90 results on '"L. MOSCOSO"'
Search Results
2. Comparación de dos dosis de FSHp en la superovulación de ovejas Pelibuey
- Author
-
Juan C. Alvarado, Daniel E. Argudo, Andrés L. Moscoso, Hugo J. Hernández-Fonseca, Fernando P. Perea, and José. M. Rodríguez
- Published
- 2022
- Full Text
- View/download PDF
3. Evaluación seminal de conejos sometidos a un programa de iluminación continua
- Author
-
Daniel Ernesto Argudo Garzon, Alexandra Eras, Juan C. Alvarado, Andrés L. Moscoso, and Dina. M. Veloz
- Published
- 2022
- Full Text
- View/download PDF
4. AQUAPONIA: PRODUÇÃO DE PEIXES E VEGETAIS
- Author
-
Marcelo Batista da, Silva, primary, Renato Miguel L. Moscoso, Pessôa, additional, Willian Ivaldo de, Moura, additional, Ricardo José Araújo, Miranda, additional, and Willy Vila Nova, Pessoa, additional
- Published
- 2018
- Full Text
- View/download PDF
5. 195 Follicular wave synchronisation with oestradiol Benzoate or gonadotrophin-releasing hormone for ovum pickup in lactating Holstein cows
- Author
-
D. F. Idrovo, J. C. Alvarado, A. L. Moscoso, C. A. Soria, J. C. Durán, and D. E. Argudo
- Subjects
Endocrinology ,Reproductive Medicine ,Genetics ,Animal Science and Zoology ,Molecular Biology ,Developmental Biology ,Biotechnology - Published
- 2022
- Full Text
- View/download PDF
6. Rapid subduction in the deep North Western Mediterranean
- Author
-
C. Richardt, D. Dornic, D. Lo Presti, G.E. Păvălaş, M. Morganti, Oleg Kalekin, Isabelle Taupier-Letage, K. Lyons, M. Circella, Uli Katz, A. Mazure, G. Halladjian, D. Zaborov, M. Ardid, A. Radu, Francisco Camarena, J. Hößl, H. Laschinsky, C. Curtil, A. Albert, M. Neff, Gisela Anton, Robert Lahmann, Vincenzo Cavasinni, C. Distefano, C. Donzaud, B. Vallage, A. Brown, U. Fritsch, Antonio Capone, P. Payre, C. M. Reed, Annarita Margiotta, J. J. Aubert, Jürgen Brunner, J.-L. Fuda, Maurizio Spurio, Anne Deschamps, R. Pillet, U. Emanuele, A.J. Heijboer, J. Carr, F. M. Schoeck, M. P. Decowski, C. Racca, F. Salesa, L. Tasca, Thierry Pradier, G. Guillard, J.J. Hernández-Rey, Gregory David Hallewell, H. Loehner, G. Lelaizant, C. Picq, S. Loucatos, Dominique Lefèvre, S.F. Biagi, E. A. De Wolf, Holger Motz, S. Basa, Vincent Bertin, M. Marcelin, N. Picot-Clemente, R. Auer, Juanan Aguilar, R. Ostasch, G. Wijnker, Manuela Vecchi, Ciro Bigongiari, Heide Costantini, Alexander Kappes, G. Riccobene, D. Castel, G.V. Russo, V. Flaminio, G. De Bonis, Giuseppina Larosa, J.P. Gómez-González, I. Dekeyser, F. Lucarelli, Jos Steijger, V. Van Elewyck, F. Fehr, Gilles Maurin, P. Vernin, Rezo Shanidze, P. Coyle, J. Zúñiga, Thomas Eberl, V. Popa, W. Kretschmer, J. P. Schuller, M.C. Bouwhuis, M. Rujoiu, Stephanie Escoffier, M. Bazzotti, J.-P. Ernenwein, P. Piattelli, Simona Toscano, K. Fratini, Manuel Bou-Cabo, Francesco Simeone, N. Cottini, Patrick Lamare, A. C.S. Assis Jesus, Tri L. Astraatmadja, Th. Stolarczyk, S. Anvar, S. Mangano, Yann Hello, Guillaume Lambard, J.A. Martínez-Mora, H. van Haren, E. Castorina, Kay Graf, Christian Tamburini, Ph. Charvis, J. Petrovic, G. Giacomelli, C. Naumann, G. Palioselitis, B. Baret, Doriane Drouhin, Antoine Kouchner, M. Melissas, H. Yepes, E. Presani, Tommaso Chiarusi, C. Kopper, Teresa Montaruli, R. Coniglione, J.D. Zornoza, Nasser Kalantar-Nayestanaki, M. de Jong, M. Anghinolfi, J. Busto, L. Moscoso, S. Cecchini, G. Lim, P. Kooijman, G. Carminati, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Paris Cité (UPCité), Institut Pluridisciplinaire Hubert Curien (IPHC), and Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Convection ,[SDU.OCEAN]Sciences of the Universe [physics]/Ocean, Atmosphere ,Subduction ,Large detector systems for particle and astroparticle physics ,Cherenkov detectors ,visible and IR photons (vacuum) ,Vortex ,Boundary current ,law.invention ,Telescope ,Acoustic Doppler current profiler ,Amplitude ,Oceanography ,Water column ,law ,[SDU]Sciences of the Universe [physics] ,Neutrino detectors ,Photon detectors for UV, visible and IR photons (vacuum) ,Photon detectors for UV ,Geology - Abstract
An Acoustic Doppler Current Profiler (ADCP) moored at the deep-sea ANTARES neutrino telescope site near Toulon, France, measured downward vertical currents of amplitudes up to 0.03 m s−1 in spring 2006. The currents were accompanied by enhanced levels of acoustic reflection by a factor of about 10 and by horizontal currents reaching 0.35 m s−1. These observations coincided with high levels of bioluminescence detected by the telescope. Although during winter 2006 deep dense-water formation occurred in this area, episodes of high levels of suspended particles and large vertical currents continuing into the summer are not direct evidence of this process. It is hypothesized that the main process allowing for particles to be moved across the entire water column (2500 m) within a few days, is local convection, triggered by small-mesoscale phenomena, such as meanders including a bipolar vortex, linked with boundary current instabilities.
- Published
- 2022
7. Administration of two doses of recombinant bovine somatotropin reduces cell damage in vitrified/warmed embryos from superovulated Pelibuey ewes
- Author
-
J C Alvarado, D E Argudo, A L Moscoso, H J Hernández, F P Perea, and J M Rodríguez
- Published
- 2021
- Full Text
- View/download PDF
8. Measurement of atmospheric neutrino oscillations with the ANTARES neutrino telescope
- Author
-
C. Vallée, V. Giordano, M. Taiuti, H. Loehner, M. Ferri, M. Circella, J.-P. Ernenwein, K. Fehn, Y. Hello, C. Richardt, R. Richter, Alexander Kappes, U. Emanuele, M. Neff, A. Rostovtsev, J. Carr, A. Sánchez-Losa, C. Donzaud, M. Morganti, S. Galatà, A. Spies, D. Zaborov, C. Carloganu, M. P. Decowski, M. de Jong, F. M. Schoeck, Miguel Ardid, U. Fritsch, I. Dekeyser, Anne Deschamps, P.M. Kooijman, C. Distefano, D. F. E. Samtleben, Anne Robert, G. De Bonis, Giuseppina Larosa, Dominique Lefèvre, H. Yepes, A. Trovato, J.P. Gómez-González, A. Kouchner, M. Anghinolfi, Jürgen Brunner, Q. Dorosti, Tri L. Astraatmadja, Z. Charif, C. M. Reed, P. Vernin, L. Core, A. Gleixner, L. Moscoso, K. Payet, S. Anvar, F. Schuessler, M. Marcelin, Vladimir Kulikovskiy, Athina Meli, S. Cecchini, Juan José Hernández-Rey, Manuel Bou-Cabo, Francesco Simeone, Jörn Wilms, D. Lo Presti, A. Capone, Jos Steijger, T. Seitz, Thomas Eberl, G. Guillard, I. Al Samarai, R. Coniglione, G.E. Păvălaş, F. Louis, Teresa Montaruli, C. Rivière, V. Bertin, S. Ferry, Th. Stolarczyk, D. Dornic, Gisela Anton, S. Mangano, Guillaume Lambard, I. Kreykenbohm, M. Vecchi, S. Loucatos, B. Baret, M. Hamal, E. Visser, H. van Haren, Oleg Kalekin, G. Lim, A. Creusot, C. Bogazzi, Matthias Kadler, Christian Tamburini, Ph. Charvis, C. C. Hsu, E. Nezri, B. Vallage, C. Curtil, K. Geyer, D. Lattuada, S. Adrián-Martínez, Holger Motz, Maurizio Spurio, F. Folger, Robert Lahmann, A.J. Heijboer, E. Presani, B. Herold, Gregory David Hallewell, Tommaso Chiarusi, C. Kopper, J. Schmid, K. Roensch, J.-L. Fuda, Paolo Fermani, S. Wagner, Michel André, O. Kavatsyuk, Arnauld Albert, S. Basa, V. Van Elewyck, J. P. Schuller, J. Petrovic, C. Racca, Rezo Shanidze, P. Coyle, G. Giacomelli, Uli Katz, D. Palioselitis, Doriane Drouhin, G.V. Russo, A. Enzenhoefer, E. A. De Wolf, Jose Busto, G. Wijnker, Annarita Margiotta, J. Zúñiga, S. Biagi, Heide Costantini, J. Ruiz-Rivas, M.C. Bouwhuis, J.A. Martínez-Mora, Piera Sapienza, V. Flaminio, B. Bouhou, V. Popa, M. Rujoiu, Stephanie Escoffier, J-J. Aubert, Giorgio Riccobene, J.D. Zornoza, Kay Graf, T. Pradier, Jutta Schnabel, J. Hoessl, Ciro Bigongiari, Paolo Piattelli, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Département d'Electronique, des Détecteurs et d'Informatique pour la Physique (ex SEDI) (DEDIP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'océanologie de Marseille (COM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de la Méditerranée - Aix-Marseille 2, Département de Physique des Particules (ex SPP) (DPP), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire des technologies de la microélectronique (LTM), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), ANTARES, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Centre National de la Recherche Scientifique (CNRS), Centre Tecnològic de Vilanova i la Geltrú, Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques, Montaruli, Teresa, Antares, Collaboration, S., Adrián-Martínez, I., Al Samarai, A., Albert, M., André, M., Anghinolfi, G., Anton, S., Anvar, M., Ardid, T., Astraatmadja, Aubert, J. -J., B., Baret, S., Basa, V., Bertin, S., Biagi, C., Bigongiari, C., Bogazzi, M., Bou-Cabo, B., Bouhou, Bouwhuis, M. C., J., Brunner, J., Busto, A., Capone, C., Cârloganu, J., Carr, S., Cecchini, Z., Charif, Ph., Charvi, T., Chiarusi, M., Circella, R., Coniglione, L., Core, H., Costantini, P., Coyle, A., Creusot, C., Curtil, G., De Boni, Decowski, M. P., I., Dekeyser, A., Deschamp, C., Distefano, C., Donzaud, D., Dornic, Q., Dorosti, D., Drouhin, T., Eberl, U., Emanuele, A., Enzenhöfer, Ernenwein, J. -P., S., Escoffier, K., Fehn, P., Fermani, M., Ferri, S., Ferry, V., Flaminio, F., Folger, U., Fritsch, Fuda, J. -L., S., Galatà, P., Gay, K., Geyer, G., Giacomelli, V., Giordano, A., Gleixner, Gómez-González, J. P., K., Graf, G., Guillard, G., Hallewell, M., Hamal, H., van Haren, Heijboer, A. J., Y., Hello, Hernández-Rey, J. J., B., Herold, J., Hößl, Hsu, C. C., M., de Jong, M., Kadler, O., Kalekin, A., Kappe, U., Katz, O., Kavatsyuk, P., Kooijman, C., Kopper, A., Kouchner, I., Kreykenbohm, V., Kulikovskiy, R., Lahmann, G., Lambard, G., Larosa, D., Lattuada, D., Lefèvre, G., Lim, D., Lo Presti, H., Loehner, S., Loucato, F., Loui, S., Mangano, M., Marcelin, A., Margiotta, Martínez-Mora, J. A., A., Meli, T., Montaruli, M., Morganti, L., Moscoso, H., Motz, M., Neff, E., Nezri, D., Palioseliti, Păvălaş, G. E., K., Payet, J., Petrovic, P., Piattelli, V., Popa, T., Pradier, E., Presani, C., Racca, C., Reed, G., Riccobene, C., Richardt, R., Richter, C., Rivière, A., Robert, K., Roensch, A., Rostovtsev, J., Ruiz-Riva, M., Rujoiu, Russo, G. V., Samtleben, D. F. E., A., Sánchez-Losa, P., Sapienza, J., Schmid, J., Schnabel, F., Schöck, Schuller, J. -P., F., Schüssler, T., Seitz, R., Shanidze, F., Simeone, A., Spie, M., Spurio, Steijger, J. J. M., Th., Stolarczyk, M., Taiuti, C., Tamburini, Trovato, A, B., Vallage, C., Vallée, V., Van Elewyck, M., Vecchi, P., Vernin, E., Visser, S., Wagner, G., Wijnker, J., Wilm, E., de Wolf, H., Yepe, D., Zaborov, Zornoza, J. D., J., Zúñiga, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Département d'Electronique, des Détecteurs et d'Informatique (ex SEDI) (DEDI), APC - Astrophysique des Hautes Energies (APC - AHE), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Commissariat à l'Énergie Atomique et aux Énergies Alternatives (CEA) - Grenoble-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), ANTARES (IHEF, IoP, FNWI), S. Adrian-Martinez, I. Al Samarai, A. Albert, M. Andre, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, T. Astraatmadja, J.-J. Aubert, B. Baret, S. Basa, V. Bertin, S. Biagi, C. Bigongiari, C. Bogazzi, M. Bou-Cabo, B. Bouhou, M. C. Bouwhui, J. Brunner, J. Busto, A. Capone, C. Carloganu, J. Carr, S. Cecchini, Z. Charif, Ph. Charvi, T. Chiarusi, M. Circella, R. Coniglione, L. Core, H. Costantini, P. Coyle, A. Creusot, C. Curtil, G. De Boni, M. P. Decowski, I. Dekeyser, A. Deschamp, C. Distefano, C. Donzaud, D. Dornic, Q. Dorosti, D. Drouhin, T. Eberl, U. Emanuele, A. Enzenhoefer, J.-P. Ernenwein, S. Escoffier, K. Fehn, P. Fermani, M. Ferri, S. Ferry, V. Flaminio, F. Folger, U. Fritsch, J.-L. Fuda, S. Galata, P. Gay, K. Geyer, G. Giacomelli, V. Giordano, A. Gleixner, J. P. Gomez-Gonzalez, K. Graf, G. Guillard, G. Hallewell, M. Hamal, H. van Haren, A. J. Heijboer, Y. Hello, J. J. Hernandez-Rey, B. Herold, J. Hoessl, C. C. Hsu, M. de Jong, M. Kadler, O. Kalekin, A. Kappe, U. Katz, O. Kavatsyuk, P. Kooijman, C. Kopper, A. Kouchner, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, G. Lambard, G. Larosa, D. Lattuada, D. Lefevre, G. Lim, D. Lo Presti, H. Loehner, S. Loucato, F. Loui, S. Mangano, M. Marcelin, A. Margiotta, J. A. Martinez-Mora, A. Meli, T. Montaruli, M. Morganti, L. Moscoso, H. Motz, M. Neff, E. Nezri, D. Palioseliti, G. E. Pavala, K. Payet, J. Petrovic, P. Piattelli, V. Popa, T. Pradier, E. Presani, C. Racca, C. Reed, G. Riccobene, C. Richardt, R. Richter, C. Riviere, A. Robert, K. Roensch, A. Rostovtsev, J. Ruiz-Riva, M. Rujoiu, G. V. Russo, D. F. E. Samtleben, A. Sanchez-Losa, P. Sapienza, J. Schmid, J. Schnabel, F. Schoeck, J.-P. Schuller, F. Schuessler, T. Seitz, R. Shanidze, F. Simeone, A. Spie, M. Spurio, J. J. M. Steijger, Th. Stolarczyk, M. Taiuti, C. Tamburini, A. Trovato, B. Vallage, C. Vallee, V. Van Elewyck, M. Vecchi, P. Vernin, E. Visser, S. Wagner, G. Wijnker, J. Wilm, E. de Wolf, H. Yepe, D. Zaborov, J. D. Zornoza, and J. Zuniga
- Subjects
Nuclear and High Energy Physics ,Particle physics ,[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Physics::Instrumentation and Detectors ,Solar neutrino ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,ddc:500.2 ,Neutrino telescope ,01 natural sciences ,Partícules (Física nuclear) ,High Energy Physics - Experiment ,Nuclear physics ,High Energy Physics - Experiment (hep-ex) ,Experiment ,0103 physical sciences ,Neutrins ,High Energy Physics ,Neutrinos ,010306 general physics ,Neutrino oscillation ,Physics ,Muon ,ANTARES ,Física [Àrees temàtiques de la UPC] ,010308 nuclear & particles physics ,Neutrino oscillations ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,High Energy Physics::Phenomenology ,Solar neutrino problem ,Neutrino astrophysics ,Cosmic neutrino background ,Neutrino detector ,FISICA APLICADA ,Measurements of neutrino speed ,Física nuclear ,High Energy Physics::Experiment ,Neutrino ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] - Abstract
The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximal mixing, a mass difference of Delta m(32)(2) = (3.1 +/- 0.9) . 10(-3) eV(2) is obtained, in good agreement with the world average value. (C) 2012 Elsevier B.V. All rights reserved., The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'energie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS-UEFISCDI), Romania; Ministerio de Ciencia e Innovacion (MICINN), Prometeo of Generalitat Valenciana and MultiDark, Spain; Agence de l'Oriental and CNRST, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.
