TY  - JOUR
A1  - Adrián-Martínez, S.
A1  - Ageron, M.
A1  - Aharonian, F.
A1  - Aiello, S.
A1  - Albert, A.
A1  - Ameli, F.
A1  - Annasontzis, E.
A1  - Andre, M.
A1  - Androulakis, G.
A1  - Anghinolfi, M.
A1  - Anton, G.
A1  - Ardid, M.
A1  - Avgitas, T.
A1  - Barbarino, G.
A1  - Baret, B.
A1  - Barrios-Martí, J.
A1  - Belhorma, B.
A1  - Belias, A.
A1  - Berbee, A.
A1  - van den Berg, A.
A1  - Bertin, V.
A1  - Beurthey, S.
A1  - van Beeveren, V.
A1  - Beverini, N.
A1  - Biagi, S.
A1  - Biagioni, A.
A1  - Billault, M.
A1  - Bondì, M.
A1  - Bormuth, R.
A1  - Bouhadef, B.
A1  - Bourlis, G.
A1  - Bourret, S.
A1  - Boutonnet, C.
A1  - Bouwhuis, M.
A1  - Bozza, C.
A1  - Bruijn, R.
A1  - Brunner, J.
A1  - Buis, E.
A1  - Busto, J.
A1  - Cacopardo, G.
A1  - Caillat, L.
A1  - Calmai, M.
A1  - Calvo, D.
A1  - Capone, A.
A1  - Caramete, L.
A1  - Cecchini, S.
A1  - Celli, S.
A1  - Champion, C.
A1  - Cherkaoui El Moursli, R.
A1  - Cherubini, S.
A1  - Chiarusi, T.
A1  - Circella, M.
A1  - Classen, L.
A1  - Cocimano, R.
A1  - Coelho, J. A. B.
A1  - Coleiro, A.
A1  - Colonges, S.
A1  - Coniglione, R.
A1  - Cordelli, M.
A1  - Cosquer, A.
A1  - Coyle, P.
A1  - Creusot, A.
A1  - Cuttone, G.
A1  - D'Amico, A.
A1  - De Bonis, G.
A1  - De Rosa, G.
A1  - De Sio, C.
A1  - Di Capua, F.
A1  - Di Palma, I.
A1  - Díaz García, A. F.
A1  - Distefano, C.
A1  - Donzaud, C.
A1  - Dornic, D.
A1  - Dorosti-Hasankiadeh, Q.
A1  - Drakopoulou, E.
A1  - Drouhin, D.
A1  - Drury, L.
A1  - Durocher, M.
A1  - Eberl, T.
A1  - Eichie, S.
A1  - van Eijk, D.
A1  - El Bojaddaini, I.
A1  - El Khayati, N.
A1  - Elsaesser, D.
A1  - Enzenhöfer, A.
A1  - Fassi, F.
A1  - Favali, P.
A1  - Fermani, P.
A1  - Ferrara, G.
A1  - Filippidis, C.
A1  - Frascadore, G.
A1  - Fusco, L. A.
A1  - Gal, T.
A1  - Galatà, S.
A1  - Garufi, F.
A1  - Gay, P.
A1  - Gebyehu, M.
A1  - Giordano, V.
A1  - Gizani, N.
A1  - Gracia, R.
A1  - Graf, K.
A1  - Grégoire, T.
A1  - Grella, G.
A1  - Habel, R.
A1  - Hallmann, S.
A1  - van Haren, H.
A1  - Harissopulos, S.
A1  - Heid, T.
A1  - Heijboer, A.
A1  - Heine, E.
A1  - Henry, S.
A1  - Hernández-Rey, J. J.
A1  - Hevinga, M.
A1  - Hofestädt, J.
A1  - Hugon, C. M. F.
A1  - Illuminati, G.
A1  - James, C. W.
A1  - Jansweijer, P.
A1  - Jongen, M.
A1  - de Jong, M.
A1  - Kadler, M.
A1  - Kalekin, O.
A1  - Kappes, A.
A1  - Katz, U. F.
A1  - Keller, P.
A1  - Kieft, G.
A1  - Kießling, D.
A1  - Koffeman, E. N.
A1  - Kooijman, P.
A1  - Kouchner, A.
A1  - Kulikovskiy, V.
A1  - Lahmann, R.
A1  - Lamare, P.
A1  - Leisos, A.
A1  - Leonora, E.
A1  - Lindsey Clark, M.
A1  - Liolios, A.
A1  - Llorenz Alvarez, C. D.
A1  - Lo Presti, D.
A1  - Löhner, H.
A1  - Lonardo, A.
A1  - Lotze, M.
A1  - Loucatos, S.
A1  - Maccioni, E.
A1  - Mannheim, K.
A1  - Margiotta, A.
A1  - Marinelli, A.
A1  - Mariş, O.
A1  - Markou, C.
A1  - Martínez-Mora, J. A.
A1  - Martini, A.
A1  - Mele, R.
A1  - Melis, K. W.
A1  - Michael, T.
A1  - Migliozzi, P.
A1  - Migneco, E.
A1  - Mijakowski, P.
A1  - Miraglia, A.
A1  - Mollo, C. M.
A1  - Mongelli, M.
A1  - Morganti, M.
A1  - Moussa, A.
A1  - Musico, P.
A1  - Musumeci, M.
A1  - Navas, S.
