Zobrazeno 1 - 10
of 89
pro vyhledávání: '"M. BONORI"'
Autor:
A. Martini, M. Osipenko, M. Taiuti, Mario Musumeci, N. Randazzo, A. Grimaldi, E. Barbarito, M. Morganti, A. D'Amico, A. Anzalone, B. Bouhadef, Ralf Wischnewski, C. Petta, Francesco Simeone, Roberto Bellotti, D. Piombo, M. Anghinolfi, L. Maccione, M. Mongelli, E. Migneco, Emanuele Castorina, Tommaso Chiarusi, M. Bazzotti, G. De Bonis, G. De Ruvo, G. Cacopardo, S. Russo, M. Circella, G. Raia, G. Carminati, G. Terreni, G. De Rosa, E. Falchini, R. Habel, R. Masullo, A. Aloisio, M. Ripani, R. De Vita, G. Osteria, M. Cordelli, L. Caponetto, M. Ruppi, Riccardo Papaleo, A. Ceres, G. C. Barbarino, G. Giacomelli, L. Trasatti, C. Distefano, S. Reito, M. Bonori, R. Coniglione, S. Urso, Alessandro Gabrielli, Annarita Margiotta, Alessandro Lonardo, G. Ricco, C. Avanzini, B. Cassano, Teresa Montaruli, A. Bersani, D. Lo Presti, C.A. Nicolau, Nicolo' Beverini, Enzo Gandolfi, F. Ameli, G.V. Russo, S. Biagi, F. Giorgi, F. Lucarelli, F. Raffaelli, P. Piattelli, S. Galeotti, G. Riccobene, E. Shirokov, V. Valente, V. Pappalardo, P. Musico, V. Flaminio, M. Battaglieri, C. De Marzo, Rosanna Cocimano, Valeria Sipala, A. Orlando, Alberto Rovelli, Antonio Capone, Maurizio Spurio, Giuseppe Longo, A. Marinelli, M. Sedita, K. Fratini, Rosario Megna, Piero Vicini, Paolo Sapienza, S. Minutoli, I. Amore, Mário Costa, Manuela Vecchi, Sebastiano Aiello, E. Leonora
The NEMO collaboration proposes to build an underwater neutrino telescope located South-East off the Sicily coast. This paper describes the concepts underlying the communication link design going over the whole data acquisition and transport from the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::922b01461ee93986d58e4191fbedff29
http://hdl.handle.net/11588/418831
http://hdl.handle.net/11588/418831
Publikováno v:
IEEE Transactions on Nuclear Science. 53:944-950
An electronic board, called floor control module (FCM), was developed for the NEMO project, an underwater neutrino telescope. The offshore FCM is in charge of providing interfaces toward instrumental control boards, collecting data from up to eight r
Autor:
C. Sollima, E. Leonora, G. Carminati, M. Circella, Alberto Rovelli, F. Lucarelli, Piera Sapienza, M. Bazzotti, S. Minutoli, F. Raffaelli, V. Flaminio, Tommaso Chiarusi, M. Costa, Manuela Vecchi, Sebastiano Aiello, G. Giacomelli, Paolo Musico, G. DeBonis, Paolo Piattelli, G. Raia, Antonio Capone, Fabio Stefani, Antonio D'Amico, Maurizio Spurio, S. Russo, Mario Musumeci, G. Giovanetti, N. Randazzo, S. Galeotti, A. Orlando, V. Pappalardo, I. Amore, G. Cacopardo, Giorgio Riccobene, L. Caponetto, M. Battaglieri, E. Shirokov, Rosanna Cocimano, D. LoPresti, C. Calì, S. Reito, F. Maugeri, R. Coniglione, M. Cordelli, S. Urso, E. Barbarito, Alberto Aloisio, M. Ripani, G. C. Barbarino, Francesco Simeone, Valeria Sipala, M. Osipenko, A. Ceres, G. DeRosa, M. Imbesi, A. Grimaldi, D. Piombo, M. Anghinolfi, Nicolo' Beverini, Enzo Gandolfi, R. DeVita, Emilio Migneco, G. Ricco, A. Grmek, G.V. Russo, M. Mongelli, A. Martini, G. Terreni, M. Morganti, S. Biagi, Ralf Wischnewski, M. Ruppi, B. Bouhdaef, B. Cassano, D. Sciliberto, M. Bonori, Piero Vicini, F. Ameli, A. Bersani, A. Marinelli, M. Sedita, K. Fratini, M. Taiuti, R. Habel, C. Distefano, L. Trasatti, Federico M. Giorgi, A. Anzalone, Annarita Margiotta, Roberto Bellotti, R. Masullo, G. DeRuvo, Riccardo Papaleo, Alessandro Lonardo, Alessandro Gabrielli
none 104 The selection of the photomultiplier plays a crucial role in the R&D activity related to a large-scale underwater neutrino telescope. This paper illustrates the main procedures and facilities used to characterize the performances of 72 large
