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)
 
Physics - Instrumentation and Detectors (9)
 
Instrumentation and Methods for Astrophysics (9)
 
High Energy Physics - Phenomenology (8)
 
Cosmology and Nongalactic Astrophysics (2)
 
Nuclear Theory (1)
 
Astrophysics of Galaxies (1)

Publications Authored By M. Taiuti

2017May
Authors: A. Albert1, M. André2, M. Anghinolfi3, G. Anton4, M. Ardid5, J. -J. Aubert6, T. Avgitas7, B. Baret8, J. Barrios-Martí9, S. Basa10, B. Belhorma11, V. Bertin12, S. Biagi13, R. Bormuth14, S. Bourret15, M. C. Bouwhuis16, R. Bruijn17, J. Brunner18, J. Busto19, A. Capone20, L. Caramete21, J. Carr22, S. Celli23, R. Cherkaoui El Moursli24, T. Chiarusi25, M. Circella26, J. A. B. Coelho27, A. Coleiro28, R. Coniglione29, H. Costantini30, P. Coyle31, A. Creusot32, A. F. Díaz33, A. Deschamps34, G. De Bonis35, C. Distefano36, I. Di Palma37, A. Domi38, C. Donzaud39, D. Dornic40, D. Drouhin41, T. Eberl42, I. El Bojaddaini43, N. El Khayati44, D. Elsässer45, A. Enzenhöfer46, A. Ettahiri47, F. Fassi48, I. Felis49, L. A. Fusco50, S. Galatà51, P. Gay52, V. Giordano53, H. Glotin54, T. Grégoire55, R. Gracia Ruiz56, K. Graf57, S. Hallmann58, H. van Haren59, A. J. Heijboer60, Y. Hello61, J. J. Hernández-Rey62, J. Hößl63, J. Hofestädt64, C. Hugon65, G. Illuminati66, C. W. James67, M. de Jong68, M. Jongen69, M. Kadler70, O. Kalekin71, U. Katz72, D. Kießling73, A. Kouchner74, M. Kreter75, I. Kreykenbohm76, V. Kulikovskiy77, C. Lachaud78, R. Lahmann79, D. Lefèvre80, E. Leonora81, M. Lotze82, S. Loucatos83, M. Marcelin84, A. Margiotta85, A. Marinelli86, J. A. Martínez-Mora87, R. Mele88, K. Melis89, T. Michael90, P. Migliozzi91, A. Moussa92, S. Navas93, E. Nezri94, M. Organokov95, G. E. Păvălaş96, C. Pellegrino97, C. Perrina98, P. Piattelli99, V. Popa100, T. Pradier101, L. Quinn102, C. Racca103, G. Riccobene104, A. Sánchez-Losa105, M. Saldaña106, I. Salvadori107, D. F. E. Samtleben108, M. Sanguineti109, P. Sapienza110, F. Schüssler111, C. Sieger112, M. Spurio113, Th. Stolarczyk114, M. Taiuti115, Y. Tayalati116, A. Trovato117, D. Turpin118, C. Tönnis119, B. Vallage120, V. Van Elewyck121, F. Versari122, D. Vivolo123, A. Vizzoca124, J. Wilms125, J. D. Zornoza126, J. Zúñiga127, D. Gaggero128, D. Grasso129
Affiliations: 1GRPHE - Université de Haute Alsace - Institut universitaire de technologie de Colmar, 34 rue du Grillenbreit BP 50568 - 68008 Colmar, France, 2Technical University of Catalonia, Laboratory of Applied Bioacoustics, Rambla Exposició, 08800 Vilanova i la Geltrú, Barcelona, Spain, 3INFN - Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy, 4Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany, 5Institut d'Investigació per a la Gestió Integrada de les Zones Costaneres, 6Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 7APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 8APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 9IFIC - Instituto de Física Corpuscular, 10LAM - Laboratoire d'Astrophysique de Marseille, Pôle de l'étoile Site de Château-Gombert, rue Frédéric Joliot-Curie 38, 13388 Marseille Cedex, 13, France, 11National Center for Energy Sciences and Nuclear Techniques, B.P.1382, R. P.10001 Rabat, Morocco, 12Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 13INFN - Laboratori Nazionali del Sud, 14Nikhef, Science Park, Amsterdam, The Netherlands, 15APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 16Nikhef, Science Park, Amsterdam, The Netherlands, 17Nikhef, Science Park, Amsterdam, The Netherlands, 18Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 19Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 20INFN - Sezione di Roma, P.le Aldo Moro 2, 00185 Roma, Italy, 21Institute for Space Science, RO-077125 Bucharest, Măgurele, Romania, 22Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 23INFN - Sezione di Roma, P.le Aldo Moro 2, 00185 Roma, Italy, 24University Mohammed V in Rabat, Faculty of Sciences, 4 av. Ibn Battouta, B.P. 1014, R.P. 10000 Rabat, Morocco, 25INFN - Sezione di Bologna, Viale Berti-Pichat 6/2, 40127 Bologna, Italy, 26INFN - Sezione di Bari, Via E. Orabona 4, 70126 Bari, Italy, 27APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 28APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 29INFN - Laboratori Nazionali del Sud, 30Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 31Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 32APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 33Department of Computer Architecture and Technology/CITIC, University of Granada, 18071 Granada, Spain, 34Géoazur, UCA, CNRS, IRD, Observatoire de la Côte d'Azur, Sophia Antipolis, France, 35INFN - Sezione di Roma, P.le Aldo Moro 2, 00185 Roma, Italy, 36INFN - Laboratori Nazionali del Sud, 37INFN - Sezione di Roma, P.le Aldo Moro 2, 00185 Roma, Italy, 38INFN - Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy, 39APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 40Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 41GRPHE - Université de Haute Alsace - Institut universitaire de technologie de Colmar, 34 rue du Grillenbreit BP 50568 - 68008 Colmar, France, 42Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany, 43University Mohammed I, Laboratory of Physics of Matter and Radiations, B.P.717, Oujda 6000, Morocco, 44University Mohammed V in Rabat, Faculty of Sciences, 4 av. Ibn Battouta, B.P. 1014, R.P. 10000 Rabat, Morocco, 45Institut für Theoretische Physik und Astrophysik, Universität Würzburg, Emil-Fischer Str. 31, 97074 Würzburg, Germany, 46Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 47University Mohammed V in Rabat, Faculty of Sciences, 4 av. Ibn Battouta, B.P. 1014, R.P. 10000 Rabat, Morocco, 48University Mohammed V in Rabat, Faculty of Sciences, 4 av. Ibn Battouta, B.P. 1014, R.P. 10000 Rabat, Morocco, 49Institut d'Investigació per a la Gestió Integrada de les Zones Costaneres, 50INFN - Sezione di Bologna, Viale Berti-Pichat 6/2, 40127 Bologna, Italy, 51APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 52Laboratoire de Physique Corpusculaire, Clermont Université, Université Blaise Pascal, CNRS/IN2P3, BP 10448, F-63000 Clermont-Ferrand, France, 53INFN - Sezione di Catania, Viale Andrea Doria 6, 95125 Catania, Italy, 54LSIS, Aix Marseille Université CNRS ENSAM LSIS UMR 7296 13397 Marseille, France, Université de Toulon CNRS LSIS UMR 7296, 83957 La Garde, France, 55APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 56APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 57Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany, 58Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany, 59Royal Netherlands Institute for Sea Research, 60Nikhef, Science Park, Amsterdam, The Netherlands, 61Géoazur, UCA, CNRS, IRD, Observatoire de la Côte d'Azur, Sophia Antipolis, France, 62IFIC - Instituto de Física Corpuscular, 63Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany, 64Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany, 65INFN - Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy, 66IFIC - Instituto de Física Corpuscular, 67Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany, 68Nikhef, Science Park, Amsterdam, The Netherlands, 69Nikhef, Science Park, Amsterdam, The Netherlands, 70Institut für Theoretische Physik und Astrophysik, Universität Würzburg, Emil-Fischer Str. 31, 97074 Würzburg, Germany, 71Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany, 72Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany, 73Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany, 74APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 75Institut für Theoretische Physik und Astrophysik, Universität Würzburg, Emil-Fischer Str. 31, 97074 Würzburg, Germany, 76Dr. Remeis-Sternwarte and ECAP, Universität Erlangen-Nürnberg, Sternwartstr. 