A1  - Nicoleau, C. A.
A1  - Olcina, I.
A1  - Olivetto, C.
A1  - Orlando, A.
A1  - Papaikonomou, A.
A1  - Papaleo, R.
A1  - Păvălaş, G. E.
A1  - Peek, H.
A1  - Pellegrino, C.
A1  - Perrina, C.
A1  - Pfutzner, M.
A1  - Piattelli, P.
A1  - Pikounis, K.
A1  - Poma, G. E.
A1  - Popa, V.
A1  - Pradier, T.
A1  - Pratolongo, F.
A1  - Pühlhofer, G.
A1  - Pulvirenti, S.
A1  - Quinn, L.
A1  - Racca, C.
A1  - Raffaelli, F.
A1  - Randazzo, N.
A1  - Rapidis, P.
A1  - Razis, P.
A1  - Real, D.
A1  - Resvanis, L.
A1  - Reubelt, J.
A1  - Riccobene, G.
A1  - Rossi, C.
A1  - Rovelli, A.
A1  - Saldaña, M.
A1  - Salvadori, I.
A1  - Samtleben, D. F. E.
A1  - Sánchez García, A.
A1  - Sánchez Losa, A.
A1  - Sanguineti, M.
A1  - Santangelo, A.
A1  - Santonocito, D.
A1  - Sapienza, P.
A1  - Schimmel, F.
A1  - Schmelling, J.
A1  - Sciacca, V.
A1  - Sedita, M.
A1  - Seitz, T.
A1  - Sgura, I.
A1  - Simeone, F.
A1  - Siotis, I.
A1  - Sipala, V.
A1  - Spisso, B.
A1  - Spurio, M.
A1  - Stavropoulos, G.
A1  - Steijger, J.
A1  - Stellacci, S. M.
A1  - Stransky, D.
A1  - Taiuti, M.
A1  - Tayalati, Y.
A1  - Tézier, D.
A1  - Theraube, S.
A1  - Thompson, L.
A1  - Timmer, P.
A1  - Tönnis, C.
A1  - Trasatti, L.
A1  - Trovato, A.
A1  - Tsirigotis, A.
A1  - Tzamarias, S.
A1  - Tzamariudaki, E.
A1  - Vallage, B.
A1  - Van Elewyk, V.
A1  - Vermeulen, J.
A1  - Vicini, P.
A1  - Viola, S.
A1  - Vivolo, D.
A1  - Volkert, M.
A1  - Voulgaris, G.
A1  - Wiggers, L.
A1  - Wilms, J.
A1  - de Wolf, E.
A1  - Zachariadou, K.
A1  - Zornoza, J. D.
A1  - Zúñiga, J.
T1  - Letter of intent for KM3NeT 2.0
JF  - Journal of Physics G-Nuclear and Particle Physics
N2  - The main objectives of the KM3NeT Collaboration are (i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and (ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: (1) the high-energy astrophysical neutrino signal reported by IceCube and (2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. A phased and distributed implementation is pursued which maximises the access to regional funds, the availability of human resources and the synergistic opportunities for the Earth and sea sciences community. Three suitable deep-sea sites are selected, namely off-shore Toulon (France), Capo Passero (Sicily, Italy) and Pylos (Peloponnese, Greece). The infrastructure will consist of three so-called building blocks. A building block comprises 115 strings, each string comprises 18 optical modules and each optical module comprises 31 photo-multiplier tubes. Each building block thus constitutes a three-dimensional array of photo sensors that can be used to detect the Cherenkov light produced by relativistic particles emerging from neutrino interactions. Two building blocks will be sparsely configured to fully explore the IceCube signal with similar instrumented volume, different methodology, improved resolution and
KW  - neutrino astronomy
KW  - eutrino physics
KW  - deep sea neutrino telescope
KW  - neutrino mass hierarchy
Y1  - 2016
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-188050
VL  - 43
IS  - 8
ER  - 
TY  - JOUR
A1  - Albert, A.
A1  - André, M.
A1  - Anghinolfi, M.
A1  - Anton, G.
A1  - Ardid, M.
A1  - Aubert, J.-J.
A1  - Aublin, J.
A1  - Avgitas, T.
A1  - Baret, B.
A1  - Barrios-Martít, J.
A1  - Basa, S.
A1  - Belhorma, B.
A1  - Bertin, V.
A1  - Biagi, S.
A1  - Bormuth, R.
A1  - Boumaaza, J
A1  - Bourret, S.
A1  - Bouwhuis, M. C.
A1  - Brânzas, H.
A1  - Bruijn, R.
A1  - Brunner, J.
A1  - Busto, J.
A1  - Capone, A.
A1  - Caramete, L.
A1  - Carr, J.
A1  - Celli, S.
A1  - Chabab, M.
A1  - Cherkaoui El Moursli, R.
A1  - Chiarusi, T.
A1  - Circella, M.
A1  - Coelho, J. A. B.
A1  - Coleiro, A.
A1  - Colomer, M
A1  - Coniglione, R.
A1  - Costantini, H.
A1  - Coyle, P.
A1  - Creusot, A.
A1  - Díaz, A. F.
A1  - Deschamps, A.
A1  - Distefano, C.
A1  - Di Palma, I.
A1  - Domi, A.
A1  - Donzaud, C.
A1  - Dornic, D.
A1  - Drouhin, D.
A1  - Eberl, T.
