y. Ilieva55, D. G. Ireland56, B. S. Ishkhanov57, E. L. Isupov58, H. Jiang59, H. S. Jo60, K. Joo61, S. Joosten62, G. Khachatryan63, M. Khandaker64, A. Kim65, W. Kim66, F. J. Klein67, S. Koirala68, V. Kubarovsky69, S. E. Kuhn70, L. Lanza71, L. A. Net72, P. Lenisa73, K. Livingston74, I. J. D. MacGregor75, M. E. McCracken76, B. McKinnon77, C. A. Meyer78, M. Mirazita79, V. I. Mokeev80, R. A. Montgomery81, E. Munevar82, C. Munoz Camacho83, G. Murdoch84, P. Nadel-Turonski85, S. Niccolai86, M. Osipenko87, A. I. Ostrovidov88, K. Park89, E. Pasyuk90, P. Peng91, W. Phelps92, S. Pisano93, O. Pogorelko94, J. W. Price95, Y. Prok96, D. Protopopescu97, B. A. Raue98, M. Ripani99, G. Rosner100, P. Rossi101, R. A. Schumacher102, Iu. Skorodumina103, G. D. Smith104, D. Sokhan105, N. Sparveris106, I. Stankovic107, I. I. Strakovsky108, S. Strauch109, M. Taiuti110, B. Torayev111, M. Ungaro112, H. Voskanyan113, E. Voutier114, X. Wei115, L. B. Weinstein116, J. Zhang117, I. Zonta118
Affiliations: 1CLAS Collaboration, 2CLAS Collaboration, 3CLAS Collaboration, 4CLAS Collaboration, 5CLAS Collaboration, 6CLAS Collaboration, 7CLAS Collaboration, 8CLAS Collaboration, 9CLAS Collaboration, 10CLAS Collaboration, 11CLAS Collaboration, 12CLAS Collaboration, 13CLAS Collaboration, 14CLAS Collaboration, 15CLAS Collaboration, 16CLAS Collaboration, 17CLAS Collaboration, 18CLAS Collaboration, 19CLAS Collaboration, 20CLAS Collaboration, 21CLAS Collaboration, 22CLAS Collaboration, 23CLAS Collaboration, 24CLAS Collaboration, 25CLAS Collaboration, 26CLAS Collaboration, 27CLAS Collaboration, 28CLAS Collaboration, 29CLAS Collaboration, 30CLAS Collaboration, 31CLAS Collaboration, 32CLAS Collaboration, 33CLAS Collaboration, 34CLAS Collaboration, 35CLAS Collaboration, 36CLAS Collaboration, 37CLAS Collaboration, 38CLAS Collaboration, 39CLAS Collaboration, 40CLAS Collaboration, 41CLAS Collaboration, 42CLAS Collaboration, 43CLAS Collaboration, 44CLAS Collaboration, 45CLAS Collaboration, 46CLAS Collaboration, 47CLAS Collaboration, 48CLAS Collaboration, 49CLAS Collaboration, 50CLAS Collaboration, 51CLAS Collaboration, 52CLAS Collaboration, 53CLAS Collaboration, 54CLAS Collaboration, 55CLAS Collaboration, 56CLAS Collaboration, 57CLAS Collaboration, 58CLAS Collaboration, 59CLAS Collaboration, 60CLAS Collaboration, 61CLAS Collaboration, 62CLAS Collaboration, 63CLAS Collaboration, 64CLAS Collaboration, 65CLAS Collaboration, 66CLAS Collaboration, 67CLAS Collaboration, 68CLAS Collaboration, 69CLAS Collaboration, 70CLAS Collaboration, 71CLAS Collaboration, 72CLAS Collaboration, 73CLAS Collaboration, 74CLAS Collaboration, 75CLAS Collaboration, 76CLAS Collaboration, 77CLAS Collaboration, 78CLAS Collaboration, 79CLAS Collaboration, 80CLAS Collaboration, 81CLAS Collaboration, 82CLAS Collaboration, 83CLAS Collaboration, 84CLAS Collaboration, 85CLAS Collaboration, 86CLAS Collaboration, 87CLAS Collaboration, 88CLAS Collaboration, 89CLAS Collaboration, 90CLAS Collaboration, 91CLAS Collaboration, 92CLAS Collaboration, 93CLAS Collaboration, 94CLAS Collaboration, 95CLAS Collaboration, 96CLAS Collaboration, 97CLAS Collaboration, 98CLAS Collaboration, 99CLAS Collaboration, 100CLAS Collaboration, 101CLAS Collaboration, 102CLAS Collaboration, 103CLAS Collaboration, 104CLAS Collaboration, 105CLAS Collaboration, 106CLAS Collaboration, 107CLAS Collaboration, 108CLAS Collaboration, 109CLAS Collaboration, 110CLAS Collaboration, 111CLAS Collaboration, 112CLAS Collaboration, 113CLAS Collaboration, 114CLAS Collaboration, 115CLAS Collaboration, 116CLAS Collaboration, 117CLAS Collaboration, 118CLAS Collaboration

Beam-target double-spin asymmetries and target single-spin asymmetries were measured for the exclusive $\pi^+$ electroproduction reaction $\gamma^* p \to n \pi^+$. The results were obtained from scattering of 6 GeV longitudinally polarized electrons off longitudinally polarized protons using the CEBAF Large Acceptance Spectrometer at Jefferson Lab. The kinematic range covered is $1. Read More