7, 96049 Bamberg, Germany, 77Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 78APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 79Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany, 80Mediterranean Institute of Oceanography, 81INFN - Laboratori Nazionali del Sud, 82IFIC - Instituto de Física Corpuscular, 83Direction des Sciences de la Matière - Institut de recherche sur les lois fondamentales de l'Univers - Service de Physique des Particules, CEA Saclay, 91191 Gif-sur-Yvette Cedex, France, 84LAM - Laboratoire d'Astrophysique de Marseille, Pôle de l'étoile Site de Château-Gombert, rue Frédéric Joliot-Curie 38, 13388 Marseille Cedex, 13, France, 85INFN - Sezione di Bologna, Viale Berti-Pichat 6/2, 40127 Bologna, Italy, 86INFN - Sezione di Pisa, Largo B. Pontecorvo 3, 56127 Pisa, Italy, 87Institut d'Investigació per a la Gestió Integrada de les Zones Costaneres, 88INFN - Sezione di Napoli, Via Cintia 80126 Napoli, Italy, 89Nikhef, Science Park, Amsterdam, The Netherlands, 90Nikhef, Science Park, Amsterdam, The Netherlands, 91INFN - Sezione di Napoli, Via Cintia 80126 Napoli, Italy, 92University Mohammed I, Laboratory of Physics of Matter and Radiations, B.P.717, Oujda 6000, Morocco, 93Dpto. de Física Teórica y del Cosmos \& C.A.F.P.E., University of Granada, 18071 Granada, Spain, 94LAM - Laboratoire d'Astrophysique de Marseille, Pôle de l'étoile Site de Château-Gombert, rue Frédéric Joliot-Curie 38, 13388 Marseille Cedex, 13, France, 95Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France, 96Institute for Space Science, RO-077125 Bucharest, Măgurele, Romania, 97INFN - Sezione di Bologna, Viale Berti-Pichat 6/2, 40127 Bologna, Italy, 98INFN - Sezione di Roma, P.le Aldo Moro 2, 00185 Roma, Italy, 99INFN - Laboratori Nazionali del Sud, 100Institute for Space Science, RO-077125 Bucharest, Măgurele, Romania, 101Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France, 102Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 103GRPHE - Université de Haute Alsace - Institut universitaire de technologie de Colmar, 34 rue du Grillenbreit BP 50568 - 68008 Colmar, France, 104INFN - Laboratori Nazionali del Sud, 105INFN - Sezione di Bari, Via E. Orabona 4, 70126 Bari, Italy, 106Institut d'Investigació per a la Gestió Integrada de les Zones Costaneres, 107Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 108Nikhef, Science Park, Amsterdam, The Netherlands, 109INFN - Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy, 110INFN - Laboratori Nazionali del Sud, 111Direction des Sciences de la Matière - Institut de recherche sur les lois fondamentales de l'Univers - Service de Physique des Particules, CEA Saclay, 91191 Gif-sur-Yvette Cedex, France, 112Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany, 113INFN - Sezione di Bologna, Viale Berti-Pichat 6/2, 40127 Bologna, Italy, 114Direction des Sciences de la Matière - Institut de recherche sur les lois fondamentales de l'Univers - Service de Physique des Particules, CEA Saclay, 91191 Gif-sur-Yvette Cedex, France, 115INFN - Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy, 116University Mohammed V in Rabat, Faculty of Sciences, 4 av. Ibn Battouta, B.P. 1014, R.P. 10000 Rabat, Morocco, 117INFN - Laboratori Nazionali del Sud, 118Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 119IFIC - Instituto de Física Corpuscular, 120Direction des Sciences de la Matière - Institut de recherche sur les lois fondamentales de l'Univers - Service de Physique des Particules, CEA Saclay, 91191 Gif-sur-Yvette Cedex, France, 121APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 122INFN - Sezione di Bologna, Viale Berti-Pichat 6/2, 40127 Bologna, Italy, 123INFN - Sezione di Napoli, Via Cintia 80126 Napoli, Italy, 124INFN - Sezione di Roma, P.le Aldo Moro 2, 00185 Roma, Italy, 125Dr. Remeis-Sternwarte and ECAP, Universität Erlangen-Nürnberg, Sternwartstr. 7, 96049 Bamberg, Germany, 126IFIC - Instituto de Física Corpuscular, 127IFIC - Instituto de Física Corpuscular, 128GRAPPA, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands, 129INFN - Sezione di Pisa, Largo B. Pontecorvo 3, 56127 Pisa, Italy

The flux of very high-energy neutrinos produced in our Galaxy by the interaction of accelerated cosmic rays with the interstellar medium is not yet determined. The characterization of this flux will shed light on Galactic accelerator features, gas distribution morphology and Galactic cosmic ray transport. The central Galactic plane can be the site of an enhanced neutrino production, thus leading to anisotropies in the extraterrestrial neutrino signal as measured by the IceCube Collaboration. Read More

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

2017Mar
Authors: A. Albert1, M. Andre2, M. Anghinolfi3, G. Anton4, M. Ardid5, J. -J. Aubert6, T. Avgitas7, B. Baret8, J. Barrios-Marti9, S. Basa10, V. Bertin11, S. Biagi12, R. Bormuth13, S. Bourret14, M. C. Bouwhuis15, R. Bruijn16, J. Brunner17, J. Busto18, A. Capone19, L. Caramete20, J. Carr21, S. Celli22, T. Chiarusi23, M. Circella24, J. A. B. Coelho25, A. Coleiro26, R. Coniglione27, H. Costantini28, P. Coyle29, A. Creusot30, A. Deschamps31, G. De Bonis32, C. Distefano33, I. Di Palma34, C. Donzaud35, D. Dornic36, D. Drouhin37, T. Eberl38, I. El Bojaddaini39, D. Elsasser40, A. Enzenhofer41, I. Felis42, L. A. Fusco43, S. Galata44, P. Gay45, V. Giordano46, H. Glotin47, T. Gregoire48, R. Gracia Ruiz49, K. Graf50, S. Hallmann51, H. van Haren52, A. J. Heijboer53, Y. Hello54, J. J. Hernandez-Rey55, J. Hoessl56, J. Hofestadt57, C. Hugon58, G. Illuminati59, C. W. James60, M. de Jong61, M. Jongen62, M. Kadler63, O. Kalekin64, U. Katz65, D. Kiessling66, A. Kouchner67, M. Kreter68, I. Kreykenbohm69, V. Kulikovskiy70, C. Lachaud71, R. Lahmann72, D. Lefevre73, E. Leonora74, M. Lotze75, S. Loucatos76, M. Marcelin77, A. Margiotta78, A. Marinelli79, J. A. Martinez-Mora80, A. Mathieu81, R. Mele82, K. Melis83, T. Michael84, P. Migliozzi85, A. Moussa86, E. Nezri87, G. E. Pavalas88, C. Pellegrino89, C. Perrina90, P. Piattelli91, V. Popa92, T. Pradier93, L. Quinn94, C. Racca95, G. Riccobene96, A. Sanchez-Losa97, M. Saldana98, I. Salvadori99, D. F. E. Samtleben100, M. Sanguineti101, P. Sapienza102, F. Schussler103, C. Sieger104, M. Spurio105, Th. Stolarczyk106, M. Taiuti107, Y. Tayalati108, A. Trovato109, D. Turpin110, C. Tonnis111, B. Vallage112, C. Vallee113, V. Van Elewyck114, F. Versari115, D. Vivolo116, A. Vizzoca117, J. Wilms118, J. D. Zornoza119, J. Zuniga120, M. G. Aartsen121, M. Ackermann122, J. Adams123, J. A. Aguilar124, M. Ahlers125, M. Ahrens126, I. Al Samarai127, D. Altmann128, K. Andeen129, T. Anderson130, I. Ansseau131, G. Anton132, M. Archinger133, C. Arguelles134, J. Auffenberg135, S. Axani136, H. Bagherpour137, X. Bai138, S. W. Barwick139, V. Baum140, R. Bay141, J. J. Beatty142, J. Becker Tjus143, K. -H. Becker144, S. BenZvi145, D. Berley146, E. Bernardini147, D. Z. Besson148, G. Binder149, D. Bindig150, E. Blaufuss151, S. Blot152, C. Bohm153, M. Borner154, F. Bos155, D. Bose156, S. Boser157, O. Botner158, F. Bradascio159, J. Braun160, L. Brayeur161, H. -P. Bretz162, S. Bron163, A. Burgman164, T. Carver165, M. Casier166, E. Cheung167, D. Chirkin168, A. Christov169, K. Clark170, L. Classen171, S. Coenders172, G. H. Collin173, J. M. Conrad174, D. F. Cowen175, R. Cross176, M. Day177, J. P. A. M. de Andre178, C. De Clercq179, E. del Pino Rosendo180, H. Dembinski181, S. De Ridder182, P. Desiati183, K. D. de Vries184, G. de Wasseige185, M. de With186, T. DeYoung187, J. C. Diaz-Velez188, V. di Lorenzo189, H. Dujmovic190, J. P. Dumm191, M. Dunkman192, B. Eberhardt193, T. Ehrhardt194, B. Eichmann195, P. Eller196, S. Euler197, P. A. Evenson198, S. Fahey199, A. R. Fazely200, J. Feintzeig201, J. Felde202, K. Filimonov203, C. Finley204, S. Flis205, C. -C. Fosig206, A. Franckowiak207, E. Friedman208, T. Fuchs209, T. K. Gaisser210, J. Gallagher211, L. Gerhardt212, K. Ghorbani213, W. Giang214, L. Gladstone215, T. Glauch216, T. Glusenkamp217, A. Goldschmidt218, J. G. Gonzalez219, D. Grant220, Z. Gri_th221, C. Haack222, A. Hallgren223, F. Halzen224, E. Hansen225, T. Hansmann226, K. Hanson227, D. Hebecker228, D. Heereman229, K. Helbing230, R. Hellauer231, S. Hickford232, J. Hignight233, G. C. Hill234, K. D. Hoffman235, R. Hoffmann236, K. Hoshina237, F. Huang238, M. Huber239, K. Hultqvist240, S. In241, A. Ishihara242, E. Jacobi243, G. S. Japaridze244, M. Jeong245, K. Jero246, B. J. P. Jones247, W. Kang248, A. Kappes249, T. Karg250, A. Karle251, U. Katz252, M. Kauer253, A. Keivani254, J. L. Kelley255, A. Kheirandish256, J. Kim257, M. Kim258, T. Kintscher259, J. Kiryluk260, T. Kittler261, S. R. Klein262, G. Kohnen263, R. Koirala264, H. 