- Published
- 2012
- Full Text
- View/download PDF
9. Management of androgenetic alopecia: a comparative clinical study between plasma rich in growth factors and topical minoxidil
- Author
-
M. R. Navarro, Ander Pino, Adel Martínez Martínez, C. Molina, M. Asín, L. Moscoso, M. A. Martínez, Gorka Orive, and Eduardo Anitua
- Subjects
medicine.medical_specialty ,integumentary system ,business.industry ,Retrospective cohort study ,medicine.disease ,Dermatology ,body regions ,Clinical study ,030207 dermatology & venereal diseases ,03 medical and health sciences ,chemistry.chemical_compound ,0302 clinical medicine ,Hair loss ,chemistry ,Minoxidil ,030220 oncology & carcinogenesis ,Hair Disorder ,Finasteride ,Medicine ,Surgery ,business ,Adverse effect ,Topical minoxidil ,medicine.drug - Abstract
Androgenetic alopecia (AGA) is a common hair disorder. Finasteride and minoxidil have been approved by the Food and Drug Administration (FDA) for the treatment of AGA. However, some side effects have been related to the intake of these drugs. Recently, plasma rich in growth factors has emerged as a safe alternative for the management of pattern hair loss. The purposes of the present study are to evaluate and compare the efficacy and safety of plasma rich in growth factors (PRGFs) versus topical minoxidil treatment in AGA-affected patients. Following a retrospective case control design, 379 patients treated with either PRGF or minoxidil were included in this study. Diagnostic trichograms at baseline and 4 months after treatment were performed with the aim of analyzing the anagen/telogen hair change improvement. PRGF-treated patients showed higher anagen hair increase improvement compared to minoxidil-treated ones (6.9 ± 0.4 and 4.6 ± 0.5 %, respectively) (p
- Published
- 2016
- Full Text
- View/download PDF
10. AQUAPONIA: PRODUÇÃO DE PEIXES E VEGETAIS
- Author
-
Miranda Ricardo José Araújo, Pessôa Renato Miguel L. Moscoso, Moura Willian Ivaldo de, Silva Marcelo Batista da, and Pessoa Willy Vila Nova
- Published
- 2018
- Full Text
- View/download PDF
11. Performance of the front-end electronics of the ANTARES neutrino telescope
- Author
-
E. Delagnes, Francisco Camarena, R. Ostasch, C. Carloganu, D. Lo Presti, M. Ardid, Annarita Margiotta, Y. Hello, Antoine Kouchner, F. Lucarelli, J. J. Aubert, Vincent Bertin, F. Fehr, J. Poinsignon, G.V. Russo, Oleg Kalekin, Nasser Kalantar-Nayestanaki, G. Vannoni, M. Circella, M. Morganti, E. Castorina, J.-P. Ernenwein, Gisela Anton, T. Legou, C. Picq, E. Falchini, Dominique Lefèvre, C. Richardt, E. A. De Wolf, D. Dornic, J. Fopma, J. Petrovic, Juanan Aguilar, G. Wijnker, U. Emanuele, G. Giacomelli, C. Naumann, M. Rujoiu, Stephanie Escoffier, M.C. Bouwhuis, W. Kretschmer, Giorgio Riccobene, Paolo Piattelli, F. Rethore, G. Halladjian, Ciro Bigongiari, H. Lafoux, U. F. Katz, D. Palioselitis, Doriane Drouhin, J.D. Zornoza, Jürgen Brunner, A. Le Van Suu, K. Fratini, V. Van Elewyck, Thierry Pradier, H. Loehner, Teresa Montaruli, J. P. Schuller, C. Hoffmann, G. Guillard, Ch Olivetto, Holger Motz, G. E. Pavala, S. Mangano, H. Costantini, C. M. Reed, Manuel Bou-Cabo, Francesco Simeone, M. Neff, F. M. Schoeck, M. de Jong, R. Auer, A. Capone, J. Hoessl, Anne Deschamps, Alain Mazure, P. Payre, B. Baret, S. Basa, Alexander Kappes, S. Biagi, Manuela Vecchi, G. Carminati, H. Yepes, S. Loucatos, H. Le Provost, L. Tasca, V. Flaminio, [No Value] Charvis, Patrick Lamare, A. C.S. Assis Jesus, G. Lim, P. Vernin, Tri L. Astraatmadja, Th. Stolarczyk, J-P Pineau, J.A. Martínez-Mora, Th. Chaleil, N. Cottini, U. Fritsch, P.M. Kooijman, Guillaume Lambard, M. Marcelin, Robert Lahmann, S. Anvar, V. Popa, H. van Haren, E. Presani, B. Herold, C. Curtil, N. Chon Sen, F. Feinstein, A. Brown, Tommaso Chiarusi, I. Dekeyser, C. Kopper, A. Radu, Jos Steijger, G. De Bonis, Giuseppina Larosa, D. Zaborov, Christian Tamburini, J.-L. Fuda, J. Zúñiga, Gregory David Hallewell, C. Donzaud, J. P. Gómez-González, D. Lachartre, Vincenzo Cavasinni, C. Distefano, E. Monmarthe, L. Caponetto, Kay Graf, B. Vallage, Arnauld Albert, M. Anghinolfi, J. Busto, Piera Sapienza, M. Bazzotti, Thomas Eberl, L. Moscoso, G. Lelaizant, F. Salesa, S. Cecchini, J. Carr, F. Druillole, N. de Botton, H. Laschinsky, Simona Toscano, C. Racca, N. Picot-Clemente, Rezo Shanidze, P. Coyle, Maurizio Spurio, A.J. Heijboer, Juan José Hernández-Rey, I. Al Samarai, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 6526), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), APC - Astrophysique des Hautes Energies (APC - AHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), ANTARES, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Département de Physique des Particules (ex SPP) (DPP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de la Méditerranée - Aix-Marseille 2, Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), ANTARES (IHEF, IoP, FNWI), KVI - Center for Advanced Radiation Technology, J.A. Aguilar, A. Albert, G. Anton, S. Anvar, M. Ardid, A.C. Assis Jesus, T. Astraatmadja, J.-J. Aubert, R. Auer, B. Baret, S. Basa, M. Bazzotti, V. Bertin, S. Biagi, C. Bigongiari, M. Bou-Cabo, M.C. Bouwhuis, A.M. Brown, J. Brunner, J. Busto, F. Camarena, A. Capone, G. Carminati, J. Carr, D. Castel, E. Castorina, V. Cavasinni, S. Cecchini, Ph. Charvis, T. Chiarusi, M. Circella, R. Coniglione, H. Costantini, N. Cottini, P. Coyle, C. Curtil, G. De Boni, M.P. Decowski, I. Dekeyser, A. Deschamps, C. Distefano, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, U. Emanuele, J.-P. Ernenwein, S. Escoffier, F. Fehr, V. Flaminio, K. Fratini, U. Fritsch, J.-L. Fuda, G. Giacomelli, J.P. Gómez-González, K. Graf, G. Guillard, G. Halladjian, G. Hallewell, H. van Haren, A.J. Heijboer, Y. Hello, J.J. Hernández-Rey, J. Hößl, M. de Jong, N. Kalantar-Nayestanaki a, O. Kalekin, A. Kappes, U. Katz, P. Kooijman, C. Kopper, A. Kouchner, W. Kretschmer, R. Lahmann, P. Lamare, G. Lambard, G. Larosa, H. Laschinsky, D. Lefèvre, G. Lelaizant, G. Lim, D. Lo Presti a, H. Loehner a, S. Loucatos, F. Lucarelli, K. Lyons, S. Mangano, M. Marcelin, A. Margiotta, J.A. Martinez-Mora, G. Maurin, A. Mazure, M. Melissas, T. Montaruli, M. Morganti, L. Moscoso, H. Motz, C. Naumann, M. Neff, R. Ostasch, D. Palioselitis, G.E. Pa˘va˘las, P. Payre, J. Petrovic, P. Piattelli, N. Picot-Clemente, C. Picq, R. Pillet, V. Popa, T. Pradier, E. Presani, C. Racca, A. Radu, C. Reed, C. Richardt, M. Rujoiu a, G.V. Russo, F. Salesa, P. Sapienza, F. Schöck, J.-P. Schuller, R. Shanidze, F. Simeone, M. Spurio, J.J.M. Steijger, Th. Stolarczyk, M. Taiuti, C. Tamburini, L. Tasca, S. Toscano, B. Vallage, V. Van Elewyck, M. Vecchi, P. Vernin, G. Wijnker, E. de Wolf, H. Yepes, D. Zaborov a, J.D. Zornoza, and J. Zúñiga
- Subjects
Nuclear and High Energy Physics ,Photomultiplier ,[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,Physics::Instrumentation and Detectors ,Optical link ,Digital data ,FOS: Physical sciences ,Analog-to-digital converter ,Neutrino telescope ,01 natural sciences ,Multiplexing ,law.invention ,Phototube ,Application-specific integrated circuit ,Photomultiplier tube ,law ,ASICs ,0103 physical sciences ,14. Life underwater ,010306 general physics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,Instrumentation ,Physics ,010308 nuclear & particles physics ,business.industry ,ASIC ,Astrophysics::Instrumentation and Methods for Astrophysics ,Electrical engineering ,CIRCUIT ,Front-end electronics ,Chip ,[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,Física nuclear ,UNDERWATER DETECTOR ,asic ,front-end electronics ,neutrino telescope ,photomultiplier tube ,Astrophysics - Instrumentation and Methods for Astrophysics ,business ,SYSTEM - Abstract
ANTARES is a high-energy neutrino telescope installed in the Mediterranean Sea at a depth of 2475 m. It consists of a three-dimensional array of optical modules, each containing a large photomultiplier tube. A total of 2700 front-end ASICs named Analogue Ring Samplers (ARS) process the phototube signals, measure their arrival time, amplitude and shape as well as perform monitoring and calibration tasks. The ARS chip processes the analogue signals from the optical modules and converts information into digital data. All the information is transmitted to shore through further multiplexing electronics and an optical link. This paper describes the performance of the ARS chip; results from the functionality and characterization tests in the laboratory are summarized and the long-term performance in the apparatus is illustrated., Comment: 20 pages, 22 figures, published in Nuclear Instruments and Methods A
- Published
- 2010
- Full Text
- View/download PDF
12. Studies of a full-scale mechanical prototype line for the ANTARES neutrino telescope and tests of a prototype instrument for deep-sea acoustic measurements
- Author
-
T. Legou, M. Ruppi, Chantal Compère, R. Ostasch, F. Urbano, Timo Karg, Diego Real, C. Gojak, V. Valente, G. Lamanna, V. Roca, V. Flaminio, C. Fiorello, I. Sokalski, J. Beltramelli, M. Taiuti, E. Kok, A. Rostovtsev, M.C. Bouwhuis, H. Loehner, A. Bigi, Chiara Roda, E. Falchini, Dominique Lefèvre, A. Le Van Suu, R. De Vita, F. Réthoré, V. Popa, H. Zaccone, J.R. Hubbard, Patrick Lamare, S. Cuneo, Julien Lavalle, Annarita Margiotta, K. Fratini, H. Laschinsky, Nicole Béthoux, R. Coniglione, Rosario Megna, C. Petta, L. Caponetto, C. Colnard, G. Wobbe, V. Niess, A. Ceres, Mario Musumeci, N. Randazzo, Thierry Pradier, G. Giacomelli, A. Heijboer, B. Vallage, B. Dinkespieler, J. Poinsignon, G. Damy, H. Le Provost, J. J. Aubert, R. Pillet, Nasser Kalantar-Nayestanaki, G. Vaudaine, G. Lelaizant, J.M. Gallone, F. Schmitt, F. Jouvenot, Paolo Sapienza, M. Jaquet, E. A. De Wolf, J. P. Schuller, G. Rusydi, Elie Aslanides, J. Carr, B. Hartmann, A. F. Yao, Holger Motz, A. Albert, P. Vernin, R. van Dantzig, R. Auer, S. Anvar, Juanan Aguilar, G. Wijnker, K. Salomon, M. de Jong, K. Streeb, Corinne Donzaud, J.J. Hernández-Rey, F. Salesa, J.-P. Pineau, D. Castel, G.V. Russo, S. Loucatos, M. Melissas, Robert Lahmann, Yvonne Becherini, Philippe Charvis, B. van Rens, J. P. Ernenwein, M. Marcelin, R. Masullo, Mohsen Harakeh, M. Circella, Alexander Kappes, F. Cafagna, L. A. M. Tasca, P. Valdy, D. Lo Presti, Gregory David Hallewell, Nathalie Palanque-Delabrouille, W. Kretschmer, V. Bertin, J. van Randwijk, Stephanie Escoffier, P. Payre, Tommaso Chiarusi, J.-L. Fuda, R. Blaes, M. Ageron, N. Cottini, G. Debonis, C. Kopper, V. Lyashuk, H. Peek, F. Lucarelli, S. Mangano, P. Lagier, J.D. Zornoza, M. Battaglieri, J.-X. Dessa, F. Fehr, G. Lim, Guillaume Lambard, Charling Tao, F.E. Ardellier-Desages, V. Rigaud, Jürgen Brunner, J.J. Destelle, E. Barbarito, U. F. Katz, C. Olivetto, S. Kuch, I. Dekeyser, L. Caillat, F. Guilloux, C. Naumann, Ana G. Pérez, F. Louis, P. Goret, C. De Marzo, Christian Tamburini, A. J. Noble, R. Bruijn, J. F. Drogou, T. Spona, F. Feinstein, J. Hößl, L. R. Sulak, M. Naumann-Godo, A. S. Cussatlegras, P. Piattelli, D. Zaborov, A. Kruijer, T. Montaruli, P. Chauchot, G. Loaec, J. Zúñiga, Anne Deschamps, S. Galeotti, Alain Mazure, J. Hogenbirk, Emanuele Castorina, C. Hoffman, G. Riccobene, D. Denans, F. Ameli, Vincenzo Cavasinni, C. Distefano, M. Billault, Y. Le Guen, M. Bazzotti, H. Kok, S. Basa, Eric Delagnes, J.-C. Languillat, M. Ripani, Jean-Francois Rolin, E. Carmona, Antoine Kouchner, G. Terreni, Dominique Durand, S. Cecchini, E. Heine, R. van Wijk, M. Morganti, Kay Graf, P. Coyle, Jean-Paul Kneib, Gisela Anton, T. Stolarczyk, C. Racca, J.-Y. Coail, Marc Régnier, S. Favard, A. Calzas, L. Moscoso, Rezo Shanidze, Antonio Capone, N. Girard, Maurizio Spurio, J. Roux, G. Venekamp, P. Kooijman, M. Jaspers, B. Verlaat, Yann Hello, P. Keller, G. van der Steenhoven, F. Mazéas, M. Anghinolfi, G. F. Burgio, J. Busto, P. Rewiersma, M. Mongelli, E. Migneco, F. Druillole, N. de Botton, High Energy Astrophys. & Astropart. Phys (API, FNWI), ANTARES (IHEF, IoP, FNWI), M. AGERON, J.A. AGUILAR, A. ALBERT, F. AMELI, M. ANGHINOLFI, G. ANTON, S. ANVAR, F. ARDELLIER-DESAGES, E. ASLANIDES, J-J. AUBERT, R. AUER, E. BARBARITO, S. BASA, M. BATTAGLIERI, M. BAZZOTTI, Y. BECHERINI, N. BETHOUX, J. BELTRAMELLI, V. BERTIN, A. BIGI, M. BILLAULT, R. BLAES, N. DE BOTTON, M.C. BOUWHUIS, R. BRUIJN, J. BRUNNER, G.F. BURGIO, J. BUSTO, F. CAFAGNA, L. CAILLAT, A. CALZAS, A. CAPONE, L. CAPONETTO, E. CARMONA, J. CARR, D. CASTEL, E. CASTORINA, V. CAVASINNI, S. CECCHINI, A. CERES, P. CHARVIS, P. CHAUCHOT, T. CHIARUSI, M. CIRCELLA, J-Y- COAIL, C. COLNARD, C. COMPERE, R. CONIGLIONE, N. COTTINI, P. COYLE, S. CUNEO, A-S. CUSSATLEGRAS, G. DAMY, R. VAN DANTZIG, G. DE BONIS, C. DE MARZO, R. DE VITA, I. DEKEYSER, E. DELAGNES, D. DENANS, A. DESCHAMPS, J.-X. DESSA, J-J. DESTELLE, B. DINKESPIELER, C. DISTEFANO, C. DONZAUD, J-F. DROGOU, F. DRUILLOLE, D. DURAND, J-P. ERNENWEIN, S. ESCOFFIER, E. FALCHINI, S. FAVARD, F. FEHR, F. FEINSTEIN, C. FIORELLO, V. FLAMINIO, K. FRATINI, J-L. FUDA, S. GALEOTTI, J-M. GALLONE, G. GIACOMELLI, N. GIRARD, C. GOJAK, PH. GORET, K. GRAF, G. HALLEWELL, M.N. HARAKEH, B. HARTMANN, A. HEIJBOER, E. HEINE, Y. HELLO, J.J. HERNANDEZ-REY, J. HOSSL, C. HOFFMAN, J. HOGENBIRK, J.R. HUBBARD, M. JAQUET, M. JASPERS, M. DE JONG, F. JOUVENOT, N. KALANTAR-NAYESTANAKI, A. KAPPES, T. KARG, U. KATZ, P. KELLER, J. P. KNEIB, E. KOK, H. KOK, P. KOOIJMAN, C. KOPPER, A. KOUCHNER, W. KRETSCHMER, A. KRUIJER, S. KUCH, P. LAGIER, R. LAHMANN, G. LAMANNA, P. LAMARE, G. LAMBARD, J-C. LANGUILLAT, H. LASCHINSKY, J. LAVALLE, Y. LE GUEN, H.LE PROVOST, A. LE VAN SUU, D. LEFEVRE, T. LEGOU, G. LELAIZANT, G. LIM, D.LO PRESTI, G. LOAEC, H. LOEHNER, S. LOUCATOS, F. LOUIS, F. LUCARELLI, V. LYASHUK, S. MANGANO, M. MARCELIN, A. MARGIOTTA, R. MASULLO, F. MAZEAS, A. MAZURE, R. MEGNA, M. MELISSAS, E. MIGNECO, M. MONGELLI, T. MONTARULI, M. MORGANTI, L. MOSCOSO, H. MOTZ, M. MUSUMECI, M. NAUMANN-GODO, C. NAUMANN, V. NIESS, T. NOBLE, C. OLIVETTO, R. OSTASCH, N. PALANQUE-DELABROUILLE, P. PAYRE, H. PEEK, A. PEREZ, C. PETTA, P. PIATTELLI, R. PILLET, J-P. PINEAU, J. POINSIGNON, V. POPA, T. PRADIER, C. RACCA, N. RANDAZZO, J. VAN RANDWIJK, D. REAL, M. REGNIER, B. VAN RENS, F. RETHORE, P. REWIERSMA, G. RICCOBENE, V. RIGAUD, M. RIPANI, V. ROCA, C. RODA, J.F. ROLIN, A. ROSTOVTSEV, J. ROUX, M. RUPPI, G.V. RUSSO, G. RUSYDI, F. SALESA, K. SALOMON, P. SAPIENZA, F. SCHMITT, J-P. SCHULLER, R. SHANIDZE, I. SOKALSKI, T. SPONA, M. SPURIO, G. VAN DER STEENHOVEN, T. STOLARCZYK, K. STREEB, L. SULAK, M. TAIUTI, C. TAMBURINI, C. TAO, L. TASCA, G. TERRENI, F. URBANO, P. VALDY, V. VALENTE, B. VALLAGE, G. VAUDAINE, G. VENEKAMP, B. VERLAAT, P. VERNIN, R. VAN WIJK, G. WIJNKER, G. WOBBE, E. DE WOLF, A-F. YAO, D. ZABOROV, H. ZACCONE, J.D. ZORNOZA, J. ZUNIGA, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), ANTARES, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), KVI - Center for Advanced Radiation Technology, and Research unit Nuclear & Hadron Physics
- Subjects
leak detection ,Nuclear and High Energy Physics ,Acoustics ,ELECTROMECHANICAL CABLES ,Full scale ,electromechanical cable ,01 natural sciences ,Optics ,Data acquisition ,Data logger ,0103 physical sciences ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,optical time domain reflectometry ,14. Life underwater ,Time domain ,Electronics ,sea deployment ,010306 general physics ,Reflectometry ,Instrumentation ,Astroparticle physics ,Physics ,ANTARES ,Hydrophone ,antares ,underwater neutrino telescope ,010308 nuclear & particles physics ,business.industry ,ANTARES, underwater neutrino telescope, leak detection, optical time domain reflectometry, electromechanical cable, sea deployment ,UNDERWATER NEUTRINO TELESCOPES ,29.40.Ka, 29.90.+r, 92.10.Vz ,business - Abstract
full-scale mechanical prototype line was deployed to a depth of 2500 m to test the leak tightness of the electronics containers and the pressure-resistant properties of an electromechanical cable under evaluation for use in the ANTARES deep-sea neutrino telescope. During a month-long immersion study, line parameter data were taken using miniature autonomous data loggers and shore-based optical time domain reflectometry. Details of the mechanical prototype line, the electromechanical cable and data acquisition are presented. Data taken during the immersion study revealed deficiencies in the pressure resistance of the electromechanical cable terminations at the entry points to the electronics containers. The improvements to the termination, which have been integrated into subsequent detection lines, are discussed. The line also allowed deep-sea acoustic measurements with a prototype hydrophone system. The technical setup of this system is described, and the first results of the data analysis are presented. (c) 2007 Elsevier B.V. All rights reserved.
- Published
- 2007
- Full Text
- View/download PDF
13. Aniba canelilla as Corrosion Inhibitor of Carbon Steel
- Author
-
Valdir Florêncio da Veiga Junior, Ivan Napoleão Bastos, Dayana L. Custódio, Iuri Bezerra de Barros, and Hugo Z. L. Moscoso
- Subjects
Corrosion inhibitor ,chemistry.chemical_compound ,Materials science ,Carbon steel ,biology ,chemistry ,engineering ,Aniba ,General Chemistry ,engineering.material ,biology.organism_classification ,Nuclear chemistry - Published
- 2015
- Full Text
- View/download PDF
14. Search for a diffuse flux of high-energy muon neutrino with the ANTARES neutrino telescope
- Author
-
J. A. Aguilar, I. Al Samarai, A. Albert, M. André, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, A. C. Assis Jesus, T. Astraatmadj, J. J. Aubert, R. Auer, B. Baret, S. Basa, V. Bertin, C. Bigongiari, C. Bogazzi, M. Bou Cabo, M. C. Bouwhuis, A. M. Brown, J. Brunner, J. Busto, F. Camarena, A. Capone, C. Cârloganu, J. Carr, P.h. Charvis, M. Circella, R. Coniglione, H. Costantini, N. Cottini, P. Coyle, C. Curtil, M. P. Decowski, I. Dekeyser, A. Deschamps, C. Donzaud, D. Dornic, Q. Dorosti, D. Drouhin, T. Eberl, U. Emanuele, J. P. Ernenwein, S. Escoffier, F. Fehr, V. Flaminio, F. Folger, U. Fritsch, J. L. Fuda, S. Galata, P. Gay, J. P. Gómez González, K. Graf, G. Guillard, G. Halladjian, G. Hallewell, H. van Haren, A. J. Heijboer, Y. Hello, J. J. Hernández Rey, B. Herold, J. Hößl, C. C. Hsu, M. de Jon, M. Kadler, N. Kalantar Nayestanaki, O. Kalekin, A. Kappes, U. Katz, P. Kooijman, C. Kopper, A. Kouchner, V. Kulikovskiy, R. Lahmann, P. Lamar, G. Larosa, D. Lefèvre, G. Lim, D. Lo Presti, H. Loehner, S. Loucatos, F. Lucarelli, S. Mangano, M. Marcelin, J. A. Martinez Mora, A. Mazure, A. Meli, T. Montaruli, M. Morganti, L. Moscoso, H. Motz, C. Naumann, M. Neff, D. Palioselitis, G. E. Pa˘va˘las¸, P. Payre, J. Petrovic, P. Piattelli, N. Picot Clemente, C. Picq, V. Popa, T. Pradier, E. Presani, C. Racca, C. Reed, G. Riccobene, C. Richardt, K. Roensch, A. Rostovtsev, M. Rujoiu, G. V. Russo, F. Salesa, P. Sapienza, F. Schöck, J. P. Schuller, R. Shanidze, F. Simeone, A. Spies, J. J. M. Steijger, T.h. Stolarczyk, M. Taiuti, C. Tamburini, L. Tasca, S. Toscano, B. Vallage, V. Van Elewyck, G. Vannoni, M. Vecchi, P. Vernin, G. Wijnker, E. de Wolf, H. Yepes, D. Zaborov, J. D. Zornoza, J. Zúñiga, BAZZOTTI, MARCO, BIAGI, SIMONE, CARMINATI, GIADA, CECCHINI, STEFANO, CHIARUSI, TOMMASO, GIACOMELLI, GIORGIO MARIA, MARGIOTTA, ANNARITA, SPURIO, MAURIZIO, J.A. Aguilar, I. Al Samarai, A. Albert, M. André, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, A.C. Assis Jesus, T. Astraatmadj, J.-J. Aubert, R. Auer, B. Baret, S. Basa, M. Bazzotti, V. Bertin, S. Biagi, C. Bigongiari, C. Bogazzi, M. Bou-Cabo, M.C. Bouwhuis, A.M. Brown, J. Brunner, J. Busto, F. Camarena, A. Capone, C. Cârloganu, G. Carminati, J. Carr, S. Cecchini, Ph. Charvis, T. Chiarusi, M. Circella, R. Coniglione, H. Costantini, N. Cottini, P. Coyle, C. Curtil, M.P. Decowski, I. Dekeyser, A. Deschamp, C. Donzaud, D. Dornic, Q. Dorosti, D. Drouhin, T. Eberl, U. Emanuele, J.-P. Ernenwein, S. Escoffier, F. Fehr, V. Flaminio, F. Folger, U. Fritsch, J.-L. Fuda, S. Galata, P. Gay, G. Giacomelli, J.P. Gómez-González, K. Graf, G. Guillard, G. Halladjian, G. Hallewell, H. van Haren, A.J. Heijboer, Y. Hello, J.J. Hernández-Rey, B. Herold, J. Hößl, C.C. Hsu, M. de Jon, M. Kadler, N. Kalantar-Nayestanaki, O. Kalekin, A. Kappe, U. Katz, P. Kooijman, C. Kopper, A. Kouchner, V. Kulikovskiy, R. Lahmann, P. Lamar, G. Larosa, D. Lefèvre, G. Lim, D. Lo Presti, H. Loehner, S. Loucato, F. Lucarelli, S. Mangano, M. Marcelin, A. Margiotta, J.A. Martinez-Mora, A. Mazure, A. Meli, T. Montaruli, M. Morganti, L. Moscoso, H. Motz, C. Naumann, M. Neff, D. Palioseliti, G.E. Pa˘va˘las¸, P. Payre, J. Petrovic, P. Piattelli, N. Picot-Clemente, C. Picq, V. Popa, T. Pradier, E. Presani, C. Racca, C. Reed, G. Riccobene, C. Richardt, K. Roensch, A. Rostovtsev, M. Rujoiu, G.V. Russo, F. Salesa, P. Sapienza, F. Schöck, J.-P. Schuller, R. Shanidze, F. Simeone, A. Spie, M. Spurio, J.J.M. Steijger, Th. Stolarczyk, M. Taiuti, C. Tamburini, L. Tasca, S. Toscano, B. Vallage, V. Van Elewyck, G. Vannoni, M. Vecchi, P. Vernin, G. Wijnker, E. de Wolf, H. Yepes, D. Zaborov, J.D. Zornoza, and J. Zúñiga
- Subjects
ANTARES ,DIFFUSE MUON NEUTRINOS ,Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics::Instrumentation and Methods for Astrophysics ,ASTROPHYSICS SOURCES ,High Energy Physics::Experiment ,NEUTRINO TELESCOPE - Abstract
A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neutrino telescope is presented. A (0.83 × 2π) sr sky was monitored for a total of 334 days of equivalent live time. The searched signal corresponds to an excess of events, produced by astrophysical sources, over the expected atmospheric neutrino background. The observed number of events is found compatible with the background expectation. Assuming an E−2 flux spectrum, a 90% c.l. upper limit on the diffuse νμ flux of E2Φ90% = 5.3 × 10−8 GeVcm−2 s−1 sr−1 in the energy range 20 TeV–2.5 PeV is obtained. Other signal models with different energy spectra are also tested and some rejected.