A1  - El Bojaddaini, I.
A1  - El Khayati, N.
A1  - Elsässer, D.
A1  - Enzenhöfer, A.
A1  - Ettahiri, A.
A1  - Fassi, F.
A1  - Felis, I.
A1  - Fermani, P.
A1  - Ferrara, G.
A1  - Fusco, L. A.
A1  - Gay, P.
A1  - Glotin, H.
A1  - Grégoire, T.
A1  - Gracia Ruiz, R.
A1  - Graf, K.
A1  - Hallmann, S.
A1  - van Haren, H.
A1  - Heijboer, A. J.
A1  - Hello, Y.
A1  - Hernández-Rey, J. J.
A1  - Hößl, J.
A1  - Hofestädt, J.
A1  - Illuminati, G.
A1  - de Jong, M.
A1  - Jongen, M.
A1  - Kadler, M.
A1  - Kalekin, O.
A1  - Katz, U.
A1  - Khan-Chowdhury, N. R.
A1  - Kouchner, A.
A1  - Kreter, M.
A1  - Kreykenbohm, I.
A1  - Kulikovskiy, V.
A1  - Lachaud, C.
A1  - Lahmann, R.
A1  - Lefèvre, D.
A1  - Leonora, E.
A1  - Levi, G.
A1  - Lotze, M.
A1  - Loucatos, S.
A1  - Marcelin, M.
A1  - Margiotta, A.
A1  - Marinelli, A.
A1  - Martínez-Mora, J. A.
A1  - Mele, R.
A1  - Melis, K.
A1  - Migliozzi, P.
A1  - Moussa, A.
A1  - Navas, S.
A1  - Nezri, E.
A1  - Nuñez, A.
A1  - Organokov, M.
A1  - Pavalas, G. E.
A1  - Pellegrino, C.
A1  - Piattelli, P.
A1  - Popa, V.
A1  - Pradier, T.
A1  - Quinn, L.
A1  - Racca, C.
A1  - Randazzo, N.
A1  - Riccobene, G.
A1  - Sánchez-Losa, A.
A1  - Saldaña, M.
A1  - Salvadori, I.
A1  - Samtleben, D. F. E.
A1  - Sanguineti, M.
A1  - Sapienza, P.
A1  - Schüssler, F.
A1  - Spurio, M.
A1  - Stolarczyk, Th.
A1  - Taiuti, M.
A1  - Tayalati, Y.
A1  - Trovato, A.
A1  - Vallage, B.
A1  - Van Elewyck, V.
A1  - Versari, F.
A1  - Vivolo, D.
A1  - Wilms, J.
A1  - Zaborov, D.
A1  - Zornoza, J. D.
A1  - Zúñiga, J.
T1  - The cosmic ray shadow of the Moon observed with the ANTARES neutrino telescope
JF  - European Physical Journal C
N2  - One of the main objectives of the ANTARES telescope is the search for point- like neutrino sources. Both the pointing accuracy and the angular resolution of the detector are important in this context and a reliableway to evaluate this performance is needed. In order to measure the pointing accuracy of the detector, one possibility is to study the shadow of the Moon, i. e. the deficit of the atmospheric muon flux from the direction of the Moon induced by the absorption of cosmic rays. Analysing the data taken between 2007 and 2016, theMoon shadow is observed with 3.5s statistical significance. The detector angular resolution for downwardgoing muons is 0.73. +/- 0.14.. The resulting pointing performance is consistent with the expectations. An independent check of the telescope pointing accuracy is realised with the data collected by a shower array detector onboard of a ship temporarily moving around the ANTARES location.
KW  - Atmospheric muons
Y1  - 2019
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-227802
VL  - 78
ER  - 
TY  - JOUR
A1  - Akshat, Puri
A1  - Aaboud, M.
A1  - Aad, G.
A1  - Abbott, B.
A1  - Abdinov, O.
A1  - Abeloos, B.
A1  - Abhayasinghe, D. K.
A1  - Abidi, S. H.
A1  - Abou Zeid, O. S.
A1  - Abraham, N. L.
A1  - Abramowicz, H.
A1  - Abreu, H.
A1  - Abulaiti, Y.
A1  - Acharya, B. S.
A1  - Adachi, S.
A1  - Adam, L.
A1  - Adamczyk, L.
A1  - Adelman, J.
A1  - Adersberger, M.
A1  - Adiguzel, A.
A1  - Adye, T.
A1  - Affolder, A. A.
A1  - Afik, Y.
A1  - Agheorghiesei, C.
A1  - Aguilar-Saavedra, J. A.
A1  - Ahmadov, F.
A1  - Aiellil, G.
A1  - Akatsuka, S.
A1  - Akesson, T. P. A.
A1  - Akilli, E.
A1  - Akimov, A. V.
A1  - Alberghi, G. L.
A1  - Albert, J.
A1  - Albicocco, P.
A1  - Alconada Verzini, M. J.
A1  - Alderweireld, S.
A1  - Aleksa, M.
A1  - Aleksandrov, I. N.
A1  - Alexa, C.
A1  - Alexopoulos, T.
A1  - Alhroob, M.
A1  - Ali, B.
A1  - Alimonti, G.
A1  - Alison, J.
A1  - Andre, S. P.
A1  - Allaire, C.
A1  - Allbrooke, B. M. M.
A1  - Allen, B. W.