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3c6eb773316fefd320c1b9a57b816c91
http://hdl.handle.net/11588/428818
http://hdl.handle.net/11588/428818
Publikováno v:
Review of Scientific Instruments. 73:4164-4168
A module was constructed for the measurement of deep sea optical activity at a sensitivity level of a single photoelectron. We describe the features of the module and a method for calibrating it. The average sensitivity in the interval from 350 to 50
Publikováno v:
The European Physical Journal C. 25:67-75
We describe the measurement of the deep sea optical background in some sites south of Capo Passero, Sicily. A continuous flux of about 440 photons cm -2 s -1 in the wavelength interval 440-550 nm is estimated due to the decays of the 40K contained in
Autor:
A. D'Amico, G. Giovanetti, P. Keller, F. Ameli, Vincent Bertin, M. Bonori, C.D. Llorens, G. Riccobene, Miguel Ardid, M. Imbesi, Manuel Bou-Cabo, Giuseppina Larosa, Salvatore Viola, R. Masullo, C. Calì, N. Randazzo, F. Speziale
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
4th International Workshop on a Very Large Volume Neutrino Telescope for the Mediterranean (VLVNT09)
4th International Workshop on a Very Large Volume Neutrino Telescope for the Mediterranean (VLVNT09), Oct 2009, Athènes, Greece. pp.S211-S213, ⟨10.1016/j.nima.2010.04.130⟩
RiuNet. Repositorio Institucional de la Universitat Politécnica de Valéncia
instname
4th International Workshop on a Very Large Volume Neutrino Telescope for the Mediterranean (VLVNT09)
4th International Workshop on a Very Large Volume Neutrino Telescope for the Mediterranean (VLVNT09), Oct 2009, Athènes, Greece. pp.S211-S213, ⟨10.1016/j.nima.2010.04.130⟩
RiuNet. Repositorio Institucional de la Universitat Politécnica de Valéncia
instname
An innovative Acoustic Positioning System for the km(3)-scale neutrino telescope has been designed and is under realization within the KM3NeT Consortium. Compared to the Acoustic Positioning Systems used for the km(3) demonstrators, ANTARES and NEMO
Autor:
Paolo Piattelli, S. Minutoli, E. Falchini, Alessandro Lonardo, G. Ricco, M. Morganti, M. Taiuti, R. De Vita, A. Capone, Manuela Vecchi, Sebastiano Aiello, Rosanna Cocimano, C. Calì, Ralf Wischnewski, F. Speziale, P. Sapienza, G. Raia, E. Castorina, S. Russo, G. De Rosa, P. Musico, Filippo Maria Giorgi, A. Orlando, M. Cordelli, Mario Musumeci, N. Randazzo, G. Giacomelli, V. D'Amato, E. Leonora, C. Sollima, A. Ceres, L. Caponetto, Antonio D'Amico, S. Biagi, G. Cacopardo, R. Masullo, B. Bouhdaef, B. Cassano, S. Galeotti, C. Distefano, V. Pappalardo, Giuseppe Longo, Alberto Rovelli, M. Osipenko, M. Ripani, E. Barbarito, E. Shirokov, A. Aloisio, C. D'Amato, R. Habel, A. Martini, A. Grimaldi, Giorgio Riccobene, M. Battaglieri, M. Ruppi, Massimo Brescia, G. C. Barbarino, M. Circella, V. Valente, Piero Vicini, Francesco Simeone, Maurizio Spurio, Riccardo Papaleo, G. Carminati, G. De Bonis, A. Anzalone, G. Giovanetti, Teresa Montaruli, Rosario Megna, A. Grmek, G. Terreni, Valeria Sipala, I. Amore, R. Coniglione, M. Bonori, F. Lucarelli, Roberto Bellotti, A. Bersani, G. Osteria, D. Piombo, L. Maccione, G. De Ruvo, M. Sedita, D. Lo Presti, K. Fratini, V. Flaminio, Alessandro Gabrielli, M. Costa, C. Petta, Annarita Margiotta, L. Trasatti, Tommaso Chiarusi, S. Reito, S. Urso, F. Ameli, G.V. Russo, M. Bazzotti, F. Maugeri, C.A. Nicolau, Nicolo' Beverini, Enzo Gandolfi, Emilio Migneco, M. Anghinolfi, M. Mongelli