- Published
- 2011
15. Time calibration of the ANTARES neutrino telescope
- Author
-
J. A. Aguilar, I. Al Samarai, A. Albert, M. André, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, A. C. Assis Jesus, T. Astraatmadj, J. J. Aubert, R. Auer, B. Baret, S. Basa, V. Bertin, C. Bigongiari, C. Bogazzi, M. Bou Cabo, M. C. Bouwhuis, A. M. Brown, J. Brunner, J. Busto, F. Camarena, A. Capone, C. Cârloganu, J. Carr, P.h. Charvis, T. Chiarusi, M. Circella, R. Coniglione, H. Costantini, N. Cottini, P. Coyle, C. Curtil, M. P. Decowski, I. Dekeyser, A. Deschamps, C. Donzaud, D. Dornic, Q. Dorosti, D. Drouhin, T. Eberl, U. Emanuele, J. P. Ernenwein, S. Escoffier, F. Fehr, V. Flaminio, F. Folger, U. Fritsch, J. L. Fuda, S. Galata, P. Gay, J. P. Gómez González, K. Graf, G. Guillard, G. Halladjian, G. Hallewell, H. van Haren, A. J. Heijboer, Y. Hello, J. J. Hernández Rey, B. Herold, J. Hößl, C. C. Hsu, M. de Jon, M. Kadler, N. Kalantar Nayestanaki, O. Kalekin, A. Kappes, U. Katz, P. Kooijman, C. Kopper, A. Kouchner, V. Kulikovskiy, R. Lahmann, P. Lamar, G. Larosa, D. Lefèvre, G. Lim, D. Lo Presti, H. Loehner, S. Loucatos, F. Lucarelli, S. Mangano, M. Marcelin, J. A. Martinez Mora, A. Mazure, A. Meli, T. Montaruli, M. Morganti, L. Moscoso, H. Motz, C. Naumann, M. Neff, D. Palioselitis, G. E. Pa˘va˘las¸, P. Payre, J. Petrovic, P. Piattelli, N. Picot Clemente, C. Picq, V. Popa, T. Pradier, E. Presani, C. Racca, C. Reed, G. Riccobene, C. Richardt, K. Roensch, A. Rostovtsev, M. Rujoiu, G. V. Russo, F. Salesa, P. Sapienza, F. Schöck, J. P. Schuller, R. Shanidze, F. Simeone, A. Spies, J. J. M. Steijger, T.h. Stolarczyk, M. Taiuti, C. Tamburini, L. Tasca, S. Toscano, B. Vallage, V. Van Elewyck, G. Vannoni, M. Vecchi, P. Vernin, G. Wijnker, E. de Wolf, H. Yepes, D. Zaborov, J. D. Zornoza, J. Zúñiga, BAZZOTTI, MARCO, BIAGI, SIMONE, CARMINATI, GIADA, CECCHINI, STEFANO, GIACOMELLI, GIORGIO MARIA, MARGIOTTA, ANNARITA, SPURIO, MAURIZIO, Instituto de Fisica Corpuscular (IFIC), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)-Universitat de València (UV), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Universitat Politècnica de Catalunya [Barcelona] (UPC), Erlangen Centre for Astroparticle Physics (ECAP), Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Universitat Politècnica de València (UPV), National Institute for Subatomic Physics [Amsterdam] (NIKHEF), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Enrico Fermi - Dipartimento di Fisica, University of Pisa - Università di Pisa, Dipartimento di Fisica [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 6526), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud 11 - Département de Physique, Université Paris-Sud - Paris 11 (UP11), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Royal Netherlands Institute for Sea Research (NIOZ), University of Groningen [Groningen], Faculteit Betawetenschappen, Universiteit Utrecht, Universiteit van Amsterdam (UvA), D.V. Skobeltsyn Institute of Nuclear Physics (SINP), Lomonosov Moscow State University (MSU), Dipartimento di Fisica e Astronomia [Catania], Università degli studi di Catania = University of Catania (Unict), University of Wisconsin-Madison, Institute of Space Science [Bucharest-Măgurele] (ISS), Institute of Theoretical and Experimental Physics [Moscow] (ITEP), National Research Center 'Kurchatov Institute' (NRC KI), KVI - Center for Advanced Radiation Technology, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Université Paris Diderot - Paris 7 (UPD7), Department of Physics [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome], Université Blaise Pascal - Clermont-Ferrand 2 (UBP), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Università degli studi di Catania [Catania], J.A. Aguilar, I. Al Samarai, A. Albert, M. André, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, A.C. Assis Jesus, T. Astraatmadj, J.-J. Aubert, R. Auer, B. Baret, S. Basa, M. Bazzotti, V. Bertin, S. Biagi, C. Bigongiari, C. Bogazzi, M. Bou-Cabo, M.C. Bouwhuis, A.M. Brown, J. Brunner, J. Busto, F. Camarena, A. Capone, C. Cârloganu, G. Carminati, J. Carr, S. Cecchini, Ph. Charvis, T. Chiarusi, M. Circella, R. Coniglione, H. Costantini, N. Cottini, P. Coyle, C. Curtil, M.P. Decowski, I. Dekeyser, A. Deschamp, C. Donzaud, D. Dornic, Q. Dorosti, D. Drouhin, T. Eberl, U. Emanuele, J.-P. Ernenwein, S. Escoffier, F. Fehr, V. Flaminio, F. Folger, U. Fritsch, J.-L. Fuda, S. Galata, P. Gay, G. Giacomelli, J.P. Gómez-González, K. Graf, G. Guillard, G. Halladjian, G. Hallewell, H. van Haren, A.J. Heijboer, Y. Hello, J.J. Hernández-Rey, B. Herold, J. Hößl, C.C. Hsu, M. de Jon, M. Kadler, N. Kalantar-Nayestanaki, O. Kalekin, A. Kappe, U. Katz, P. Kooijman, C. Kopper, A. Kouchner, V. Kulikovskiy, R. Lahmann, P. Lamar, G. Larosa, D. Lefèvre, G. Lim, D. Lo Presti, H. Loehner, S. Loucato, F. Lucarelli, S. Mangano, M. Marcelin, A. Margiotta, J.A. Martinez-Mora, A. Mazure, A. Meli, T. Montaruli, M. Morganti, L. Moscoso, H. Motz, C. Naumann, M. Neff, D. Palioseliti, G.E. Pa˘va˘las¸, P. Payre, J. Petrovic, P. Piattelli, N. Picot-Clemente, C. Picq, V. Popa, T. Pradier, E. Presani, C. Racca, C. Reed, G. Riccobene, C. Richardt, K. Roensch, A. Rostovtsev, M. Rujoiu, G.V. Russo, F. Salesa, P. Sapienza, F. Schöck, J.-P. Schuller, R. Shanidze, F. Simeone, A. Spie, M. Spurio, J.J.M. Steijger, Th. Stolarczyk, M. Taiuti, C. Tamburini, L. Tasca, S. Toscano, B. Vallage, V. Van Elewyck, G. Vannoni, M. Vecchi, P. Vernin, G. Wijnker, E. de Wolf, H. Yepes, D. Zaborov, J.D. Zornoza, J. Zúñiga., and ANTARES (IHEF, IoP, FNWI)
- Subjects
Optical telescopes ,Physics - Instrumentation and Detectors ,[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Physics::Instrumentation and Detectors ,01 natural sciences ,Optimal performance ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,Calibration procedure ,Dimensional arrays ,Angular resolution ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,Neutrino energy ,NEUTRINO TELESCOPE ,010303 astronomy & astrophysics ,Physics ,Detector ,Astrophysics::Instrumentation and Methods for Astrophysics ,Instrumentation and Detectors (physics.ins-det) ,Deep sea ,Neutrino detector ,Relative time ,Calibration ,Física nuclear ,Neutrino ,Astrophysics - Instrumentation and Methods for Astrophysics ,Time calibration ,Photomultiplier ,[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,Cherenkov light ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Scattering length ,Neutrino Telescopes ,Optical telescope ,Nuclear physics ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Tellurium compounds ,0103 physical sciences ,Optical systems ,14. Life underwater ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,DETECTOR ,Cherenkov radiation ,time calibration ,neutrino telescopes ,antares ,ANTARES ,010308 nuclear & particles physics ,Neutrino interactions ,Astronomy ,Elementary particles ,Astronomy and Astrophysics ,Photomultipliers ,FISICA APLICADA ,High Energy Physics::Experiment ,UNDERWATER DETECTOR ,Neutrino telescopes ,SYSTEM - Abstract
The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the vicinity of the detector. The large scattering length of light in the deep sea facilitates an angular resolution of a few tenths of a degree for neutrino energies exceeding 10 TeV. In order to achieve this optimal performance, the time calibration procedures should ensure a relative time calibration between the photomultipliers at the level of ~1 ns. The methods developed to attain this level of precision are described., The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'energie atomique et aux energies alternatives (CEA), Agence National de la Recherche (ANR), Commission Europeenne (FEDER fund and Marie Curie Program), Region Alsace (contract CPER), Region Provence-Alpes-Cote d'Azur, Departe-ment du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Ciencia e Innovacion (MICINN), Prometeo of Generalitat Valenciana (GVA) and MultiDark, Spain. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.
- Published
- 2011
- Full Text
- View/download PDF
16. Erratum to ‘‘Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope'
- Author
-
M. Ageron, J. A. Aguilar, A. Albert, F. Ameli, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, J. J. Aubert, J. Aublin, R. Auer, S. Basa, M. Bazzotti, V. Bertin, C. Bigongiari, M. Bou Cabo, M. C. Bouwhuis, R. Bruijn, J. Brunner, G. F. Burgio, J. Busto, F. Camarena, A. Capone, J. Carr, D. Castel, E. C.a.s.t.o.r.i.n.a., .V. Cavasinni, P.h. Charvis, M. Circella, C. Colnard, R. Coniglione, H. Costantini, N. Cottini, P. Coyle, G. De Bonis, P. Decowski, I. Dekeyser, A. D.e.s.c.h.a.m.p.s., .C. Donzaud, D. D.o.r.n.i.c., .D. Drouhin, F. Druillole, T. Eberl, J. P. Ernenwein, S. Escoffier, E. F.a.l.c.h.i.n.i., .F. Fehr, V. Flaminio, K. Fratini, J. L. Fuda, K. Graf, G. Guillard, G. Hallewell, Y. Hello, J. J. Hernández Rey, J. Hößl, M. de Jong, N. Kalantar Nayestanaki, O. Kalekin, A. Kappes, U. Katz, P. Kooijman, C. Kopper, A. Kouchner, W. K.r.e.t.s.c.h.m.e.r., .S. Kuch, R. Lahmann, P. Lamare, G. L.a.m.b.a.r.d., .H. Laschinsky, J. Lavalle, H. Le Provost, D. Lefèvre, G. Lelaizant, G. Lim, D. Lo Presti, H. Loehner, S. L.o.u.c.a.t.o.s., .F. Louis, F. L.u.c.a.r.e.l.l.i., .K. Lyons, S. M.a.n.g.a.n.o., .M. Marcelin, J. A. Martinez Mora, G. M.a.u.r.i.n., .A. Mazure, M. Melissas, E. Migneco, T. Montaruli, M. M.o.r.g.a.n.t.i., .L. Moscoso, H. Motz, C. N.a.u.m.a.n.n., .R. Ostasch, G. E. Pa, 728, va, 728, l.a.s., P. Payre, J. Petrovic, C. Petta, P. Piattelli, C. Picq, R. Pillet, V. Popa, T. P.r.a.d.i.e.r., .E. Presani, C. R.a.c.c.a., .A. Radu, C. Reed, C. Richardt, M. Rujoiu, M. Ruppi, G. V. Russo, F. S.a.l.e.s.a., .P. Sapienza, F. Schoeck, J. P. Schuller, R. Shanidze, G. van der Steenhoven, C. T.a.m.b.u.r.i.n.i., .L. Tasca, S. Toscano, M. Vecchi, P. Vernin, G. Wijnker, E. de Wolf, D. Zaborov, J. D. Zornoza, J. Zúñiga, BIAGI, SIMONE, CARMINATI, GIADA, CECCHINI, STEFANO, CHIARUSI, TOMMASO, GIACOMELLI, GIORGIO MARIA, MARGIOTTA, ANNARITA, SPURIO, MAURIZIO, M. Ageron, J.A. Aguilar , A. Albert , F. Ameli , M. Anghinolfi , G. Anton, S. Anvar , M. Ardid , J.-J. Aubert , J. Aublin ,R. Auer ,S. Basa ,M. Bazzotti ,V. Bertin ,S. Biagi,A. Bigi,C. Bigongiari , M. Bou-Cabo ,M.C. Bouwhuis ,R. Bruijn ,J. Brunner ,G.F. Burgio ,J. Busto ,F. Camarena ,A. Capone , G. Carminati ,J. Carr ,D. Castel ,E. Castorina,V. Cavasinni,S. Cecchini ,Ph. Charvis ,T. Chiarusi ,M. Circella ,C. Colnard ,R. Coniglione ,H. Costantini ,N. Cottini ,P. Coyle ,G. De Bonis ,P. Decowski , I. Dekeyser ,A. Deschamps,C. Donzaud,D. Dornic,D. Drouhin,F. Druillole ,T. Eberl,J.-P. Ernenwein , S. Escoffier ,E. Falchini,F. Fehr,V. Flaminio,K. Fratini ,J.-L. Fuda,G. Giacomelli ,K. Graf ,G. Guillard, G. Hallewell ,Y. Hello ,J.J. Hernández-Rey ,J. Hößl,M. de Jong,N. Kalantar-Nayestanaki ,O. Kalekin , A. Kappes ,U. Katz,P. Kooijman ,C. Kopper ,A. Kouchner ,W. Kretschmer,S. Kuch,R. Lahmann, P. Lamare ,G. Lambard,H. Laschinsky,J. Lavalle,H.Le Provost,D. Lefèvre ,G. Lelaizant ,G. Lim, D. Lo Presti ,H. Loehner ,S. Loucatos,F. Louis,F. Lucarelli,K. Lyons,S. Mangano,M. Marcelin,A. Margiotta ,J.A. Martinez-Mora ,G. Maurin,A. Mazure,M. Melissas ,E.Migneco,T. Montaruli, M. Morganti,L. Moscoso,H. Motz ,C. Naumann,R. Ostasch,G.E. Pa˘, va˘, and las,P. Payre,J. Petrovic , C. Petta ,P. Piattelli ,C. Picq,R. Pillet ,V. Popa ,T. Pradier,E. Presani,C. Racca,A. Radu,C. Reed, C. Richardt ,M. Rujoiu ,M. Ruppi,G.V. Russo ,F. Salesa,P. Sapienza,F. Schoeck ,J.-P. Schuller , R. Shanidze ,F. Simeone,M. Spurio,G. van der Steenhoven ,C. Tamburini,L. Tasca,S. Toscano , M. Vecchi ,P. Vernin,G. Wijnker ,E. de Wolf,D. Zaborov,J.D. Zornoza ,J. Zúñiga.
- Subjects
ATMOSPHERIC MUONS - Published
- 2010
17. Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope
- Author
-
B. Baret, H. Yepes, Thomas Eberl, L. Tasca, S. Loucatos, Patrick Lamare, A. C.S. Assis Jesus, S. Basa, Tri L. Astraatmadja, M. Ardid, S. Biagi, P. Payre, Hans van Haren, S. Anvar, A. Albert, D. Zaborov, V. Bertin, M. Rujoiu, Stephanie Escoffier, R. Ostasch, I. Dekeyser, F. Lucarelli, Thierry Pradier, F. Fehr, A. M. Brown, D. Lo Presti, Manuela Vecchi, J-J. Aubert, Th. Stolarczyk, G.E. Păvălaş, Juanan Aguilar, Teresa Montaruli, R. Auer, Antoine Kouchner, C. Picq, Damien Dornic, Jos Steijger, G. Wijnker, J.D. Zornoza, M. P. Decowski, Y. Hello, Dominique Lefèvre, Guillaume Lambard, Alexander Kappes, C. Richardt, Jose Busto, C. Naumann, S. Mangano, F. M. Schoeck, J. Carr, G. Lelaizant, M. Neff, Anne Deschamps, Oleg Kalekin, Alain Mazure, J.A. Martínez-Mora, J. Hoessl, Christian Tamburini, Antonio Capone, Maurizio Spurio, E. Castorina, E. Wolf, J. Zúñiga, A.J. Heijboer, J. Petrovic, C. Racca, Kay Graf, Ph. Charvis, V. Flaminio, G. Giacomelli, G. Palioselitis, M. Marcelin, V. Van Elewyck, Doriane Drouhin, N. Picot-Clemente, E. Presani, B. Herold, Tommaso Chiarusi, C. Kopper, Jürgen Brunner, V. Popa, U. Fritsch, J. P. Schuller, H. Costantini, A. Radu, Manuel Bou-Cabo, Francesco Simeone, Robert Lahmann, R. Coniglione, Rezo Shanidze, Ciro Bigongiari, Nasser Kalantar-Nayestanaki, Gregory David Hallewell, U. Emanuele, U. F. Katz, Vincenzo Cavasinni, C. Distefano, R. Pillet, M.C. Bouwhuis, M. Jong, J.-L. Fuda, K. Fratini, Piera Sapienza, M. Bazzotti, Francisco Camarena, Annarita Margiotta, Juan José Hernández-Rey, I. Al Samarai, Gisela Anton, G. Lim, N. Chon Sen, C. Donzaud, G. Carminati, Paolo Piattelli, F. Salesa, H. Loehner, M. Circella, J.-P. Ernenwein, G. Halladjian, P. Vernin, C. Cârloganu, B. Vallage, V. Russo, G. Guillard, Holger Motz, N. Cottini, M. Morganti, Simona Toscano, P. Coyle, H. Laschinsky, P.M. Kooijman, G. De Bonis, Giuseppina Larosa, W. Kretschmer, C. M. Reed, C. Curtil, J. P. Gómez-González, M. Anghinolfi, L. Moscoso, S. Cecchini, M. Ageron, J.A. Aguilar , A. Albert , F. Ameli , M. Anghinolfi , G. Anton, S. Anvar , M. Ardid , J.-J. Aubert , J. Aublin ,R. Auer ,S. Basa ,M. Bazzotti ,V. Bertin ,S. Biagi,A. Bigi,C. Bigongiari , M. Bou-Cabo ,M.C. Bouwhuis ,R. Bruijn ,J. Brunner ,G.F. Burgio ,J. Busto ,F. Camarena ,A. Capone , G. Carminati ,J. Carr ,D. Castel ,E. Castorina,V. Cavasinni,S. Cecchini ,Ph. Charvis ,T. Chiarusi ,M. Circella ,C. Colnard ,R. Coniglione ,H. Costantini ,N. Cottini ,P. Coyle ,G. De Bonis ,P. Decowski , I. Dekeyser ,A. Deschamps,C. Donzaud,D. Dornic,D. Drouhin,F. Druillole ,T. Eberl,J.-P. Ernenwein , S. Escoffier ,E. Falchini,F. Fehr,V. Flaminio,K. Fratini ,J.-L. Fuda,G. Giacomelli ,K. Graf ,G. Guillard, G. Hallewell ,Y. Hello ,J.J. Hernández-Rey ,J. Hößl,M. de Jong,N. Kalantar-Nayestanaki ,O. Kalekin , A. Kappes ,U. Katz,P. Kooijman ,C. Kopper ,A. Kouchner ,W. Kretschmer,S. Kuch,R. Lahmann, P. Lamare ,G. Lambard,H. Laschinsky,J. Lavalle,H.Le Provost,D. Lefèvre ,G. Lelaizant ,G. Lim, D. Lo Presti ,H. Loehner ,S. Loucatos,F. Louis,F. Lucarelli,K. Lyons,S. Mangano,M. Marcelin,A. Margiotta ,J.A. Martinez-Mora ,G. Maurin,A. Mazure,M. Melissas ,E.Migneco,T. Montaruli, M. Morganti,L. Moscoso,H. Motz ,C. Naumann,R. Ostasch,G.E. Pa˘, va˘, las,P. Payre,J. Petrovic , C. Petta ,P. Piattelli ,C. Picq,R. Pillet ,V. Popa ,T. Pradier,E. Presani,C. Racca,A. Radu,C. Reed, C. Richardt ,M. Rujoiu ,M. Ruppi,G.V. Russo ,F. Salesa,P. Sapienza,F. Schoeck ,J.-P. Schuller , R. Shanidze ,F. Simeone,M. Spurio,G. van der Steenhoven ,C. Tamburini,L. Tasca,S. Toscano , M. Vecchi ,P. Vernin,G. Wijnker ,E. de Wolf,D. Zaborov,J.D. Zornoza ,J. Zúñiga, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Erlangen Centre for Astroparticle Physics (ECAP), Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Universitat Politècnica de València (UPV), National Institute for Subatomic Physics [Amsterdam] (NIKHEF), Université Paris Diderot - Paris 7 (UPD7), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Enrico Fermi - Dipartimento di Fisica, University of Pisa - Università di Pisa, Instituto de Fisica Corpuscular (IFIC), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)-Universitat de València (UV), Dipartimento di Fisica [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Dipartimento di Fisica [Bologna], Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Géoazur (GEOAZUR 6526), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratori Nazionali del Sud (INFN), Istituto Nazionale di Fisica Nucleare (INFN), Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Domaines Océaniques (LDO), Institut national des sciences de l'Univers (INSU - CNRS)-Université de Brest (UBO)-Observatoire des Sciences de l'Univers-Institut d'écologie et environnement-Centre National de la Recherche Scientifique (CNRS), Département de Physique, Université Paris-Sud - Paris 11 (UP11), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), University of Groningen [Groningen], Dept. of Physics, University of Wisconsin-Madison, Faculteit Betawetenschappen, Universiteit Utrecht, Universiteit van Amsterdam (UvA), Dipartimento di Fisica e Astronomia [Catania], Università degli studi di Catania = University of Catania (Unict), Science Faculty CP230, Université libre de Bruxelles (ULB), Institutul de Ştiinţe Spaţiale, National Institute for Laser, Plasma and Radiation Physics (INFLPR), Institute of Space Science [Bucharest-Măgurele] (ISS), APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Institute of Theoretical and Experimental Physics [Moscow] (ITEP), National Research Center 'Kurchatov Institute' (NRC KI), KVI - Center for Advanced Radiation Technology, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Universitat Politecnica de Valencia (UPV), National Institute for Subatomic Physics Nikhef [Amsterdam] (NIKHEF), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Consejo Superior de Investigaciones Científicas [Spain] (CSIC)-Universitat de València (UV), Department of Physics [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' [Rome], Università di Bologna [Bologna] (UNIBO), Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), National Institute for Nuclear Physics (INFN), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de la Méditerranée - Aix-Marseille 2, Centre National de la Recherche Scientifique (CNRS)-Institut d'écologie et environnement-Observatoire des Sciences de l'Univers-Université de Brest (UBO)-Institut national des sciences de l'Univers (INSU - CNRS), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Università degli studi di Catania [Catania], Université Libre de Bruxelles [Bruxelles] (ULB), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Institute for Theoretical and Experimental Physics [Moscow] (ITEP), Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome], Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, and Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)
- Subjects