A1  - Allport, P. P.
A1  - Aloisio, A.
A1  - Alonso, A.
A1  - Alonso, F.
A1  - Alpigiani, C.
A1  - Alshehri, A. A.
A1  - Alstaty, M. I.
A1  - Alvarez, Gonzalez B.
A1  - Alvarez Piqueras, D.
A1  - Alviggi, M. G.
A1  - Amadio, B. T.
A1  - Amaral, Coutinho, Y.
A1  - Ambler, A.
A1  - Ambroz, L.
A1  - Amelung, C.
A1  - Amidei, D.
A1  - Amor Dos Santos, S. P.
A1  - Amoroso, S.
A1  - Amrouche, C. S.
A1  - Anastopoulos, C.
A1  - Ancu, L. S.
A1  - Andari, N.
A1  - Andeen, T.
A1  - Anders, C. F.
A1  - Anders, J. K.
A1  - Anderson, K. J.
A1  - Andreazza, A.
A1  - Andrei, V.
A1  - et al, 
T1  - Measurement of angular and momentum distributions of charged particles within and around jets in Pb plus Pb and pp collisions at root s(NN)=5.02 TeV with ATLAS at the LHC : XXVIIth International Conference on Ultrarelativistic Nucleus-Nucleus Collisions
(Quark Matter 2018)
JF  - Nuclear Physics A
N2  - Studies of the fragmentation of jets into charged particles in heavy-ion collisions can help in understanding the mechanism of jet quenching by the hot and dense QCD matter created in such collisions, the quark-gluon plasma. These proceedings present a measurement of the angular distribution of charged particles around the jet axis in root s(NN) = 5.02 TeV Pb+Pb and pp collisions, done using the ATLAS detector at the LHC. The measurement is performed inside jets reconstructed with the anti-k(t) algorithm with radius parameter R = 0.4, and is extended to regions outside the jet cone. Results are presented as a function of Pb+Pb collision centrality, and both jet and charged-particle transverse momenta.
KW  - jets
KW  - fragmentation functions
KW  - jet shapes
Y1  - 2019
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-224703
VL  - 982
IS  - 2
ER  - 
TY  - JOUR
A1  - Adrián-Martínez, S.
A1  - Albert, A.
A1  - André, M.
A1  - Anton, G.
A1  - Ardid, M.
A1  - Aubert, J.-J.
A1  - Avgitas, T.
A1  - Baret, B.
A1  - Barrios-Martí, J.
A1  - Basa, S.
A1  - Bertin, V.
A1  - Biagi, S.
A1  - Bormuth, R.
A1  - Bou-Cabo, M.
A1  - Bouwhuis, M.C.
A1  - Bruijn, R.
A1  - Brunner, J.
A1  - Busto, J.
A1  - Capone, A.
A1  - Caramete, L.
A1  - Carr, J.
A1  - Celli, S.
A1  - Chiarusi, T.
A1  - Circella, M.
A1  - Coleiro, A.
A1  - Coniglione, R.
A1  - Costantini, H.
A1  - Coyle, P.
A1  - Creusot, A.
A1  - Deschamps, A.
A1  - De Bonis, G.
A1  - Distefano, C.
A1  - Donzaud, C.
A1  - Dornic, D.
A1  - Drouhin, D.
A1  - Eberl, T.
A1  - El Bojaddaini, I.
A1  - Elsässer, D.
A1  - Enzenhöfer, A.
A1  - Fehn, K.
A1  - Felis, I.
A1  - Fusco, L.A.
A1  - Galatà, S.
A1  - Gay, P.
A1  - Geißelsöder, S.
A1  - Geyer, K.
A1  - Giordano, V.
A1  - Gleixner, A.
A1  - Glotin, H.
A1  - Gracia-Ruiz, R.
A1  - Graf, K.
A1  - Hallmann, S.
A1  - van Haren, H.
A1  - Heijboer, A.J.
A1  - Hello, Y.
A1  - Hernández-Rey, J.-J.
A1  - Hößl, J.
A1  - Hofestädt, J.
A1  - Hugon, C.
A1  - Illuminati, G.
A1  - James, C.W.
A1  - de Jong, M.
A1  - Kadler, M.
A1  - Kalekin, O.
A1  - Katz, U.
A1  - Kießling, D.
A1  - Kouchner, A.
A1  - Kreter, M.
A1  - Kreykenbohm, I.
A1  - Kulikovskiy, V.
A1  - Lachaud, C.
A1  - Lahmann, R.
A1  - Lefèvre, D.
A1  - Leonora, E.
A1  - Loucatos, S.
A1  - Marcelin, M.
A1  - Margiotta, A.
A1  - Marinelli, A.
A1  - Martínez-Mora, J.A.
A1  - Mathieu, A.
A1  - Michael, T.
A1  - Migliozzi, P.
A1  - Moussa, A.
A1  - Mueller, C.
A1  - Nezri, E.
A1  - Păvălaș, G.E.
A1  - Pellegrino, C.
A1  - Perrina, C.
A1  - Piattelli, P.
A1  - Popa, V.
A1  - Pradier, T.
A1  - Racca, C.
A1  - Riccobene, G.
A1  - Roensch, K.
A1  - Saldaña, M.
A1  - Samtleben, D.F.E.
A1  - Sanguineti, M.
A1  - Sapienza, P.
A1  - Schnabel, J.