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Affiliations: 1ANTARES Collaboration, 2ANTARES Collaboration, 3ANTARES Collaboration, 4ANTARES Collaboration, 5ANTARES Collaboration, 6ANTARES Collaboration, 7ANTARES Collaboration, 8ANTARES Collaboration, 9ANTARES Collaboration, 10ANTARES Collaboration, 11ANTARES Collaboration, 12ANTARES Collaboration, 13ANTARES Collaboration, 14ANTARES Collaboration, 15ANTARES Collaboration, 16ANTARES Collaboration, 17ANTARES Collaboration, 18ANTARES Collaboration, 19ANTARES Collaboration, 20ANTARES Collaboration, 21ANTARES Collaboration, 22ANTARES Collaboration, 23ANTARES Collaboration, 24ANTARES Collaboration, 25ANTARES Collaboration, 26ANTARES Collaboration, 27ANTARES Collaboration, 28ANTARES Collaboration, 29ANTARES Collaboration, 30ANTARES Collaboration, 31ANTARES Collaboration, 32ANTARES Collaboration, 33ANTARES Collaboration, 34ANTARES Collaboration, 35ANTARES Collaboration, 36ANTARES Collaboration, 37ANTARES Collaboration, 38ANTARES Collaboration, 39ANTARES Collaboration, 40ANTARES Collaboration, 41ANTARES Collaboration, 42ANTARES Collaboration, 43ANTARES Collaboration, 44ANTARES Collaboration, 45ANTARES Collaboration, 46ANTARES Collaboration, 47ANTARES Collaboration, 48ANTARES Collaboration, 49ANTARES Collaboration, 50ANTARES Collaboration, 51ANTARES Collaboration, 52ANTARES Collaboration, 53ANTARES Collaboration, 54ANTARES Collaboration, 55ANTARES Collaboration, 56ANTARES Collaboration, 57ANTARES Collaboration, 58ANTARES Collaboration, 59ANTARES Collaboration, 60ANTARES Collaboration, 61ANTARES Collaboration, 62ANTARES Collaboration, 63ANTARES Collaboration, 64ANTARES Collaboration, 65ANTARES Collaboration, 66ANTARES Collaboration, 67ANTARES Collaboration, 68ANTARES Collaboration, 69ANTARES Collaboration, 70ANTARES Collaboration, 71ANTARES Collaboration, 72ANTARES Collaboration, 73ANTARES Collaboration, 74ANTARES Collaboration, 75ANTARES Collaboration, 76ANTARES Collaboration, 77ANTARES Collaboration, 78ANTARES Collaboration, 79ANTARES Collaboration, 80ANTARES Collaboration, 81ANTARES Collaboration, 82ANTARES Collaboration, 83ANTARES Collaboration, 84ANTARES Collaboration, 85ANTARES Collaboration, 86ANTARES Collaboration, 87ANTARES Collaboration, 88ANTARES Collaboration, 89ANTARES Collaboration, 90ANTARES Collaboration, 91ANTARES Collaboration, 92ANTARES Collaboration, 93ANTARES Collaboration, 94ANTARES Collaboration, 95ANTARES Collaboration, 96ANTARES Collaboration, 97ANTARES Collaboration, 98ANTARES Collaboration, 99ANTARES Collaboration, 100ANTARES Collaboration, 101ANTARES Collaboration, 102ANTARES Collaboration, 103ANTARES Collaboration, 104ANTARES Collaboration, 105ANTARES Collaboration, 106ANTARES Collaboration, 107ANTARES Collaboration, 108ANTARES Collaboration, 109ANTARES Collaboration, 110ANTARES Collaboration, 111ANTARES Collaboration, 112ANTARES Collaboration, 113ANTARES Collaboration, 114ANTARES Collaboration, 115ANTARES Collaboration, 116ANTARES Collaboration, 117ANTARES Collaboration, 118ANTARES Collaboration, 119ANTARES Collaboration, 120ANTARES Collaboration, 121IceCube Collaboration, 122IceCube Collaboration, 123IceCube Collaboration, 124IceCube Collaboration, 125IceCube Collaboration, 126IceCube Collaboration, 127IceCube Collaboration, 128IceCube Collaboration, 129IceCube Collaboration, 130IceCube Collaboration, 131IceCube Collaboration, 132IceCube Collaboration, 133IceCube Collaboration, 134IceCube Collaboration, 135IceCube Collaboration, 136IceCube Collaboration, 137IceCube Collaboration, 138IceCube Collaboration, 139IceCube Collaboration, 140IceCube Collaboration, 141IceCube Collaboration, 142IceCube Collaboration, 143IceCube Collaboration, 144IceCube Collaboration, 145IceCube Collaboration, 146IceCube Collaboration, 147IceCube Collaboration, 148IceCube Collaboration, 149IceCube Collaboration, 150IceCube Collaboration, 151IceCube Collaboration, 152IceCube Collaboration, 153IceCube Collaboration, 154IceCube Collaboration, 155IceCube Collaboration, 156IceCube Collaboration, 157IceCube Collaboration, 158IceCube Collaboration, 159IceCube Collaboration, 160IceCube Collaboration, 161IceCube Collaboration, 162IceCube Collaboration, 163IceCube Collaboration, 164IceCube Collaboration, 165IceCube Collaboration, 166IceCube Collaboration, 167IceCube Collaboration, 168IceCube Collaboration, 169IceCube Collaboration, 170IceCube Collaboration, 171IceCube Collaboration, 172IceCube Collaboration, 173IceCube Collaboration, 174IceCube Collaboration, 175IceCube Collaboration, 176IceCube Collaboration, 177IceCube Collaboration, 178IceCube Collaboration, 179IceCube Collaboration, 180IceCube Collaboration, 181IceCube Collaboration, 182IceCube Collaboration, 183IceCube Collaboration, 184IceCube Collaboration, 185IceCube Collaboration, 186IceCube Collaboration, 187IceCube Collaboration, 188IceCube Collaboration, 189IceCube Collaboration, 190IceCube Collaboration, 191IceCube Collaboration, 192IceCube Collaboration, 193IceCube Collaboration, 194IceCube Collaboration, 195IceCube Collaboration, 196IceCube Collaboration, 197IceCube Collaboration, 198IceCube Collaboration, 199IceCube Collaboration, 200IceCube Collaboration, 201IceCube Collaboration, 202IceCube Collaboration, 203IceCube Collaboration, 204IceCube Collaboration, 205IceCube Collaboration, 206IceCube Collaboration, 207IceCube Collaboration, 208IceCube Collaboration, 209IceCube Collaboration, 210IceCube Collaboration, 211IceCube Collaboration, 212IceCube Collaboration, 213IceCube Collaboration, 214IceCube Collaboration, 215IceCube Collaboration, 216IceCube Collaboration, 217IceCube Collaboration, 218IceCube Collaboration, 219IceCube Collaboration, 220IceCube Collaboration, 221IceCube Collaboration, 222IceCube Collaboration, 223IceCube Collaboration, 224IceCube Collaboration, 225IceCube Collaboration, 226IceCube Collaboration, 227IceCube Collaboration, 228IceCube Collaboration, 229IceCube Collaboration, 230IceCube Collaboration, 231IceCube Collaboration, 232IceCube Collaboration, 233IceCube 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Collaboration, 272IceCube Collaboration, 273IceCube Collaboration, 274IceCube Collaboration, 275IceCube Collaboration, 276IceCube Collaboration, 277IceCube Collaboration, 278IceCube Collaboration, 279IceCube Collaboration, 280IceCube Collaboration, 281IceCube Collaboration, 282IceCube Collaboration, 283IceCube Collaboration, 284IceCube Collaboration, 285IceCube Collaboration, 286IceCube Collaboration, 287IceCube Collaboration, 288IceCube Collaboration, 289IceCube Collaboration, 290IceCube Collaboration, 291IceCube Collaboration, 292IceCube Collaboration, 293IceCube Collaboration, 294IceCube Collaboration, 295IceCube Collaboration, 296IceCube Collaboration, 297IceCube Collaboration, 298IceCube Collaboration, 299IceCube Collaboration, 300IceCube Collaboration, 301IceCube Collaboration, 302IceCube Collaboration, 303IceCube Collaboration, 304IceCube Collaboration, 305IceCube Collaboration, 306IceCube Collaboration, 307IceCube Collaboration, 308IceCube Collaboration, 309IceCube Collaboration, 310IceCube Collaboration, 311IceCube Collaboration, 312IceCube Collaboration, 313IceCube Collaboration, 314IceCube Collaboration, 315IceCube Collaboration, 316IceCube Collaboration, 317IceCube Collaboration, 318IceCube Collaboration, 319IceCube Collaboration, 320IceCube Collaboration, 321IceCube Collaboration, 322IceCube Collaboration, 323IceCube Collaboration, 324IceCube Collaboration, 325IceCube Collaboration, 326IceCube Collaboration, 327IceCube Collaboration, 328IceCube Collaboration, 329IceCube Collaboration, 330IceCube Collaboration, 331IceCube Collaboration, 332IceCube Collaboration, 333IceCube Collaboration, 334IceCube Collaboration, 335IceCube Collaboration, 336IceCube Collaboration, 337IceCube Collaboration, 338IceCube Collaboration, 