2016Jul
Authors: X. Zheng1, K. P. Adhikari2, P. Bosted3, A. Deur4, V. Drozdov5, L. El Fassi6, Hyekoo Kang7, K. Kovacs8, S. Kuhn9, E. Long10, S. K. Phillips11, M. Ripani12, K. Slifer13, L. C. Smith14, D. Adikaram15, Z. Akbar16, M. J. Amaryan17, S. Anefalos Pereira18, G. Asryan19, H. Avakian20, R. A. Badui21, J. Ball22, N. A. Baltzell23, M. Battaglieri24, V. Batourine25, I. Bedlinskiy26, A. S. Biselli27, W. J. Briscoe28, S. Bültmann29, V. D. Burkert30, D. S. Carman31, A. Celentano32, S. Chandavar33, G. Charles34, J. -P. Chen35, T. Chetry36, Seonho Choi37, G. Ciullo38, L. Clark39, L. Colaneri40, P. L. Cole41, N. Compton42, M. Contalbrigo43, V. Crede44, A. D'Angelo45, N. Dashyan46, R. De Vita47, E. De Sanctis48, C. Djalali49, G. E. Dodge50, R. Dupre51, H. Egiyan52, A. El Alaoui53, L. Elouadrhiri54, P. Eugenio55, E. Fanchini56, G. Fedotov57, R. Fersch58, A. Filippi59, J. A. Fleming60, N. Gevorgyan61, Y. Ghandilyan62, G. P. Gilfoyle63, K. L. Giovanetti64, F. X. Girod65, C. Gleason66, E. Golovach67, R. W. Gothe68, K. A. Griffioen69, M. Guidal70, N. Guler71, L. Guo72, C. Hanretty73, N. Harrison74, M. Hattawy75, K. Hicks76, M. Holtrop77, S. M. Hughes78, Y. Ilieva79, D. G. Ireland80, B. S. Ishkhanov81, E. L. Isupov82, D. Jenkins83, H. Jiang84, H. S. Jo85, S. Joosten86, D. Keller87, G. Khachatryan88, M. Khandaker89, A. Kim90, W. Kim91, F. J. Klein92, V. Kubarovsky93, L. Lanza94, P. Lenisa95, K. Livingston96, I . J . D. MacGregor97, N. Markov98, B. McKinnon99, M. Mirazita100, V. Mokeev101, A. Movsisyan102, E. Munevar103, C. Munoz Camacho104, G. Murdoch105, P. Nadel-Turonski106, L. A. Net107, A. Ni108, S. Niccolai109, G. Niculescu110, I. Niculescu111, M. Osipenko112, A. I. Ostrovidov113, M. Paolone114, R. Paremuzyan115, K. Park116, E. Pasyuk117, P. Peng118, S. Pisano119, O. Pogorelko120, J. W. Price121, A. J. R. Puckett122, B. A. Raue123, A. Rizzo124, G. Rosner125, P. Rossi126, P. Roy127, F. Sabatié128, C. Salgado129, R. A. Schumacher130, Y. G. Sharabian131, Iu. Skorodumina132, G. D. Smith133, D. Sokhan134, N. Sparveris135, I. Stankovic136, I. I. Strakovsky137, S. Strauch138, M. Taiuti139, Ye Tian140, M. Ungaro141, H. Voskanyan142, E. Voutier143, N. K. Walford144, D. P. Watts145, X. Wei146, L. B. Weinstein147, M. H. Wood148, N. Zachariou149, J. Zhang150
Affiliations: 1The CLAS Collaboration, 2The CLAS Collaboration, 3The CLAS Collaboration, 4The CLAS Collaboration, 5The CLAS Collaboration, 6The CLAS Collaboration, 7The CLAS Collaboration, 8The CLAS Collaboration, 9The CLAS Collaboration, 10The CLAS Collaboration, 11The CLAS Collaboration, 12The CLAS Collaboration, 13The CLAS Collaboration, 14The CLAS Collaboration, 15The CLAS Collaboration, 16The CLAS Collaboration, 17The CLAS Collaboration, 18The CLAS Collaboration, 19The CLAS Collaboration, 20The CLAS Collaboration, 21The CLAS Collaboration, 22The CLAS Collaboration, 23The CLAS Collaboration, 24The CLAS Collaboration, 25The CLAS Collaboration, 26The CLAS Collaboration, 27The CLAS Collaboration, 28The CLAS Collaboration, 29The CLAS Collaboration, 30The CLAS Collaboration, 31The CLAS Collaboration, 32The CLAS Collaboration, 33The CLAS Collaboration, 34The CLAS Collaboration, 35The CLAS Collaboration, 36The CLAS Collaboration, 37The CLAS Collaboration, 38The CLAS Collaboration, 39The CLAS Collaboration, 40The CLAS Collaboration, 41The CLAS Collaboration, 42The CLAS Collaboration, 43The CLAS Collaboration, 44The CLAS Collaboration, 45The CLAS Collaboration, 46The CLAS Collaboration, 47The CLAS Collaboration, 48The CLAS Collaboration, 49The CLAS Collaboration, 50The CLAS Collaboration, 51The CLAS Collaboration, 52The CLAS Collaboration, 53The CLAS Collaboration, 54The CLAS Collaboration, 55The CLAS Collaboration, 56The CLAS Collaboration, 57The CLAS Collaboration, 58The CLAS Collaboration, 59The CLAS Collaboration, 60The CLAS Collaboration, 61The CLAS Collaboration, 62The CLAS Collaboration, 63The CLAS Collaboration, 64The CLAS Collaboration, 65The CLAS Collaboration, 66The CLAS Collaboration, 67The CLAS Collaboration, 68The CLAS Collaboration, 69The CLAS Collaboration, 70The CLAS Collaboration, 71The CLAS Collaboration, 72The CLAS Collaboration, 73The CLAS Collaboration, 74The CLAS Collaboration, 75The CLAS Collaboration, 76The CLAS Collaboration, 77The CLAS Collaboration, 78The CLAS Collaboration, 79The CLAS Collaboration, 80The CLAS Collaboration, 81The CLAS Collaboration, 82The CLAS Collaboration, 83The CLAS Collaboration, 84The CLAS Collaboration, 85The CLAS Collaboration, 86The CLAS Collaboration, 87The CLAS Collaboration, 88The CLAS Collaboration, 89The CLAS Collaboration, 90The CLAS Collaboration, 91The CLAS Collaboration, 92The CLAS Collaboration, 93The CLAS Collaboration, 94The CLAS Collaboration, 95The CLAS Collaboration, 96The CLAS Collaboration, 97The CLAS Collaboration, 98The CLAS Collaboration, 99The CLAS Collaboration, 100The CLAS Collaboration, 101The CLAS Collaboration, 102The CLAS Collaboration, 103The CLAS Collaboration, 104The CLAS Collaboration, 105The CLAS Collaboration, 106The CLAS Collaboration, 107The CLAS Collaboration, 108The CLAS Collaboration, 109The CLAS Collaboration, 110The CLAS Collaboration, 111The CLAS Collaboration, 112The CLAS Collaboration, 113The CLAS Collaboration, 114The CLAS Collaboration, 115The CLAS Collaboration, 116The CLAS Collaboration, 117The CLAS Collaboration, 118The CLAS Collaboration, 119The CLAS Collaboration, 120The CLAS Collaboration, 121The CLAS Collaboration, 122The CLAS Collaboration, 123The CLAS Collaboration, 124The CLAS Collaboration, 125The CLAS Collaboration, 126The CLAS Collaboration, 127The CLAS Collaboration, 128The CLAS Collaboration, 129The CLAS Collaboration, 130The CLAS Collaboration, 131The CLAS Collaboration, 132The CLAS Collaboration, 133The CLAS Collaboration, 134The CLAS Collaboration, 135The CLAS Collaboration, 136The CLAS Collaboration, 137The CLAS Collaboration, 138The CLAS Collaboration, 139The CLAS Collaboration, 140The CLAS Collaboration, 141The CLAS Collaboration, 142The CLAS Collaboration, 143The CLAS Collaboration, 144The CLAS Collaboration, 145The CLAS Collaboration, 146The CLAS Collaboration, 147The CLAS Collaboration, 148The CLAS Collaboration, 149The CLAS Collaboration, 150The CLAS Collaboration

We report measurements of target- and double-spin asymmetries for the exclusive channel $\vec e\vec p\to e\pi^+ (n)$ in the nucleon resonance region at Jefferson Lab using the CEBAF Large Acceptance Spectrometer (CLAS). These asymmetries were extracted from data obtained using a longitudinally polarized NH$_3$ target and a longitudinally polarized electron beam with energies 1.1, 1. Read More

2016Jul

MeV-GeV dark matter (DM) is theoretically well motivated but remarkably unexplored. This proposal presents the MeV-GeV DM discovery potential for a $\sim$1 m$^3$ segmented CsI(Tl) scintillator detector placed downstream of the Hall A beam-dump at Jefferson Lab, receiving up to 10$^{22}$ electrons-on-target (EOT) in 285 days. This experiment (Beam-Dump eXperiment or BDX) would be sensitive to elastic DM-electron and to inelastic DM scattering at the level of 10 counts per year, reaching the limit of the neutrino irreducible background. Read More