A1  - Schüssler, F.
A1  - Seitz, T.
A1  - Sieger, C.
A1  - Spurio, M.
A1  - Stolarczyk, Th.
A1  - Sánchez-Losa, A.
A1  - Taiuti, M.
A1  - Trovato, A.
A1  - Tselengidou, M.
A1  - Turpin, D.
A1  - Tönnis, C.
A1  - Vallage, B.
A1  - Vallée, C.
A1  - Van Elewyck, V.
A1  - Vivolo, D.
A1  - Wagner, S.
A1  - Wilms, J.
A1  - Zornoza, J.D.
A1  - Zúñiga, J.
T1  - A search for Secluded Dark Matter in the Sun with the ANTARES neutrino telescope
JF  - Journal of Cosmology and Astroparticle Physics
N2  - 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.
KW  - dark matter experiments
KW  - neutrino detectors
KW  - dark matter detectors
KW  - neutrino astronomy
Y1  - 2016
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-189035
VL  - 2016
IS  - 5
ER  - 
TY  - JOUR
A1  - Adrián-Martínez, S.
A1  - Albert, A.
A1  - André, M.
A1  - Anton, G.
A1  - Ardid, M.
A1  - Aubert, J.-J.
A1  - Avgitas, T.
A1  - Baret, B.
A1  - Barrios-Martí, J.
A1  - Basa, S.
A1  - Bertin, V.
A1  - Biagi, S.
A1  - Bormuth, R.
A1  - Bouwhuis, M.C.
A1  - Bruijn, R.
A1  - Brunner, J.
A1  - Busto, J.
A1  - Capone, A.
A1  - Caramete, L.
A1  - Carr, J.
A1  - Celli, S.
A1  - Chiarusi, T.
A1  - Circella, M.
A1  - Coleiro, A.
A1  - Coniglione, R.
A1  - Costantini, H.
A1  - Coyle, P.
A1  - Creusot, A.
A1  - Deschamps, A.
A1  - De Bonis, G.
A1  - Distefano, C.
A1  - Donzaud, C.
A1  - Dornic, D.
A1  - Drouhin, D.
A1  - Eberl, T.
A1  - El Bojaddaini, I.
A1  - Elsässer, D.
A1  - Enzenhöfer, A.
A1  - Fehn, K.
A1  - Felis, I.
A1  - Fusco, L.A.
A1  - Galatà, S.
A1  - Gay, P.
A1  - Geißelsöder, S.
A1  - Geyer, K.
A1  - Giordano, V.
A1  - Gleixner, A.
A1  - Glotin, H.
A1  - Gracia-Ruiz, R.
A1  - Graf, K.
A1  - Hallmann, S.
A1  - van Haren, H.
A1  - Heijboer, A.J.
A1  - Hello, Y.
A1  - Hernández-Rey, J.J.
A1  - Hößl, J.
A1  - Hofestädt, J.
A1  - Hugon, C.
A1  - Illuminati, G.
A1  - James, C.W.
A1  - de Jong, M.
A1  - Jongen, M.
A1  - Kadler, M.
A1  - Kalekin, O.
A1  - Katz, U.
A1  - Kießling, D.
A1  - Kouchner, A.
A1  - Kreter, M.
A1  - Kreykenbohm, I.
A1  - Kulikovskiy, V.
A1  - Lachaud, C.
A1  - Lahmann, R.
A1  - Lefèvre, D.
A1  - Leonora, E.
A1  - Loucatos, S.
A1  - Marcelin, M.
A1  - Margiotta, A.
A1  - Marinelli, A.
A1  - Martínez-Mora, J.A.
A1  - Mathieu, A.
A1  - Melis, K.
A1  - Michael, T.
A1  - Migliozzi, P.
A1  - Moussa, A.
A1  - Mueller, C.
A1  - Nezri, E.
A1  - Pavalas, G.E.
A1  - Pellegrino, C.
A1  - Perrina, C.
A1  - Piattelli, P.
A1  - Popa, V.
A1  - Pradier, T.
A1  - Racca, C.
A1  - Riccobene, G.
A1  - Roensch, K.
A1  - Saldaña, M.
A1  - Samtleben, D.F.E.
A1  - Sánchez-Losa, A.
A1  - Sanguineti, M.
A1  - Sapienza, P.
A1  - Schnabel, J.
A1  - Schüssler, F.
A1  - Seitz, T.
A1  - Sieger, C.
A1  - Spurio, M.
A1  - Stolarczyk, Th.
A1  - Taiuti, M.
A1  - Tönnis, C.
A1  - Trovato, A.
A1  - Tselengidou, M.
A1  - Turpin, D.
A1  - Vallage, B.
A1  - Vallée, C.
A1  - Van Elewyck, V.
A1  - Vivolo, D.
A1  - Wagner, S.
A1  - Wilms, J.
A1  - Zornoza, J.D.
A1  - Zúñiga, J.
T1  - Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope
JF  - Physics Letters B
N2  - 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.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP→ b\(\overline{b}\), W\(^{+}\)W\(^{−}\) and τ\(^{+}\)τ\(^{−}\).
KW  - dark matter
KW  - WIMP
KW  - neutralino
KW  - indirect detection
KW  - neutrino telescope
KW  - sun
Y1  - 2016
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-166642
VL  - 759
ER  - 
TY  - JOUR
A1  - Adrián-Martínez, S.