Photomultiplier ,Physics::Instrumentation and Detectors ,Astrophysics::High Energy Astrophysical Phenomena ,Atmospheric muons ,FOS: Physical sciences ,LINE ,Cosmic ray ,Potassium-40 ,01 natural sciences ,Particle detector ,Nuclear physics ,POTASSIUM-40 ,NEUTRINO TELESCOPES ,atmospheric muons ,depth intensity relation ,potassium-40 ,0103 physical sciences ,Depth intensity relation ,14. Life underwater ,010306 general physics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,ATMOSPHERIC MUONS ,Physics ,High Energy Astrophysical Phenomena (astro-ph.HE) ,010308 nuclear & particles physics ,Detector ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy and Astrophysics ,PERFORMANCE ,DEPTH INTENSITY RELATION ,LIGHT ,Neutrino detector ,13. Climate action ,ddc:540 ,Física nuclear ,High Energy Physics::Experiment ,Neutrino ,Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Instrumentation and Methods for Astrophysics ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,SYSTEM ,Lepton - Abstract
A new method for the measurement of the muon flux in the deep-sea ANTARES neutrino telescope and its dependence on the depth is presented. The method is based on the observation of coincidence signals in adjacent storeys of the detector. This yields an energy threshold of about 4 GeV. The main sources of optical background are the decay of 40K and the bioluminescence in the sea water. The 40K background is used to calibrate the efficiency of the photo-multiplier tubes., 10 pages, 4 figures
- Published
- 2010
- Full Text
- View/download PDF
18. Performance of the First ANTARES Detector Line
- Author
-
C. Colnard, Robert Lahmann, Antoine Kouchner, P. Vernin, J. P. Schuller, Gregory David Hallewell, A. Bigi, C. Picq, F. Louis, Paolo Piattelli, Jean-Pierre Ernenwein, H. Loehner, M. Anghinolfi, C. Naumann, E. Falchini, Dominique Lefèvre, J. Busto, E. A. De Wolf, J.-L. Fuda, M. Circella, M. Ruppi, G.E. Ip # v # la, G. Wijnker, Corinne Donzaud, P. Payre, M. de Jong, F. Druillole, Kay Graf, Jürgen Brunner, Guillaume Lambard, L. A. M. Tasca, Piera Sapienza, M. Bazzotti, Gilles Maurin, Manuel Bou-Cabo, Francesco Simeone, Christian Tamburini, Holger Motz, A. Radu, Ph. Charvis, G. van der Steenhoven, J. Zúñiga, K. Lyons, J. Jeffrey Carr, R. Coniglione, Vincenzo Cavasinni, G. F. Burgio, M. Ageron, E. Castorina, M. Ardid, S. Basa, R. Bruijn, Yann Hello, Nasser Kalantar-Nayestanaki, J. Petrovic, G. Carminati, G. Giacomelli, V. Bertin, N. Cottini, Francisco Camarena, S. Kuch, C. M. Reed, H. Costantini, Juan A. Aguilar, F. Ischoeck, Ciro Bigongiari, Doriane Drouhin, R. Auer, U. F. Katz, F. Salesa, Annarita Margiotta, C. Petta, Alexander Kappes, Simona Toscano, M. Melissas, Julien Lavalle, Thomas Eberl, G. Lim, E. Presani, Tommaso Chiarusi, C. Kopper, G. Guillard, Juan José Hernández-Rey, Arnauld Albert, P.M. Kooijman, D. Zaborov, V. Flaminio, G. De Bonis, S. Mangano, V. Popa, M. Morganti, H. Laschinsky, C. Richardt, M. Rujoiu, Stephanie Escoffier, J.D. Zornoza, D. Castel, G.V. Russo, T. Pradier, W. Kretschmer, R. Ostasch, G. Lelaizant, Patrick Lamare, S. Biagi, D. Dornic, S. Anvar, Yvonne Becherini, Oleg Kalekin, Emilio Migneco, Anne Deschamps, Alain Mazure, F. Ameli, F. Lucarelli, D. Lo Presti, F. Fehr, S. Cecchini, S. Loucatos, M. Vecchi, J. J. Aubert, M. Marcelin, T. Montaruli, Gisela Anton, R. Pillet, C. Racca, H. Leiprovost, P. Coyle, R. Ishanidze, Julien Aublin, M.C. Bouwhuis, P. Decowski, K. Fratini, A. Capone, Maurizio Spurio, Ivan Dekeyser, J.A. Martínez-Mora, L. Moscoso, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Département de Physique des Particules (ex SPP) (DPP), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Géoazur (GEOAZUR 6526), Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), APC - Astrophysique des Hautes Energies (APC - AHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), ANTARES, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), KVI - Center for Advanced Radiation Technology, High Energy Astrophys. & Astropart. Phys (API, FNWI), ANTARES (IHEF, IoP, FNWI), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de la Méditerranée - Aix-Marseille 2, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), M. Ageron, J.A. Aguilar, A. Albert, F. Ameli, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, J.-J. Aubert, J. Aublin, R. Auer, S. Basa, M. Bazzotti, Y. Becherini, V. Bertin, S. Biagi, A. Bigi, C. Bigongiari, M. Bou-Cabo, M.C. Bouwhui, R. Bruijn, J. Brunner, G.F. Burgio, J. Busto, F. Camarena, A. Capone, G. Carminati, J. Carr, D. Castel, E. Castorina, V. Cavasinni, S. Cecchini, Ph. Charvi, T. Chiarusi, M. Circella, C. Colnard, R. Coniglione, H. Costantini, N. Cottini, P. Coyle, G. De Boni, P. Decowski, I. Dekeyser, A. Deschamp, C. Donzaud, D. Dornic, D. Drouhin, F. Druillole, T. Eberl, J.-P. Ernenwein, S. Escoffier, E. Falchini, F. Fehr, V. Flaminio, K. Fratini, J.-L. Fuda, G. Giacomelli, K. Graf, G. Guillard, G. Hallewell, Y. Hello, J.J. Hernández-Rey, J. Hößl, M. de Jong, N. Kalantar-Nayestanaki, O. Kalekin, A. Kappe, U. Katz, P. Kooijman, C. Kopper, A. Kouchner, W. Kretschmer, S. Kuch, R. Lahmann, P. Lamare, G. Lambard, H. Laschinsky, J. Lavalle, H.Le Provost, D. Lefèvre, G. Lelaizant, G. Lim, D. Lo Presti, H. Loehner, S. Loucato, F. Loui, F. Lucarelli, K. Lyon, S. Mangano, M. Marcelin, A. Margiotta, J.A. Martinez-Mora, G. Maurin, A. Mazure, M. Melissa, E.Migneco, T. Montaruli, M. Morganti, L. Moscoso, H. Motz, C. Naumann, R. Ostasch, G.E. Pa˘va˘la, P. Payre, J. Petrovic, C. Petta, P. Piattelli, C. Picq, R. Pillet, V. Popa, T. Pradier, E. Presani, C. Racca, A. Radu, C. Reed, C. Richardt, M. Rujoiu, M. Ruppi, G.V. Russo, F. Salesa, P. Sapienza, F. Schoeck, J.-P. Schuller, R. Shanidze, F. Simeone, M. Spurio, G. van der Steenhoven, C. Tamburini, L. Tasca, S. Toscano, M. Vecchi, P. Vernin, G. Wijnker, E. de Wolf, D. Zaborov, J.D. Zornoza, and J. Zúñiga
- Subjects
MODULE ,Physics::Instrumentation and Detectors ,FOS: Physical sciences ,Astrophysics ,01 natural sciences ,Nuclear physics ,NEUTRINO TELESCOPES ,Angular distribution ,antares ,deep-sea ,first line ,neutrino ,0103 physical sciences ,Neutrino ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,WATER ,Angular resolution ,NEUTRINO TELESCOPE ,010306 general physics ,ATMOSPHERIC MUONS ,Astroparticle physics ,Physics ,Muon ,ANTARES ,010308 nuclear & particles physics ,Astrophysics (astro-ph) ,Detector ,Deep-sea ,Astronomy and Astrophysics ,Time resolution ,Geodesy ,MUON FLUX ,First line ,SINGLE ,Física nuclear ,UNDERWATER DETECTOR ,Line (text file) ,SYSTEM - Abstract
In this paper we report on the data recorded with the first Antares detector line. The line was deployed on the 14th of February 2006 and was connected to the readout two weeks later. Environmental data for one and a half years of running are shown. Measurements of atmospheric muons from data taken from selected runs during the first six months of operation are presented. Performance figures in terms of time residuals and angular resolution are given. Finally the angular distribution of atmospheric muons is presented and from this the depth profile of the muon intensity is derived., Comment: 14 pages, 9 figures
- Published
- 2009
- Full Text
- View/download PDF
19. Dark Matter Searches with the ANTARES Neutrino Telescope
- Author
-
A. Calzas, G. V. Russo, V. Roca-Blay, C. Ferdi, Elie Aslanides, E.-M. Clarke, A. Romeyer, H. Peek, C. Hoffmann, J.-F. Rollin, V. Lyashuk, Gisela Anton, T. Stolarczyk, M. Battaglieri, V. Niess, P. Keller, M. Ardid, F. Réthoré, F. Jouvenot, R. Bruyn, E. A. De Wolf, C. De Marzo, Antoine Kouchner, F. Mazéas, V. Bertin, J. Hoessl, E. Heine, P. Amram, J.-C. Languillat, Y. Le Guen, J.-L. Michel, E. Salusti, J. Jeffrey Carr, A. Usik, J.J. Destelle, De D.Zornoza, J. Boulesteix, A. Rostovtsev, A. Kruijer, M.C. Bouwhuis, S. Ferry, M. Billault, Alessia Capone, P.M. Kooijman, F. Burgio, F. Feinstein, D. Lo Presti, D. Zaborov, H. Le Provost, G. de Vries, J. Croquette, P. Piattelli, G. Venekamp, U. Katz, S. Loucatos, C. Racca, G. Giacomelli, J. E. McMillan, S. Saouter, P. Goret, I. Sokalski, Patrick Lamare, J.-F. Drougou, L. Laubier, V. Valente, J.J. Hernández-Rey, F. Louis, P. Coyle, Y. Benhammou, J.M. Gallone, G. Raia, T. Legou, A. Milovanovic, B. Dinkelspiler, S. Favard, E. V. Korolkova, M. Anghinolfi, Chantal Compère, L Lo Nigro, M. Romita, V. Popa, F. Sukowski, V. A. Kudryavtsev, A. Massol, M. Danilov, Philippe Charvis, Lester D.R. Thompson, S. Anvar, Yvonne Becherini, F. Bugeon, S. Cuneo, C. Petta, Fabrizio Ameli, H. Alleyne, J.J. Engelen, L. Caponetto, M. Ripani, E. Carmona, C. Olivetto, P. Vernin, F.E. Ardellier-Desages, S. L. Cartwright, Timo Karg, C. L. Naumann, B. Vallage, E. Migneco, Y. Sacquin, A. Bersani, K. Yearby, Anne Deschamps, J. Beltramelli, Alain Mazure, B. Hartmann, J. Hogenbirk, M. Godo, S. Cecchini, Sandra Zavatarelli, P.K.A. de Witt Huberts, M. Taiuti, E. Kok, G. Riccobene, R. van Wijk, T. Montaruli, Diego Real, M. Jaquet, J. Brunner, Yann Hello, O. Suvorova, Thierry Pradier, J.-P. Morel, G. Damy, D. Stubert, G. Herrouin, H. Zaccone, L. Moscoso, M. Circella, Annarita Margiotta, Maurizio Spurio, V. Zakharov, F. Cafagna, A.J. Heijboer, S. Karkar, W. Kretschmer, Alexander Kappes, J. J. Aubert, C. Millot, M. de Jong, P. Lagier, R. Blaes, P. Valdy, J.-P. Pineau, S. M. Bradbury, R. Masullo, Riccardo Papaleo, Roberto Bellotti, J. Zúñiga, M. Marcelin, J. P. Schuller, Mario Musumeci, A. Le Van Suu, R. De Vita, E. Vladimirsky, Gerardus Nooren, N. Randazzo, F. Druillole, D. Morgan, Elizabeth Winstanley, Jean Virieux, P. Payre, Gregory David Hallewell, H. J. Rose, Nathalie Palanque-Delabrouille, D. Festy, J. A. Aguilar, J.-L. Fuda, Van Rens, G. Vaudaine, R. van Dantzig, I. Varlamov, C. Maron, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Antares Collaboration
- Subjects
Nuclear and High Energy Physics ,Particle physics ,WIMP ,Astrophysics::High Energy Astrophysical Phenomena ,Dark matter ,Bubble Chamber ,neutrino telescopes ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,7. Clean energy ,0103 physical sciences ,Bubble chamber ,Dark Matter ,010306 general physics ,010303 astronomy & astrophysics ,Cherenkov radiation ,Physics ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,Geyser detector ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,Supersymmetry ,[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,Neutrino detector ,FISICA APLICADA ,Weakly interacting massive particles ,High Energy Physics::Experiment ,Neutrino - Abstract
[EN] The MOSCAB experiment (Materia OSCura A Bolle) uses the Geyser technique for dark matter search. The results of the first 0.5 kg mass prototype detector using superheated C3F8 liquid were very encouraging, achieving a 5 keV nuclear recoil threshold with high insensitivity to gamma radiation. Additionally, the technique seems to be easily scalable to higher masses for both in terms of complexity and costs, resulting in a very competitive technique for direct dark matter search, especially for the spin dependent case. Here, we report as well in the construction and commissioning of the big detector of 40 kg at the Milano-Bicocca University. The detector, the calibration tests and the evaluation of the background will be presented. Once demonstrated the functionality of the detector, it will be operated at the Gran Sasso National Laboratory in 2015., We acknowledge the financial support of the Spanish Ministerio de Ciencia e Innovación (MICINN) and Ministerio de Economía y Competitividad (MINECO), Grants FPA2012-37528-C02-02, and Consolider MultiDark CSD2009-00064, and of the Generalitat Valenciana, Grants ACOMP/2014/153 and PrometeoII/2014/079.
- Published
- 2014
- Full Text
- View/download PDF
20. High energy neutrino astronomy
- Author
-
L. Moscoso
- Subjects
Physics ,Nuclear and High Energy Physics ,Physics::Instrumentation and Detectors ,Solar neutrino ,Astronomy ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Solar neutrino problem ,Atomic and Molecular Physics, and Optics ,Particle detector ,Nuclear physics ,Neutrino detector ,Measurements of neutrino speed ,High Energy Physics::Experiment ,Neutrino ,Neutrino astronomy ,Lepton - Abstract
The sky survey with high energy neutrinos is complementary to the survey with photons. The method of the detection of ν μ is described and the expected sensitivity to high energy neutrino sources with a kilometer-scale detector is estimated. The status of the current under-water(ice) detector projects is reported.
- Published
- 2000
- Full Text
- View/download PDF
21. The data acquisition system for the ANTARES neutrino telescope
- Author
-
D. Zaborov, G.D. Hallewell, M. Morganti, Anne Deschamps, S. Galeotti, P. Chauchot, K. Salomon, V. Rigaud, C. Racca, Philippe Charvis, B. van Rens, J. Hogenbirk, S. L. Cartwright, M. Billault, C. Hoffman, H. Le Provost, P. Coyle, J.-C. Languillat, R. Bruijn, Chantal Compère, V. Flaminio, J.R. Hubbard, J. van Randwijk, L Lo Nigro, M. Romita, Paolo Sapienza, V. Roca, A. Calzas, V. Popa, M. Jaspers, C. Donzaud, V. Niess, S. Anvar, Yvonne Becherini, D. Lo Presti, Roberto Bellotti, J. Zúñiga, J. F. Drogou, M. Anghinolfi, P. Rewiersma, Robert Lahmann, C. Petta, P.K.A. de Witt Huberts, S. Basa, L. Caillat, U. F. Katz, D. Lachartre, H. Peek, T. Legou, Nathalie Palanque-Delabrouille, F. Lucarelli, Yann Hello, J. Carr, J. Busto, M. Ripani, Jean-Francois Rolin, E. Carmona, N. Cottini, A. Capone, S. Loucatos, Stephanie Escoffier, J-J. Aubert, Giorgio Riccobene, G. van der Steenhoven, F. Mazéas, G. F. Burgio, I. Sokalski, J. P. Schuller, M. Jaquet, M. Mongelli, E. Migneco, L. Moscoso, Eric Delagnes, F. Réthoré, J. P. Pineau, G. Venekamp, P. Kooijman, P. Goret, V. Lyashuk, J.D. Zornoza, M. Battaglieri, R. Ostasch, Emanuele Castorina, E. A. De Wolf, L. Caponetto, J. P. Ernenwein, Rosario Megna, Charling Tao, F. Louis, Juanan Aguilar, Timo Karg, G. Damy, V. A. Kudryavstev, F. Schmitt, T. Pradier, Diego Real, G. Lamanna, C. De Marzo, M. de Jong, V. Valente, T. Spona, I. Dekeyser, Tommaso Chiarusi, M. Naumann-Godo, A.-S. Cussatlegras, E. Falchini, A. Le Van Suu, R. De Vita, B. Dinkespieler, J. Hößl, F. Druillole, H. Lafoux, P. Piattelli, N. de Botton, F. Ameli, P. Payre, A.-F. Yao, J. Roux, C. Kopper, J.-J. Destelle, A. Milovanovic, M. Melissas, Chiara Roda, F. Feinstein, Mohsen Harakeh, Kay Graf, Lester D.R. Thompson, B. Vallage, P. Valdy, S. Cecchini, M.C. Bouwhuis, A. Heijboer, M. Circella, T. Montaruli, H. Zaccone, G. Wobbe, D. Denans, N. Girard, J. Beltramelli, Vincenzo Cavasinni, C. Distefano, H. Kok, R. van Wijk, Juan José Hernández-Rey, Maurizio Spurio, P. Keller, J. M. Gallone, R. Coniglione, G. de Vries, F. Dessages-Ardellier, H. Laschinsky, M. Ruppi, C. Olivetto, B. Hartmann, C. Gojak, M. Taiuti, M. Marcelin, Annarita Margiotta, R. van Dantzig, F. Jouvenot, A. Albert, K. Streeb, J. E. McMillan, H. J. Rose, S. M. Bradbury, Gisela Anton, T. Stolarczyk, J. Poinsignon, Nasser Kalantar-Nayestanaki, G. Terreni, V. Bertin, P. Lagier, G. Lim, F. Cafagna, R. Masullo, S. Favard, Elie Aslanides, Christian Tamburini, B. Verlaat, D. Festy, Alexander Kappes, Rezo Shanidze, S. Kuch, C. Naumann, F. Salesa, C. Colnard, Mario Musumeci, N. Randazzo, A. Kruijer, A. Rostovtsev, C. Fiorello, P. Vernin, E. V. Korolkova, A. Ceres, H. Loehner, Jürgen Brunner, E. Barbarito, S. Ferry, Y. Le Guen, D. Castel, G.V. Russo, G. Giacomelli, S. Karkar, W. Kretschmer, Antoine Kouchner, R. Blaes, Dominique Durand, S. Cuneo, Lawrence Sulak, E. Heine, P. Lamare, A. Mazure, A. Bigi, D. Stubert, KVI - Center for Advanced Radiation Technology, J.A. AGUILAR, A. ALBERT, F. AMELI, M. ANGHINOLFI, G. ANTON, S. ANVAR, E. ASLANIDES, J.-J. AUBERT, E. BARBARITO, S. BASA, M. BATTAGLIERI, Y. BECHERINI, R. BELLOTTI, J. BELTRAMELLI, V. BERTIN, A. BIGI, M. BILLAULT, R. BLAES, N. DE BOTTON, M.C. BOUWHUIS, S.M. BRADBURY, R. BRUIJN, J. BRUNNER, G.F. BURGIO, J. BUSTO, F. CAFAGNA, L. CAILLAT, A. CALZAS, A. CAPONE, L. CAPONETTO, E. CARMONA, J. CARR, S.L. CARTWRIGHT, D. CASTEL, E. CASTORINA, V. CAVASINNI, S. CECCHINI, A. CERES, P. CHARVIS, P. CHAUCHOT, T. CHIARUSI, M. CIRCELLA, C. COLNARD, C. COMPÈRE, R. CONIGLIONE, N. COTTINI, P. COYLE, S. CUNEO, A.-S. CUSSATLEGRAS, G. DAMY, R. VAN DANTZIG, C. DE MARZO, I. DEKEYSER, E. DELAGNES, D. DENANS, A. DESCHAMPS, F. DESSAGES-ARDELLIER, J.-J. DESTELLE, B. DINKESPIELER, C. DISTEFANO, C. DONZAUD, J.-F. DROGOU, F. DRUILLOLE, D. DURAND, J.-P. ERNENWEIN, S. ESCOFFIER, E. FALCHINI, S. FAVARD, F. FEINSTEIN, S. FERRY, D. FESTY, C. FIORELLO, V. FLAMINIO, S. GALEOTTI, J.-M. GALLONE, G. GIACOMELLI, N. GIRARD, C. GOJAK, PH. GORET, K. GRAF, G. HALLEWELL, M.N. HARAKEH, B. HARTMANN, A. HEIJBOER, E. HEINE, Y. HELLO, J.J. HERNÁNDEZ-REY, J. HÖßL, C. HOFFMAN, J. HOGENBIRK, J.R. HUBBARD, M. JAQUET, M. JASPERS, M. DE JONG, F. JOUVENOT, N. KALANTAR-NAYESTANAKI, A. KAPPES, T. KARG, S. KARKAR, U. KATZ, P. KELLER, H. KOK, P. KOOIJMAN, C. KOPPER, E.V. KOROLKOVA, A. KOUCHNER, W. KRETSCHMER, A. KRUIJER, S. KUCH, V.A. KUDRYAVSTEV, D. LACHARTRE, H. LAFOUX, P. LAGIER, R. LAHMANN, G. LAMANNA, P. LAMARE, J.C. LANGUILLAT, H. LASCHINSKY, Y. LE GUEN, H. LE PROVOST, A. LE VAN SUU, T. LEGOU, G. LIM, L. LO NIGRO, D. LO PRESTI, H. LOEHNER, S. LOUCATOS, F. LOUIS, F. LUCARELLI, V. LYASHUK, M. MARCELIN, A. MARGIOTTA, R. MASULLO, F. MAZÉAS, A. MAZURE, J.E. MCMILLAN, R. MEGNA, M. MELISSAS, E. MIGNECO, A. MILOVANOVIC, M. MONGELLI, T. MONTARULI, M. MORGANTI, L. MOSCOSO, M. MUSUMECI, C. NAUMANN, M. NAUMANN-GODO, V. NIESS, C. OLIVETTO, R. OSTASCH, N. PALANQUE-DELABROUILLE, P. PAYRE, H. PEEK, C. PETTA, P. PIATTELLI, J.-P. PINEAU, J. POINSIGNON, V. POPA, T. PRADIER, C. RACCA, N.RANDAZZO, J. VAN RANDWIJK, D. REAL, B. VAN RENS, F. RÉTHORÉ, P. REWIERSMA, G. RICCOBENE, V. RIGAUD, M. RIPANI, V. ROCA, C. RODA, J.F. ROLIN, M. ROMITA, H.J. ROSE, A. ROSTOVTSEV, J. ROUX, M. RUPPI, G.V. RUSSO, F. SALESA, K. SALOMON, P. SAPIENZA, F. SCHMITT, J.-P. SCHULLER, R. SHANIDZE, I. SOKALSKI, T. SPONA, M. SPURIO, G. VAN DER STEENHOVEN, T. STOLARCZYK, K. STREEB, D. STUBERT, L. SULAK, M. TAIUTI, C. TAMBURINI, C. TAO, G. TERRENI, L.F. THOMPSON, P. VALDY, V. VALENTE, B. VALLAGE, G. VENEKAMP, B. VERLAAT, P. VERNIN, R. DE VITA, G. DE VRIES, R. VAN WIJK, P. DE WITT HUBERTS, G. WOBBE, E. DE WOLF, A.-F. YAO, D. ZABOROV, H. ZACCONE, J.D. ZORNOZA, J. ZÚÑIGA, Groupe de Recherche en Physique des Hautes Energies (GRPHE), Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 6526), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut Français de Recherche pour l'Exploitation de la Mer - Brest (IFREMER Centre de Bretagne), Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER), Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), IFREMER - Centre de Toulon/La Seyne Sur Mer (IFREMER), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), ANTARES, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut Français de Recherche pour l'Exploitation de la Mer - Brest (IFREMER), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de la Méditerranée - Aix-Marseille 2, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
- Subjects