2016Apr
Authors: P. E. Bosted1, A. S. Biselli2, S. Careccia3, G. Dodge4, R. Fersch5, S. E. Kuhn6, J. Pierce7, Y. Prok8, X. Zheng9, K. P. Adhikari10, D. Adikaram11, Z. Akbar12, M. J. Amaryan13, S. Anefalos Pereira14, G. Asryan15, H. Avakian16, R. A. Badui17, J. Ball18, N. A. Baltzell19, M. Battaglieri20, V. Batourine21, I. Bedlinskiy22, S. Boiarinov23, W. J. Briscoe24, S. Bültmann25, V. D. Burkert26, T. Cao27, D. S. Carman28, A. Celentano29, S. Chandavar30, G. Charles31, T. Chetry32, G. Ciullo33, L. Clark34, L. Colaneri35, P. L. Cole36, M. Contalbrigo37, O. Cortes38, V. Crede39, A. D'Angelo40, N. Dashyan41, R. De Vita42, A. Deur43, C. Djalali44, R. Dupre45, H. Egiyan46, A. El Alaoui47, L. El Fassi48, P. Eugenio49, E. Fanchini50, G. Fedotov51, A. Filippi52, J. A. Fleming53, T. A. Forest54, A. Fradi55, M. Garçon56, N. Gevorgyan57, Y. Ghandilyan58, G. P. Gilfoyle59, K. L. Giovanetti60, F. X. Girod61, C. Gleason62, W. Gohn63, E. Golovatch64, R. W. Gothe65, K. A. Griffioen66, N. Guler67, L. Guo68, K. Hafidi69, C. Hanretty70, N. Harrison71, M. Hattawy72, D. Heddle73, K. Hicks74, M. Holtrop75, S. M. Hughes76, Y. Ilieva77, D. G. Ireland78, B. S. Ishkhanov79, E. L. Isupov80, D. Jenkins81, H. Jiang82, H. S. Jo83, K. Joo84, S. Joosten85, D. Keller86, M. Khandaker87, W. Kim88, A. Klein89, F. J. Klein90, V. Kubarovsky91, S. V. Kuleshov92, L. Lanza93, P. Lenisa94, K. Livingston95, H. Y. Lu96, I . J . D. MacGregor97, N. Markov98, M. E. McCracken99, B. McKinnon100, C. A. Meyer101, R. Minehart102, M. Mirazita103, V. Mokeev104, A Movsisyan105, E. Munevar106, C. Munoz Camacho107, P. Nadel-Turonski108, L. A. Net109, A. Ni110, S. Niccolai111, G. Niculescu112, I. Niculescu113, M. Osipenko114, A. I. Ostrovidov115, R. Paremuzyan116, K. Park117, E. Pasyuk118, P. Peng119, W. Phelps120, S. Pisano121, O. Pogorelko122, J. W. Price123, S. Procureur124, D. Protopopescu125, A. J. R. Puckett126, B. A. Raue127, M. Ripani128, A. Rizzo129, G. Rosner130, P. Rossi131, P. Roy132, F. Sabatié133, C. Salgado134, R. A. Schumacher135, E. Seder136, Y. G. Sharabian137, A. Simonyan138, Iu. Skorodumina139, G. D. Smith140, N. Sparveris141, Ivana Stankovic142, S. Stepanyan143, I. I. Strakovsky144, S. Strauch145, V. Sytnik146, M. Taiuti147, Ye Tian148, B. Torayev149, M. Ungaro150, H. Voskanyan151, E. Voutier152, N. K. Walford153, D. P. Watts154, X. Wei155, L. B. Weinstein156, M. H. Wood157, N. Zachariou158, L. Zana159, J. Zhang160, Z. W. Zhao161, I. Zonta162
Affiliations: 1CLAS Collaboration, 2CLAS Collaboration, 3CLAS Collaboration, 4CLAS Collaboration, 5CLAS Collaboration, 6CLAS Collaboration, 7CLAS Collaboration, 8CLAS Collaboration, 9CLAS Collaboration, 10CLAS Collaboration, 11CLAS Collaboration, 12CLAS Collaboration, 13CLAS Collaboration, 14CLAS Collaboration, 15CLAS Collaboration, 16CLAS Collaboration, 17CLAS Collaboration, 18CLAS Collaboration, 19CLAS Collaboration, 20CLAS Collaboration, 21CLAS Collaboration, 22CLAS Collaboration, 23CLAS Collaboration, 24CLAS Collaboration, 25CLAS Collaboration, 26CLAS Collaboration, 27CLAS Collaboration, 28CLAS Collaboration, 29CLAS Collaboration, 30CLAS Collaboration, 31CLAS Collaboration, 32CLAS Collaboration, 33CLAS Collaboration, 34CLAS Collaboration, 35CLAS Collaboration, 36CLAS Collaboration, 37CLAS Collaboration, 38CLAS Collaboration, 39CLAS Collaboration, 40CLAS Collaboration, 41CLAS Collaboration, 42CLAS Collaboration, 43CLAS Collaboration, 44CLAS Collaboration, 45CLAS Collaboration, 46CLAS Collaboration, 47CLAS Collaboration, 48CLAS Collaboration, 49CLAS Collaboration, 50CLAS Collaboration, 51CLAS Collaboration, 52CLAS Collaboration, 53CLAS Collaboration, 54CLAS Collaboration, 55CLAS Collaboration, 56CLAS Collaboration, 57CLAS Collaboration, 58CLAS Collaboration, 59CLAS Collaboration, 60CLAS Collaboration, 61CLAS Collaboration, 62CLAS Collaboration, 63CLAS Collaboration, 64CLAS Collaboration, 65CLAS Collaboration, 66CLAS Collaboration, 67CLAS Collaboration, 68CLAS Collaboration, 69CLAS Collaboration, 70CLAS Collaboration, 71CLAS Collaboration, 72CLAS Collaboration, 73CLAS Collaboration, 74CLAS Collaboration, 75CLAS Collaboration, 76CLAS Collaboration, 77CLAS Collaboration, 78CLAS Collaboration, 79CLAS Collaboration, 80CLAS Collaboration, 81CLAS Collaboration, 82CLAS Collaboration, 83CLAS Collaboration, 84CLAS Collaboration, 85CLAS Collaboration, 86CLAS Collaboration, 87CLAS Collaboration, 88CLAS Collaboration, 89CLAS Collaboration, 90CLAS Collaboration, 91CLAS Collaboration, 92CLAS Collaboration, 93CLAS Collaboration, 94CLAS Collaboration, 95CLAS Collaboration, 96CLAS Collaboration, 97CLAS Collaboration, 98CLAS Collaboration, 99CLAS Collaboration, 100CLAS Collaboration, 101CLAS Collaboration, 102CLAS Collaboration, 103CLAS Collaboration, 104CLAS Collaboration, 105CLAS Collaboration, 106CLAS Collaboration, 107CLAS Collaboration, 108CLAS Collaboration, 109CLAS Collaboration, 110CLAS Collaboration, 111CLAS Collaboration, 112CLAS Collaboration, 113CLAS Collaboration, 114CLAS Collaboration, 115CLAS Collaboration, 116CLAS Collaboration, 117CLAS Collaboration, 118CLAS Collaboration, 119CLAS Collaboration, 120CLAS Collaboration, 121CLAS Collaboration, 122CLAS Collaboration, 123CLAS Collaboration, 124CLAS Collaboration, 125CLAS Collaboration, 126CLAS Collaboration, 127CLAS Collaboration, 128CLAS Collaboration, 129CLAS Collaboration, 130CLAS Collaboration, 131CLAS Collaboration, 132CLAS Collaboration, 133CLAS Collaboration, 134CLAS Collaboration, 135CLAS Collaboration, 136CLAS Collaboration, 137CLAS Collaboration, 138CLAS Collaboration, 139CLAS Collaboration, 140CLAS Collaboration, 141CLAS Collaboration, 142CLAS Collaboration, 143CLAS Collaboration, 144CLAS Collaboration, 145CLAS Collaboration, 146CLAS Collaboration, 147CLAS Collaboration, 148CLAS Collaboration, 149CLAS Collaboration, 150CLAS Collaboration, 151CLAS Collaboration, 152CLAS Collaboration, 153CLAS Collaboration, 154CLAS Collaboration, 155CLAS Collaboration, 156CLAS Collaboration, 157CLAS Collaboration, 158CLAS Collaboration, 159CLAS Collaboration, 160CLAS Collaboration, 161CLAS Collaboration, 162CLAS Collaboration

Beam-target double spin asymmetries and target single-spin asymmetries in exclusive $\pi^+$ and $\pi^-$ electroproduction were obtained from scattering of 1.6 to 5.7 GeV longitudinally polarized electrons from longitudinally polarized protons (for $\pi^+$) and deuterons (for $\pi^-$) using the CEBAF Large Acceptance Spectrometer (CLAS) at Jefferson Lab. Read More

2016Mar
Authors: ANTARES collaboration, S. Adrián-Martínez, A. Albert, M. André, G. Anton, M. Ardid, J. -J. Aubert, T. Avgitas, B. Baret, J. Barrios-Martí, S. Basa, V. Bertin, S. Biagi, R. Bormuth, M. C. Bouwhuis, R. Bruijn, J. Brunner, J. Busto, A. Capone, L. Caramete, J. Carr, S. Celli, T. Chiarusi, M. Circella, A. Coleiro, R. Coniglione, H. Costantini, P. Coyle, A. Creusot, A. Deschamps, G. De Bonis, C. Distefano, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, I. El Bojaddaini, D. Elsässer, A. Enzenhöfer, K. Fehn, I. Felis, L. A. Fusco, S. Galatà, P. Gay, S. Geißelsöder, K. Geyer, V. Giordano, A. Gleixner, H. Glotin, 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. Lefèver, E. Leonora, S. Loucatos, M. Marcelin, A. Margiotta, A. Marinelli, J. A. Martínez-Mora, A. Mathieu, 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, C. Racca, G. Riccobene, K. Roensch, M. Saldana, D. F. E. Samtleben, A. Sánchez-Losa, M. Sanguineti, P. Sapienza, J. Schnabel, F. Schüssler, T. Seitz, C. Sieger, M. Spurio, Th. Stolarczyk, M. Taiuti, C. Tönnis, A. Trovato, M. Tselengidou, D. Turpin, B. Vallage, C. Vallée, V. Van Elewyck, D. Vivolo, S. Wagner, J. Wilms, J. D. Zornoza, J. Zúñiga

A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and $90\%$ C. Read More

2016Mar
Authors: S. Croft, D. L. Kaplan, S. J. Tingay, T. Murphy, M. E. Bell, A. Rowlinson, S. Adrian-Martinez, M. Ageron, A. Albert, M. Andre, G. Anton, M. Ardid, J. -J. Aubert, T. Avgitas, B. Baret, J. Barrios-Marti, S. Basa, V. Bertin, S. Biagi, R. Bormuth, M. C. Bouwhuis, R. Bruijn, J. Brunner, J. Busto, A. Capone, L. Caramete, J. Carr, T. Chiarusi, M. Circella, A. Coleiro, R. Coniglione, H. Costantini, P. Coyle, A. Creusot, I. Dekeyser, A. Deschamps, G. De Bonis, C. Distefano, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, I. El Bojaddaini, D. Elsasser, A. Enzenhofer, K. Fehn, I. Felis, P. Fermani, L. A. Fusco, S. Galata, P. Gay, S. Geisselsoder, K. Geyer, V. Giordano, A. Gleixner, H. Glotin, R. Gracia-Ruiz, K. Graf, S. Hallmann, H. van Haren, A. J. Heijboer, Y. Hello, J. J. Hernandez-Rey, J. Hossl, J. Hofestadt, C. Hugon, C. W James, M. de Jong, M. Kadler, O. Kalekin, U. Katz, D. Kiessling, P. Kooijman, A. Kouchner, M. Kreter, I. Kreykenbohm, V. Kulikovskiy, C. Lachaud, R. Lahmann, D. Lefevre, E. Leonora, S. Loucatos, M. Marcelin, A. Margiotta, A. Marinelli, J. A. Martinez-Mora, A. Mathieu, T. Michael, P. Migliozzi, A. Moussa, C. Mueller, E. Nezri, G. E. Pavalas, C. Pellegrino, C. Perrina, P. Piattelli, V. Popa, T. Pradier, C. Racca, G. Riccobene, K. Roensch, M. Saldana, D. F. E. Samtleben, A. Sanchez-Losa, M. Sanguineti, P. Sapienza, J. Schmid, J. Schnabel, F. Schussler, T. Seitz, C. Sieger, M. Spurio, J. J. M. Steijger, T. Stolarczyk, M. Taiuti, C. Tamburini, A. Trovato, M. Tselengidou, D. Turpin, C. Tonnis, B. Vallage, C. Vallee, V. Van Elewyck, E. Visser, D. Vivolo, S. Wagner, J. Wilms, J. D. Zornoza, J. Zuniga, A. Klotz, M. Boer, A. Le Van Suu, C. Akerlof, W. Zheng