A1  - Albert, A.
A1  - André, M.
A1  - Anghinolfi, M.
A1  - Anton, G.
A1  - Ardid, M.
A1  - Aubert, J.-J.
A1  - Avgitas, T.
A1  - Baret, B.
A1  - Barrios-Martí, J.
A1  - Basa, S.
A1  - Bertin, V.
A1  - Biagi, S.
A1  - Bormuth, R.
A1  - Bouwhuis, M.C.
A1  - Bruijn, R.
A1  - Brunner, J.
A1  - Busto, J.
A1  - Capone, A.
A1  - Caramete, L.
A1  - Carr, J.
A1  - Celli, S.
A1  - Chiarusi, T.
A1  - Circella, M.
A1  - Coleiro, A.
A1  - Coniglione, R.
A1  - Constantini, H.
A1  - Coyle, P.
A1  - Creusot, A.
A1  - Deschamps, A.
A1  - De Bonis, G.
A1  - Distefano, C.
A1  - Donzaud, C.
A1  - Dornic, D.
A1  - Drouhin, D.
A1  - Eberl, T.
A1  - El Bojaddaini, I.
A1  - Elsässer, D.
A1  - Enzenhöfer, A.
A1  - Fehn, K.
A1  - Felis, I.
A1  - Fusco, L.A.
A1  - Galatà, S.
A1  - Gay, P.
A1  - Geißelsöder, S.
A1  - Geyer, K.
A1  - Giordano, V.
A1  - Gleixner, A.
A1  - Glotin, H.
A1  - Gracia-Ruiz, R.
A1  - Graf, K.
A1  - Hallmann, S.
A1  - van Haren, H.
A1  - Heijboer, A.J.
A1  - Hello, Y.
A1  - Hernández-Rey, J.J.
A1  - Hößl, J.
A1  - Hofestädt, J.
A1  - Hugon, C.
A1  - Illuminati, G.
A1  - James, C.W.
A1  - de Jong, M.
A1  - Kadler, M.
A1  - Kalekin, O.
A1  - Katz, U.
A1  - Kießling, D.
A1  - Kouchner, A.
A1  - Kreter, M.
A1  - Kreykenbohm, I.
A1  - Kulikovskiy, V.
A1  - Lachaud, C.
A1  - Lahmann, R.
A1  - Lefèvre, D.
A1  - Leonora, E.
A1  - Loucatos, S.
A1  - Marcelin, M.
A1  - Margiotta, A.
A1  - Marinelli, A.
A1  - Martínez-Mora, J.A.
A1  - Mathieu, A.
A1  - Michael, T.
A1  - Migliozzi, P.
A1  - Moussa, A.
A1  - Mueller, C.
A1  - Nezri, E.
A1  - Pavalas, G.E.
A1  - Pellegrino, C.
A1  - Perrina, C.
A1  - Piattelli, P.
A1  - Popa, V.
A1  - Pradier, T.
A1  - Racca, C.
A1  - Riccobene, G.
A1  - Roensch, K.
A1  - Saldaña, M.
A1  - Samtleben, D.F.E.
A1  - Sánchez-Losa, A.
A1  - Sanguineti, M.
A1  - Sapienza, P.
A1  - Schnabel, J.
A1  - Schüssler, F.
A1  - Seitz, T.
A1  - Sieger, C.
A1  - Spurio, M.
A1  - Stolarczyk, Th.
A1  - Taiuti, M.
A1  - Trovato, A.
A1  - Tselengidou, M.
A1  - Turpin, D.
A1  - Tönnis, C.
A1  - Vallage, B.
A1  - Vallée, C.
A1  - Van Elewyck, V.
A1  - Visser, E.
A1  - Vivolo, D.
A1  - Wagner, S.
A1  - Wilms, J.
A1  - Zornoza, J.D.
A1  - Zúñiga, J.
T1  - Constraints on the neutrino emission from the Galactic Ridge with the ANTARES telescope
JF  - Physics Letters B
N2  - A highly significant excess of high-energy astrophysical neutrinos has been reported by the IceCube Collaboration. Some features of the energy and declination distributions of IceCube events hint at a North/South asymmetry of the neutrino flux. This could be due to the presence of the bulk of our Galaxy in the Southern hemisphere. The ANTARES neutrino telescope, located in the Mediterranean Sea, has been taking data since 2007. It offers the best sensitivity to muon neutrinos produced by galactic cosmic ray interactions in this region of the sky. In this letter a search for an extended neutrino flux from the Galactic Ridge region is presented. Different models of neutrino production by cosmic ray propagation are tested. No excess of events is observed and upper limits for different neutrino flux spectral indices Γ are set. For Γ=2.4 the 90% confidence level flux upper limit at 100 TeV for one neutrino flavour corresponds to Φ\(^{1f}_{0}\) (100 TeV) = 2.0 · 10\(^{−17}\) GeV\(^{−1}\) cm\(^{−2}\)s\(^{−1}\)sr\(^{−1}\). Under this assumption, at most two events of the IceCube cosmic candidates can originate from the Galactic Ridge. A simple power-law extrapolation of the Fermi-LAT flux to account for IceCube High Energy Starting Events is excluded at 90% confidence level.
KW  - neutrino emission
KW  - Galactic Ridge
KW  - ANTARES telescope
Y1  - 2016
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-166608
VL  - 760
ER  - 
TY  - JOUR
A1  - Dimopoulos, Meletios A.