339IceCube Collaboration, 340IceCube Collaboration, 341IceCube Collaboration, 342IceCube Collaboration, 343IceCube Collaboration, 344IceCube Collaboration, 345IceCube Collaboration, 346IceCube Collaboration, 347IceCube Collaboration, 348IceCube Collaboration, 349IceCube Collaboration, 350IceCube Collaboration, 351IceCube Collaboration, 352IceCube Collaboration, 353IceCube Collaboration, 354IceCube Collaboration, 355IceCube Collaboration, 356IceCube Collaboration, 357IceCube Collaboration, 358IceCube Collaboration, 359IceCube Collaboration, 360IceCube Collaboration, 361IceCube Collaboration, 362IceCube Collaboration, 363IceCube Collaboration, 364IceCube Collaboration, 365IceCube Collaboration, 366IceCube Collaboration, 367IceCube Collaboration, 368IceCube Collaboration, 369IceCube Collaboration, 370IceCube Collaboration, 371IceCube Collaboration, 372IceCube Collaboration, 373IceCube Collaboration, 374IceCube Collaboration, 375IceCube Collaboration, 376IceCube Collaboration, 377IceCube Collaboration, 378IceCube Collaboration, 379IceCube Collaboration, 380IceCube Collaboration, 381IceCube Collaboration, 382IceCube Collaboration, 383IceCube Collaboration, 384IceCube Collaboration, 385IceCube 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, 429LIGO Scientific Collaboration and Virgo Collaboration, 430LIGO Scientific Collaboration and Virgo Collaboration, 431LIGO Scientific Collaboration and Virgo Collaboration, 432LIGO Scientific Collaboration and Virgo Collaboration, 433LIGO Scientific Collaboration and Virgo Collaboration, 434LIGO Scientific Collaboration and Virgo Collaboration, 435LIGO Scientific Collaboration and Virgo Collaboration, 436LIGO Scientific Collaboration and Virgo Collaboration, 437LIGO Scientific Collaboration and Virgo Collaboration, 438LIGO Scientific Collaboration and Virgo Collaboration, 439LIGO Scientific Collaboration and Virgo Collaboration, 440LIGO Scientific Collaboration and Virgo Collaboration, 441LIGO Scientific Collaboration and Virgo Collaboration, 442LIGO Scientific Collaboration and Virgo Collaboration, 443LIGO Scientific Collaboration and Virgo 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Scientific Collaboration and Virgo Collaboration, 651LIGO Scientific Collaboration and Virgo Collaboration, 652LIGO Scientific Collaboration and Virgo Collaboration, 653LIGO Scientific Collaboration and Virgo Collaboration, 654LIGO Scientific Collaboration and Virgo Collaboration, 655LIGO Scientific Collaboration and Virgo Collaboration, 656LIGO Scientific Collaboration and Virgo Collaboration, 657LIGO Scientific Collaboration and Virgo Collaboration, 658LIGO Scientific Collaboration and Virgo Collaboration, 659LIGO Scientific Collaboration and Virgo Collaboration, 660LIGO Scientific Collaboration and Virgo Collaboration, 661LIGO Scientific Collaboration and Virgo Collaboration, 662LIGO Scientific Collaboration and Virgo Collaboration, 663LIGO Scientific Collaboration and Virgo Collaboration, 664LIGO Scientific Collaboration and Virgo Collaboration, 665LIGO Scientific Collaboration and Virgo Collaboration, 666LIGO Scientific Collaboration and Virgo Collaboration, 667LIGO Scientific Collaboration and Virgo Collaboration, 668LIGO Scientific Collaboration and Virgo Collaboration, 669LIGO Scientific Collaboration and Virgo Collaboration, 670LIGO Scientific Collaboration and Virgo Collaboration, 671LIGO Scientific Collaboration and Virgo Collaboration, 672LIGO Scientific Collaboration and Virgo Collaboration, 673LIGO Scientific Collaboration and Virgo Collaboration, 674LIGO Scientific Collaboration and Virgo Collaboration, 675LIGO Scientific Collaboration and Virgo Collaboration, 676LIGO Scientific Collaboration and Virgo Collaboration, 677LIGO Scientific Collaboration and Virgo Collaboration, 678LIGO Scientific Collaboration and Virgo Collaboration, 679LIGO Scientific Collaboration and Virgo Collaboration, 680LIGO Scientific Collaboration and Virgo Collaboration, 681LIGO Scientific Collaboration and Virgo Collaboration, 682LIGO Scientific Collaboration and Virgo Collaboration, 683LIGO Scientific Collaboration and Virgo Collaboration, 684LIGO Scientific Collaboration and Virgo Collaboration, 685LIGO Scientific Collaboration and Virgo Collaboration, 686LIGO Scientific Collaboration and Virgo Collaboration, 687LIGO Scientific Collaboration and Virgo Collaboration, 688LIGO Scientific Collaboration and Virgo Collaboration, 689LIGO Scientific Collaboration and Virgo Collaboration, 690LIGO Scientific Collaboration and Virgo Collaboration, 691LIGO Scientific Collaboration and Virgo Collaboration, 692LIGO Scientific Collaboration and Virgo Collaboration, 693LIGO Scientific Collaboration and Virgo Collaboration, 694LIGO Scientific Collaboration and Virgo Collaboration, 695LIGO Scientific Collaboration and Virgo Collaboration, 696LIGO Scientific Collaboration and Virgo Collaboration, 697LIGO Scientific Collaboration and Virgo Collaboration, 698LIGO Scientific Collaboration and Virgo Collaboration, 699LIGO Scientific Collaboration and Virgo Collaboration, 700LIGO Scientific Collaboration and Virgo Collaboration, 701LIGO Scientific Collaboration and Virgo Collaboration, 702LIGO Scientific Collaboration and Virgo Collaboration, 703LIGO Scientific Collaboration and Virgo Collaboration, 704LIGO Scientific Collaboration and Virgo Collaboration, 705LIGO Scientific Collaboration and Virgo Collaboration, 706LIGO Scientific Collaboration and Virgo Collaboration, 707LIGO Scientific Collaboration and Virgo Collaboration, 708LIGO Scientific Collaboration and Virgo Collaboration, 709LIGO Scientific Collaboration and Virgo Collaboration, 710LIGO Scientific Collaboration and Virgo Collaboration, 711LIGO Scientific Collaboration and Virgo Collaboration, 712LIGO Scientific Collaboration and Virgo Collaboration, 713LIGO Scientific Collaboration and Virgo Collaboration, 714LIGO Scientific Collaboration and Virgo Collaboration, 715LIGO Scientific Collaboration and Virgo Collaboration, 716LIGO Scientific Collaboration and Virgo Collaboration, 717LIGO Scientific Collaboration and Virgo Collaboration, 718LIGO Scientific Collaboration and Virgo Collaboration, 719LIGO Scientific Collaboration and Virgo Collaboration, 720LIGO Scientific Collaboration and Virgo Collaboration, 721LIGO Scientific Collaboration and Virgo Collaboration, 722LIGO Scientific Collaboration and Virgo Collaboration, 723LIGO Scientific Collaboration and Virgo Collaboration, 724LIGO Scientific Collaboration and Virgo Collaboration, 725LIGO Scientific Collaboration and Virgo Collaboration, 726LIGO Scientific Collaboration and Virgo Collaboration, 727LIGO Scientific Collaboration and Virgo Collaboration, 728LIGO Scientific Collaboration and Virgo Collaboration, 729LIGO Scientific Collaboration and Virgo Collaboration, 730LIGO Scientific Collaboration and Virgo Collaboration, 731LIGO Scientific Collaboration and Virgo Collaboration, 732LIGO Scientific Collaboration and Virgo Collaboration, 733LIGO Scientific Collaboration and Virgo Collaboration, 734LIGO Scientific Collaboration and Virgo Collaboration, 735LIGO Scientific Collaboration and Virgo Collaboration, 736LIGO Scientific Collaboration and Virgo Collaboration, 737LIGO Scientific Collaboration and Virgo Collaboration, 738LIGO Scientific Collaboration and Virgo Collaboration, 739LIGO Scientific Collaboration and Virgo Collaboration, 740LIGO Scientific Collaboration and Virgo Collaboration, 741LIGO Scientific Collaboration and Virgo Collaboration, 742LIGO Scientific Collaboration and Virgo Collaboration, 743LIGO Scientific Collaboration and Virgo Collaboration, 744LIGO Scientific Collaboration and Virgo Collaboration, 745LIGO Scientific Collaboration and Virgo Collaboration, 746LIGO Scientific Collaboration and Virgo Collaboration, 747LIGO Scientific Collaboration and Virgo Collaboration, 748LIGO Scientific Collaboration and Virgo Collaboration, 749LIGO Scientific Collaboration and Virgo Collaboration, 750LIGO Scientific Collaboration and Virgo Collaboration, 751LIGO Scientific Collaboration and Virgo Collaboration, 752LIGO