We present a search, using the Murchison Widefield Array (MWA), for electromagnetic counterparts to two candidate high energy neutrino events detected by the ANTARES neutrino telescope in 2013 November and 2014 March. These events were selected by ANTARES because they are consistent, within 0.4 degrees, with the locations of galaxies within 20 Mpc of Earth. Read More

2016Mar
Authors: D. Rimal, D. Adikaram, B. A. Raue, L. B. Weinstein, J. Arrington, W. K. Brooks, M. Ungaro, K. P. Adhikari, Z. Akbar, S. Anefalos Pereira, R. A. Badui, J. Ball, N. A. Baltzell, M. Battaglieri, V. Batourine, I. Bedlinskiy, R. P. Bennett, A. S. Biselli, S. Boiarinov, W. J. Briscoe, S. Bültmann, D. S. Carman, A. Celentano, T. Chetry, G. Ciullo, L. Clark, L. Colaneri, P. L. Cole, N. Compton, M. Contalbrigo, O. Cortes, V. Crede, A. D'Angelo, N. Dashyan, R. De Vita, A. Deur, C. Djalali, R. Dupre, H. Egiyan, A. El Alaoui, L. El Fassi, P. Eugenio, G. Fedotov, R. Fersch, A. Filippi, J. A. Fleming, T. A. Forest, A. Fradi, N. Gevorgyan, Y. Ghandilyan, G. P. Gilfoyle, K. L. Giovanetti, F. X. Girod, C. Gleason, W. Gohn, E. Golovatch, R. W. Gothe, K. A. Griffioen, L. Guo, K. Hafidi, C. Hanretty, N. Harrison, M. Hattawy, D. Heddle, K. Hicks, M. Holtrop, S. M. Hughes, Y. Ilieva, D. G. Ireland, B. S. Ishkhanov, E. L. Isupov, D. Jenkins, H. Jiang, S. Joosten, D. Keller, P. Khetarpal, G. Khachatryan, M. Khandaker, W. Kim, A. Klein, F. J. Klein, V. Kubarovsky, S. E. Kuhn, S. V. Kuleshov, L. Lanza, P. Lenisa, K. Livingston, H. Y. Lu, I . J . D. MacGregor, N. Markov, B. McKinnon, M. D. Mestayer, M. Mirazita, V. Mokeev, A Movsisyan, E. Munevar, C. Munoz Camacho, P. Nadel-Turonski, A. Ni, S. Niccolai, G. Niculescu, I. Niculescu, M. Osipenko, A. I. Ostrovidov, M. Paolone, R. Paremuzyan, K. Park, E. Pasyuk, W. Phelps, S. Pisano, O. Pogorelko, J. W. Price, Y. Prok, D. Protopopescu, A. J. R. Puckett, A. Rizzo, G. Rosner, P. Rossi, P. Roy, F. Sabatié, C. Salgado, R. A. Schumacher, E. Seder, Y. G. Sharabian, Iu. Skorodumina, G. D. Smith, D. Sokhan, N. Sparveris, Ivana Stankovic, S. Stepanyan, S. Strauch, V. Sytnik, M. Taiuti, B. Torayev, H. Voskanyan, E. Voutier, N. K. Walford, D. P. Watts, X. Wei, M. H. Wood, N. Zachariou, L. Zana, J. Zhang, Z. W. Zhao, I. Zonta

[Background] The electromagnetic form factors of the proton measured by unpolarized and polarized electron scattering experiments show a significant disagreement that grows with the squared four momentum transfer ($Q^{2}$). Calculations have shown that the two measurements can be largely reconciled by accounting for the contributions of two-photon exchange (TPE). TPE effects are not typically included in the standard set of radiative corrections since theoretical calculations of the TPE effects are highly model dependent, and, until recently, no direct evidence of significant TPE effects has been observed. Read More

2016Feb
Authors: S. Adrián-Martínez, A. Albert, M. André, G. Anton, M. Ardid, J. -J. Aubert, T. Avgitas, B. Baret, J. Barrios-Martí, S. Basa, V. Bertin, S. Biagi, R. Bormuth, M. Bou-Cabo, M. C. Bouwhuis, R. Bruijn, J. Brunner, J. Busto, A. Capone, L. Caramete, J. Carr, S. Celli, T. Chiarusi, M. Circella, A. Coleiro, R. Coniglione, H. Costantini, P. Coyle, A. Creusot, A. Deschamps, G. De Bonis, C. Distefano, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, I. El Bojaddaini, D. Elsässer, A. Enzenhöfer, K. Fehn, I. Felis, L. A. Fusco, S. Galatà, P. Gay, S. Geißelsöder, K. Geyer, V. Giordano, A. Gleixner, H. Glotin, 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. Kadler, O. Kalekin, U. Katz, D. Kießling, A. Kouchner, M. Kreter, I. Kreykenbohm, V. Kulikovskiy, C. Lachaud, R. Lahmann, D. Lefèvre, E. Leonora, S. Loucatos, M. Marcelin, A. Margiotta, A. Marinelli, J. A. Martínez-Mora, A. Mathieu, T. Michael, P. Migliozzi, A. Moussa, C. Mueller, E. Nezri, G. E. Păvălaş, C. Pellegrino, C. Perrina, P. Piattelli, V. Popa, T. Pradier, C. Racca, G. Riccobene, K. Roensch, M. Saldaña, D. F. E. Samtleben, M. Sanguineti, P. Sapienza, J. Schnabel, F. Schüssler, T. Seitz, C. Sieger, M. Spurio, Th. Stolarczyk, A. Sánchez-Losa, M. Taiuti, A. Trovato, M. Tselengidou, D. Turpin, C. Tönnis, B. Vallage, C. Vallée, V. Van Elewyck, D. Vivolo, S. Wagner, J. Wilms, J. D. Zornoza, J. Zúñiga

A search for Secluded Dark Matter annihilation in the Sun using 2007-2012 data of the ANTARES neutrino telescope is presented. Three different cases are considered: a) detection of dimuons that result from the decay of the mediator, or neutrino detection from: b) mediator that decays into a dimuon and, in turn, into neutrinos, and c) mediator that decays directly into neutrinos. As no significant excess over background is observed, constraints are derived on the dark matter mass and the lifetime of the mediator. Read More