A1  - Weisel, Katja C.
A1  - Song, Kevin W.
A1  - Delforge, Michel
A1  - Karlin, Lionel
A1  - Goldschmidt, Hartmut
A1  - Moreau, Philippe
A1  - Banos, Anne
A1  - Oriol, Albert
A1  - Garderet, Laurent
A1  - Cavo, Michele
A1  - Ivanova, Valentina
A1  - Alegre, Adrian
A1  - Martinez-Lopez, Joaquin
A1  - Chen, Christine
A1  - Spencer, Andrew
A1  - Knop, Stefan
A1  - Bahlis, Nizar J.
A1  - Renner, Christoph
A1  - Yu, Xin
A1  - Hong, Kevin
A1  - Sternas, Lars
A1  - Jacques, Christian
A1  - Zaki, Mohamed H.
A1  - San Miguel, Jesus F.
T1  - Cytogenetics and long-term survival of patients with refractory or relapsed and refractory multiple myeloma treated with pomalidomide and low-dose dexamethasone
JF  - Haematologica
N2  - Patients with refractory or relapsed and refractory multiple myeloma who no longer receive benefit from novel agents have limited treatment options and short expected survival. del(17p) and t(4;14) are correlated with shortened survival. The phase 3 MM-003 trial demonstrated significant progression-free and overall survival benefits from treatment with pomalidomide plus low-dose dexamethasone compared to high-dose dexamethasone among patients in whom bortezomib and lenalidomide treatment had failed. At an updated median follow-up of 15.4 months, the progression-free survival was 4.0 versus 1.9 months (HR, 0.50; P<0.001), and median overall survival was 13.1 versus 8.1 months (HR, 0.72; P=0.009). Pomalidomide plus low-dose dexamethasone, compared with high-dose dexamethasone, improved progression-free survival in patients with del(17p) (4.6 versus 1.1 months; HR, 0.34; P < 0.001), t(4;14) (2.8 versus 1.9 months; HR, 0.49; P=0.028), and in standard-risk patients (4.2 versus 2.3 months; HR, 0.55; P<0.001). Although the majority of patients treated with high-dose dexamethasone took pomalidomide after discontinuation, the overall survival of patients treated with pomalidomide plus low-dose dexamethasone or highdose dexamethasone was 12.6 versus 7.7 months (HR, 0.45; P=0.008) in patients with del(17p), 7.5 versus 4.9 months (HR, 1.12; P=0.761) in those with t(4;14), and 14.0 versus 9.0 months (HR, 0.85; P=0.380) in standard-risk subjects. The overall response rate was higher in patients treated with pomalidomide plus low-dose dexamethasone than in those treated with high-dose dexamethasone both among standard-risk patients (35.2% versus 9.7%) and those with del(17p) (31.8% versus 4.3%), whereas it was similar in patients with t(4; 14) (15.9% versus 13.3%). The safety of pomalidomide plus low-dose dexamethasone was consistent with initial reports. In conclusion, pomalidomide plus low-dose dexamethasone is efficacious in patients with relapsed/refractory multiple myeloma and del(17p) and/or t(4;14).
KW  - translocation
KW  - plus dexamethasone
KW  - deletion 17P
KW  - bortezomib
KW  - therapy
KW  - abnormalities
KW  - stem-cell transplantation
KW  - growth-factor receptor 3
KW  - high-risk cytogenetics
KW  - intergroupe francophone
Y1  - 2015
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-140349
VL  - 100
IS  - 10
SP  - 1327
EP  - 1333
ER  - 
TY  - JOUR
A1  - Kasprzak, J.
A1  - Sivalertporn, K.
A1  - Albert, F.
A1  - Schneider, C.
A1  - Höfling, S.
A1  - Kamp, M.
A1  - Forchel, A.
A1  - Muljarov, E. A.
A1  - Langbein, W.
T1  - Coherence dynamics and quantum-to-classical crossover in an exciton-cavity system in the quantum strong coupling regime
JF  - New Journal of Physics
N2  - Interaction between light and matter generates optical nonlinearities, which are particularly pronounced in the quantum strong coupling regime. When a single bosonic mode couples to a single fermionic mode, a Jaynes-Cummings (JC) ladder is formed, which we realize here using cavity photons and quantum dot excitons. We measure and model the coherent anharmonic response of this strongly coupled exciton-cavity system at resonance. Injecting two photons into the cavity, we demonstrate a \(\sqrt 2\) larger polariton splitting with respect to the vacuum Rabi splitting. This is achieved using coherent nonlinear spectroscopy, specifically four-wave mixing, where the coherence between the ground state and the first (second) rung of the JC ladder can be interrogated for positive (negative) delays. With increasing excitation intensity and thus rising average number of injected photons, we observe spectral signatures of the quantum-to-classical crossover of the strong coupling regime.
KW  - Jaynes-Cummings ladder
KW  - spectral interferometry
KW  - photon
KW  - dot
KW  - spectroscopy
KW  - oscillations
KW  - microcavity
KW  - resonance
KW  - light
Y1  - 2013
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-123005
SN  - 1367-2630
VL  - 15
IS  - 045013
ER  - 
TY  - JOUR
A1  - Hopfmann, C.
A1  - Albert, F.
A1  - Schneider, C.