Scientific Collaboration and Virgo Collaboration, 753LIGO Scientific Collaboration and Virgo Collaboration, 754LIGO Scientific Collaboration and Virgo Collaboration, 755LIGO Scientific Collaboration and Virgo Collaboration, 756LIGO Scientific Collaboration and Virgo Collaboration, 757LIGO Scientific Collaboration and Virgo Collaboration, 758LIGO Scientific Collaboration and Virgo Collaboration, 759LIGO Scientific Collaboration and Virgo Collaboration, 760LIGO Scientific Collaboration and Virgo Collaboration, 761LIGO Scientific Collaboration and Virgo Collaboration, 762LIGO Scientific Collaboration and Virgo Collaboration, 763LIGO Scientific Collaboration and Virgo Collaboration, 764LIGO Scientific Collaboration and Virgo Collaboration, 765LIGO Scientific Collaboration and Virgo Collaboration, 766LIGO Scientific Collaboration and Virgo Collaboration, 767LIGO Scientific Collaboration and Virgo Collaboration, 768LIGO Scientific Collaboration and Virgo Collaboration, 769LIGO Scientific Collaboration and Virgo Collaboration, 770LIGO Scientific Collaboration and Virgo Collaboration, 771LIGO Scientific Collaboration and Virgo Collaboration, 772LIGO Scientific Collaboration and Virgo Collaboration, 773LIGO Scientific Collaboration and Virgo Collaboration, 774LIGO Scientific Collaboration and Virgo Collaboration, 775LIGO Scientific Collaboration and Virgo Collaboration, 776LIGO Scientific Collaboration and Virgo Collaboration, 777LIGO Scientific Collaboration and Virgo Collaboration, 778LIGO Scientific Collaboration and Virgo Collaboration, 779LIGO Scientific Collaboration and Virgo Collaboration, 780LIGO Scientific Collaboration and Virgo Collaboration, 781LIGO Scientific Collaboration and Virgo Collaboration, 782LIGO Scientific Collaboration and Virgo Collaboration, 783LIGO Scientific Collaboration and Virgo Collaboration, 784LIGO Scientific Collaboration and Virgo Collaboration, 785LIGO Scientific Collaboration and Virgo Collaboration, 786LIGO Scientific Collaboration and Virgo Collaboration, 787LIGO Scientific Collaboration and Virgo Collaboration, 788LIGO Scientific Collaboration and Virgo Collaboration, 789LIGO Scientific Collaboration and Virgo Collaboration, 790LIGO Scientific Collaboration and Virgo Collaboration, 791LIGO Scientific Collaboration and Virgo Collaboration, 792LIGO Scientific Collaboration and Virgo Collaboration, 793LIGO Scientific Collaboration and Virgo Collaboration, 794LIGO Scientific Collaboration and Virgo Collaboration, 795LIGO Scientific Collaboration and Virgo Collaboration, 796LIGO Scientific Collaboration and Virgo Collaboration, 797LIGO Scientific Collaboration and Virgo Collaboration, 798LIGO Scientific Collaboration and Virgo Collaboration, 799LIGO Scientific Collaboration and Virgo Collaboration, 800LIGO Scientific Collaboration and Virgo Collaboration, 801LIGO Scientific Collaboration and Virgo Collaboration, 802LIGO Scientific Collaboration and Virgo Collaboration, 803LIGO Scientific Collaboration and Virgo Collaboration, 804LIGO Scientific Collaboration and Virgo Collaboration, 805LIGO Scientific Collaboration and Virgo Collaboration, 806LIGO Scientific Collaboration and Virgo Collaboration, 807LIGO Scientific Collaboration and Virgo Collaboration, 808LIGO Scientific Collaboration and Virgo Collaboration, 809LIGO Scientific Collaboration and Virgo Collaboration, 810LIGO Scientific Collaboration and Virgo Collaboration, 811LIGO Scientific Collaboration and Virgo Collaboration, 812LIGO Scientific Collaboration and Virgo Collaboration, 813LIGO Scientific Collaboration and Virgo Collaboration, 814LIGO Scientific Collaboration and Virgo Collaboration, 815LIGO Scientific Collaboration and Virgo Collaboration, 816LIGO Scientific Collaboration and Virgo Collaboration, 817LIGO Scientific Collaboration and Virgo Collaboration, 818LIGO Scientific Collaboration and Virgo Collaboration, 819LIGO Scientific Collaboration and Virgo Collaboration, 820LIGO Scientific Collaboration and Virgo Collaboration, 821LIGO Scientific Collaboration and Virgo Collaboration, 822LIGO Scientific Collaboration and Virgo Collaboration, 823LIGO Scientific Collaboration and Virgo Collaboration, 824LIGO Scientific Collaboration and Virgo Collaboration, 825LIGO Scientific Collaboration and Virgo Collaboration, 826LIGO Scientific Collaboration and Virgo Collaboration, 827LIGO Scientific Collaboration and Virgo Collaboration, 828LIGO Scientific Collaboration and Virgo Collaboration, 829LIGO Scientific Collaboration and Virgo Collaboration, 830LIGO Scientific Collaboration and Virgo Collaboration, 831LIGO Scientific Collaboration and Virgo Collaboration, 832LIGO Scientific Collaboration and Virgo Collaboration, 833LIGO Scientific Collaboration and Virgo Collaboration, 834LIGO Scientific Collaboration and Virgo Collaboration, 835LIGO Scientific Collaboration and Virgo Collaboration, 836LIGO Scientific Collaboration and Virgo Collaboration, 837LIGO Scientific Collaboration and Virgo Collaboration, 838LIGO Scientific Collaboration and Virgo Collaboration, 839LIGO Scientific Collaboration and Virgo Collaboration, 840LIGO Scientific Collaboration and Virgo Collaboration, 841LIGO Scientific Collaboration and Virgo Collaboration, 842LIGO Scientific Collaboration and Virgo Collaboration, 843LIGO Scientific Collaboration and Virgo Collaboration, 844LIGO Scientific Collaboration and Virgo Collaboration, 845LIGO Scientific Collaboration and Virgo Collaboration, 846LIGO Scientific Collaboration and Virgo Collaboration, 847LIGO Scientific Collaboration and Virgo Collaboration, 848LIGO Scientific Collaboration and Virgo Collaboration, 849LIGO Scientific Collaboration and Virgo Collaboration, 850LIGO Scientific Collaboration and Virgo Collaboration, 851LIGO Scientific Collaboration and Virgo Collaboration, 852LIGO Scientific Collaboration and Virgo Collaboration, 853LIGO Scientific Collaboration and Virgo Collaboration, 854LIGO Scientific Collaboration and Virgo Collaboration, 855LIGO Scientific Collaboration and Virgo Collaboration, 856LIGO Scientific Collaboration and Virgo Collaboration, 857LIGO Scientific Collaboration and Virgo Collaboration, 858LIGO Scientific Collaboration and Virgo Collaboration, 859LIGO Scientific Collaboration and Virgo Collaboration, 860LIGO Scientific Collaboration and Virgo Collaboration, 861LIGO Scientific Collaboration and Virgo Collaboration, 862LIGO Scientific Collaboration and Virgo Collaboration, 863LIGO Scientific Collaboration and Virgo Collaboration, 864LIGO Scientific Collaboration and Virgo Collaboration, 865LIGO Scientific Collaboration and Virgo Collaboration, 866LIGO Scientific Collaboration and Virgo Collaboration, 867LIGO Scientific Collaboration and Virgo Collaboration, 868LIGO Scientific Collaboration and Virgo Collaboration, 869LIGO Scientific Collaboration and Virgo Collaboration, 870LIGO Scientific Collaboration and Virgo Collaboration, 871LIGO Scientific Collaboration and Virgo Collaboration, 872LIGO Scientific Collaboration and Virgo Collaboration, 873LIGO Scientific Collaboration and Virgo Collaboration, 874LIGO Scientific Collaboration and Virgo Collaboration, 875LIGO Scientific Collaboration and Virgo Collaboration, 876LIGO Scientific Collaboration and Virgo Collaboration, 877LIGO Scientific Collaboration and Virgo Collaboration, 878LIGO Scientific Collaboration and Virgo Collaboration, 879LIGO Scientific Collaboration and Virgo Collaboration, 880LIGO Scientific Collaboration and Virgo Collaboration, 881LIGO Scientific Collaboration and Virgo Collaboration, 882LIGO Scientific Collaboration and Virgo Collaboration, 883LIGO Scientific Collaboration and Virgo Collaboration, 884LIGO Scientific Collaboration and Virgo Collaboration, 885LIGO Scientific Collaboration and Virgo Collaboration, 886LIGO Scientific Collaboration and Virgo Collaboration, 887LIGO Scientific Collaboration and Virgo Collaboration, 888LIGO Scientific Collaboration and Virgo Collaboration, 889LIGO Scientific Collaboration and Virgo Collaboration, 890LIGO Scientific Collaboration and Virgo Collaboration, 891LIGO Scientific Collaboration and Virgo