Nuclear and High Energy Physics ,[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Physics::Instrumentation and Detectors ,Data management ,Astrophysics::High Energy Astrophysical Phenomena ,Neutrino telescope ,ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION ,FOS: Physical sciences ,Astrophysics ,01 natural sciences ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Data filtering ,Data acquisition ,0103 physical sciences ,14. Life underwater ,Electronics ,010306 general physics ,Instrumentation ,data acquisition system ,neutrino telescope ,Remote sensing ,Astroparticle physics ,Physics ,neutrino telescope, data acquisition system ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,010308 nuclear & particles physics ,business.industry ,Detector ,Astrophysics (astro-ph) ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,Computer data storage ,Física nuclear ,business - Abstract
The ANTARES neutrino telescope is being constructed in the Mediterranean Sea. It consists of a large three-dimensional array of photo-multiplier tubes. The data acquisition system of the detector takes care of the digitisation of the photo-multiplier tube signals, data transport, data filtering, and data storage. The detector is operated using a control program interfaced with all elements. The design and the implementation of the data acquisition system are described., 20 pages, 6 figures, accepted for publication in Nucl. Instrum. Meth. A
- Published
- 2007
- Full Text
- View/download PDF
22. The ANTARES Optical Beacon System
- Author
-
E. Falchini, Dominique Lefèvre, J. F. Drogou, H. J. Rose, R. De Vita, A. Rostovtsev, D. Zaborov, J. P. Ernenwein, G. Lim, Guillaume Lambard, S. Cuneo, Lawrence Sulak, D. Lo Presti, Anne Deschamps, S. Galeotti, G. de Vries-Uiterweerd, Antoine Kouchner, H. Laschinsky, Christian Tamburini, H. Peek, Chantal Compère, J. Hogenbirk, V. Flaminio, A. S. Cussatlegras, V. Popa, Eric Delagnes, C. Petta, K. Streeb, Dominique Durand, F. Cafagna, E. Heine, G. Lelaizant, P. Lamare, C. Hoffman, M. Morganti, Stephanie Escoffier, H. Le Provost, E. Castorina, B. Vallage, Giorgio Riccobene, V. Lyashuk, J.D. Zornoza, M. Battaglieri, J. M. Gallone, R. Coniglione, T. Pradier, C. De Marzo, J. Beltramelli, G. Giacomelli, P. Goret, A. Capone, G. Venekamp, P. Kooijman, C. Olivetto, F. Urbano, A. Mazure, S. Kuch, Charling Tao, F. Louis, F. Jouvenot, I. Dekeyser, M. Jaquet, Annarita Margiotta, S. Favard, A. Milovanovic, M. Billault, Philippe Charvis, B. van Rens, J.-C. Languillat, R. Ostasch, J.R. Hubbard, G. Damy, F. Ameli, A. Albert, C. Fiorello, A. Bigi, D. Denans, E. A. De Wolf, C. Gojak, Timo Karg, J. Poinsignon, D. Castel, Nasser Kalantar-Nayestanaki, S. Anvar, G.V. Russo, Lester D.R. Thompson, Robert Lahmann, Juanan Aguilar, S. Cecchini, G. Wijnker, Chiara Roda, Vincenzo Cavasinni, C. Distefano, Jürgen Brunner, H. Kok, E. Barbarito, F. Réthoré, R. van Wijk, Juan José Hernández-Rey, J. P. Schuller, V. Valente, S. Loucatos, Nathalie Palanque-Delabrouille, P. Lagier, Paolo Piattelli, F.E. Ardellier-Desages, A. Calzas, J. P. Pineau, Diego Real, S. Ferry, J. van Randwijk, Julien Lavalle, J.-L. Fuda, E. V. Korolkova, Yvonne Becherini, F. Lucarelli, V. Bertin, F. Fehr, N. Girard, Elie Aslanides, W. Kretschmer, M. Taiuti, G. De Bonis, Y. Le Guen, I. Sokalski, J. Roux, R. Blaes, H. Zaccone, J.J. Destelle, T. Legou, A. Ceres, E. Kok, P. Valdy, G. Wobbe, V. Niess, T. Spona, L. Moscoso, A. Heijboer, G. Vaudaine, V. A. Kudryavstev, M. Melissas, Maurizio Spurio, M. Naumann-Godo, B. Verlaat, V. Roca, J. Hößl, P. Coyle, Rosario Megna, H. Loehner, B. Dinkespieler, Gregory David Hallewell, V. Rigaud, R. Auer, L. Caponetto, Paolo Sapienza, C. Racca, M. Ripani, Jean-Francois Rolin, E. Carmona, G. van der Steenhoven, Kay Graf, R. van Dantzig, Alexander Kappes, F. Mazéas, G. Terreni, S. L. Cartwright, C. Donzaud, G. F. Burgio, Tommaso Chiarusi, C. Kopper, M. Ruppi, S. Basa, Mohsen Harakeh, M. Circella, M. Jaspers, M. Ageron, Gisela Anton, T. Stolarczyk, R. Bruijn, M. Anghinolfi, J. Busto, P. Rewiersma, P. Keller, U. F. Katz, T. Noble, C. Naumann, P.K.A. de Witt Huberts, A. Le Van Suu, Yann Hello, C. Colnard, Mario Musumeci, N. Randazzo, J. J. Aubert, N. Cottini, L. Caillat, R. Pillet, P. Vernin, G. Lamanna, M. Mongelli, E. Migneco, J. Carr, F. Schmitt, K. Salomon, M. de Jong, F. Druillole, P. Payre, N. de Botton, M. Marcelin, Rezo Shanidze, M.C. Bouwhuis, G. Rusydi, A. F. Yao, K. Fratini, T. Montaruli, A. Perez, F. Salesa, A. Kruijer, F. Feinstein, P. Chauchot, J. Zúñiga, B. Hartmann, J. E. McMillan, S. M. Bradbury, R. Masullo, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Géoazur (GEOAZUR 6526), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut Français de Recherche pour l'Exploitation de la Mer - Brest (IFREMER Centre de Bretagne), Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER), Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), IFREMER - Centre de Toulon/La Seyne sur Mer (IFREMER - CENTRE DE TOULON/LA SEYNE SUR MER), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), ANTARES, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Biogéochimie des Contaminants Métalliques (LBCM), Biogéochimie et Ecotoxicologie (BE), Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER)-Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), M. AGERON, J.A. AGUILAR, A. ALBERT, F. AMELI, M. ANGHINOLFI, G. ANTON, S. ANVAR, F. ARDELLIER-DESAGES, E. ASLANIDES, J-J. AUBERT, R. AUER, E. BARBARITO, S. BASA, M. BATTAGLIERI, Y. BECHERINI, J. BELTRAMELLI, V. BERTIN, A. BIGI, M. BILLAULT, R. BLAES, N. DE BOTTON, M.C. BOUWHUIS, S.M. BRADBURY, R. BRUIJN, J. BRUNNER, G.F. BURGIO, J. BUSTO, F. CAFAGNA, L. CAILLAT, A. CALZAS, A. CAPONE, L. CAPONETTO, E. CARMONA, J. CARR, S.L. CARTWRIGHT, D. CASTEL, E. CASTORINA, V. CAVASINNI, S. CECCHINI, A. CERES, P. CHARVIS, P. CHAUCHOT, T. CHIARUSI, M. CIRCELLA, C. COLNARD, C. COMPERE, R. CONIGLIONE, N. COTTINI, P. COYLE, S. CUNEO, A-S. CUSSATLEGRAS, G. DAMY, R. VAN DANTZIG, G. DE BONIS, C. DE MARZO, R. DE VITA, I. DEKEYSER, E. DELAGNES, D. DENANS, A. DESCHAMPS, J-J. DESTELLE, B. DINKESPIELER, C. DISTEFANO, C. DONZAUD, J-F. DROGOU, F. DRUILLOLE, D. DURAND, J-P. ERNENWEIN, S. ESCOFFIER, E. FALCHINI, S. FAVARD, F. FEHR, F. FEINSTEIN, S. FERRY, C. FIORELLO, V. FLAMINIO, K. FRATINI, J-L. FUDA, S. GALEOTTI, J-M. GALLONE, G. GIACOMELLI, N. GIRARD, C. GOJAK, PH. GORET, K. GRAF, G. HALLEWELL, M.N. HARAKEH, B. HARTMANN, A. HEIJBOER, E. HEINE, Y. HELLO, J.J. HERNANDEZ-REY, J. HOSSL, C. HOFFMAN, J. HOGENBIRK, J.R. HUBBARD, M. JAQUET, M. JASPERS, M. DE JONG, F. JOUVENOT, N. KALANTAR-NAYESTANAKI, A. KAPPES, T. KARG, U. KATZ, P. KELLER, E. KOK, H. KOK, P. KOOIJMAN, C. KOPPER, E.V. KOROLKOVA, A. KOUCHNER, W. KRETSCHMER, A. KRUIJER, S. KUCH, V.A. KUDRYAVSTEV, P. LAGIER, R. LAHMANN, G. LAMANNA, P. LAMARE, G. LAMBARD, J-C. LANGUILLAT, H. LASCHINSKY, J. LAVALLE, Y. LE GUEN, H.LE PROVOST, A. LE VAN SUU, D. LEFEVRE, T. LEGOU, G. LELAIZANT, G. LIM, D.LO PRESTI, H. LOEHNER, S. LOUCATOS, F. LOUIS, F. LUCARELLI, V. LYASHUK, M. MARCELIN, A. MARGIOTTA, R. MASULLO, F. MAZEAS, MAZURE A.R, J.E. MCMILLAN, R. MEGNA, M. MELISSAS, E. MIGNECO, A. MILOVANOVIC, M. MONGELLI, T. MONTARULI, M. MORGANTI, L. MOSCOSO, M. MUSUMECI, M. NAUMANN-GODO, C. NAUMANN, V. NIESS, T. NOBLE, C. OLIVETTO, R. OSTASCH, N. PALANQUE-DELABROUILLE, P. PAYRE, H. PEEK, A. PEREZ, C. PETTA, P. PIATTELLI, R. PILLET, J-P. PINEAU, J. POINSIGNON, V. POPA, T. PRADIER, C. RACCA, N. RANDAZZO, J. VAN RANDWIJK, D. REAL, B. VAN RENS, F. RETHORE, P. REWIERSMA, G. RICCOBENE, V. RIGAUD, M. RIPANI, V. ROCA, C. RODA, J.F. ROLIN, H.J. ROSE, A. ROSTOVTSEV, J. ROUX, M. RUPPI, G.V. RUSSO, G. RUSYDI, F. SALESA, K. SALOMON, P. SAPIENZA, F. SCHMITT, J-P. SCHULLER, R. SHANIDZE, I. SOKALSKI, T. SPONA, M. SPURIO, G. VAN DER STEENHOVEN, T. STOLARCZYK, K. STREEB, L. SULAK, M. TAIUTI, C. TAMBURINI, C. TAO, G. TERRENI, L.F. THOMPSON, F. URBANO, P. VALDY, V. VALENTE, B. VALLAGE, G. VAUDAINE, G. VENEKAMP, B. VERLAAT, P. VERNIN, G. DE VRIES-UITERWEERD, R. VAN WIJK, G. WIJNKER, P. DE WITT HUBERTS, G. WOBBE, E. DE WOLF, A-F. YAO, D. ZABOROV, H. ZACCONE, J.D. ZORNOZA, J. ZUNIGA, KVI - Center for Advanced Radiation Technology, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut Français de Recherche pour l'Exploitation de la Mer - Brest (IFREMER), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de la Méditerranée - Aix-Marseille 2, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
- Subjects
Nuclear and High Energy Physics ,Photomultiplier ,Physics::Instrumentation and Detectors ,[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,neutrino telescope ,optical beacon ,time calibration ,Astrophysics ,01 natural sciences ,law.invention ,Telescope ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Optics ,law ,0103 physical sciences ,Calibration ,Angular resolution ,14. Life underwater ,010306 general physics ,Instrumentation ,Cherenkov radiation ,Physics ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,neutrino telescope, time calibration, optical beacon ,010308 nuclear & particles physics ,business.industry ,Detector ,Astrophysics (astro-ph) ,Astrophysics::Instrumentation and Methods for Astrophysics ,SITE ,Astronomy ,Beacon ,LIGHT ,Física nuclear ,Neutrino ,business - Abstract
ANTARES is a neutrino telescope being deployed in the Mediterranean Sea. It consists of a three dimensional array of photomultiplier tubes that can detect the Cherenkov light induced by charged particles produced in the interactions of neutrinos with the surrounding medium. High angular resolution can be achieved, in particular when a muon is produced, provided that the Cherenkov photons are detected with sufficient timing precision. Considerations of the intrinsic time uncertainties stemming from the transit time spread in the photomultiplier tubes and the mechanism of transmission of light in sea water lead to the conclusion that a relative time accuracy of the order of 0.5 ns is desirable. Accordingly, different time calibration systems have been developed for the ANTARES telescope. In this article, a system based on Optical Beacons, a set of external and well-controlled pulsed light sources located throughout the detector, is described. This calibration system takes into account the optical properties of sea water, which is used as the detection volume of the ANTARES telescope. The design, tests, construction and first results of the two types of beacons, LED and laser-based, are presented., 21 pages, 18 figures, submitted to Nucl. Instr. and Meth. Phys. Res. A
- Published
- 2007
- Full Text
- View/download PDF
23. First results of the Instrumentation Line for the deep-sea ANTARES neutrino telescope
- Author
-
Philippe Charvis, R. De Vita, C. Kopper, B. van Rens, A. F. Yao, E. Castorina, S. Cecchini, G. Lim, E. A. De Wolf, E. Barbarito, V. A. Kudryavtsev, C. De Marzo, Corinne Donzaud, J. P. Schuller, C. Racca, F. Ameli, J. Beltramelli, V. Roca, J.-C. Languillat, P. Piattelli, P. Valdy, R. Bruijn, Annarita Margiotta, K. Streeb, S. Cuneo, W. Kretschmer, R. Ostasch, M. de Jong, G. Damy, Teresa Montaruli, M. Jaspers, J. E. Mcmillan, G. V. Russo, J.A. Aguilar, Gregory David Hallewell, F. Druillole, A. Capone, Nathalie Palanque-Delabrouille, M. Mongelli, S. Favard, N. de Botton, Yann Hello, N. Cottini, P. Chauchot, E. Falchini, H. J. Rose, F. Lucarelli, J. F. Drogou, F. Rethore, M. Morganti, D. Lo Presti, S. Kuch, Christian Tamburini, J.J. Destelle, L. Caillat, C. Gojak, Eric Delagnes, V. Cavasinni, A. Rostovtsev, S. Loucatos, R. Masullo, M. Jaquet, M. Melissas, C. Petta, I. Sokalski, H. Laschinsky, Roberto Bellotti, N. Girard, Gisela Anton, T. Stolarczyk, D. Real, Maurizio Spurio, N. Kalantar-Nayestanaki, V. Lyashuk, M. Ruppi, F. Feinstein, Rosario Megna, D. Stubert, M. Ripani, J. Zúñiga, H. Peek, J. Busto, J. J. Aubert, R. van Dantzig, J. Carr, P. Rewiersma, V. Rigaud, C. Olivetto, S. L. Cartwright, M.C. Bouwhuis, J.-P. Pineau, U. F. Katz, A.J. Heijboer, Ivan Dekeyser, P. Coyle, J. van Randwijk, K. Graf, P. Sapienza, H. Zaccone, F. Salesa, V. Flaminio, Alexander Kappes, Ch. Naumann, M. Naumann-Godo, M. Battaglieri, F. Jouvenot, A. Albert, D. Zaborov, A. Ceres, R. Shadnize, M. Billault, B. Vallage, A. S. Cussatlegras, P. Keller, P. Goret, C. Roda, A. Levan Suu, P. Payre, A. Milovanovic, G. de Vries, Anne Deschamps, M. Romita, Y. Leguen, R. Coniglione, G. van der Steenhoven, Alain Mazure, J. Hogenbirk, D. Festy, L. Moscoso, B. Dinkespieler, D. Denans, T. Spona, M. Marcelin, E. Korolkova, C. Hoffman, R. Lahmann, G. Terreni, H. Kok, F. Mazéas, C. Fiorello, S. M. Bradbury, J.R. Hubbard, Patrick Lamare, R. van Wijk, Juan José Hernández-Rey, M. Circella, H. Le Provost, J.M. Gallone, J. Roux, S. Anvar, Charling Tao, F. Louis, S. Basa, D. Lachartre, Yvonne Becherini, G. F. Burgio, J. Poinsignon, Jean-Francois Rolin, V. Bertin, B. Verlaat, Lester D.R. Thompson, Elie Aslanides, A. Kruijer, G. Wobbe, P. K. A. de Witt-Huberts, S. Ferry, A. Calzas, L. Caponetto, S. Galeotti, N. Randazzo, G. Venekamp, M. Musumeci, H. Lafoux, Jean-Pierre Ernenwein, E. Migneco, T. Karg, C. Colnard, P. Vernin, V. Valente, Mohsen Harakeh, B. Hartmann, F. Dessages-Ardellier, P. Lagier, M. Taiuti, P. Kooijman, T. Legou, F. Schmitt, G. Giacomelli, G. Lamanna, J. Hossl, Stephanie Escoffier, Giorgio Riccobene, J.D. Zornoza, Antoine Kouchner, V. Niess, T. Pradier, E. Carmona, Dominique Durand, D. Castel, M. Anghinolfi, C. Distefano, S. Karkar, K. Salomon, R. Blaes, E. Heine, T. Chiarusi, A. Bigi, Lawrence Sulak, Jürgen Brunner, F. Cafagna, Chantal Compère, H. Löhner, L Lo Nigro, V. Popa, Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Géoazur (GEOAZUR 6526), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut Français de Recherche pour l'Exploitation de la Mer - Brest (IFREMER Centre de Bretagne), Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER), Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), IFREMER - Centre de Toulon/La Seyne Sur Mer (IFREMER), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), ANTARES, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut Français de Recherche pour l'Exploitation de la Mer - Brest (IFREMER), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de la Méditerranée - Aix-Marseille 2, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), J.A. AGUILAR, A. ALBERT, F. AMELI, P. AMRAM, M. ANGHINOLFI, G. ANTON, S. ANVAR, F.E. ARDELLIER-DESAGES, E. ASLANIDES, J.J. AUBERT, D. BAILEY, S. BASA, M. BATTAGLIERI, Y. BECHERINI, R. BELLOTTI, J. BELTRAMELLI, V. BERTIN, M. BILLAULT, R. BLAES, F. BLANC, N. DE BOTTON, J. BOULESTEIX, M.C. BOUWHUIS, C.B. BROOKS, S.M. BRADBURY, R. BRUIJN, J. BRUNNER, G.F. BURGIO, F. CAFAGNA, A. CALZAS, A. CAPONE, L. CAPONETTO, E. CARMONA, J. CARR, S.L. CARTWRIGHT, E. CASTORINA, V. CAVASINNI, S. CECCHINI, P. CHARVIS, M. CIRCELLA, C. COLNARD, C. COMPERE, R. CONIGLIONE, S. COOPER, P. COYLE, S. CUNEO, G. DAMY, R. VAN DANTZIG, A. DESCHAMPS, C. DE MARZO, D. DENANS, J.J. DESTELLE, R. DE VITA, B. DINKELSPILER, C. DISTEFANO, J.F. DROGOU, F. DRUILLOLE, J. ENGELEN, J.P. ERNENWEIN, E. FALCHINI, S. FAVARD, F. FEINSTEIN, S. FERRY, D. FESTY, V. FLAMINIO, J. FOPMA, J.L. FUDA, J.M. GALLONE, G. GIACOMELLI, N. GIRARD, P. GORET, K. GRAF, G. HALLEWELL, B. HARTMANN, A. HEIJBOER, Y. HELLO, J.J. HERNANDEZ-REY, G. HERROUIN, J. HÖßL, C. HOFFMANN, J.R. HUBBARD, M. JAQUET, M. DE JONG, F. JOUVENOT, A. KAPPES, T. KARG, S. KARKAR, M. KAROLAK, U. KATZ, P. KELLER, P. KOOIJMAN, E.V. KOROLKOVA, A. KOUCHNER, W. KRETSCHMER, S. KUCH, V.A. KUDRYAVTSEV, H. LAFOUX, P. LAGIER, R. LAHMANN, P. LAMARE, J.C. LANGUILLAT, H. LASCHINSKY, L. LAUBIER, T. LEGOU, Y. LE GUEN, H. LE PROVOST, A. LE VAN SUU, L. LO NIGRO, D. LO PRESTI, S. LOUCATOS, F. LOUIS, V. LYASHUK, M. MARCELIN, A. MARGIOTTA, C. MARON, A. MASSOL, R. MASULLO, F. MAZÉAS, A. MAZURE, J.E. MCMILLAN, E. MIGNECO, C. MILLOT, A. MILOVANOVIC, F. MONTANET, T. MONTARULI, J.-P. MOREL, M. MORGANTI, L. MOSCOSO, M. MUSUMECI, C. NAUMANN, M. NAUMANN-GODO, E. NEZRI, V. NIESS, G.J. NOOREN, P. OGDEN, C. OLIVETTO, N. PALANQUE-DELABROUILLE, R. PAPALEO, P. PAYRE, C. PETTA, P. PIATTELLI, J.P. PINEAU, J. POINSIGNON, V. POPA, R. POTHEAU, T. PRADIER, C. RACCA, G. RAIA, N. RANDAZZO, D. REAL, B.A.P. VAN RENS, F. RÉTHORÉ, G. RICCOBENE, V. RIGAUD, M. RIPANI, V. ROCA-BLAY, J.F. ROLIN, M. ROMITA, H.J. ROSE, A. ROSTOVTSEV, M. RUPPI, G.V. RUSSO, Y. SACQUIN, F. SALESA, K. SALOMON, S. SAOUTER, P. SAPIENZA, R. SHANIDZE, J.-P. SCHULLER, W. SCHUSTER, I. SOKALSKI, M. SPURIO, T. STOLARCZYK, D. STUBERT, M. TAIUTI, L.F. THOMPSON, S. TILAV, P. VALDY, V. VALENTE, B. VALLAGE, P. VERNIN, J. VIRIEUX, G. DE VRIES, P. DE WITT HUBERTS, E. DE WOLF, D. ZABOROV, H. ZACCONE, V. ZAKHAROV, J.D. ZORNOZA, J. ZUÑIGA, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), and KVI - Center for Advanced Radiation Technology
- Subjects
Photomultiplier ,neutrino astronomy ,photon detection ,underwater detector ,Positioning system ,Instrumentation ,Astrophysics::High Energy Astrophysical Phenomena ,Neutrino astronomy, Underwater detector, Photon detection ,FOS: Physical sciences ,Astrophysics ,01 natural sciences ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,0103 physical sciences ,Calibration ,Angular resolution ,010306 general physics ,Remote sensing ,Astroparticle physics ,Physics ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,010308 nuclear & particles physics ,Detector ,Astrophysics (astro-ph) ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,SITE ,Astronomy and Astrophysics ,LIGHT ,PHOTON DETECTION ,NEUTRINO ASTRONOMY ,Física nuclear ,UNDERWATER DETECTOR ,Neutrino astronomy - Abstract
In 2005, the ANTARES Collaboration deployed and operated at a depth of 2500 m a so-called Mini Instrumentation Line equipped with Optical Modules (MILOM) at the ANTARES site. The various data acquired during the continuous operation from April to December 2005 of the MILOM confirm the satisfactory performance of the Optical Modules, their front-end electronics and readout system, as well as the calibration devices of the detector. The in-situ measurement of the Optical Module time response yields a resolution better than 0.5 ns. The performance of the acoustic positioning system, which enables the spatial reconstruction of the ANTARES detector with a precision of about 10 cm, is verified. These results demonstrate that with the full ANTARES neutrino telescope the design angular resolution of better than $0.3^\circ$ can be realistically achieved., Comment: 18 pages, 12 figures, submitted to Astroparticle Physics
- Published
- 2006
- Full Text
- View/download PDF
24. Study of Large Hemispherical Photomultiplier Tubes for the ANTARES Neutrino Telescope
- Author
-