A1  - Höfling, S.
A1  - Kamp, M.
A1  - Forchel, A.
A1  - Kanter, I.
A1  - Reizenstein, S.
T1  - Nonlinear emission characteristics of quantum dot-micropillar lasers in the presence of polarized optical feedback
JF  - New Journal of Physics
N2  - We report on electrically pumped quantum dot-microlasers in the presence of polarized self-feedback. The high-\(\beta\) microlasers show two orthogonal, linearly polarized emission modes which are coupled via the common gain medium. This coupling is explained in terms of gain competition between the two lasing modes and leads to distinct differences in their input-output characteristics. By applying polarized self-feedback via an external mirror, we are able to control the laser characteristics of the emission modes in terms of the output power, the coherence time and the photon statistics. We find that linearly polarized self-feedback stabilizes the lasing of a given mode, while cross-polarized feedback between the two modes reduces strongly the intensity of the other emission mode showing particular high-intensity fluctuations and even super-thermal values of the photon autocorrelation function \(g^{(2)} (\tau)\) at zero delay. Measurements of \(g^{(2)} (\tau)\) under external feedback also allow us to detect revival peaks associated with the round trip time of the external cavity. Analyzing the damping and shape of the \(g^{(2)} (\tau)\) revival peaks by a phenomenological model provides us insight into the underlying physics such as the effective exciton lifetime and gain characteristics of the quantum dots in the active region of these microlasers.
KW  - semiconductor lasers
KW  - coherence
KW  - system
KW  - gain
Y1  - 2013
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-123127
SN  - 1367-2630
VL  - 15
IS  - 025030
ER  - 
TY  - JOUR
A1  - van Koolwijk, Leonieke M. E.
A1  - Ramdas, Wishal D.
A1  - Ikram, M. Kamran
A1  - Jansonius, Nomdo M.
A1  - Pasutto, Francesca
A1  - Hys, Pirro G.
A1  - Macgregor, Stuart
A1  - Janssen, Sarah F.
A1  - Hewitt, Alex W.
A1  - Viswanathan, Ananth C.
A1  - ten Brink, Jacoline B.
A1  - Hosseini, S. Mohsen
A1  - Amin, Najaf
A1  - Despriet, Dominiek D. G.
A1  - Willemse-Assink, Jacqueline J. M.
A1  - Kramer, Rogier
A1  - Rivadeneira, Fernando
A1  - Struchalin, Maksim
A1  - Aulchenko, Yurii S.
A1  - Weisschuh, Nicole
A1  - Zenkel, Matthias
A1  - Mardin, Christian Y.
A1  - Gramer, Eugen
A1  - Welge-Lüssen, Ulrich
A1  - Montgomery, Grant W.
A1  - Carbonaro, Francis
A1  - Young, Terri L.
A1  - Bellenguez, Céline
A1  - McGuffin, Peter
A1  - Foster, Paul J.
A1  - Topouzis, Fotis
A1  - Mitchell, Paul
A1  - Wang, Jie Jin
A1  - Wong, Tien Y.
A1  - Czudowska, Monika A.
A1  - Hofman, Albert
A1  - Uitterlinden, Andre G.
A1  - Wolfs, Roger C. W.
A1  - de Jong, Paulus T. V. M.
A1  - Oostra, Ben A.
A1  - Paterson, Andrew D.
A1  - Mackey, David A.
A1  - Bergen, Arthur A. B.
A1  - Reis, Andre
A1  - Hammond, Christopher J.
A1  - Vingerling, Johannes R.
A1  - Lemij, Hans G.
A1  - Klaver, Caroline C. W.
A1  - van Duijn, Cornelia M.
T1  - Common Genetic Determinants of Intraocular Pressure and Primary Open-Angle Glaucoma
JF  - PLoS Genetics
N2  - Intraocular pressure (IOP) is a highly heritable risk factor for primary open-angle glaucoma and is the only target for current glaucoma therapy. The genetic factors which determine IOP are largely unknown. We performed a genome-wide association study for IOP in 11,972 participants from 4 independent population-based studies in The Netherlands. We replicated our findings in 7,482 participants from 4 additional cohorts from the UK, Australia, Canada, and the Wellcome Trust Case-Control Consortium 2/Blue Mountains Eye Study. IOP was significantly associated with rs11656696, located in GAS7 at 17p13.1 (p = 1.4 x 10\(^{-8}\)), and with rs7555523, located in TMCO1 at 1q24.1 (p = 1.6 x 10\(^{-8}\)). In a meta-analysis of 4 case-control studies (total N = 1,432 glaucoma cases), both variants also showed evidence for association with glaucoma (p = 2.4 x 10\(^{-2}\) for rs11656696 and p = 9.1 x 10\(^{-4}\) for rs7555523). GAS7 and TMCO1 are highly expressed in the ciliary body and trabecular meshwork as well as in the lamina cribrosa, optic nerve, and retina. Both genes functionally interact with known glaucoma disease genes. These data suggest that we have identified two clinically relevant genes involved in IOP regulation.
KW  - expression
KW  - goldmann applanation tonometer
KW  - central corneal thickness
KW  - genome-wide scan
KW  - beaver-dam eye
KW  - to-disc ratio
KW  - onset
KW  - association
KW  - identification
KW  - population
Y1  - 2012
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-131378
VL  - 8
IS  - 5
ER  -