Collaboration, 892LIGO Scientific Collaboration and Virgo Collaboration, 893LIGO Scientific Collaboration and Virgo Collaboration, 894LIGO Scientific Collaboration and Virgo Collaboration, 895LIGO Scientific Collaboration and Virgo Collaboration, 896LIGO Scientific Collaboration and Virgo Collaboration, 897LIGO Scientific Collaboration and Virgo Collaboration, 898LIGO Scientific Collaboration and Virgo Collaboration, 899LIGO Scientific Collaboration and Virgo Collaboration, 900LIGO Scientific Collaboration and Virgo Collaboration, 901LIGO Scientific Collaboration and Virgo Collaboration, 902LIGO Scientific Collaboration and Virgo Collaboration, 903LIGO Scientific Collaboration and Virgo Collaboration, 904LIGO Scientific Collaboration and Virgo Collaboration, 905LIGO Scientific Collaboration and Virgo Collaboration, 906LIGO Scientific Collaboration and Virgo Collaboration, 907LIGO Scientific Collaboration and Virgo Collaboration, 908LIGO Scientific Collaboration and Virgo Collaboration, 909LIGO Scientific Collaboration and Virgo Collaboration, 910LIGO Scientific Collaboration and Virgo Collaboration, 911LIGO Scientific Collaboration and Virgo Collaboration, 912LIGO Scientific Collaboration and Virgo Collaboration, 913LIGO Scientific Collaboration and Virgo Collaboration, 914LIGO Scientific Collaboration and Virgo Collaboration, 915LIGO Scientific Collaboration and Virgo Collaboration, 916LIGO Scientific Collaboration and Virgo Collaboration, 917LIGO Scientific Collaboration and Virgo Collaboration, 918LIGO Scientific Collaboration and Virgo Collaboration, 919LIGO Scientific Collaboration and Virgo Collaboration, 920LIGO Scientific Collaboration and Virgo Collaboration, 921LIGO Scientific Collaboration and Virgo Collaboration, 922LIGO Scientific Collaboration and Virgo Collaboration, 923LIGO Scientific Collaboration and Virgo Collaboration, 924LIGO Scientific Collaboration and Virgo Collaboration, 925LIGO Scientific Collaboration and Virgo Collaboration, 926LIGO Scientific Collaboration and Virgo Collaboration, 927LIGO Scientific Collaboration and Virgo Collaboration, 928LIGO Scientific Collaboration and Virgo Collaboration, 929LIGO Scientific Collaboration and Virgo Collaboration, 930LIGO Scientific Collaboration and Virgo Collaboration, 931LIGO Scientific Collaboration and Virgo Collaboration, 932LIGO Scientific Collaboration and Virgo Collaboration, 933LIGO Scientific Collaboration and Virgo Collaboration, 934LIGO Scientific Collaboration and Virgo Collaboration, 935LIGO Scientific Collaboration and Virgo Collaboration, 936LIGO Scientific Collaboration and Virgo Collaboration, 937LIGO Scientific Collaboration and Virgo Collaboration, 938LIGO Scientific Collaboration and Virgo Collaboration, 939LIGO Scientific Collaboration and Virgo Collaboration, 940LIGO Scientific Collaboration and Virgo Collaboration, 941LIGO Scientific Collaboration and Virgo Collaboration, 942LIGO Scientific Collaboration and Virgo Collaboration, 943LIGO Scientific Collaboration and Virgo Collaboration, 944LIGO Scientific Collaboration and Virgo Collaboration, 945LIGO Scientific Collaboration and Virgo Collaboration, 946LIGO Scientific Collaboration and Virgo Collaboration, 947LIGO Scientific Collaboration and Virgo Collaboration, 948LIGO Scientific Collaboration and Virgo Collaboration, 949LIGO Scientific Collaboration and Virgo Collaboration, 950LIGO Scientific Collaboration and Virgo Collaboration, 951LIGO Scientific Collaboration and Virgo Collaboration, 952LIGO Scientific Collaboration and Virgo Collaboration, 953LIGO Scientific Collaboration and Virgo Collaboration, 954LIGO Scientific Collaboration and Virgo Collaboration, 955LIGO Scientific Collaboration and Virgo Collaboration, 956LIGO Scientific Collaboration and Virgo Collaboration, 957LIGO Scientific Collaboration and Virgo Collaboration, 958LIGO Scientific Collaboration and Virgo Collaboration, 959LIGO Scientific Collaboration and Virgo Collaboration, 960LIGO Scientific Collaboration and Virgo Collaboration, 961LIGO Scientific Collaboration and Virgo Collaboration, 962LIGO Scientific Collaboration and Virgo Collaboration, 963LIGO Scientific Collaboration and Virgo Collaboration, 964LIGO Scientific Collaboration and Virgo Collaboration, 965LIGO Scientific Collaboration and Virgo Collaboration, 966LIGO Scientific Collaboration and Virgo Collaboration, 967LIGO Scientific Collaboration and Virgo Collaboration, 968LIGO Scientific Collaboration and Virgo Collaboration, 969LIGO Scientific Collaboration and Virgo Collaboration, 970LIGO Scientific Collaboration and Virgo Collaboration, 971LIGO Scientific Collaboration and Virgo Collaboration, 972LIGO Scientific Collaboration and Virgo Collaboration, 973LIGO Scientific Collaboration and Virgo Collaboration, 974LIGO Scientific Collaboration and Virgo Collaboration, 975LIGO Scientific Collaboration and Virgo Collaboration, 976LIGO Scientific Collaboration and Virgo Collaboration, 977LIGO Scientific Collaboration and Virgo Collaboration, 978LIGO Scientific Collaboration and Virgo Collaboration, 979LIGO Scientific Collaboration and Virgo Collaboration, 980LIGO Scientific Collaboration and Virgo Collaboration, 981LIGO Scientific Collaboration and Virgo Collaboration, 982LIGO Scientific Collaboration and Virgo Collaboration, 983LIGO Scientific Collaboration and Virgo Collaboration, 984LIGO Scientific Collaboration and Virgo Collaboration, 985LIGO Scientific Collaboration and Virgo Collaboration, 986LIGO Scientific Collaboration and Virgo Collaboration, 987LIGO Scientific Collaboration and Virgo Collaboration, 988LIGO Scientific Collaboration and Virgo Collaboration, 989LIGO Scientific Collaboration and Virgo Collaboration, 990LIGO Scientific Collaboration and Virgo Collaboration, 991LIGO Scientific Collaboration and Virgo Collaboration, 992LIGO Scientific Collaboration and Virgo Collaboration, 993LIGO Scientific Collaboration and Virgo Collaboration, 994LIGO Scientific Collaboration and Virgo Collaboration, 995LIGO Scientific Collaboration and Virgo Collaboration, 996LIGO Scientific Collaboration and Virgo Collaboration, 997LIGO Scientific Collaboration and Virgo Collaboration, 998LIGO Scientific Collaboration and Virgo Collaboration, 999LIGO Scientific Collaboration and Virgo Collaboration, 1000LIGO Scientific Collaboration and Virgo Collaboration, 1001LIGO Scientific Collaboration and Virgo Collaboration, 1002LIGO Scientific Collaboration and Virgo Collaboration, 1003LIGO Scientific Collaboration and Virgo Collaboration, 1004LIGO Scientific Collaboration and Virgo Collaboration, 1005LIGO Scientific Collaboration and Virgo Collaboration, 1006LIGO Scientific Collaboration and Virgo Collaboration, 1007LIGO Scientific Collaboration and Virgo Collaboration, 1008LIGO Scientific Collaboration and Virgo Collaboration, 1009LIGO Scientific Collaboration and Virgo Collaboration, 1010LIGO Scientific Collaboration and Virgo Collaboration, 1011LIGO Scientific Collaboration and Virgo Collaboration, 1012LIGO Scientific Collaboration and Virgo Collaboration, 1013LIGO Scientific Collaboration and Virgo Collaboration, 1014LIGO Scientific Collaboration and Virgo Collaboration, 1015LIGO Scientific Collaboration and Virgo Collaboration, 1016LIGO Scientific Collaboration and Virgo Collaboration, 1017LIGO Scientific Collaboration and Virgo Collaboration, 1018LIGO Scientific Collaboration and Virgo Collaboration, 1019LIGO Scientific Collaboration and Virgo Collaboration, 1020LIGO Scientific Collaboration and Virgo Collaboration, 1021LIGO Scientific Collaboration and Virgo Collaboration, 1022LIGO Scientific Collaboration and Virgo Collaboration, 1023LIGO Scientific Collaboration and Virgo Collaboration, 1024LIGO Scientific Collaboration and Virgo Collaboration, 1025LIGO Scientific Collaboration and Virgo Collaboration, 1026LIGO Scientific Collaboration and Virgo Collaboration, 1027LIGO Scientific Collaboration and Virgo Collaboration, 1028LIGO Scientific Collaboration and Virgo Collaboration, 1029LIGO Scientific Collaboration and Virgo Collaboration, 1030LIGO Scientific Collaboration and Virgo Collaboration, 