2016Feb
Authors: S. Adrián-Martínez1, A. Albert2, M. André3, G. Anton4, M. Ardid5, J. -J. Aubert6, T. Avgitas7, B. Baret8, J. Barrios-Martí9, S. Basa10, V. Bertin11, S. Biagi12, R. Bormuth13, M. C. Bouwhuis14, R. Bruijn15, J. Brunner16, J. Busto17, A. Capone18, L. Caramete19, J. Carr20, S. Celli21, T. Chiarusi22, M. Circella23, A. Coleiro24, R. Coniglione25, H. Costantini26, P. Coyle27, A. Creusot28, A. Deschamps29, G. De Bonis30, C. Distefano31, C. Donzaud32, D. Dornic33, D. Drouhin34, T. Eberl35, I. El Bojaddaini36, D. Elsässer37, A. Enzenhöfer38, K. Fehn39, I. Felis40, L. A. Fusco41, S. Galatà42, P. Gay43, S. Geißelsöder44, K. Geyer45, V. Giordano46, V. Giordano47, A. Gleixner48, H. Glotin49, R. Gracia-Ruiz50, K. Graf51, S. Hallmann52, H. van Haren53, A. J. Heijboer54, Y. Hello55, J. J. Hernández-Rey56, J. Hößl57, J. Hofestädt58, C. Hugon59, G. Illuminati60, C. W James61, M. de Jong62, M. Jongen63, M. Kadler64, O. Kalekin65, U. Katz66, D. Kießling67, A. Kouchner68, M. Kreter69, I. Kreykenbohm70, V. Kulikovskiy71, C. Lachaud72, R. Lahmann73, D. Lefèvre74, E. Leonora75, S. Loucatos76, M. Marcelin77, A. Margiotta78, A. Marinelli79, J. A. Martínez-Mora80, A. Mathieu81, K. Melis82, T. Michael83, P. Migliozzi84, A. Moussa85, C. Mueller86, E. Nezri87, G. E. Păvălaş88, C. Pellegrino89, C. Perrina90, P. Piattelli91, V. Popa92, T. Pradier93, C. Racca94, G. Riccobene95, K. Roensch96, M. Saldaña97, D. F. E. Samtleben98, M. Sanguineti99, P. Sapienza100, J. Schnabel101, F. Schüssler102, T. Seitz103, C. Sieger104, M. Spurio105, Th. Stolarczyk106, A. Sánchez-Losa107, M. Taiuti108, A. Trovato109, M. Tselengidou110, D. Turpin111, C. T\112, B. Vallage113, C. Vallée114, V. Van Elewyck115, D. Vivolo116, S. Wagner117, J. Wilms118, J. D. Zornoza119, J. Zúñiga120, . M. G. Aartsen121, K. Abraham122, M. Ackermann123, J. Adams124, J. A. Aguilar125, M. Ahlers126, M. Ahrens127, D. Altmann128, T. Anderson129, I. Ansseau130, G. Anton131, M. Archinger132, C. Arguelles133, T. C. Arlen134, J. Auffenberg135, X. Bai136, S. W. Barwick137, V. Baum138, R. Bay139, J. J. Beatty140, J. Becker Tjus141, K. -H. Becker142, E. Beiser143, S. BenZvi144, P. Berghaus145, D. Berley146, E. Bernardini147, A. Bernhard148, D. Z. Besson149, G. Binder150, D. Bindig151, M. Bissok152, E. Blaufuss153, J. Blumenthal154, D. J. Boersma155, C. Bohm156, M. Börner157, F. Bos158, D. Bose159, S. Böser160, O. Botner161, J. Braun162, L. Brayeur163, H. -P. Bretz164, N. Buzinsky165, J. Casey166, M. Casier167, E. Cheung168, D. Chirkin169, A. Christov170, K. Clark171, L. Classen172, S. Coenders173, G. H. Collin174, J. M. Conrad175, D. F. Cowen176, A. H. Cruz Silva177, J. Daughhetee178, J. C. Davis179, M. Day180, J. P. A. M. de André181, C. De Clercq182, E. del Pino Rosendo183, H. Dembinski184, S. De Ridder185, P. Desiati186, K. D. de Vries187, G. de Wasseige188, M. de With189, T. DeYoung190, J. C. Díaz-Vélez191, V. di Lorenzo192, H. Dujmovic193, J. P. Dumm194, M. Dunkman195, B. Eberhardt196, T. Ehrhardt197, B. Eichmann198, S. Euler199, P. A. Evenson200, S. Fahey201, A. R. Fazely202, J. Feintzeig203, J. Felde204, K. Filimonov205, C. Finley206, S. Flis207, C. -C. Fösig208, T. Fuchs209, T. K. Gaisser210, R. Gaior211, J. Gallagher212, L. Gerhardt213, K. Ghorbani214, D. Gier215, L. Gladstone216, M. Glagla217, T. Glüsenkamp218, A. Goldschmidt219, G. Golup220, J. G. Gonzalez221, D. Góra222, D. Grant223, Z. Griffith224, C. Ha225, C. Haack226, A. Haj Ismail227, A. Hallgren228, F. Halzen229, E. Hansen230, B. Hansmann231, T. Hansmann232, K. Hanson233, D. Hebecker234, D. Heereman235, K. Helbing236, R. Hellauer237, S. Hickford238, J. Hignight239, G. C. Hill240, K. D. Hoffman241, R. Hoffmann242, K. Holzapfel243, A. Homeier244, K. Hoshina245, F. Huang246, M. Huber247, W. Huelsnitz248, P. O. Hulth249, K. Hultqvist250, S. In251, A. Ishihara252, E. Jacobi253, G. S. Japaridze254, M. Jeong255, K. Jero256, B. J. P. Jones257, M. Jurkovic258, A. Kappes259, T. Karg260, A. Karle261, U. Katz262, M. Kauer263, A. Keivani264, J. L. Kelley265, J. Kemp266, A. Kheirandish267, M. Kim268, T. Kintscher269, J. Kiryluk270, S. R. Klein271, G. Kohnen272, R. Koirala273, H. Kolanoski274, R. Konietz275, L. Köpke276, C. Kopper277, S. Kopper278, D. J. Koskinen279, M. Kowalski280, K. Krings281, G. Kroll282, M. Kroll283, G. Krückl284, J. Kunnen285, S. Kunwar286, N. Kurahashi287, T. Kuwabara288, M. Labare289, J. L. Lanfranchi290, M. J. Larson291, D. Lennarz292, M. Lesiak-Bzdak293, M. Leuermann294, J. Leuner295, L. Lu296, J. Lünemann297, J. Madsen298, G. Maggi299, K. B. M. Mahn300, M. Mandelartz301, R. Maruyama302, K. Mase303, H. S. Matis304, R. Maunu305, F. McNally306, K. Meagher307, M. Medici308, M. Meier309, A. Meli310, T. Menne311, G. Merino312, T. Meures313, S. Miarecki314, E. Middell315, L. Mohrmann316, T. Montaruli317, R. Morse318, R. Nahnhauer319, U. Naumann320, G. Neer321, H. Niederhausen322, S. C. Nowicki323, D. R. Nygren324, A. Obertacke Pollmann325, A. Olivas326, A. Omairat327, A. O'Murchadha328, T. Palczewski329, H. Pandya330, D. V. Pankova331, L. Paul332, J. A. Pepper333, C. Pérez de los Heros334, C. Pfendner335, D. Pieloth336, E. Pinat337, J. Posselt338, P. B. Price339, G. T. Przybylski340, M. Quinnan341, C. Raab342, L. Rädel343, M. Rameez344, K. Rawlins345, R. Reimann346, M. Relich347, E. Resconi348, W. Rhode349, M. Richman350, S. Richter351, B. Riedel352, S. Robertson353, M. Rongen354, C. Rott355, T. Ruhe356, D. Ryckbosch357, L. Sabbatini358, H. -G. Sander359, A. Sandrock360, J. Sandroos361, S. Sarkar362, K. Schatto363, M. Schimp364, P. Schlunder365, T. Schmidt366, S. Schoenen367, S. Schöneberg368, A. Schönwald369, L. Schumacher370, D. Seckel371, S. Seunarine372, D. Soldin373, M. Song374, G. M. Spiczak375, C. Spiering376, M. Stahlberg377, M. Stamatikos378, T. Stanev379, A. Stasik380, A. Steuer381, T. Stezelberger382, R. G. Stokstad383, A. Stößl384, R. Ström385, N. L. Strotjohann386, G. W. Sullivan387, M. Sutherland388, H. Taavola389, I. Taboada390, J. Tatar391, S. Ter-Antonyan392, A. Terliuk393, G. Tešić394, S. Tilav395, P. A. Toale396, M. N. Tobin397, S. Toscano398, D. Tosi399, M. Tselengidou400, A. Turcati401, E. Unger402, M. Usner403, S. Vallecorsa404, J. Vandenbroucke405, N. van Eijndhoven406, S. Vanheule407, J. van Santen408, J. Veenkamp409, M. Vehring410, M. Voge411, M. Vraeghe412, C. Walck413, A. Wallace414, M. Wallraff415, N. Wandkowsky416, Ch. Weaver417, C. Wendt418, S. Westerhoff419, B. J. Whelan420, K. Wiebe421, C. H. Wiebusch422, L. Wille423, D. R. Williams424, L. Wills425, H. Wissing426, M. Wolf427, T. R. Wood428, K. Woschnagg429, D. L. Xu430, X. W. Xu431, Y. Xu432, J. P. Yanez433, G. Yodh434, S. Yoshida435, M. Zoll436, . B. P. Abbott437, R. Abbott438, T. D. Abbott439, M. R. Abernathy440, F. Acernese441, K. Ackley442, C. Adams443, T. Adams444, P. Addesso445, R. X. Adhikari446, V. B. Adya447, C. Affeldt448, M. Agathos449, K. Agatsuma450, N. Aggarwal451, O. D. Aguiar452, L. Aiello453, A. Ain454, P. Ajith455, B. Allen456, A. Allocca457, P. A. Altin458, S. B. Anderson459, W. G. Anderson460, K. Arai461, M. C. Araya462, C. C. Arceneaux463, J. S. Areeda464, N. Arnaud465, K. G. Arun466, S. Ascenzi467, G. Ashton468, M. Ast469, S. M. Aston470, P. Astone471, P. Aufmuth472, C. Aulbert473, S. Babak474, P. Bacon475, M. K. M. Bader476, P. T. Baker477, F. Baldaccini478, G. Ballardin479, S. W. Ballmer480, J. C. Barayoga481, S. E. Barclay482, B. C. Barish483, D. Barker484, F. Barone485, B. Barr486, L. Barsotti487, M. Barsuglia488, D. Barta489, J. Bartlett490, I. Bartos491, R. Bassiri492, A. Basti493, J. C. Batch494, C. Baune495, V. Bavigadda496, M. Bazzan497, B. Behnke498, M. Bejger499, A. S. Bell500, C. J. Bell501, B. K. Berger502, J. Bergman503, G. Bergmann504, C. P. L. Berry505, D. Bersanetti506, A. Bertolini507, J. Betzwieser508, S. Bhagwat509, R. Bhandare510, I. A. Bilenko511, G. Billingsley512, J. Birch513, R. Birney514, S. Biscans515, A. Bisht516, M. Bitossi517, C. Biwer518, M. A. Bizouard519, J. K. Blackburn520, C. D. Blair521, D. G. Blair522, R. M. Blair523, S. Bloemen524, O. Bock525, T. P. Bodiya526, M. Boer527, G. Bogaert528, C. Bogan529, A. Bohe530, P. Bojtos531, C. Bond532, F. Bondu533, R. Bonnand534, B. A. Boom535, R. Bork536, V. Boschi537, S. Bose538, Y. Bouffanais539, A. Bozzi540, C. Bradaschia541, P. R. Brady542, V. B. Braginsky543, M. Branchesi544, J. E. Brau545, T. Briant546, A. Brillet547, M. Brinkmann548, V. Brisson549, P. Brockill550, A. F. Brooks551, D. D. Brown552, N. M. Brown553, C. C. Buchanan554, A. Buikema555, T. Bulik556, H. J. Bulten557, A. Buonanno558, D. Buskulic559, C. Buy560, R. L. Byer561, L. Cadonati562, G. Cagnoli563, C. Cahillane564, J. Calderón Bustillo565, T. Callister566, E. Calloni567, J. B. Camp568, K. C. Cannon569, J. Cao570, C. D. Capano571, E. Capocasa572, F. Carbognani573, S. Caride574, J. Casanueva Diaz575, C. Casentini576, S. Caudill577, M. Cavaglià578, F. Cavalier579, R. Cavalieri580, G. Cella581, C. B. Cepeda582, L. Cerboni Baiardi583, G. Cerretani584, E. Cesarini585, R. Chakraborty586, T. Chalermsongsak587, S. J. Chamberlin588, M. Chan589, S. Chao590, P. Charlton591, E. Chassande-Mottin592, H. Y. Chen593, Y. Chen594, C. Cheng595, A. Chincarini596, A. Chiummo597, H. S. Cho598, M. Cho599, J. H. Chow600, N. Christensen601, Q. Chu602, S. Chua603, S. Chung604, G. Ciani605, F. Clara606, J. A. Clark607, F. Cleva608, E. Coccia609, P. -F. Cohadon610, A. Colla611, C. G. Collette612, L. Cominsky613, M. Constancio Jr.614, A. Conte615, L. Conti616, D. Cook617, T. R. Corbitt618, N. Cornish619, A. Corsi620, S. Cortese621, C. A. Costa622, M. W. Coughlin623, S. B. Coughlin624, J. -P. Coulon625, S. T. Countryman626, P. Couvares627, E. E. Cowan628, D. M. Coward629, M. J. Cowart630, D. C. Coyne631, R. Coyne632, K. Craig633, J. D. E. Creighton634, J. Cripe635, S. G. Crowder636, A. Cumming637, L. Cunningham638, E. Cuoco639, T. Dal Canton640, S. L. Danilishin641, S. D'Antonio642, K. Danzmann643, N. S. Darman644, V. Dattilo645, I. Dave646, H. P. Daveloza647, M. Davier648, G. S. Davies649, E. J. Daw650, R. Day651, D. DeBra652, G. Debreczeni653, J. Degallaix654, M. De Laurentis655, S. Deléglise656, W. Del Pozzo657, T. Denker658, H. Dereli659, V. Dergachev660, R. T. DeRosa661, R. De Rosa662, R. DeSalvo663, S. Dhurandhar664, M. C. Díaz665, L. Di Fiore666, M. Di Giovanni667, A. Di Lieto668, S. Di Pace669, I. Di Palma670, A. Di Virgilio671, G. Dojcinoski672, V. Dolique673, F. Donovan674, K. L. Dooley675, S. Doravari676, R. Douglas677, T. P. Downes678, M. Drago679, R. W. P. Drever680, J. C. Driggers681, Z. Du682, M. Ducrot683, S. E. Dwyer684, T. B. Edo685, M. C. Edwards686, A. Effler687, H. -B. Eggenstein688, P. Ehrens689, J. Eichholz690, S. S. Eikenberry691, W. Engels692, R. C. Essick693, T. Etzel694, M. Evans695, T. M. Evans696, R. Everett697, M. Factourovich698, V. Fafone699, H. Fair700, S. Fairhurst701, X. Fan702, Q. Fang703, S. Farinon704, B. Farr705, W. M. Farr706, M. Favata707, M. Fays708, H. Fehrmann709, M. M. Fejer710, I. Ferrante711, E. C. Ferreira712, F. Ferrini713, F. Fidecaro714, I. Fiori715, D. Fiorucci716, R. P. Fisher717, R. Flaminio718, M. Fletcher719, J. -D. Fournier720, S. Franco721, S. Frasca722, F. Frasconi723, Z. Frei724, A. Freise725, R. Frey726, V. Frey727, T. T. Fricke728, P. Fritschel729, V. V. Frolov730, P. Fulda731, M. Fyffe732, H. A. G. Gabbard733, J. R. Gair734, L. Gammaitoni735, S. G. Gaonkar736, F. Garufi737, A. Gatto738, G. Gaur739, N. Gehrels740, G. Gemme741, B. Gendre742, E. Genin743, A. Gennai744, J. George745, L. Gergely746, V. Germain747, Archisman Ghosh748, S. Ghosh749, J. A. Giaime750, K. D. Giardina751, A. Giazotto752, K. Gill753, A. Glaefke754, E. Goetz755, R. Goetz756, L. Gondan757, G. González758, J. M. Gonzalez Castro759, A. Gopakumar760, N. A. Gordon761, M. L. Gorodetsky762, S. E. Gossan763, M. Gosselin764, R. Gouaty765, C. Graef766, P. B. Graff767, M. Granata768, A. Grant769, S. Gras770, C. Gray771, G. Greco772, A. C. Green773, P. Groot774, H. Grote775, S. Grunewald776, G. M. Guidi777, X. Guo778, A. Gupta779, M. K. Gupta780, K. E. Gushwa781, E. K. Gustafson782, R. Gustafson783, J. J. Hacker784, B. R. Hall785, E. D. Hall786, G. Hammond787, M. Haney788, M. M. Hanke789, J. Hanks790, C. Hanna791, M. D. Hannam792, J. Hanson793, T. Hardwick794, J. Harms795, G. M. Harry796, I. W. Harry797, M. J. Hart798, M. T. Hartman799, C. -J. Haster800, K. Haughian801, A. Heidmann802, M. C. Heintze803, H. Heitmann804, P. Hello805, G. Hemming806, M. Hendry807, I. S. Heng808, J. Hennig809, A. W. Heptonstall810, M. Heurs811, S. Hild812, D. Hoak813, K. A. Hodge814, D. Hofman815, S. E. Hollitt816, K. Holt817, D. E. Holz818, P. Hopkins819, D. J. Hosken820, J. Hough821, E. A. Houston822, E. J. Howell823, Y. M. Hu824, S. Huang825, E. A. Huerta826, D. Huet827, B. Hughey828, S. Husa829, S. H. Huttner830, T. Huynh-Dinh831, A. Idrisy832, N. Indik833, D. R. Ingram834, R. Inta835, H. N. Isa836, J. -M. Isac837, M. Isi838, G. Islas839, T. Isogai840, B. R. Iyer841, K. Izumi842, T. Jacqmin843, H. Jang844, K. Jani845, P. Jaranowski846, S. Jawahar847, F. Jiménez-Forteza848, W. W. Johnson849, D. I. Jones850, R. Jones851, R. J. G. Jonker852, L. Ju853, Haris K854, C. V. Kalaghatgi855, V. Kalogera856, S. Kandhasamy857, G. Kang858, J. B. Kanner859, S. Karki860, M. Kasprzack861, E. Katsavounidis862, W. Katzman863, S. Kaufer864, T. Kaur865, K. Kawabe866, F. Kawazoe867, F. Kéfélian868, M. S. Kehl869, D. Keitel870, D. B. Kelley871, W. Kells872, R. Kennedy873, J. S. Key874, A. Khalaidovski875, F. Y. Khalili876, I. Khan877, S. Khan878, Z. Khan879, E. A. Khazanov880, N. Kijbunchoo881, C. Kim882, J. Kim883, K. Kim884, Nam-Gyu Kim885, Namjun Kim886, Y. -M. Kim887, E. J. King888, P. J. King889, D. L. Kinzel890, J. S. Kissel891, L. Kleybolte892, S. Klimenko893, S. M. Koehlenbeck894, K. Kokeyama895, S. Koley896, V. Kondrashov897, A. Kontos898, M. Korobko899, W. Z. Korth900, I. Kowalska901, D. B. Kozak902, V. Kringel903, B. Krishnan904, A. Królak905, C. Krueger906, G. Kuehn907, P. Kumar908, L. Kuo909, A. Kutynia910, B. D. Lackey911, M. Landry912, J. Lange913, B. Lantz914, P. D. Lasky915, A. Lazzarini916, C. Lazzaro917, P. Leaci918, S. Leavey919, E. O. Lebigot920, C. H. Lee921, H. K. Lee922, H. M. Lee923, K. Lee924, A. Lenon925, M. Leonardi926, J. R. Leong927, N. Leroy928, N. Letendre929, Y. Levin930, B. M. Levine931, T. G. F. Li932, A. Libson933, T. B. Littenberg934, N. A. Lockerbie935, J. Logue936, A. L. Lombardi937, J. E. Lord938, M. Lorenzini939, V. Loriette940, M. Lormand941, G. Losurdo942, J. D. Lough943, H. Lück944, A. P. Lundgren945, J. Luo946, R. Lynch947, Y. Ma948, T. MacDonald949, B. Machenschalk950, M. MacInnis951, D. M. Macleod952, F. Magaña-Sandoval953, R. M. Magee954, M. Mageswaran955, E. Majorana956, I. Maksimovic957, V. Malvezzi958, N. Man959, I. Mandel960, V. Mandic961, V. Mangano962, G. L. Mansell963, M. Manske964, M. Mantovani965, F. Marchesoni966, F. Marion967, S. Márka968, Z. Márka969, A. S. 