F. Salesa, F. Ameli, I. Sokalski, Jean Virieux, T. Legou, Robert Lahmann, J. Carr, G.V. Russo, Lester D.R. Thompson, Nathalie Palanque-Delabrouille, F. Montanet, C. Hoffmann, A. Calzas, J. Fopma, V. Roca-Blay, E. Falchini, A. Le Van Suu, E. Nezri, L. Caponetto, W. Kretschmer, D. Lo Presti, R. Coniglione, R. De Vita, V. Rigaud, F. Réthoré, C. Racca, S. Saouter, P. Goret, R. Blaes, S. L. Cartwright, J. Poinsignon, L. Moscoso, J-J. Aubert, E. Castorina, M. Jaquet, U. F. Katz, Jean-Luc Fuda, V. Bertin, Elie Aslanides, Giorgio Riccobene, M. Anghinolfi, A. Mazure, C. Olivetto, C.B. Brooks, H. Lafoux, Timo Karg, L. Laubier, D. Denans, Vincenzo Cavasinni, V. A. Kudryavtsev, C. Distefano, Yann Hello, V. Valente, S. Favard, P.M. Kooijman, P. A. Ogden, R. Potheau, R. van Dantzig, G. Giacomelli, V. Lyashuk, J.D. Zornoza, Nunzio Randazzo, M. Battaglieri, S. Loucatos, J.-P. Ernenwein, R. Bruijn, F.E. Ardellier-Desages, E. Migneco, Rezo Shanidze, G. Damy, M. Taiuti, T. Pradier, C. De Marzo, P. Coyle, S. Cuneo, G. de Vries, M. Karolak, Paolo Sapienza, F. Jouvenot, V. Niess, F. Mazéas, S. Kuch, F. Blanc, S. Basa, A. Albert, H. J. Rose, Teresa Montaruli, P.K.A. de Witt Huberts, G. F. Burgio, G. Raia, Y. Sacquin, Jürgen Brunner, A. Rostovtsev, M. Ripani, Jean-Francois Rolin, E. Carmona, M.C. Bouwhuis, J.-C. Languillat, D. S. Bailey, J.-J. Destelle, J. Hößl, F. Louis, P. Lamare, M. Naumann-Godo, S. Tilav, S. Ferry, E. A. De Wolf, Juanan Aguilar, Philippe Charvis, P. Valdy, E. V. Korolkova, Alexander Kappes, B. van Rens, C. Maron, S. Cecchini, H. Le Provost, Juan José Hernández-Rey, P. Keller, F. Feinstein, Y. Le Guen, S. Karkar, Antonio Capone, N. Girard, Maurizio Spurio, A.J. Heijboer, J.J. Engelen, Kay Graf, F. Cafagna, Chantal Compère, M. Ruppi, Roberto Bellotti, V. Flaminio, Antoine Kouchner, M. Morganti, L Lo Nigro, B. Vallage, B. Dinkelspiler, J. Zúñiga, Jean-Pierre Morel, M. Romita, V. Popa, B. Hartmann, D. Festy, J. E. McMillan, S. M. Bradbury, R. Masullo, J. Beltramelli, Riccardo Papaleo, C. Petta, Wolfgang Schuster, H. Laschinsky, P. Amram, J. Boulesteix, J. F. Drogou, Annarita Margiotta, Gisela Anton, T. Stolarczyk, A. Milovanovic, D. Stubert, G.D. Hallewell, J. P. Schuller, P. Payre, K. Salomon, C. Millot, J.-P. Pineau, C. Naumann, P. Piattelli, D. Zaborov, Anne Deschamps, A. Massol, M. Marcelin, M. Billault, V. Zakharov, J.R. Hubbard, Diego Real, J.M. Gallone, Susan Cooper, S. Anvar, Yvonne Becherini, M. de Jong, F. Druillole, N. de Botton, G. Herrouin, H. Zaccone, C. Colnard, Mario Musumeci, Gerardus Nooren, P. Vernin, M. Circella, P. Lagier, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 6526), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), ANTARES, J.A. AGUILAR, A. ALBERT, F. AMELI, P. AMRAM, M. ANGHINOLFI, G. ANTON, S. ANVAR, F.E. ARDELLIER-DESAGES, E. ASLANIDES, J.J. AUBERT, D. BAILEY, S. BASA, M. BATTAGLIERI, Y. BECHERINI, R. BELLOTTI, J. BELTRAMELLI, V. BERTIN, M. BILLAULT, R. BLAES, F. BLANC, N. DE BOTTON, J. BOULESTEIX, M.C. BOUWHUIS, C.B. BROOKS, S.M. BRADBURY, R. BRUIJN, J. BRUNNER, G.F. BURGIO, F. CAFAGNA, A. CALZAS, A. CAPONE, L. CAPONETTO, E. CARMONA, J. CARR, S.L. CARTWRIGHT, E. CASTORINA, V. CAVASINNI, S. CECCHINI, P. CHARVIS, M. CIRCELLA, C. COLNARD, C. COMPERE, R. CONIGLIONE, S. COOPER, P. COYLE, S. CUNEO, G. DAMY, R. VAN DANTZIG, A. DESCHAMPS, C. DE MARZO, D. DENANS, J.J. DESTELLE, R. DE VITA, B. DINKELSPILER, C. DISTEFANO, J.F. DROGOU, F. DRUILLOLE, J. ENGELEN, J.P. ERNENWEIN, E. FALCHINI, S. FAVARD, F. FEINSTEIN, S. FERRY, D. FESTY, V. FLAMINIO, J. FOPMA, J.L. FUDA, J.M. GALLONE, G. GIACOMELLI, N. GIRARD, P. GORET, K. GRAF, G. HALLEWELL, B. HARTMANN, A. HEIJBOER, Y. HELLO, J.J. HERNANDEZ-REY, G. HERROUIN, J. HÖßL, C. HOFFMANN, J.R. HUBBARD, M. JAQUET, M. DE JONG, F. JOUVENOT, A. KAPPES, T. KARG, S. KARKAR, M. KAROLAK, U. KATZ, P. KELLER, P. KOOIJMAN, E.V. KOROLKOVA, A. KOUCHNER, W. KRETSCHMER, S. KUCH, V.A. KUDRYAVTSEV, H. LAFOUX, P. LAGIER, R. LAHMANN, P. LAMARE, J.C. LANGUILLAT, H. LASCHINSKY, L. LAUBIER, T. LEGOU, Y. LE GUEN, H. LE PROVOST, A. LE VAN SUU, L. LO NIGRO, D. LO PRESTI, S. LOUCATOS, F. LOUIS, V. LYASHUK, M. MARCELIN, A. MARGIOTTA, C. MARON, A. MASSOL, R. MASULLO, F. MAZÉAS, A. MAZURE, J.E. MCMILLAN, E. MIGNECO, C. MILLOT, A. MILOVANOVIC, F. MONTANET, T. MONTARULI, J.-P. MOREL, M. MORGANTI, L. MOSCOSO, M. MUSUMECI, C. NAUMANN, M. NAUMANN-GODO, E. NEZRI, V. NIESS, G.J. NOOREN, P. OGDEN, C. OLIVETTO, N. PALANQUE-DELABROUILLE, R. PAPALEO, P. PAYRE, C. PETTA, P. PIATTELLI, J.P. PINEAU, J. POINSIGNON, V. POPA, R. POTHEAU, T. PRADIER, C. RACCA, G. RAIA, N. RANDAZZO, D. REAL, B.A.P. VAN RENS, F. RÉTHORÉ, G. RICCOBENE, V. RIGAUD, M. RIPANI, V. ROCA-BLAY, J.F. ROLIN, M. ROMITA, H.J. ROSE, A. ROSTOVTSEV, M. RUPPI, G.V. RUSSO, Y. SACQUIN, F. SALESA, K. SALOMON, S. SAOUTER, P. SAPIENZA, R. SHANIDZE, J.-P. SCHULLER, W. SCHUSTER, I. SOKALSKI, M. SPURIO, T. STOLARCZYK, D. STUBERT, M. TAIUTI, L.F. THOMPSON, S. TILAV, P. VALDY, V. VALENTE, B. VALLAGE, P. VERNIN, J. VIRIEUX, G. DE VRIES, P. DE WITT HUBERTS, E. DE WOLF, D. ZABOROV, H. ZACCONE, V. ZAKHAROV, J.D. ZORNOZA, J. ZUÑIGA, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)
- Subjects
Nuclear and High Energy Physics ,Photomultiplier ,Physics - Instrumentation and Detectors ,Neutrino detection ,Neutrino telescope ,FOS: Physical sciences ,01 natural sciences ,large area photosensor, hemispherical photomultiplier, neutrino detection ,Nuclear physics ,Optics ,Intensive Phase ,0103 physical sciences ,14. Life underwater ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,010306 general physics ,Instrumentation ,Astroparticle physics ,Physics ,010308 nuclear & particles physics ,business.industry ,Hemispherical photomultiplier ,Instrumentation and Detectors (physics.ins-det) ,Large area photosensor ,Glass spheres ,Neutrino detector ,95.55.Vj ,85.60.Ha ,Física nuclear ,business ,hemispherical photomultiplier ,large area photosensor ,neutrino detection - Abstract
The ANTARES neutrino telescope, to be immersed depth in the Mediterranean Sea, will consist of a 3 dimensional matrix of 900 large area photomultiplier tubes housed in pressure resistant glass spheres. The selection of the optimal photomultiplier was a critical step for the project and required an intensive phase of tests and developments carried out in close collaboration with the main manufacturers worldwide. This paper provides an overview of the tests performed by the collaboration and describes in detail the features of the PMT chosen for ANTARES., Comment: 21 pages, 10 figures. To be published in Nuclear Inst. and Methods in Physics Research, A
- Published
- 2005
- Full Text
- View/download PDF
25. First search for neutrinos in correlation with gamma-ray bursts with the ANTARES neutrino telescope
- Author
-
C. Richardt, C. Carloganu, R. Richter, A. C.S. Assis Jesus, Tri L. Astraatmadja, S. Loucatos, C. Racca, S. Basa, I. Al Samarai, Vladimir Kulikovskiy, M. Hamal, S. Anvar, Z. Charif, Holger Motz, B. Vallage, M. Ferri, A. Capone, Dominique Lefèvre, D. Lo Presti, S. Mangano, M. Neff, A. Trovato, J. P. Gómez-González, Jürgen Brunner, Manuela Vecchi, M. Anghinolfi, J. Busto, G.E. Păvălaş, V. Flaminio, Paolo Sapienza, A. Rostovtsev, Rezo Shanidze, Q. Dorosti, K. Payet, Manuel Bou-Cabo, Francesco Simeone, Paolo Piattelli, Anne Deschamps, F. Salesa, Heide Costantini, F. Schüssler, Thomas Eberl, P. Vernin, G.V. Russo, Juan José Hernández-Rey, B. Bouhou, C. Bogazzi, J. Jeffrey Carr, Kay Graf, P.M. Kooijman, J. Hossl, V. Popa, C. Distefano, D. F. E. Samtleben, M. de Jong, E. A. De Wolf, G. Wijnker, E. Presani, F. M. Schöck, B. Herold, A. Spies, Tommaso Chiarusi, G. De Bonis, Giuseppina Larosa, M. Taiuti, Corinne Donzaud, G. Riccobene, Jutta Schnabel, C. Kopper, S. Adrián-Martínez, J.A. Martínez-Mora, Matthias Kadler, Maurizio Spurio, Antoine Kouchner, Ciro Bigongiari, A.J. Heijboer, S. Galatà, Ivan Dekeyser, Jean-Pierre Ernenwein, V. Bertin, C. C. Hsu, M. Rujoiu, Thierry Pradier, U. F. Katz, Stephanie Escoffier, V. Van Elewyck, J. Ruiz-Rivas, S. Ferry, K. Fehn, A. Sánchez-Losa, M. Ardid, S. Biagi, J.D. Zornoza, C. Curtil, D. Lattuada, Philippe Charvis, U. Emanuele, G. Lim, Alexander Kappes, R. Coniglione, D. Dornic, Yann Hello, M. Morganti, H. Loehner, E. Nezri, M.C. Bouwhuis, A. Albert, L. Moscoso, J. Petrovic, K. Roensch, G. Giacomelli, F. Louis, J. J. Aubert, S. Wagner, E. Visser, C. Vallée, P. Coyle, J. Zúñiga, Oleg Kalekin, Jörn Wilms, S. Cecchini, D. Palioselitis, Doriane Drouhin, O. Kavatsyuk, M. Marcelin, L. Core, D. Zaborov, J. L. Fuda, A. Creusot, V. Giordano, K. Geyer, F. Folger, C. M. Reed, M. Circella, Bruny Baret, M. P. Decowski, I. Kreykenbohm, G. Guillard, Robert Lahmann, Gregory David Hallewell, Guillaume Lambard, H. van Haren, Christian Tamburini, Annarita Margiotta, Michel André, J. P. Schuller, A. Enzenhöfer, H. Yepes, C. Rivière, Teresa Montaruli, Jos Steijger, Gisela Anton, T. Stolarczyk, A. Robert, T. Seitz, U. Fritsch, Paolo Fermani, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Département d'Electronique, des Détecteurs et d'Informatique pour la Physique (ex SEDI) (DEDIP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 6526), Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut méditerranéen d'océanologie (MIO), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPP), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ANTARES, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Département d'Electronique, des Détecteurs et d'Informatique (ex SEDI) (DEDI), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN)-Aix Marseille Université (AMU)-Institut de Recherche pour le Développement (IRD), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), S. Adrián-Martínez, I. Al Samarai, A. Albert, M. André, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, T. Astraatmadja, J-J. Aubert, B. Baret, S. Basa, V. Bertin, S. BIAGI, C. Bigongiari, C. Bogazzi, M. Bou-Cabo, B. Bouhou, M. C. Bouwhui, J. Brunner, J. Busto, A. Capone, C. Cârloganu, J. Carr, S. CECCHINI, Z. Charif, Ph. Charvi, T. CHIARUSI, M. Circella, R. Coniglione, L. Core, H. Costantini, P. Coyle, A. Creusot, C. Curtil, G. De Boni, M. P. Decowski, I. Dekeyser, A. Deschamp, C. Distefano, C. Donzaud, D. Dornic, Q. Dorosti, D. Drouhin, T. Eberl, U. Emanuele, A. Enzenhöfer, J-P. Ernenwein, S. Escoffier, K. Fehn, P. Fermani, M. Ferri, S. Ferry, V. Flaminio, F. Folger, U. Fritsch, J-L. Fuda, S. Galatà, P. Gay, K. Geyer, G. GIACOMELLI, V. Giordano, A. Gleixner, J. P. Gómez-González, K. Graf, G. Guillard, G. Hallewell, M. Hamal, H. van Haren, A. J. Heijboer, Y. Hello, J. J. Hernández-Rey, B. Herold, J. Hößl, C. C. Hsu, M. de Jong, M. Kadler, O. Kalekin, A. Kappe, U. Katz, O. Kavatsyuk, P. Kooijman, C. Kopper, A. Kouchner, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, G. Lambard, G. Larosa, D. Lattuada, E. Leonora, D. Lefèvre, G. Lim, D. Lo Presti, H. Loehner, S. Loucato, F. Loui, S. Mangano, M. Marcelin, A. MARGIOTTA, J. A. Martínez-Mora, A. Meli, T. Montaruli, M. Morganti, H. Motz, M. Neff, E. Nezri, D. Palioseliti, G. E. Pavala, V. POPA, J. Petrovic, P. Piattelli, V. Popa, T. Pradier, E. Presani, C. Racca, C. Reed, G. Riccobene, R. Richter, C. Rivière, A. Robert, K. Roensch, A. Rostovtsev, J. Ruiz-Riva, M. Rujoiu, D. F. E. Samtleben, P. Sapienza, J. Schmid, J. Schnabel, J-P. Schuller, F. Schüssler, T. Seitz, M. SPURIO, F. Simeone, A. Spie, M. Spurio, J. J. M. Steijger, Th. Stolarczyk, A. Sánchez-Losa, M. Taiuti, C. Tamburini, A. Trovato, B. Vallage, C. Vallée, V. Van Elewyck, M. Vecchi, P. Vernin, E. Visser, S. Wagner, G. Wijnker, J. Wilm, E. de Wolf, H. Yepe, D. Zaborov, J. D. Zornoza, and J. Zúñiga, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), KVI - Center for Advanced Radiation Technology, ANTARES (IHEF, IoP, FNWI), Centre National de la Recherche Scientifique (France), and Ministerio de Ciencia e Innovación (España)
- Subjects
Astrofísica ,FLUX ,[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,neutrino experiments ,neutrino astronomy ,gamma ray bursts theory ,POINT SOURCES ,Physics::Instrumentation and Detectors ,Solar neutrino ,Astrophysics::High Energy Astrophysical Phenomena ,REDSHIFT ,Flux ,FOS: Physical sciences ,Astrophysics ,01 natural sciences ,ICECUBE ,0103 physical sciences ,010303 astronomy & astrophysics ,Neutrino experiments ,ATMOSPHERIC MUONS ,Physics ,High Energy Astrophysical Phenomena (astro-ph.HE) ,Muon ,Gamma ray bursts theory ,010308 nuclear & particles physics ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,High Energy Physics::Phenomenology ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,Astronomy and Astrophysics ,gamma ray bursts ,CATALOG ,Redshift ,Neutrino detector ,Neutrino astronomy ,FISICA APLICADA ,neutrino experiment ,High Energy Physics::Experiment ,Neutrino ,Astrophysics - High Energy Astrophysical Phenomena ,Gamma-ray burst ,SYSTEM - Abstract
A search for neutrino-induced muons in correlation with a selection of 40 gamma-ray bursts that occurred in 2007 has been performed with the ANTARES neutrino telescope. During that period, the detector consisted of 5 detection lines. The ANTARES neutrino telescope is sensitive to TeV-PeV neutrinos that are predicted from gamma-ray bursts. No events were found in correlation with the prompt photon emission of the gamma-ray bursts and upper limits have been placed on the flux and fluence of neutrinos for different models., The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat à l’ énergie atomique et aux énergies alter-natives (CEA), Agence National de la Recherche (ANR), Commission Européenne (FEDER fund and Marie Curie Program), Région Alsace (contrat CPER), Région Provence-Alpes-Côte d’Azur, Département du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fúr Bildung und Forschung (BMBF), Germany; Instituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS - UEFI SCDI), Romania; Ministerio de Ciencia e Innovación (MICINN), Brometeo of Generalitat Valenciana and MultiDark, Spain; Agence de l’Oriental, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.
- Published
- 2013
- Full Text
- View/download PDF
26. Colloquium: Multimessenger astronomy with gravitational waves and high-energy neutrinos
- Author
-
Vuk Mandic, A. Dietz, Antoine Kouchner, Shin'ichiro Ando, B. Bouhou, Dafne Guetta, Imre Bartos, L. Moscoso, Francis Halzen, Kei Kotake, David Eichler, Bruny Baret, Veronique Van Elewyck, I. Di Palma, S. Kandhasamy, Eli Waxman, Thierry Pradier, Patrick J. Sutton, E. Chassande-Mottin, S. Márka, Chad Finley, G. E. Romero, E. Thrane, Tsvi Piran, Z. Márka, Maria Alessandra Papa, Alessandra Corsi, Gareth Jones, Corinne Donzaud, and String Theory (ITFA, IoP, FNWI)
- Subjects
Physics ,Photon ,010308 nuclear & particles physics ,Gravitational wave ,media_common.quotation_subject ,Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics::Instrumentation and Methods for Astrophysics ,General Physics and Astronomy ,Astronomy ,Cosmic ray ,Astrophysics ,01 natural sciences ,7. Clean energy ,LIGO ,Universe ,Neutrino detector ,13. Climate action ,0103 physical sciences ,Neutrino ,Gamma-ray burst ,010303 astronomy & astrophysics ,media_common - Abstract
Many of the astrophysical sources and violent phenomena observed in our Universe are potential emitters of gravitational waves and high-energy cosmic radiation, including photons, hadrons, and presumably also neutrinos. Both gravitational waves (GW) and high-energy neutrinos (HEN) are cosmic messengers that may escape much denser media than photons. They travel unaffected over cosmological distances, carrying information from the inner regions of the astrophysical engines from which they are emitted (and from which photons and charged cosmic rays cannot reach us). For the same reasons, such messengers could also reveal new, hidden sources that have not been observed by conventional photon-based astronomy. Coincident observation of GWs and HENs may thus play a critical role in multimessenger astronomy. This is particularly true at the present time owing to the advent of a new generation of dedicated detectors: the neutrino telescopes IceCube at the South Pole and ANTARES in the Mediterranean Sea, as well as the GW interferometers Virgo in Italy and LIGO in the United States. Starting from 2007, several periods of concomitant data taking involving these detectors have been conducted. More joint data sets are expected with the next generation of advanced detectors that are to be operational by 2015, with other detectors, such as KAGRA in Japan, joining in the future. Combining information from these independent detectors can provide original ways of constraining the physical processes driving the sources and also help confirm the astrophysical origin of a GW or HEN signal in case of coincident observation. Given the complexity of the instruments, a successful joint analysis of this combined GW and HEN observational data set will be possible only if the expertise and knowledge of the data is shared between the two communities. This Colloquium aims at providing an overview of both theoretical and experimental state of the art and perspectives for GW and HEN multimessenger astronomy.
- Published
- 2013
27. Determination of the atmospheric neutrino spectra with the Fr�jus detector
- Author
-
P. Bareyre, J. Ernwein, S. Tisserant, K. Daum, Michael Schubnell, B. Kuznik, L. Mosca, O. Perdereau, B. Degrange, Wolfgang Rhode, L. Moscoso, Y. Wei, G. Chardin, R. Barloutaud, and H. J. Meyer
- Subjects
Physics ,Particle physics ,Spectral index ,Muon ,Physics and Astronomy (miscellaneous) ,Physics::Instrumentation and Detectors ,Flux ,Electron ,Spectral line ,Nuclear physics ,High Energy Physics::Experiment ,Neutrino ,Neutrino oscillation ,Engineering (miscellaneous) ,Energy (signal processing) - Abstract
The combined analysis of the final event set of data on neutrino interactions inside the detector, upward going stopping muons and horizontal muons recorded in the Frejus experiment is presented. The absolute atmospheric neutrino spectra in the energy range $$320{\rm M}eV< E_{v_e }< 30GeV$$ for electron neutrinos and $$320{\rm M}eV< E_{v_\mu }< 30GeV$$ for muon neutrinos are determined. Based on the parameterization of Volkova for thev µ a spectral index of γ=2.66±0.05 is obtained from the ratio of horizontal muons over upward going stopping muons and from the measurement of the energy loss of horizontal muons inside the detector. The neutrino spectra are compared with various flux calculations. They do not show any evidence for neutrino oscillations in agreement with earlier analyses of the Frejus data.
- Published
- 1995
- Full Text
- View/download PDF
28. Microlensing evidence from eros
- Author
-
L. Moscoso
- Subjects
Physics ,Nuclear and High Energy Physics ,Solar mass ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Gravitational microlensing ,Atomic and Molecular Physics, and Optics ,law.invention ,Telescope ,Stars ,law ,Data analysis ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,Halo ,Large Magellanic Cloud ,Low Mass ,Astrophysics::Galaxy Astrophysics - Abstract
Two possible gravitational microlensing events have been detected on stars of the Large Magellanic Cloud by the EROS experiment. The time scales of the observed events imply that masses of the lensing objects lie between few hundredths and one solar mass. No candidate has been found in the analysis of data taken in 91–93 by the EROS programme using a CCD camera installed on a 40cm telescope devoted to the search of low mass compact halo objects.