1031LIGO Scientific Collaboration and Virgo Collaboration, 1032LIGO Scientific Collaboration and Virgo Collaboration, 1033LIGO Scientific Collaboration and Virgo Collaboration, 1034LIGO Scientific Collaboration and Virgo Collaboration, 1035LIGO Scientific Collaboration and Virgo Collaboration, 1036LIGO Scientific Collaboration and Virgo Collaboration, 1037LIGO Scientific Collaboration and Virgo Collaboration, 1038LIGO Scientific Collaboration and Virgo Collaboration, 1039LIGO Scientific Collaboration and Virgo Collaboration, 1040LIGO Scientific Collaboration and Virgo Collaboration, 1041LIGO Scientific Collaboration and Virgo Collaboration, 1042LIGO Scientific Collaboration and Virgo Collaboration, 1043LIGO Scientific Collaboration and Virgo Collaboration, 1044LIGO Scientific Collaboration and Virgo Collaboration, 1045LIGO Scientific Collaboration and Virgo Collaboration, 1046LIGO Scientific Collaboration and Virgo Collaboration, 1047LIGO Scientific Collaboration and Virgo Collaboration, 1048LIGO Scientific Collaboration and Virgo Collaboration, 1049LIGO Scientific Collaboration and Virgo Collaboration, 1050LIGO Scientific Collaboration and Virgo Collaboration, 1051LIGO Scientific Collaboration and Virgo Collaboration, 1052LIGO Scientific Collaboration and Virgo Collaboration, 1053LIGO Scientific Collaboration and Virgo Collaboration, 1054LIGO Scientific Collaboration and Virgo Collaboration, 1055LIGO Scientific Collaboration and Virgo Collaboration, 1056LIGO Scientific Collaboration and Virgo Collaboration, 1057LIGO Scientific Collaboration and Virgo Collaboration, 1058LIGO Scientific Collaboration and Virgo Collaboration, 1059LIGO Scientific Collaboration and Virgo Collaboration, 1060LIGO Scientific Collaboration and Virgo Collaboration, 1061LIGO Scientific Collaboration and Virgo Collaboration, 1062LIGO Scientific Collaboration and Virgo Collaboration, 1063LIGO Scientific Collaboration and Virgo Collaboration, 1064LIGO Scientific Collaboration and Virgo Collaboration, 1065LIGO Scientific Collaboration and Virgo Collaboration, 1066LIGO Scientific Collaboration and Virgo Collaboration, 1067LIGO Scientific Collaboration and Virgo Collaboration, 1068LIGO Scientific Collaboration and Virgo Collaboration, 1069LIGO Scientific Collaboration and Virgo Collaboration, 1070LIGO Scientific Collaboration and Virgo Collaboration, 1071LIGO Scientific Collaboration and Virgo Collaboration, 1072LIGO Scientific Collaboration and Virgo Collaboration, 1073LIGO Scientific Collaboration and Virgo Collaboration, 1074LIGO Scientific Collaboration and Virgo Collaboration, 1075LIGO Scientific Collaboration and Virgo Collaboration, 1076LIGO Scientific Collaboration and Virgo Collaboration, 1077LIGO Scientific Collaboration and Virgo Collaboration, 1078LIGO Scientific Collaboration and Virgo Collaboration, 1079LIGO Scientific Collaboration and Virgo Collaboration, 1080LIGO Scientific Collaboration and Virgo Collaboration, 1081LIGO Scientific Collaboration and Virgo Collaboration, 1082LIGO Scientific Collaboration and Virgo Collaboration, 1083LIGO Scientific Collaboration and Virgo Collaboration, 1084LIGO Scientific Collaboration and Virgo Collaboration, 1085LIGO Scientific Collaboration and Virgo Collaboration, 1086LIGO Scientific Collaboration and Virgo Collaboration, 1087LIGO Scientific Collaboration and Virgo Collaboration, 1088LIGO Scientific Collaboration and Virgo Collaboration, 1089LIGO Scientific Collaboration and Virgo Collaboration, 1090LIGO Scientific Collaboration and Virgo Collaboration, 1091LIGO Scientific Collaboration and Virgo Collaboration, 1092LIGO Scientific Collaboration and Virgo Collaboration, 1093LIGO Scientific Collaboration and Virgo Collaboration, 1094LIGO Scientific Collaboration and Virgo Collaboration, 1095LIGO Scientific Collaboration and Virgo Collaboration, 1096LIGO Scientific Collaboration and Virgo Collaboration, 1097LIGO Scientific Collaboration and Virgo Collaboration, 1098LIGO Scientific Collaboration and Virgo Collaboration, 1099LIGO Scientific Collaboration and Virgo Collaboration, 1100LIGO Scientific Collaboration and Virgo Collaboration, 1101LIGO Scientific Collaboration and Virgo Collaboration, 1102LIGO Scientific Collaboration and Virgo Collaboration, 1103LIGO Scientific Collaboration and Virgo Collaboration, 1104LIGO Scientific Collaboration and Virgo Collaboration, 1105LIGO Scientific Collaboration and Virgo Collaboration, 1106LIGO Scientific Collaboration and Virgo Collaboration, 1107LIGO Scientific Collaboration and Virgo Collaboration, 1108LIGO Scientific Collaboration and Virgo Collaboration, 1109LIGO Scientific Collaboration and Virgo Collaboration, 1110LIGO Scientific Collaboration and Virgo Collaboration, 1111LIGO Scientific Collaboration and Virgo Collaboration, 1112LIGO Scientific Collaboration and Virgo Collaboration, 1113LIGO Scientific Collaboration and Virgo Collaboration, 1114LIGO Scientific Collaboration and Virgo Collaboration, 1115LIGO Scientific Collaboration and Virgo Collaboration, 1116LIGO Scientific Collaboration and Virgo Collaboration, 1117LIGO Scientific Collaboration and Virgo Collaboration, 1118LIGO Scientific Collaboration and Virgo Collaboration, 1119LIGO Scientific Collaboration and Virgo Collaboration, 1120LIGO Scientific Collaboration and Virgo Collaboration, 1121LIGO Scientific Collaboration and Virgo Collaboration, 1122LIGO Scientific Collaboration and Virgo Collaboration, 1123LIGO Scientific Collaboration and Virgo Collaboration, 1124LIGO Scientific Collaboration and Virgo Collaboration, 1125LIGO Scientific Collaboration and Virgo Collaboration, 1126LIGO Scientific Collaboration and Virgo Collaboration, 1127LIGO Scientific Collaboration and Virgo Collaboration, 1128LIGO Scientific Collaboration and Virgo Collaboration, 1129LIGO Scientific Collaboration and Virgo Collaboration, 1130LIGO Scientific Collaboration and Virgo Collaboration, 1131LIGO Scientific Collaboration and Virgo Collaboration, 1132LIGO Scientific Collaboration and Virgo Collaboration, 1133LIGO Scientific Collaboration and Virgo Collaboration, 1134LIGO Scientific Collaboration and Virgo Collaboration, 1135LIGO Scientific Collaboration and Virgo Collaboration, 1136LIGO Scientific Collaboration and Virgo Collaboration, 1137LIGO Scientific Collaboration and Virgo Collaboration, 1138LIGO Scientific Collaboration and Virgo Collaboration, 1139LIGO Scientific Collaboration and Virgo Collaboration, 1140LIGO Scientific Collaboration and Virgo Collaboration, 1141LIGO Scientific Collaboration and Virgo Collaboration, 1142LIGO Scientific Collaboration and Virgo Collaboration, 1143LIGO Scientific Collaboration and Virgo Collaboration, 1144LIGO Scientific Collaboration and Virgo Collaboration, 1145LIGO Scientific Collaboration and Virgo Collaboration, 1146LIGO Scientific Collaboration and Virgo Collaboration, 1147LIGO Scientific Collaboration and Virgo Collaboration, 1148LIGO Scientific Collaboration and Virgo Collaboration, 1149LIGO Scientific Collaboration and Virgo Collaboration, 1150LIGO Scientific Collaboration and Virgo Collaboration, 1151LIGO Scientific Collaboration and Virgo Collaboration, 1152LIGO Scientific Collaboration and Virgo Collaboration, 1153LIGO Scientific Collaboration and Virgo Collaboration, 1154LIGO Scientific Collaboration and Virgo Collaboration, 1155LIGO Scientific Collaboration and Virgo Collaboration, 1156LIGO Scientific Collaboration and Virgo Collaboration, 1157LIGO Scientific Collaboration and Virgo Collaboration, 1158LIGO Scientific Collaboration and Virgo Collaboration, 1159LIGO Scientific Collaboration and Virgo Collaboration, 1160LIGO Scientific Collaboration and Virgo Collaboration, 1161LIGO Scientific Collaboration and Virgo Collaboration, 1162LIGO Scientific Collaboration and Virgo Collaboration, 1163LIGO Scientific Collaboration and Virgo Collaboration, 1164LIGO Scientific Collaboration and Virgo Collaboration, 1165LIGO Scientific Collaboration and Virgo Collaboration, 1166LIGO Scientific Collaboration and Virgo Collaboration, 1167LIGO Scientific Collaboration and Virgo Collaboration, 1168LIGO