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Collaboration, 386IceCube Collaboration, 387IceCube Collaboration, 388IceCube Collaboration, 389IceCube Collaboration, 390IceCube Collaboration, 391IceCube Collaboration, 392IceCube Collaboration, 393IceCube Collaboration, 394IceCube Collaboration, 395IceCube Collaboration, 396IceCube Collaboration, 397IceCube Collaboration, 398IceCube Collaboration, 399IceCube Collaboration, 400IceCube Collaboration, 401IceCube Collaboration, 402IceCube Collaboration, 403IceCube Collaboration, 404IceCube Collaboration, 405IceCube Collaboration, 406IceCube Collaboration, 407IceCube Collaboration, 408IceCube Collaboration, 409IceCube Collaboration, 410IceCube Collaboration, 411IceCube Collaboration, 412IceCube Collaboration, 413IceCube Collaboration, 414IceCube Collaboration, 415IceCube Collaboration, 416IceCube Collaboration, 417IceCube Collaboration, 418IceCube Collaboration, 419IceCube Collaboration, 420IceCube Collaboration, 421IceCube Collaboration, 422IceCube Collaboration, 423IceCube Collaboration, 424IceCube Collaboration, 425IceCube Collaboration, 426IceCube Collaboration, 427IceCube Collaboration, 428IceCube Collaboration, 429IceCube Collaboration, 430IceCube Collaboration, 431IceCube Collaboration, 432IceCube Collaboration, 433IceCube Collaboration, 434IceCube Collaboration, 435IceCube Collaboration, 436IceCube Collaboration, 437ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 438ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 439ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 440ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 441ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 442ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 443ANTARES Collaboration, IceCube 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Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1141ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1142ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1143ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1144ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1145ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1146ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1147ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1148ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1149ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1150ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1151ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1152ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1153ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1154ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1155ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1156ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1157ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1158ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1159ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1160ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1161ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1162ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1163ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1164ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1165ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1166ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1167ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1168ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1169ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1170ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1171ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1172ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1173ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1174ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1175ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1176ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1177ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1178ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1179ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1180ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1181ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1182ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1183ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1184ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1185ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1186ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1187ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1188ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1189ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1190ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1191ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1192ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1193ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1194ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1195ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1196ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1197ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1198ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1199ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1200ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1201ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1202ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1203ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1204ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1205ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1206ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1207ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1208ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1209ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1210ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1211ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1212ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1213ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1214ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1215ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1216ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1217ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1218ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1219ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1220ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1221ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1222ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1223ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1224ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1225ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1226ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1227ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1228ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1229ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1230ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1231ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1232ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1233ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1234ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1235ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1236ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1237ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1238ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1239ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1240ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1241ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1242ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1243ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1244ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1245ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1246ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1247ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1248ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1249ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1250ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1251ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1252ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1253ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1254ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1255ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1256ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1257ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1258ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1259ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1260ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1261ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1262ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1263ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1264ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1265ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1266ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1267ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1268ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1269ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1270ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1271ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1272ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1273ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1274ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1275ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1276ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1277ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1278ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1279ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1280ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1281ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1282ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1283ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1284ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1285ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1286ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1287ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1288ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1289ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1290ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1291ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1292ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1293ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1294ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1295ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1296ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1297ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1298ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1299ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1300ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1301ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1302ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1303ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1304ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1305ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1306ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1307ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1308ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1309ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1310ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1311ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1312ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1313ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1314ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1315ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1316ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1317ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1318ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1319ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1320ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1321ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1322ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1323ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1324ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1325ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1326ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1327ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1328ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1329ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1330ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1331ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1332ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1333ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1334ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1335ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1336ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1337ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1338ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1339ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1340ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1341ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1342ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1343ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1344ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1345ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1346ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1347ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1348ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1349ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1350ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1351ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1352ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1353ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1354ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1355ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1356ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1357ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1358ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1359ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1360ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1361ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1362ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1363ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1364ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1365ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1366ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1367ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1368ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1369ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1370ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1371ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1372ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1373ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1374ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1375ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1376ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1377ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1378ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1379ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1380ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1381ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1382ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1383ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1384ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1385ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1386ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1387ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1388ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1389ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1390ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1391ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1392ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1393ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1394ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1395ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration

We present the high-energy-neutrino follow-up observations of the first gravitational wave transient GW150914 observed by the Advanced LIGO detectors on Sept. 14th, 2015. We search for coincident neutrino candidates within the data recorded by the IceCube and ANTARES neutrino detectors. Read More

2016Feb
Authors: S. Adrián-Martínez1, A. Albert2, M. André3, M. Anghinolfi4, G. Anton5, M. Ardid6, J. -J. Aubert7, T. Avgitas8, B. Baret9, J. Barrios-Martí10, S. Basa11, V. Bertin12, S. Biagi13, R. Bormuth14, M. C. Bouwhuis15, R. Bruijn16, J. Brunner17, J. Busto18, A. Capone19, L. Caramete20, J. Carr21, S. Celli22, T. Chiarusi23, M. Circella24, A. Coleiro25, R. Coniglione26, H. Costantini27, P. Coyle28, A. Creusot29, A. Deschamps30, G. De Bonis31, C. Distefano32, C. Donzaud33, D. Dornic34, D. Drouhin35, T. Eberl36, I. El Bojaddaini37, D. Elsässer38, A. Enzenhöfer39, K. Fehn40, I. Felis41, L. A. Fusco42, S. Galatà43, P. Gay44, S. Geißelsöder45, K. Geyer46, V. Giordano47, A. Gleixner48, H. Glotin49, R. Gracia-Ruiz50, K. Graf51, S. Hallmann52, H. van Haren53, A. J. Heijboer54, Y. Hello55, J. J. Hernández-Rey56, J. Hößl57, J. Hofestädt58, C. Hugon59, G. Illuminati60, C. W James61, M. de Jong62, M. Kadler63, O. Kalekin64, U. Katz65, D. Kießling66, A. Kouchner67, M. Kreter68, I. Kreykenbohm69, V. Kulikovskiy70, C. Lachaud71, R. Lahmann72, D. Lefèvre73, E. Leonora74, S. Loucatos75, M. Marcelin76, A. Margiotta77, A. Marinelli78, J. A. Martínez-Mora79, A. Mathieu80, T. Michael81, P. Migliozzi82, A. Moussa83, C. Mueller84, E. Nezri85, G. E. Păvălaş86, C. Pellegrino87, C. Perrina88, P. Piattelli89, V. Popa90, T. Pradier91, C. Racca92, G. Riccobene93, K. Roensch94, M. Saldaña95, D. F. E. Samtleben96, A. Sánchez-Losa97, M. Sanguineti98, P. Sapienza99, J. Schnabel100, F. Schüssler101, T. Seitz102, C. Sieger103, M. Spurio104, Th. Stolarczyk105, M. Taiuti106, A. Trovato107, M. Tselengidou108, D. Turpin109, C. Tönnis110, B. Vallage111, C. Vallée112, V. Van Elewyck113, E. Visser114, D. Vivolo115, S. Wagner116, J. Wilms117, J. D. Zornoza118, J. Zúñiga119
Affiliations: 1The ANTARES Collaboration, 2The ANTARES Collaboration, 3The ANTARES Collaboration, 4The ANTARES Collaboration, 5The ANTARES Collaboration, 6The ANTARES Collaboration, 7The ANTARES Collaboration, 8The ANTARES Collaboration, 9The ANTARES Collaboration, 10The ANTARES Collaboration, 11The ANTARES Collaboration, 12The ANTARES Collaboration, 13The ANTARES Collaboration, 14The ANTARES Collaboration, 15The ANTARES Collaboration, 16The ANTARES Collaboration, 17The ANTARES Collaboration, 18The ANTARES Collaboration, 19The ANTARES Collaboration, 20The ANTARES Collaboration, 21The ANTARES Collaboration, 22The ANTARES Collaboration, 23The ANTARES Collaboration, 24The ANTARES Collaboration, 25The ANTARES Collaboration, 26The ANTARES Collaboration, 27The ANTARES Collaboration, 28The ANTARES Collaboration, 29The ANTARES Collaboration, 30The ANTARES Collaboration, 31The ANTARES Collaboration, 32The ANTARES Collaboration, 33The ANTARES Collaboration, 34The ANTARES Collaboration, 35The ANTARES Collaboration, 36The ANTARES Collaboration, 37The ANTARES Collaboration, 38The ANTARES Collaboration, 39The ANTARES Collaboration, 40The ANTARES Collaboration, 41The ANTARES Collaboration, 42The ANTARES Collaboration, 43The ANTARES Collaboration, 44The ANTARES Collaboration, 45The ANTARES Collaboration, 46The ANTARES Collaboration, 47The ANTARES Collaboration, 48The ANTARES Collaboration, 49The ANTARES Collaboration, 50The ANTARES Collaboration, 51The ANTARES Collaboration, 52The ANTARES Collaboration, 53The ANTARES Collaboration, 54The ANTARES Collaboration, 55The ANTARES Collaboration, 56The ANTARES Collaboration, 57The ANTARES Collaboration, 58The ANTARES Collaboration, 59The ANTARES Collaboration, 60The ANTARES Collaboration, 61The ANTARES Collaboration, 62The ANTARES Collaboration, 63The ANTARES Collaboration, 64The ANTARES Collaboration, 65The ANTARES Collaboration, 66The ANTARES Collaboration, 67The ANTARES Collaboration, 68The ANTARES Collaboration, 69The ANTARES Collaboration, 70The ANTARES Collaboration, 71The ANTARES Collaboration, 72The ANTARES Collaboration, 73The ANTARES Collaboration, 74The ANTARES Collaboration, 75The ANTARES Collaboration, 76The ANTARES Collaboration, 77The ANTARES Collaboration, 78The ANTARES Collaboration, 79The ANTARES Collaboration, 80The ANTARES Collaboration, 81The ANTARES Collaboration, 82The ANTARES Collaboration, 83The ANTARES Collaboration, 84The ANTARES Collaboration, 85The ANTARES Collaboration, 86The ANTARES Collaboration, 87The ANTARES Collaboration, 88The ANTARES Collaboration, 89The ANTARES Collaboration, 90The ANTARES Collaboration, 91The ANTARES Collaboration, 92The ANTARES Collaboration, 93The ANTARES Collaboration, 94The ANTARES Collaboration, 95The ANTARES Collaboration, 96The ANTARES Collaboration, 97The ANTARES Collaboration, 98The ANTARES Collaboration, 99The ANTARES Collaboration, 100The ANTARES Collaboration, 101The ANTARES Collaboration, 102The ANTARES Collaboration, 103The ANTARES Collaboration, 104The ANTARES Collaboration, 105The ANTARES Collaboration, 106The ANTARES Collaboration, 107The ANTARES Collaboration, 108The ANTARES Collaboration, 109The ANTARES Collaboration, 110The ANTARES Collaboration, 111The ANTARES Collaboration, 112The ANTARES Collaboration, 113The ANTARES Collaboration, 114The ANTARES Collaboration, 115The ANTARES Collaboration, 116The ANTARES Collaboration, 117The ANTARES Collaboration, 118The ANTARES Collaboration, 119The ANTARES Collaboration