- Published
- 1995
- Full Text
- View/download PDF
29. The ANTARES telescope neutrino alert system
- Author
-
V. Bertin, G. Halladjian, P. Payre, F. M. Schoeck, G. Lim, Francisco Camarena, Kay Graf, D. Zaborov, Jos Steijger, C. Bogazzi, Z. Charif, J.-P. Ernenwein, Maurizio Spurio, Thomas Eberl, C. Distefano, Jürgen Brunner, A.J. Heijboer, Annarita Margiotta, D. Lo Presti, K. Payet, Simona Toscano, C. Racca, G.E. Păvălaş, N. Picot-Clemente, A. Enzenhoefer, E. A. De Wolf, Juanan Aguilar, G. Wijnker, Michel André, G.V. Russo, A. Spies, Manuel Bou-Cabo, Francesco Simeone, D. Dornic, Holger Motz, I. Kreykenbohm, V. Van Elewyck, M. Taiuti, M. Circella, Patrick Lamare, A. C.S. Assis Jesus, Ciro Bigongiari, A. Rostovtsev, Tri L. Astraatmadja, U. F. Katz, S. Galatà, J. Hartman, P.M. Kooijman, A. Bigi, Giuseppina Larosa, A. Sánchez-Losa, C. Carloganu, F. Salesa, Rezo Shanidze, Oleg Kalekin, Antoine Kouchner, Thierry Pradier, Vladimir Kulikovskiy, M. Ardid, Matthias Kadler, M. P. Decowski, Piera Sapienza, Athina Meli, S. Anvar, U. Fritsch, Paolo Fermani, A. Capone, Th. Stolarczyk, A. Albert, C. C. Hsu, Teresa Montaruli, V. Giordano, G. Vannoni, K. Roensch, Y. Hello, Manuela Vecchi, H. van Haren, F. Folger, Anne Deschamps, C. Donzaud, I. Al Samarai, Christian Tamburini, Alexander Kappes, R. Coniglione, F. Schuessler, J. Carr, Dominique Lefèvre, Paolo Piattelli, B. Baret, S. Loucatos, J. Petrovic, G. Giacomelli, B. Vallage, M. Ferri, H. Yepes, D. Palioselitis, Doriane Drouhin, O. Kavatsyuk, C. Rivière, V. Flaminio, H. Loehner, Jp Schuller, I. Dekeyser, Jose Busto, Robert Lahmann, S. Basa, J. Zúñiga, E. Presani, B. Herold, S. Biagi, Tommaso Chiarusi, C. Kopper, Gregory David Hallewell, B. Bouhou, M. Marcelin, Gisela Anton, A. Robert, V. Popa, J.-L. Fuda, P. Coyle, M. Rujoiu, Stephanie Escoffier, C. Curtil, D. Lattuada, J-J. Aubert, C. Reed, J.D. Zornoza, J. Hoessl, G. Guillard, C. Richardt, R. Richter, S. Mangano, M. Neff, Heide Costantini, M. Ageron, J.A. Martínez-Mora, J. Ruiz-Rivas, U. Emanuele, E. Nezri, M.C. Bouwhuis, Juan José Hernández-Rey, Ph. Charvis, M. de Jong, G. Carminati, Jörn Wilms, S. Cecchini, J. P. Gómez-González, M. Anghinolfi, Q. Dorosti, P. Vernin, L. Moscoso, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 6526), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ANTARES, KVI - Center for Advanced Radiation Technology, Ageron, M., Aguilar, J.A., Samarai, I. AL, Albert, A., André, M., Anghinolfi, M., Anton, G., Anvar, S., Ardid, M., ASSIS JESUS, A.C., Astraatmadja, T., Aubert, J.-J., Baret, B., Basa, S., Bertin, V., Biagi, S., Bigi, A., Bigongiari, C., Bogazzi, C., BOU-CABO, M., Bouhou, B., Bouwhuis, M.C., Brunner, J., Busto, J., Camarena, F., Capone, A., Cârloganu, C., Carminati, G., Carr, J., Cecchini, S., Charif, Z., Charvis, Ph., Chiarusi, T., Circella, M., Coniglione, R., Costantini, H., Coyle, P., Curtil, C., Decowski, M.P., Dekeyser, I., Deschamps, A., Distefano, C., Donzaud, C., Dornic, D., Dorosti, Q., Drouhin, D., Eberl, T., Emanuele, U., Enzenhöfer, A., Ernenwein, J-P., Escoffier, S., Fermani, P., Ferri, M., Flaminio, V., Folger, F., Fritsch, U., Fuda, J-L., Galatà, S., Gay, P., Giacomelli, G., Giordano, V., GÓMEZ-GONZÁLEZ, J.P., Graf, K., Guillard, G., Halladjian, G., Hallewell, G., Haren, H. VAN, Hartman, J., Heijboer, A.J., Hello, Y., HERNÁNDEZ-REY, J.J., Herold, B., Hößl, J., Hsu, C.C., Jong, M. DE, KADLER A, M., Kalekin, O., Kappes, A., Katz, U., Kavatsyuk, O., Kooijman, P., Kopper, C., Kouchner, A., KREYKENBOHM A, I., KULIKOVSKIY A, V., Lahmann, R., Lamare, P., Larosa, G., Lattuada, D., Lefèvre, D., Lim, G., Presti, D. LO, Loehner, H., LOUCATOS A, S., Mangano, S., Marcelin, M., Margiotta, A., MARTÍNEZ-MORA, J.A., Meli, A., Montaruli, T., Moscoso, L., Motz, H., Neff, M., Nezri, E., Palioselitis, D., Pa˘va˘las, G.E., Payet, K., Payre, P., Petrovic, J., Piattelli, P., PICOT-CLEMENTE, N., Popa, V., Pradier, T., Presani, E., Racca, C., Reed, C., Richardt, C., Richter, R., Rivière, C., Robert, A., Roensch, K., Rostovtsev, A., RUIZ-RIVAS, J., RUJOIU A, M., Russo, G.V., Salesa, F., Sapienza, P., Schöck, F., Schuller, J-P., Schüssler, F., Shanidze, R., Simeone, F., Spies, A., Spurio, M., Steijger, J.J.M., Stolarczyk, Th., SÁNCHEZ-LOSA, A., Taiuti, M., Tamburini, C., Toscano, S., VALLAGE A, B., Elewyck, V. VAN, Vannoni, G., Vecchi, M., Vernin, P., Wijnker, G., Wilms, J., Wolf, E. DE, Yepes, H., Zaborov, D., Zornoza, J.D., Zúñiga, J., ANTARES (IHEF, IoP, FNWI), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de la Méditerranée - Aix-Marseille 2, Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), APC - Astrophysique des Hautes Energies (APC - AHE), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), and Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Optical telescopes ,Physics::Instrumentation and Detectors ,Astrophysics ,7. Clean energy ,01 natural sciences ,Gamma ray bursts ,FOLLOW-UP OBSERVATIONS ,law.invention ,law ,Flaring active ,Very high energies ,High Energy Astrophysical Phenomena (astro-ph.HE) ,Physics ,GAMMA-RAY BURSTS ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Astrophysics::Instrumentation and Methods for Astrophysics ,Supernova ,Neutrino detector ,Neutrino astronomy ,Física nuclear ,Neutrino ,Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena ,FLUX ,[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Optical telescope ,Telescope ,Muon tracks ,Coincident ,SEARCH ,Detection methods ,0103 physical sciences ,Core collapse supernovae ,010306 general physics ,Optical follow-up ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,Neutrons ,antares ,neutrino astronomy ,optical follow-up ,transient sources ,ANTARES ,010308 nuclear & particles physics ,Gamma rays ,Astronomy ,Astronomy and Astrophysics ,Alert systems ,Stars ,Transient sources ,[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,Optical signals ,Potential sources ,13. Climate action ,FISICA APLICADA ,High Energy Physics::Experiment ,Gamma-ray burst - Abstract
The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are generated for special events, such as two or more neutrinos, coincident in time and direction, or single neutrinos of very high energy., Comment: 17 pages, 9 figures submitted to Astroparticle Physics
- Published
- 2012
- Full Text
- View/download PDF
30. A method for detection of muon induced electromagnetic showers with the ANTARES detector
- Author
-
J. Ruiz-Rivas, U. Emanuele, M.C. Bouwhuis, Gregory David Hallewell, J.A. Martínez-Mora, S. Biagl, C. Donzaud, S. Loucatos, V. Flaminio, B. Bouhou, A. Bigi, I. Dekeyser, F. M. Schoeck, V. Popa, Antoine Kouchner, M. Rujoiu, Stephanie Escoffier, I. Kreykenbohm, J.D. Zornoza, C. Curtil, D. Lattuada, C. Reed, Teresa Montaruli, Z. Charif, A. Rostovtsev, G. Carminati, J. Hoessl, G. Vannoni, Simona Toscano, M. Circella, J.-P. Ernenwein, M. Ferri, Guido Russo, A. Enzenhoefer, G. Lim, Thomas Eberl, E. A. De Wolf, Oleg Kalekin, F. Schuessler, M. de Jong, G. Wijnker, J. Petrovic, B. Baret, C. Bogazzi, P.M. Kooijman, Giuseppina Larosa, E. Nezri, Matthias Kadler, G. Giacomelli, H. Yepes, Antonio Capone, Michel André, K. Roensch, Philippe Charvis, F. Folger, C. C. Hsu, Maurizio Spurio, Juan A. Aguilar, A. Spies, A.J. Heijboer, V. Van Elewyck, G. Halladjian, V. Giordano, P. Coyle, J. P. Schuller, J. P. Gómez-González, Juan José Hernández-Rey, D. Palioselitis, M. Anghinolfi, Doriane Drouhin, J. Busto, J. Carr, Ciro Bigongiari, G. Guillard, O. Kavatsyuk, M. Marcelin, U. F. Katz, Q. Dorosti, P. Vernin, Vladimir Kulikovskiy, Jürgen Brunner, P. Payre, Paolo Piattelli, Athina Meli, A. Sánchez-Losa, C. Distefano, Anne Robert, F. Salesa, M. Taiuti, L. Moscoso, S. Galata, H. Loehner, C. Carloganu, Manuela Vecchi, Francisco Camarena, M. Ardid, C. Racca, S. Basa, K. Payet, C. Koppe, Thierry Pradier, Kay Graf, J. Zúñiga, H. Costantini, I. Al Samarai, D. Lo Presti, Piera Sapienza, G.E. Păvălaş, A. Albert, Manuel Bou-Cabo, Francesco Simeone, N. Picot-Clemente, Annarita Margiotta, Jörn Wilms, S. Cecchini, Y. Hello, Alexander Kappes, H. van Haren, Christian Tamburini, Patrick Lamare, A. C.S. Assis Jesus, Tri L. Astraatmadja, C. Riviere, J. Hartman, S. Anvar, D. Zaborov, Rezo Shanidze, Dominique Lefèvre, Anne Deschamps, B. Vallage, J. J. Auberth, Holger Motz, C. Richardt, R. Richter, S. Mangano, M. Neff, Gisela Anton, T. Stolarczyk, M. P. Decowski, R. Coniglione, Paolo Fermani, V. Bertin, Robert Lahmann, J.-L. Fuda, E. Presani, B. Herold, Tommaso Chiarusi, U. Fritsch, Jos Steijger, D. Dornic, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ANTARES, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de la Méditerranée - Aix-Marseille 2, Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), APC - Astrophysique des Hautes Energies (APC - AHE), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Research unit Nuclear & Hadron Physics, KVI - Center for Advanced Radiation Technology, ANTARES (IHEF, IoP, FNWI), J.A. Aguilar, I.AlSamarai, A.Albert, M.Andre´, M.Anghinolfi, G.Anton, S.Anvar, M.Ardid, A.C. Assis Jesus, T.Astraatmadja, J.J.Aubert, B.Baret, S.Basa, V.Bertin, S.Biagi, A.Bigi, C. Bigongiari, C.Bogazzi, M.Bou-Cabo, B.Bouhou, M.C.Bouwhuis, J.Brunner, J.Busto, F. Camarena, A.Capone, C.Cˆarloganu, G.Carminati, J.Carr, S.Cecchini, Z.Charif, P. Charvis, T.Chiarusi, M.Circella, R.Coniglione, H.Costantini, P.Coyle, C.Curtil, M.P. Decowski, I.Dekeyser, A.Deschamps, C.Distefano, C.Donzaud, D.Dornic, Q.Dorosti, D. Drouhin, T.Eberl, U.Emanuele, A.Enzenh¨ofer, J.P.Ernenwein, S.Escoffier, P.Fermani, M. Ferri, V.Flaminio, F.Folger, U.Fritsch, J.L.Fuda, S.Galata, P.Gay, G.Giacomelli, V. Giordano, J.P.Gomez-Gonza lez, K.Graf, G.Guillard, G.Halladjian, G.Hallewell, H.vanHaren, J. Hartman, A.J.Heijboer, Y.Hello, J.J.Hernandez-Rey, B.Herold, J.H¨oßl, C.C.Hsu, M.de Jong, M. Kadler, O.Kalekin, A.Kappes, U.Katz, O.Kavatsyuk, P.Kooijman, C.Kopper, A.Kouchner, I. Kreykenbohm, V.Kulikovskiy, R.Lahmann, P.Lamare, G.Larosa, D.Lattuada, D.Lefevre, G. Lim, D.LoPresti, H.Loehner, S.Loucatos, S.Mangano, M.Marcelin, A.Margiotta, J.A. Martinez-Mora, A.Meli, T.Montaruli, L.Moscoso, H.Motz, M.Neff, E.Nezri, D. Palioselitis, G.E.P˘av˘alas, K.Payet, P.Payre, J.Petrovic, P.Piattelli, N.Picot-Clemente, V. Popa, T.Pradier, E.Presani, C.Racca, C.Reed, C.Richardt, R.Richter, C.Rivi_ere, A.Robert, K. Roensch, A.Rostovtsev, J.Ruiz-Rivas, M.Rujoiu, G.V.Russo, F.Salesa, P.Sapienza, F. Sch¨ock, J.P.Schuller, F.Sch ¨ ussler, R.Shanidze, F.Simeone, A.Spies, M.Spurio, J.J.M. Steijger, T.Stolarczyk, A.Sa´nchez-Losa, M.Taiuti, C.Tamburini, S.Toscano, B.Vallage, V. VanElewyck, G.Vannoni, M.Vecchi, P.Vernin, G.Wijnker, J.Wilms, E.deWolf, H. Yepes, D.Zaborov, J.D.Zornoza, and J.Zuniga
- Subjects
Physics::Instrumentation and Detectors ,Atmospheric muons ,Decay products ,Neutrino telescope ,Electromagnetic shower identification ,01 natural sciences ,7. Clean energy ,neutrino telescope electromagnetic shower identification high energy muons energy reconstruction ,high energy muons ,neutrino telescope ,electromagnetic shower identification ,energy reconstruction ,Muon neutrino ,NEUTRINO TELESCOPE ,010303 astronomy & astrophysics ,Instrumentation ,Energy reconstruction ,Physics ,High Energy Astrophysical Phenomena (astro-ph.HE) ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Detector ,Astrophysics::Instrumentation and Methods for Astrophysics ,Detectors ,High energy muon ,Neutrino detector ,Muon collider ,Neutrino astronomy ,Física nuclear ,Neutrino ,High energy muons ,Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena ,FLUX ,Nuclear and High Energy Physics ,Particle physics ,[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Charged current ,[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Cosmic ray ,Nuclear physics ,Electromagnetism ,0103 physical sciences ,High energy physics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,Muon ,ANTARES ,010308 nuclear & particles physics ,Charged particles ,[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,FISICA APLICADA ,TEV ,Physics::Accelerator Physics ,High Energy Physics::Experiment ,Neutrino telescopes ,Electro-magnetic showers - Abstract
The primary aim of ANTARES is neutrino astronomy with upward going muons created in charged current muon neutrino interactions in the detector and its surroundings. Downward going muons are background for neutrino searches. These muons are the decay products of cosmic-ray collisions in the Earths atmosphere far above the detector. This paper presents a method to identify and count electromagnetic showers induced along atmospheric muon tracks with the ANTARES detector. The method is applied to both cosmic muon data and simulations and its applicability to the reconstruction of muon event energies is demonstrated. © 2012 Elsevier B.V. All rights reserved., The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'enegie atomique et aux energies alternatives (CEA), Agence National de la Recherche (ANR), Commission Europeenne (FEDER fund and Marie Curie Program), Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Ciencia e Innovacion (MICINN), Prometeo of Generalitat Valenciana and MultiDark, Spain. We also acknowledge the technical support of Ifremer. AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.
- Published
- 2012
- Full Text
- View/download PDF
31. A 20 cm2 CCD mosaic camera for a dark matter search part I : Mechanics, optics and cryogeny
- Author
-
Christophe Magneville, G. Dispau, M. Gros, L. Prevot, Roger Ferlet, B. Laurent, P. Bareyre, D. Kohler, M. Moniez, L. Moscoso, A. Richaud, Michel Spiro, F. Queinnec, A. Milsztajn, J. C. Delclite, G. Adrianzyk, M. Arnaud, Y. Piret, Y. Laigneau, S. Zylberajch, B. Mazeau, R. Ansari, Jean-Philippe Berger, R. Magnan, P. Grison, Cecile Gry, K. Djidi, L. Vigroux, J. de Trogoff, Éric Aubourg, J. de Kat, A. Baranne, Ph. Lavocat, J. Rich, O. Moreau, J. Petibon, J. Guibert, E. Maurice, Alfred Vidal-Madjar, R. Burnage, Jean-Philippe Beaulieu, F. Cavalier, J. Pasquaud, E. Lesquoy, P. Perrin, S. ehin, F. Tajahmady, R. Caridroit, M. Lachieze-Rey, and B. Paul
- Subjects
Physics ,Reflector (photography) ,Pixel ,business.industry ,Reflecting telescope ,Dark matter ,Astronomy ,Astronomy and Astrophysics ,Gravitational microlensing ,Galactic halo ,Optics ,Cardinal point ,Space and Planetary Science ,Observatory ,business - Abstract
A 20cm 2 CCD mosaic camera has been especially built to search for dark galactic halo objects by the gravitational microlensing effect. The sensitive area is made of 16 edge-buttable CCDs developped by Thomson-CTS, with 23×23 µm 2 pixels. The 35 kg camera housing and mechanical equipment is presented. The associated electronics and data acquisition system are described in a separate paper. The camera resides at the focal plane of a 40 cm, f/10, Ferson reflector. The instrument has been in operation since December 1991 at the La Silla Observatory (ESO).
- Published
- 1994
- Full Text
- View/download PDF
32. A 20cm 2 CCD mosaic camera for a dark matter search part II : Electronics, data acquisition and performance
- Author
-
Christophe Magneville, R. Magnan, J. Guibert, L. Moscoso, E. Maurice, Alfred Vidal-Madjar, F. Tajahmady, Ph. Lavocat, G. Adrianzyk, A. Milsztajn, E. Lesquoy, P. Bareyre, Jean-Philippe Berger, M. Moniez, J. Pasquaud, Michel Spiro, B. Mazeau, O. Moreau, P. Perrin, S. ehin, G. Dispau, J. de Kat, B. Laurent, K. Djidi, R. Caridroit, M. Lachieze-Rey, Éric Aubourg, B. Paul, Roger Ferlet, J. Rich, A. Baranne, Y. Laigneau, R. Burnage, L. Prevot, M. Gros, L. Vigroux, F. Cavalier, M. Arnaud, S. Zylberajch, J. C. Delclite, A. Richaud, P. Grison, R. Ansari, Cecile Gry, J. de Trogoff, D. Kohler, Y. Piret, J. Petibon, F. Queinnec, and Jean-Philippe Beaulieu
- Subjects
Physics ,business.industry ,Dark matter ,Astronomy and Astrophysics ,Mosaic (geodemography) ,Control equipment ,Electronic equipment ,Optics ,Data acquisition ,Space and Planetary Science ,Observatory ,Computer graphics (images) ,Electronics ,Overall performance ,business - Abstract
To summarize, the readout and the control system of the CCD mosaic camera are running since December 1991 at the La Silla Observatory (ESO). The overall performance of the camera has been good. About 12000 pictures (data and flat-fields) have been successfully registered up to now. We will report in the near future preliminary scientific results of the EROS experiment.
- Published
- 1994
- Full Text
- View/download PDF
33. Bounding the time delay between high-energy neutrinos and gravitational-wave transients from gamma-ray bursts
- Author
-
Bartos, I., Baret, B., Sutton, P., Rollins, J., Raffai, P., Pradier, T., Papa, M.A., Chassande-Mottin, E., Moscoso, L., Márka, Z., Márka, S., Kouchner, A., Jones, G., Finley, C., Elewyck, V.V., Donzaud, C., Palma, I.D., Corsi, A., Bouhou, B., B, Baret, I, Bartos, B, Bouhoua, A, Corsi, I, Di Palma, C, Donzauda, V, Van Elewyck, C, Finley, G, Jones, A, Kouchnera, S, Márka, Z, Márka, L, Moscoso, E, Chassande-Mottin, M A, Papa, T, Pradier, P, Raffai, J, Rollins, P, Sutton, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), APC - Astrophysique des Hautes Energies (APC - AHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI)
- Subjects
[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Cosmic ray ,Astrophysics ,General Relativity and Quantum Cosmology (gr-qc) ,01 natural sciences ,7. Clean energy ,Upper and lower bounds ,General Relativity and Quantum Cosmology ,0103 physical sciences ,Emission spectrum ,010303 astronomy & astrophysics ,Physics ,High Energy Astrophysical Phenomena (astro-ph.HE) ,010308 nuclear & particles physics ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Astronomy and Astrophysics ,Light curve ,Massless particle ,13. Climate action ,[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] ,Neutrino ,Astrophysics - High Energy Astrophysical Phenomena ,Gamma-ray burst ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Fermi Gamma-ray Space Telescope - Abstract
We derive a conservative coincidence time window for joint searches of gravitational-wave (GW) transients and high-energy neutrinos (HENs, with energies ≳100 GeV), emitted by gamma-ray bursts (GRBs). The last are among the most interesting astrophysical sources for coincident detections with current and near-future detectors. We take into account a broad range of emission mechanisms. We take the upper limit of GRB durations as the 95% quantile of the T90’s of GRBs observed by BATSE, obtaining a GRB duration upper limit of ∼150 s. Using published results on high-energy (>100 MeV) photon light curves for 8 GRBs detected by Fermi LAT, we verify that most high-energy photons are expected to be observed within the first ∼150 s of the GRB. Taking into account the breakout-time of the relativistic jet produced by the central engine, we allow GW and HEN emission to begin up to 100 s before the onset of observable gamma photon production. Using published precursor time differences, we calculate a time upper bound for precursor activity, obtaining that 95% of precursors occur within ∼250 s prior to the onset of the GRB. Taking the above different processes into account, we arrive at a time window of tHEN − tGW ∈ [−500 s, +500 s]. Considering the above processes, an upper bound can also be determined for the expected time window of GW and/or HEN signals coincident with a detected GRB, tGW − tGRB ≈ tHEN − tGRB ∈ [−350 s, +150 s]. These upper bounds can be used to limit the coincidence time window in multimessenger searches, as well as aiding the interpretation of the times of arrival of measured signals.
- Published
- 2011
- Full Text
- View/download PDF
34. Searches for massive dark matter objects
- Author
-
L. Moscoso
- Subjects
Physics ,Nuclear and High Energy Physics ,Hot dark matter ,Dark matter ,Scalar field dark matter ,Astronomy ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Gravitational microlensing ,Galactic tide ,Atomic and Molecular Physics, and Optics ,Galactic halo ,Dark matter halo ,Baryonic dark matter ,Physics::Space Physics ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Galaxy Astrophysics - Abstract
A status report of the French experiment to search for dark objects in the galactic halo via gravitational micro-lensing of stars in the Large Magellanic Cloud is presented. The search uses combination of Schmidt photographic plates and CCD images and is sensitive to lensing by objects in the range of 10−7 to 10−1 solar masses.
- Published
- 1993
- Full Text
- View/download PDF
35. Lifetime limits on (B-L)-violating nucleon decay and di-nucleon decay modes from the Fréjus experiment
- Author
-
O. Perdereau, C. Paulot, J. Löffler, C. Boudarios, Peter Schleper, B. Kuznik, H. Mönch, L. Mosca, B. Dudelzack, D. Lalanne, H. J. Meyer, U. Nguyen-Khac, K. Daum, R. Barloutaud, C. Arpesella, G. Szklarz, Ch. Berger, P. Eschstruth, J. Ernwein, J. F. Glicenstein, James T. Becker, Richard Nisius, L. Moscoso, L. Behr, M. Fröhlich, G. Chardin, B. Jacobi, Frank Raupach, P. Bareyre, D. Blum, Wolfgang Rhode, A. Borg, S. Tisserant, Y. Wei, Michael Schubnell, Y. Benadjal, F. Laplanche, K.-H. Becker, Ph. Roy, B. Degrange, S. Jullian, C. Longemare, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), and FREJUS
- Subjects
Semileptonic decay ,Physics ,Nuclear and High Energy Physics ,Particle physics ,010308 nuclear & particles physics ,Branching fraction ,Nuclear Theory ,7. Clean energy ,01 natural sciences ,Delta baryon ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Nuclear physics ,Particle decay ,Pion ,0103 physical sciences ,High Energy Physics::Experiment ,Neutron ,Nuclear Experiment ,010306 general physics ,Nucleon ,Radioactive decay - Abstract
The fully contained events recorded in the Frejus detector are used to search for (B-L)-violating nucleon decay and di-nucleon decay processes. No signal is found for a sensitivity of 2.0 kiloton year. The lower limits on the partial lifetime for the various nucleon decay modes range from 5.4×1030 yr for p→μ−π+K+ to 1.0×1032 yr for pn→e+n. We also quote limits on neutron and di-neutron decay into three and two neutrinos respectively.
- Published
- 1991
- Full Text
- View/download PDF
36. Results from the Fr�jus experiment on nucleon decay modes with charged leptons
- Author
-
H. J. Daum, L. Moscoso, D. Blum, S. Tisserant, G. Chardin, J. Löffler, B. Jacobi, J. F. Glicenstein, Claire Bourdarios, Michael Schubnell, Ph. Roy, Peter Schleper, James T. Becker, Y. Benadjal, R. Möller, A. Borg, F. Laplanche, B. Kuznik, P. Wintgen, Frank Raupach, Ch. Berger, S. Jullian, L. Behr, P. Bareyre, D. Lalanne, H. Mönch, K.-H. Becker, C. Longuemare, H. J. Meyer, B. Degrange, C. Paulot, U. Nguyen-Khac, O. Perdereau, G. Szklarz, J. Ernwein, C. Arpesella, M. Fröhlich, R. Nisius, R. Barloutaud, P. Eschstruth, Y. Wei, L. Mosca, and B. Dudelzak
- Subjects
Massless particle ,Baryon ,Nuclear physics ,Physics ,Particle physics ,Particle decay ,Muon ,Physics and Astronomy (miscellaneous) ,Branching fraction ,Neutrino ,Nucleon ,Engineering (miscellaneous) ,Lepton - Abstract
Lower limits on the nucleon lifetime in channels containing at least one positron or muon are given. The analysis is based on 4 years of data taking with the Frejus detector. Various approaches to determine the background from atmospheric neutrinos are discussed and two different nuclear models are used in event simulations. The limits obtained range from 1031 years forp→e + K *0 to 1.5·1032 years forp→e + K *0 to 1.5·1032 years forp→µ + γ.
- Published
- 1991
- Full Text
- View/download PDF
37. Experimental determination of υ background expected in the Fréjus nucleon decay detector
- Author
-
G. Chardin, B. Jacobi, J. F. Glicenstein, Claire Bourdarios, S. Tisserant, R. Nisius, Ph. Roy, R. Barloutaud, P. Eschstruth, K.-H. Becker, James T. Becker, A. Borg, Y. Wei, G. Szklarz, Ch. Berger, P. Bareyre, B. Degrange, H. J. Daum, L. Moscoso, J. Ernwein, H. Mönch, C. Longuemare, L. Behr, M. Fröhlich, S. Jullian, Michael Schubnell, B. Dudelzak, B. Kuznik, Y. Benadjal, F. Laplanche, H. J. Meyer, D. Lalanne, U. Nguyen-Khac, O. Perdereau, D. Blum, C. Paulot, Peter Schleper, C. Arpesella, L. Mosca, W. Kolton, and Frank Raupach
- Subjects
Semileptonic decay ,Physics ,Nuclear and High Energy Physics ,Particle physics ,Large Hadron Collider ,Physics::Instrumentation and Detectors ,Elementary particle ,Nuclear physics ,Particle decay ,High Energy Physics::Experiment ,Neutrino ,Nuclear Experiment ,Nucleon ,Instrumentation ,Lepton ,Background radiation - Abstract
We present an experimental estimate of the background due to atmospheric neutrino interactions in the Frejus underground nucleon decay experiment. The data of a CERN neutrino experiment of the Aachen-Padova collaboration are re-analyzed for this purpose. The large statistics available, some 60 kt yr of equivalent sensitivity, allows for a detailed topological study of most nucleon decay channels with a charged lepton.