Scientific Collaboration and Virgo Collaboration, 1169LIGO Scientific Collaboration and Virgo Collaboration, 1170LIGO Scientific Collaboration and Virgo Collaboration, 1171LIGO Scientific Collaboration and Virgo Collaboration, 1172LIGO Scientific Collaboration and Virgo Collaboration, 1173LIGO Scientific Collaboration and Virgo Collaboration, 1174LIGO Scientific Collaboration and Virgo Collaboration, 1175LIGO Scientific Collaboration and Virgo Collaboration, 1176LIGO Scientific Collaboration and Virgo Collaboration, 1177LIGO Scientific Collaboration and Virgo Collaboration, 1178LIGO Scientific Collaboration and Virgo Collaboration, 1179LIGO Scientific Collaboration and Virgo Collaboration, 1180LIGO Scientific Collaboration and Virgo Collaboration, 1181LIGO Scientific Collaboration and Virgo Collaboration, 1182LIGO Scientific Collaboration and Virgo Collaboration, 1183LIGO Scientific Collaboration and Virgo Collaboration, 1184LIGO Scientific Collaboration and Virgo Collaboration, 1185LIGO Scientific Collaboration and Virgo Collaboration, 1186LIGO Scientific Collaboration and Virgo Collaboration, 1187LIGO Scientific Collaboration and Virgo Collaboration, 1188LIGO Scientific Collaboration and Virgo Collaboration, 1189LIGO Scientific Collaboration and Virgo Collaboration, 1190LIGO Scientific Collaboration and Virgo Collaboration, 1191LIGO Scientific Collaboration and Virgo Collaboration, 1192LIGO Scientific Collaboration and Virgo Collaboration, 1193LIGO Scientific Collaboration and Virgo Collaboration, 1194LIGO Scientific Collaboration and Virgo Collaboration, 1195LIGO Scientific Collaboration and Virgo Collaboration, 1196LIGO Scientific Collaboration and Virgo Collaboration, 1197LIGO Scientific Collaboration and Virgo Collaboration, 1198LIGO Scientific Collaboration and Virgo Collaboration, 1199LIGO Scientific Collaboration and Virgo Collaboration, 1200LIGO Scientific Collaboration and Virgo Collaboration, 1201LIGO Scientific Collaboration and Virgo Collaboration, 1202LIGO Scientific Collaboration and Virgo Collaboration, 1203LIGO Scientific Collaboration and Virgo Collaboration, 1204LIGO Scientific Collaboration and Virgo Collaboration, 1205LIGO Scientific Collaboration and Virgo Collaboration, 1206LIGO Scientific Collaboration and Virgo Collaboration, 1207LIGO Scientific Collaboration and Virgo Collaboration, 1208LIGO Scientific Collaboration and Virgo Collaboration, 1209LIGO Scientific Collaboration and Virgo Collaboration, 1210LIGO Scientific Collaboration and Virgo Collaboration, 1211LIGO Scientific Collaboration and Virgo Collaboration, 1212LIGO Scientific Collaboration and Virgo Collaboration, 1213LIGO Scientific Collaboration and Virgo Collaboration, 1214LIGO Scientific Collaboration and Virgo Collaboration, 1215LIGO Scientific Collaboration and Virgo Collaboration, 1216LIGO Scientific Collaboration and Virgo Collaboration, 1217LIGO Scientific Collaboration and Virgo Collaboration, 1218LIGO Scientific Collaboration and Virgo Collaboration, 1219LIGO Scientific Collaboration and Virgo Collaboration, 1220LIGO Scientific Collaboration and Virgo Collaboration, 1221LIGO Scientific Collaboration and Virgo Collaboration, 1222LIGO Scientific Collaboration and Virgo Collaboration, 1223LIGO Scientific Collaboration and Virgo Collaboration, 1224LIGO Scientific Collaboration and Virgo Collaboration, 1225LIGO Scientific Collaboration and Virgo Collaboration, 1226LIGO Scientific Collaboration and Virgo Collaboration, 1227LIGO Scientific Collaboration and Virgo Collaboration, 1228LIGO Scientific Collaboration and Virgo Collaboration, 1229LIGO Scientific Collaboration and Virgo Collaboration, 1230LIGO Scientific Collaboration and Virgo Collaboration, 1231LIGO Scientific Collaboration and Virgo Collaboration, 1232LIGO Scientific Collaboration and Virgo Collaboration, 1233LIGO Scientific Collaboration and Virgo Collaboration, 1234LIGO Scientific Collaboration and Virgo Collaboration, 1235LIGO Scientific Collaboration and Virgo Collaboration, 1236LIGO Scientific Collaboration and Virgo Collaboration, 1237LIGO Scientific Collaboration and Virgo Collaboration, 1238LIGO Scientific Collaboration and Virgo Collaboration, 1239LIGO Scientific Collaboration and Virgo Collaboration, 1240LIGO Scientific Collaboration and Virgo Collaboration, 1241LIGO Scientific Collaboration and Virgo Collaboration, 1242LIGO Scientific Collaboration and Virgo Collaboration, 1243LIGO Scientific Collaboration and Virgo Collaboration, 1244LIGO Scientific Collaboration and Virgo Collaboration, 1245LIGO Scientific Collaboration and Virgo Collaboration, 1246LIGO Scientific Collaboration and Virgo Collaboration, 1247LIGO Scientific Collaboration and Virgo Collaboration, 1248LIGO Scientific Collaboration and Virgo Collaboration, 1249LIGO Scientific Collaboration and Virgo Collaboration, 1250LIGO Scientific Collaboration and Virgo Collaboration, 1251LIGO Scientific Collaboration and Virgo Collaboration, 1252LIGO Scientific Collaboration and Virgo Collaboration, 1253LIGO Scientific Collaboration and Virgo Collaboration, 1254LIGO Scientific Collaboration and Virgo Collaboration, 1255LIGO Scientific Collaboration and Virgo Collaboration, 1256LIGO Scientific Collaboration and Virgo Collaboration, 1257LIGO Scientific Collaboration and Virgo Collaboration, 1258LIGO Scientific Collaboration and Virgo Collaboration, 1259LIGO Scientific Collaboration and Virgo Collaboration, 1260LIGO Scientific Collaboration and Virgo Collaboration, 1261LIGO Scientific Collaboration and Virgo Collaboration, 1262LIGO Scientific Collaboration and Virgo Collaboration, 1263LIGO Scientific Collaboration and Virgo Collaboration, 1264LIGO Scientific Collaboration and Virgo Collaboration, 1265LIGO Scientific Collaboration and Virgo Collaboration, 1266LIGO Scientific Collaboration and Virgo Collaboration, 1267LIGO Scientific Collaboration and Virgo Collaboration, 1268LIGO Scientific Collaboration and Virgo Collaboration, 1269LIGO Scientific Collaboration and Virgo Collaboration, 1270LIGO Scientific Collaboration and Virgo Collaboration, 1271LIGO Scientific Collaboration and Virgo Collaboration, 1272LIGO Scientific Collaboration and Virgo Collaboration, 1273LIGO Scientific Collaboration and Virgo Collaboration, 1274LIGO Scientific Collaboration and Virgo Collaboration, 1275LIGO Scientific Collaboration and Virgo Collaboration, 1276LIGO Scientific Collaboration and Virgo Collaboration, 1277LIGO Scientific Collaboration and Virgo Collaboration, 1278LIGO Scientific Collaboration and Virgo Collaboration, 1279LIGO Scientific Collaboration and Virgo Collaboration, 1280LIGO Scientific Collaboration and Virgo Collaboration, 1281LIGO Scientific Collaboration and Virgo Collaboration, 1282LIGO Scientific Collaboration and Virgo Collaboration, 1283LIGO Scientific Collaboration and Virgo Collaboration, 1284LIGO Scientific Collaboration and Virgo Collaboration, 1285LIGO Scientific Collaboration and Virgo Collaboration, 1286LIGO Scientific Collaboration and Virgo Collaboration, 1287LIGO Scientific Collaboration and Virgo Collaboration, 1288LIGO Scientific Collaboration and Virgo Collaboration, 1289LIGO Scientific Collaboration and Virgo Collaboration, 1290LIGO Scientific Collaboration and Virgo Collaboration, 1291LIGO Scientific Collaboration and Virgo Collaboration, 1292LIGO Scientific Collaboration and Virgo Collaboration, 1293LIGO Scientific Collaboration and Virgo Collaboration, 1294LIGO Scientific Collaboration and Virgo Collaboration, 1295LIGO Scientific Collaboration and Virgo Collaboration, 1296LIGO Scientific Collaboration and Virgo Collaboration, 1297LIGO Scientific 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Scientific Collaboration and Virgo Collaboration, 1416LIGO Scientific Collaboration and Virgo Collaboration

The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find 2 and 4 neutrino candidates detected by IceCube, and 1 and 0 detected by ANTARES, within $\pm500$ s around the respective gravitational wave signals, consistent with the expected background rate. 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,