Compelling evidence for the existence of astrophysical neutrinos has been reported by the IceCube collaboration. Some features of the energy and declination distributions of IceCube events hint at a North/South asymmetry of the neutrino flux. This could be due to the presence of the bulk of our Galaxy in the Southern hemisphere. Read More

2016Jan
Authors: S. Adrián-Martínez, M. Ageron, F. Aharonian, S. Aiello, A. Albert, F. Ameli, E. Anassontzis, M. Andre, G. Androulakis, M. Anghinolfi, G. Anton, M. Ardid, T. Avgitas, G. Barbarino, E. Barbarito, B. Baret, J. Barrios-Martí, B. Belhorma, A. Belias, E. Berbee, A. van den Berg, V. Bertin, S. Beurthey, V. van Beveren, N. Beverini, S. Biagi, A. Biagioni, M. Billault, M. Bond, R. Bormuth, B. Bouhadef, G. Bourlis, S. Bourret, C. Boutonnet, M. Bouwhuis, C. Bozza, R. Bruijn, J. Brunner, E. Buis, J. Busto, G. Cacopardo, L. Caillat, M. Calamai, D. Calvo, A. Capone, L. Caramete, S. Cecchini, S. Celli, C. Champion, R. Cherkaoui El Moursli, S. Cherubini, T. Chiarusi, M. Circella, L. Classen, R. Cocimano, J. A. B. Coelho, A. Coleiro, S. Colonges, R. Coniglione, M. Cordelli, A. Cosquer, P. Coyle, A. Creusot, G. Cuttone, A. D'Amico, G. De Bonis, G. De Rosa, C. De Sio, F. Di Capua, I. Di Palma, A. F. Díaz García, C. Distefano, C. Donzaud, D. Dornic, Q. Dorosti-Hasankiadeh, E. Drakopoulou, D. Drouhin, L. Drury, M. Durocher, T. Eberl, S. Eichie, D. van Eijk, I. El Bojaddaini, N. El Khayati, D. Elsaesser, A. Enzenhöfer, F. Fassi, P. Favali, P. Fermani, G. Ferrara, G. Frascadore, C. Filippidis, L. A. Fusco, T. Gal, S. Galatà, F. Garufi, P. Gay, M. Gebyehu, V. Giordano, N. Gizani, R. Gracia, K. Graf, T. Grégoire, G. Grella, R. Habel, S. Hallmann, H. van Haren, S. Harissopulos, T. Heid, A. Heijboer, E. Heine, S. Henry, J. J. Hernández-Rey, M. Hevinga, J. Hofestädt, C. M. F. Hugon, G. Illuminati, C. W. James, P. Jansweijer, M. Jongen, M. de Jong, M. Kadler, O. Kalekin, A. Kappes, U. F. Katz, P. Keller, G. Kieft, D. Kießling, E. N. Koffeman, P. Kooijman, A. Kouchner, V. Kulikovskiy, R. Lahmann, P. Lamare, A. Leisos, E. Leonora, M. Lindsey Clark, A. Liolios, C. D. Llorens Alvarez, D. Lo Presti, H. Löhner, A. Lonardo, M. Lotze, S. Loucatos, E. Maccioni, K. Mannheim, A. Margiotta, A. Marinelli, O. Mariş, C. Markou, J. A. Martínez-Mora, A. Martini, R. Mele, K. W. Melis, T. Michael, P. Migliozzi, E. Migneco, P. Mijakowski, A. Miraglia, C. M. Mollo, M. Mongelli, M. Morganti, A. Moussa, P. Musico, M. Musumeci, S. Navas, C. A. Nicolau, I. Olcina, C. Olivetto, A. Orlando, A. Papaikonomou, R. Papaleo, G. E. Păvălaş, H. Peek, C. Pellegrino, C. Perrina, M. Pfutzner, P. Piattelli, K. Pikounis, G. E. Poma, V. Popa, T. Pradier, F. Pratolongo, G. Pühlhofer, S. Pulvirenti, L. Quinn, C. Racca, F. Raffaelli, N. Randazzo, P. Rapidis, P. Razis, D. Real, L. Resvanis, J. Reubelt, G. Riccobene, C. Rossi, A. Rovelli, M. Saldaña, I. Salvadori, D. F. E. Samtleben, A. Sánchez García, A. Sánchez Losa, M. Sanguineti, A. Santangelo, D. Santonocito, P. Sapienza, F. Schimmel, J. Schmelling, V. Sciacca, M. Sedita, T. Seitz, I. Sgura, F. Simeone, I. Siotis, V. Sipala, B. Spisso, M. Spurio, G. Stavropoulos, J. Steijger, S. M. Stellacci, D. Stransky, M. Taiuti, Y. Tayalati, D. Tézier, S. Theraube, L. Thompson, P. Timmer, C. Tönnis, L. Trasatti, A. Trovato, A. Tsirigotis, S. Tzamarias, E. Tzamariudaki, B. Vallage, V. Van Elewyck, J. Vermeulen, P. Vicini, S. Viola, D. Vivolo, M. Volkert, G. Voulgaris, L. Wiggers, J. Wilms, E. de Wolf, K. Zachariadou, J. D. Zornoza, J. Zúñiga

The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The high-energy astrophysical neutrino signal reported by IceCube and 2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. Read More