- Published
- 1991
- Full Text
- View/download PDF
38. A study of atmospheric neutrino oscillations in the Fréjus experiment
- Author
-
Michael Schubnell, D. Lalanne, S. Jullian, James T. Becker, F. Laplanche, B. Dudelzak, Y. Wei, G. Szklarz, M. Fröhlich, H. J. Meyer, Ch. Berger, U. Nguyen-Khac, S. Tisserant, Richard Nisius, B. Degrange, C. Longuemare, O. Perdereau, H. Mönch, A. Borg, L. Behr, C. Paulot, R. Möller, J. Ernwein, H. J. Daum, L. Moscoso, K.-H. Becker, G. Chardin, B. Jacobi, Claire Bourdarios, Ph. Roy, D. Blum, J. F. Glicenstein, Frank Raupach, C. Arpesella, B. Kuznik, P. Bareye, R. Barloutaud, P. Eschstruth, and L. Mosca
- Subjects
Nuclear physics ,Physics ,Nuclear and High Energy Physics ,Particle physics ,Muon ,Measurements of neutrino speed ,High Energy Physics::Experiment ,Elementary particle ,Electron ,Neutrino ,Neutrino oscillation ,Charged current ,Lepton - Abstract
Atmospheric neutrino interactions have been studied with the Frejus proton decay detector using a total fiducial sensitivity of 1.56 kT yr. The atmospheric neutrino interaction sample has been compared to a Monte Carlo simulation which includes neutrino oscillations. The v e ( v e ) ∌v μ , ( v μ ), v e ( v e ) ∌v τ v μ ( v μ ) ∌v τ ( v τ) oscillations channels have been studied using the ratio of electron to muon charged current events. Three independent analyses have been performed and no evidence for neutrino oscillations has been found. The resulting limits on Δm2 for maximal mixing are more restrictive by more than one order of magnitude with respect to earlier measurements.
- Published
- 1990
- Full Text
- View/download PDF
39. A search for high energy neutrinos from SN 1987A, the Carb, Hercules X-1, and Cygnus X-3 with the Fr�jus detector
- Author
-
C. Arpesella, Ph. Roy, H. Mönch, C. Longuemare, P. Bareyre, R. Barloutaud, P. Eschstruth, C. Paulot, S. Tisserant, M. Fröhlich, G. Chardin, B. Jacobi, B. Kuznik, J. F. Glicenstein, R. Nisius, Claire Bourdarios, D. Blum, Ch. Berger, H. J. Meyer, H. J. Daum, K.-H. Becker, James T. Becker, L. Moscoso, L. Mosca, Michael Schubnell, B. Degrange, J. Ernwein, U. Nguyen-Khac, Y. Minet, A. Borg, O. Perdereau, Y. Wei, G. Szklarz, S. Jullian, B. Dudelzak, R. Möller, Y. Benadjal, F. Laplanche, L. Behr, D. Lalanne, and Frank Raupach
- Subjects
Physics ,Spectral index ,Antiparticle ,Physics and Astronomy (miscellaneous) ,High Energy Physics::Phenomenology ,Astrophysics ,Massless particle ,Supernova ,Antimatter ,High Energy Physics::Experiment ,Neutrino ,Engineering (miscellaneous) ,Lepton ,Bar (unit) - Abstract
With the Frejus detector we studied four astrophysical point-like sources by using\(v_e (\bar v_e )\) and\(v_\mu (\bar v_\mu )\) interactions in the detector and\(v_\mu (\bar v_\mu )\) interactions in the surrounding rock. No excess of events was found. Therefore upper limits of neutrino fluxes and source luminositics are quoted. These limits confirm results from other experiments. In addition new limits are presented for spectral indices above 3.
- Published
- 1990
- Full Text
- View/download PDF
40. Search for neutron-antineutron oscillations in the Fréjus detector
- Author
-
K.-H. Becker, B. Kuznik, Y. Benadjal, H. Mönch, S. Tisserant, B. Dudelzak, C. Arpesella, R. Nisius, M. Fröhlich, A. Borg, H. J. Meyer, H. J. Daum, L. Moscoso, P. Roy, L. Behr, G. Chardin, U. Nguyen-Khac, R. Möller, B. Jacobi, S. Jullian, O. Perdereau, James T. Becker, J. F. Glicenstein, Peter Schleper, Claire Bourdarios, C. Longuemare, Michael Schubnell, D. Lalanne, Frank Raupach, D. Blum, C. Paulot, B. Degrange, J. Ernwein, G. Szklarz, P. Bareyre, Y. Wei, F. Laplanche, R. Barloutaud, P. Eschstruth, L. Mosca, and Ch. Berger
- Subjects
Physics ,Nuclear physics ,Nuclear and High Energy Physics ,Antiparticle ,Oscillation ,Antimatter ,Detector ,Hadron ,Neutron ,Nucleon ,Antineutron - Abstract
From the analysis of the fully contained events recorded in the underground Frejus detector, a lower limit of 1.2×108s at 90% CL is derived for the free neutron-antineutron oscillation time.
- Published
- 1990
- Full Text
- View/download PDF
41. The ANTARES optical module
- Author
-
M. Taiuti, R.W. Bland, D. Stubert, M. Anghinolfi, V. Roca-Blay, A. Le Van Suu, J. Carr, R. De Vita, V. Bertin, Elie Aslanides, E. Migneco, C. Millot, Sandra Zavatarelli, F. Mazéas, François Montanet, J. Poinsignon, D. Zornoza J. De, B. Mazeau, V.A. Kudryatsev, P. Deck, F. Feinstein, M. de Jong, F. Bernard, R. Berthier, F. Druillole, F. Blondeau, A. Massol, J.P. Soirat, J.-F. Drougou, N. de Botton, O. Suvorova, P. Goret, A. Rostovtsev, G. Herrouin, C. Carloganu, Y. Tayalati, N. J. C. Spooner, D. Lachartre, J.-S Ricol, Roland Triay, A. Calzas, J.E.J. Oberski, Nathalie Palanque-Delabrouille, E. Nezri, Jean-Pierre Morel, Lester D.R. Thompson, Roberto Bellotti, J.F. Gournay, J. Zúñiga, L. Lemoine, S. Loucatos, E. A. De Wolf, V. Valente, C. Olivetto, M. Circella, M. Karolak, R. Potheau, M. Danilov, S. L. Cartwright, D. Festy, M. Marcelin, D. Lo Presti, M. Ripani, Jean-Francois Rolin, E. Carmona, J. Fopma, P. Mols, L. Gosset, V. Zakharov, Annarita Margiotta, C. Racca, J.J. Engelen, T. Montaruli, J.R. Hubbard, M. Billault, P.M. Kooijman, P. Petta, G. Raia, J.M. Gallone, Th. Stolarczyk, Susan Cooper, H. Le Provost, S. Anvar, F. Réthoré, G. Vaudaine, Gerardus Nooren, S. Cecchini, Y. Queinec, A. Kouchner, M. Petruccetti, P. Amram, Juan José Hernández-Rey, R. van Dantzig, F. Cafagna, Chantal Compère, J.J. Destelle, L. Moscoso, P. Vernin, J. Boulesteix, M. Jaquet, Maurizio Spurio, L Lo Nigro, A.J. Heijboer, F. Ciacio, P. Coyle, Charling Tao, F. Louis, P. Piattelli, V. Popa, Wolfgang Schuster, F.E. Ardellier-Desages, F. Cassol, J. P. Laugier, S. Basa, J. P. Schuller, Y. Benhammou, D. S. Bailey, J-J. Aubert, Giorgio Riccobene, H. Lafoux, L. Laubier, J. E. McMillan, P. Magnier, P. Payre, V. Lyashuk, Nunzio Randazzo, M. Battaglieri, A. Oppelt-Pohl, R. Masullo, C. De Marzo, J.-L. Michel, E. Salusti, Y. Sacquin, A. Mazure, S. Cuneo, P.K.A. de Witt Huberts, P. Lamare, S. Tilav, G.V. Russo, R. Blaes, J. Croquette, L. Caponetto, J.-C. Languillat, P. Perrin, P.H. Carton, G. Dispau, G. Giacomelli, A. Capone, Jürgen Brunner, S. Sánchez Navas, Y. Le Guen, R. Azoulay, B. Brooks, I. Varlamov, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), ANTARES, ANTARES (IHEF, IoP, FNWI), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Amram P., Anghinolfi M., Anvar S., Ardellier-Desages F.E, Aslanides E., Aubert J.-J., Azoulay R., Bailey D., Basa S., Battaglieri M., Bellotti R., Benhammou Y., Bernard F., Berthier R., Bertin V., Billault M., Blaes R., Bland R.W, Blondeau F., De Botton N., Boulesteix J., Brooks C.B, Brunner J., Cafagna F., Calzas A., Capone A., Caponetto L., Carloganu C., Carmona E., Carr J., Carton P.-H., Cartwright S.L, Cassol F., Cecchini S., Ciacio F., Circella M., Compere C., Cooper S., Coyle P., Croquette J., Cuneo S., Danilov M., Van Dantzig R., De Marzo C., DeVita R., Deck P., Destelle J.-J., Dispau G., Drougou J.F, Druillole F., Engelen J., Feinstein F., Festy D., Fopma J., Gallone J.-M., Giacomelli G., Goret P., Gosset L., Gournay J.-F., Heijboer A., Hernandez-Rey J.J, Herrouin G., Hubbard J.R, Jaquet M., De Jong M., Karolak M., Kooijman P., Kouchner A., Kudryavtsev V.A, Lachartre D., Lafoux H., Lamare P., Languillat J.-C., Laubier L., Laugier J.-P., Le Guen Y., Le Provost H., Le Van Suu A., Lemoine L., Lo Nigro L., Lo Presti D., Loucatos S., Louis F., Lyashuk V., Magnier P., Marcelin M., Margiotta A., Massol A., Masullo R., Mazeas F., Mazeau B., Mazure A., and Spurio
- Subjects
Nuclear and High Energy Physics ,Photomultiplier ,Astrophysics and Astronomy ,Physics::Instrumentation and Detectors ,Astrophysics::High Energy Astrophysical Phenomena ,Neutrino telescope ,FOS: Physical sciences ,Astrophysics ,01 natural sciences ,High Energy Physics - Experiment ,Nuclear physics ,Optical Module ,neutrino astronomy ,High Energy Physics - Experiment (hep-ex) ,deep sea detector ,Mediterranean sea ,0103 physical sciences ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,14. Life underwater ,Electronics ,Detectors and Experimental Techniques ,010306 general physics ,Instrumentation ,Remote sensing ,Physics ,010308 nuclear & particles physics ,Detector ,Astrophysics (astro-ph) ,Astrophysics::Instrumentation and Methods for Astrophysics ,Neutrino detector ,Física nuclear ,Neutrino astronomy - Abstract
The ANTARES collaboration is building a deep sea neutrino telescope in the Mediterranean Sea. This detector will cover a sensitive area of typically 0.1 km-squared and will be equipped with about 1000 optical modules. Each of these optical modules consists of a large area photomultiplier and its associated electronics housed in a pressure resistant glass sphere. The design of the ANTARES optical module, which is a key element of the detector, has been finalized following extensive R & D studies and is reviewed here in detail., 26 pages, 15 figures, to be published in NIM
- Published
- 2002
42. Underwater Neutrino Detectors
- Author
-
L. Moscoso
- Subjects
Physics ,Particle physics ,Astrophysics::High Energy Astrophysical Phenomena ,Solar neutrino ,Cosmic microwave background ,Dark matter ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Solar neutrino problem ,Neutrino detector ,Measurements of neutrino speed ,Neutrino ,Neutrino astronomy - Abstract
Due to their weak interaction with matter and to the absence of their interaction with the electro-magnetic radiations, neutrinos can travel in the Universe without being absorbed. This is not the case for photons which interact with matter, with the infra-red (IR) radiation and with the cosmic microwave background (CMB).
- Published
- 2001
- Full Text
- View/download PDF
43. Neutrino telescopes under the ocean: The case for ANTARES
- Author
-
L. Moscoso
- Subjects
Physics ,Nuclear and High Energy Physics ,Particle physics ,Physics::Instrumentation and Detectors ,Astrophysics::High Energy Astrophysical Phenomena ,Detector ,Astrophysics (astro-ph) ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,FOS: Physical sciences ,Astrophysics ,Atomic and Molecular Physics, and Optics ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,High Energy Physics - Phenomenology ,High Energy Physics - Phenomenology (hep-ph) ,Angular resolution ,High Energy Physics::Experiment ,Neutrino - Abstract
Neutrino telescopes offer an alternative way to explore the Universe. Several projects are in operation or under construction. A detector under the ocean is very promising because of the very accurate angular resolution that it provides. The ANTARES project is intended to demonstrate the feasibilty of such a detector., Talk given at the Neutrino98 conference, Takayama, Japan, June 4-9, 1998
- Published
- 1998
44. EROS and MACHO Combined Limits on Planetary Mass Dark Matter in the Galactic Halo
- Author
-
Pratt, A. Tomaney, C Renault, R. A. Allsman, F. Cavalier, L. Prevot, Dante Minniti, Kenneth C. Freeman, Christopher W. Stubbs, A. Milsztajn, Bruce A. Peterson, Charles Alcock, P. Bareyre, L. Vigroux, Peter J. Quinn, B Laurent, F Queinnec, Éric Aubourg, J. Guibert, E. Maurice, Nathalie Palanque-Delabrouille, David P. Bennett, Michel Spiro, David R. Alves, M Lachieze-Rey, P. Grison, L Moscoso, Andrew C. Becker, Christophe Magneville, William J. Sutherland, R. Ansari, J. Fernandez, Matthew J. Lehner, Kem H Cook, T. Vandehei, Roger Ferlet, Cecile Gry, M. Gros, S. Zylberajch, S. L. Marshall, Tim Axelrod, É. Lesquoy, Alfred Vidal-Madjar, S. Char, J. P. Beaulieu, O. Moreau, Kim Griest, M. Moniez, S. Brehin, J. Rich, Astronomy, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF (institution))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), EROS, and Lantz, Simone
- Subjects
stars ,gravitational lensing ,Scalar field dark matter ,FOS: Physical sciences ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,dark matter ,Galactic halo ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Baryonic dark matter ,0103 physical sciences ,low-mass ,Astrophysics::Solar and Stellar Astrophysics ,Massive compact halo object ,010303 astronomy & astrophysics ,Light dark matter ,Astrophysics::Galaxy Astrophysics ,Physics ,010308 nuclear & particles physics ,stars, low-mass, brown dwarfs ,Hot dark matter ,Astrophysics (astro-ph) ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,Astronomy and Astrophysics ,Dark matter halo ,Space and Planetary Science ,[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Cuspy halo problem ,OBJECTS ,Astrophysics::Earth and Planetary Astrophysics ,brown dwarfs - Abstract
The EROS and MACHO collaborations have each published upper limits on the amount of planetary mass dark matter in the Galactic Halo obtained from gravitational microlensing searches. In this paper the two limits are combined to give a much stronger constraint on the abundance of low mass MACHOs., 8 pages, 4 figures, submitted to ApJ Letters
- Published
- 1998
45. Pre-Main-Sequence Star Candidates in the Bar of the Large Magellanic Cloud
- Author
-
E. Aubourg, R. Julien, F. Queinnec, A. Milsztajn, J. de Kat, P. Bareyre, Alfred Vidal-Madjar, Roger Ferlet, C. Magneville, L. Moscoso, M. Gros, L. Vigroux, H. J. G. L. M. Lamers, M. Moniez, S. Zylberajch, Cecile Gry, E. Bertin, C. Renault, Jean-Philippe Beaulieu, P. Grison, L. Prevot, M. Lachieze-Rey, O. Moreau, B. Laurent, C. Lanciaux, R. Ansari, J. Rich, E. Lesquoy, M. Spiro, F. Cavalier, F. Tajhmady, J. Guibert, and E. Maurice
- Subjects
Physics ,Multidisciplinary ,Spiral galaxy ,K-type main-sequence star ,Astronomy ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Star count ,Astrophysics ,Herbig Ae/Be star ,Galaxy ,Blue straggler ,T Tauri star ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics::Galaxy Astrophysics ,Dwarf galaxy - Abstract
Candidate pre-main-sequence stars were observed in the bar of the Large Magellanic Cloud during the search for dark matter in the galactic halo. Seven blue stars of apparent visual magnitude 15 to 17 had irregular photometric variations and hydrogen emission lines in their optical spectra, which suggested that these stars are pre-main-sequence stars of about 10 solar masses. These stars are slightly more massive and definitely more luminous than are Herbig AeBe pre-main-sequence stars in our own galaxy. Continued observations of these very young stars from another galaxy, which are probably at the pre-hydrogen-burning stage, should provide important clues about early stages of star formation.
- Published
- 1996
46. Limits on the flux of very high energy neutrinos with the FREJUS detector
- Author
-
B. Kuznik, H. J. Meyer, S. Tisserant, L. Moscoso, B. Degrange, R. Barloutaud, O. Perdereau, J. Ernwein, Wolfgang Rhode, Michael Schubnell, G. Chardin, Y. Wei, P. Bareyre, L. Mosca, K. Daum, Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), FREJUS, and Kerec, Hélène
- Subjects
Physics ,Particle physics ,Physics::Instrumentation and Detectors ,010308 nuclear & particles physics ,Astrophysics::High Energy Astrophysical Phenomena ,Solar neutrino ,Astronomy and Astrophysics ,Solar neutrino problem ,01 natural sciences ,Cosmic neutrino background ,Nuclear physics ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Neutrino detector ,[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,0103 physical sciences ,Measurements of neutrino speed ,High Energy Physics::Experiment ,Neutrino ,Neutrino astronomy ,010306 general physics ,Neutrino oscillation - Abstract
The final data set of muons recorded with the Frejus detector has been analyzed to determine the atmospheric neutrino ν μ -flux. From the depth intensity relation of the muon flux a region of almost horizontal neutrino induced muons has been identified. The measurement of the energy loss inside the detector of these through-going muons allows a search for deviations from the expected energy spectrum of the atmospheric neutrinos with two independent methods. No evidence of any extra ν μ -flux at energies > 1 TeV has been found thus enabling significant limits to be set on the extragalactic ν μ -flux predicted by several models of cosmological sources. These limits do not depend on the particular atmospheric neutrino flux model considered.
- Published
- 1996
47. Multimessenger Sources of Gravitational Waves and High-energy Neutrinos: Science Reach and Analysis Method
- Author
-
Francesco Salemi, V. Re, Thierry Pradier, J. G. Rollins, P. J. Sutton, S. Márka, Z. Márka, P. Raffai, E. Chassande-Mottin, M Alessandra Papa, L. Moscoso, M. Tse, Gareth Jones, Antoine Kouchner, Corinne Donzaud, Chad Finley, B. Bouhou, I. Di Palma, Alessandra Corsi, Imre Bartos, G. Vedovato, V. Van Elewyck, M. Drago, G. A. Prodi, S. Klimenko, Bruny Baret, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Department of Physics, Columbia University, Columbia University [New York], Laser Interferometer Gravitational-Wave Observatory (LIGO), Max-Planck-Institut für Gravitationsphysik, Université Paris-Sud - Paris 11 (UP11), Gruppo Collegato di Trento (INFN), Oskar Klein Centre, Physics Department, Cardiff University, University of Florida, Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata (INFN), and Istituto Nazionale di Fisica Nucleare, Sezione di Padova (INFN)
- Subjects
Physics ,History ,Gravitational-wave observatory ,Gravitational wave ,Astrophysics::High Energy Astrophysical Phenomena ,Astronomy ,Observable ,Astrophysics ,Gravitational-wave astronomy ,Computer Science Applications ,Education ,Gravitational energy ,Massless particle ,General Relativity and Quantum Cosmology ,Neutrino ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,Lepton - Abstract
International audience; Sources of gravitational waves are often expected to be observable through several messengers, such as gamma-rays, X-rays, optical, radio, and/or neutrino emission. The simultaneous observation of electromagnetic or neutrino emission with a gravitational-wave signal could be a crucial aspect for the first direct detection of gravitational waves. Furthermore, combining gravitational waves with electromagnetic and neutrino observations will enable the extraction of scientific insight that was hidden from us before. We discuss the method that enables the joint search with the LIGO-Virgo-IceCube-ANTARES global network, as well as its methodology, science reach, and outlook for the next generation of gravitational-wave detectors.
- Published
- 2012
- Full Text
- View/download PDF
48. Evidence for gravitational microlensing by dark objects in the galactic halo
- Author
-
Michel Spiro, Roger Ferlet, Jean-Philippe Beaulieu, Éric Aubourg, M. Gros, L. Vigroux, P. Bareyre, L. Prevot, P. Grison, A. Milsztajn, R. Ansari, S. Brehin, Cecile Gry, L. Moscoso, J. Rich, Alfred Vidal-Madjar, E. Lesquoy, S. Zylberajch, O. Moreau, B. Laurent, M. Lachieze-Rey, F. Cavalier, M. Moniez, Christophe Magneville, F. Tajahmady, J. Guibert, E. Maurice, F. Queinnec, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), and EROS
- Subjects
Physics ,Multidisciplinary ,Spiral galaxy ,010308 nuclear & particles physics ,Dark matter ,Astronomy ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Gravitational microlensing ,01 natural sciences ,Galactic tide ,Galaxy ,Galactic halo ,Dark matter halo ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Galaxy rotation curve - Abstract
THE flat rotation curves of spiral galaxies, including our own, indicate that they are surrounded by unseen haloes of ‘dark matter’1,2. In the absence of a massive halo, stars and gas in the outer portions of a galaxy would orbit the centre more slowly, just as the outer planets in the Solar System circle the Sun more slowly than the inner ones. So far, however, there has been no direct observational evidence for the dark matter, or its characteristics. Paczynski3suggested that dark bodies in the halo of our Galaxy can be detected when they act as gravitational ‘microlenses’, amplifying the light from stars in nearby galaxies. The duration of such an event depends on the mass, distance and velocity of the dark object. We have been monitoring the brightness of three million stars in the Large Magellanic Cloud for over three years, and here report the detection of two possible microlensing events. The brightening of the stars was symmetrical in time, achromatic and not repeated during the monitoring period. The timescales of the two events are about thirty days and imply that the masses of the lensing objects lie between a few hundredths and one solar mass. The number of events observed is consistent with the number expected if the halo is dominated by objects with masses in this range. In 1986, Bohdan Paczynski suggested that dark, compact objects in the halo of our Galaxy — the local cousins of similar objects conjectured to contribute dark matter to the haloes of other galaxies — could be detected on Earth, as their gravitation might occasionally amplify the light arriving from more distant stars. In 1993, in surveys of several million stars in the Large Magellanic Cloud, C. Alcock et al. and E. Aubourg et al. observed several candidate events. In total, the two groups detected three stars for which the brightness increased by two magnitudes over an interval of roughly one month.
- Published
- 1993
49. Search for long-lived particles in 200 GeV/c proton-nucleon collisions
- Author
-
L. Moscoso, G. Giacomelli, A. Bussière, W. Bozzoli, D. E. Plane, R. Meunier, S. Zylberajch, E. Lesquoy, Achim Müller, and Franco Rimondi
- Subjects
Physics ,Nuclear physics ,Nuclear and High Energy Physics ,Particle physics ,Pion ,Proton ,Hadron ,High Energy Physics::Experiment ,Nuclear Experiment ,Nucleon ,Beam (structure) ,Lepton - Abstract
A search for long-lived particles (τ ≳ 10−8 sec), with changes ±23, ± 1, ±43 and ± 2, produced in 200 GeV pN collisions was performed at the CERN-SPS in a secondary beam equipped with superconducting r.f. separators. Upper limits were obtained for the production of long-lived hadrons and leptons. For charge - 1 particles the limits are at the level of 10−7 of the pions at a mass m = 0.2 GeV and reach the 10−11 level from 3 to 8 GeV. The production of light antinuclei was measured. The cross sections for 3He production are (1.3 ± 0.3) and (1.9 ± 0.3) × 10−34 cm2/sr · GeV/c at 21 and 47.4 GeV/c respectively; for t the cross section is (7.6 ± 0.9) × 10−34 cm2/sr · GeV/c at 23.7 GeV/c.
- Published
- 1979
- Full Text
- View/download PDF
50. Production of d, t, 3He, and by 200 GeV protons
- Author
-
R. Meunier, L. Moscoso, Franco Rimondi, G. Giacomelli, E. Lesquoy, Achim Müller, S. Zylberajch, A. Bussière, and W. Bozzoli
- Subjects
Physics ,Nuclear and High Energy Physics ,Nuclear Theory ,chemistry.chemical_element ,Charged particle ,Nuclear physics ,medicine.anatomical_structure ,chemistry ,Deuterium ,Yield (chemistry) ,Antimatter ,Helium-3 ,medicine ,Beryllium ,Atomic physics ,Nuclear Experiment ,Nucleus ,Isotopes of helium - Abstract
Data are presented on the yields of d, t, 3 He, d , t and 3 He with laboratory momenta between 12 and 37 GeV/ c produced by 200 GeV protons on beryllium and aluminium. The production yield of nuclei depends significantly on the target nucleus, while the d production is independent of target material. The mass dependence of the production cross section is exponential for both nuclei and antinuclei.
- Published
- 1978
- Full Text
- View/download PDF
Catalog
Discovery Service for Jio Institute Digital Library
For full access to our library's resources, please sign in.