The status of the activities towards the realization of a km3 Cherenkov neutrino detector carried out by the NEMO Collaboration is described. The realization of a Phase-1 project, which is under way, will validate the proposed technologies for the re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c99d0fb53177262a88b1ef2f8194e0df
http://hdl.handle.net/11585/126723
http://hdl.handle.net/11585/126723
Autor:
A. Anzalone, B. Bouhadef, R. Masullo, R. Habel, C. Distefano, Mario Musumeci, N. Randazzo, V. Valente, Riccardo Papaleo, I. Amore, V. Pappalardo, M. Taiuti, Mário Costa, A. D'Amico, A. Orlando, F. Lucarelli, C. Petta, M. Ambriola, M. Ruppi, G. De Bonis, Roberto Bellotti, M. Mongelli, G. C. Barbarino, S. Reito, Piero Vicini, M. Anghinolfi, R. De Vita, S. Cuneo, R. Coniglione, S. Urso, P. Piattelli, V. Flaminio, Annarita Margiotta, Teresa Montaruli, M. Circella, E. Migneco, Giuseppe Longo, S. Galeotti, S. Russo, M. Bonori, Massimo Brescia, M. Morganti, D. Lo Presti, M. Sedita, M. Osipenko, G. Osteria, Alessandro Lonardo, G. Ricco, G. Riccobene, E. Shirokov, Enrico Maccioni, Alessandro Gabrielli, L. Caponetto, Rosario Megna, L. Trasatti, Valeria Sipala, Sebastiano Aiello, K. Fratini, Tommaso Chiarusi, A. Grimaldi, E. Falchini, G. Cacopardo, Filippo Maria Giorgi, F. Ameli, Alberto Rovelli, F. Cafagna, Paolo Sapienza, M. Ripani, M. Battaglieri, C. De Marzo, E. Leonora, G. Terreni, Antonio Capone, Rosanna Cocimano, Maurizio Spurio, E. Castorina, G. Giacomelli, E. Barbarito, G. Raia, Francesco Simeone, G. De Rosa, C. Fiorello, M. Cordelli, A. Ceres, A. Martini, G.V. Russo, C.A. Nicolau, Nicolo' Beverini, Enzo Gandolfi
In this paper are presented the results of Monte Carlo simulations on the capability of the proposed NEMO-km$^3$ telescope to detect TeV muon neutrinos from Galactic microquasars. For each known microquasar we compute the number of detectable events,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c37d6b9455cc150583faac6ef7b640b3
http://hdl.handle.net/11588/418905
http://hdl.handle.net/11588/418905
Autor:
M. Ruppi, S. Aiello, F. Ameli, I. Amore, M. Anghinolfi, A. Anzalone, C. Avanzini, E. Barbarito, M. Battaglieri, M. Bazzotti, R. Bellotti, A. Bersani, N. Beverini, S. Biagi, M. Bonori, B. Bouhadef, G. Cacopardo, A. Capone, L. Caponetto, G. Carminati, E. Castorina, A. Ceres, T. Chiarusi, M. Circella, R. Cocimano, R. Coniglione, M. Cordelli, M. Costa, A. D'Amico, G. De Bonis, C. De Marzo, G. De Ruvo, R. De Vita, C. Distefano, E. Falchini, V. Flaminio, K. Fratini, A. Gabrielli, S. Galeotti, E. Gandolfi, G. Giacomelli, F. Giorgi, A. Grimaldi, R. Habel, E. Leonora, D. Lo Presti, A. Lonardo, LONGO, GIUSEPPE, F. Lucarelli, L. Maccione, A. Margiotta, A. Marinelli, A. Martini, R. Masullo, R. Megna, E. Migneco, M. Mongelli, T. Montaruli, M. Morganti, S. Minutoli, P. Musico, M. Musumeci, C. A. Nicolau, A. Orlando, M. Osipenko, G. Osteria, R. Papaleo, V. Pappalardo, C. Petta, P. Piattelli, D. Piombo, F. Raffaelli, G. Raia, N. Randazzo, S. Reito, G. Ricco, G. Riccobene, M. Ripani, A. Rovelli, G. V. Russo, S. Russo, P. Sapienza, M. Sedita, E. Shirokov, F. Simeone, V. Sipala, M. Spurio, M. Taiuti, G. Terreni, L. Trasatti, S. Urso, V. Valente, M. Vecchi, P. Vicini, R. Wischnewski, BARBARINO, GIANCARLO, DE ROSA, GIANFRANCA
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3730::0595efd07b27c35510091ce1481d2ea3
http://hdl.handle.net/11588/518518
http://hdl.handle.net/11588/518518
Autor:
E. MIGNECO, S. AIELLO, A. ALOISIO, F. AMELI, I. AMORE, M. ANGHINOLFI, A. ANZALONE, G. BARBARINO, E. BARBARITO, M. BATTAGLIERI, M. BAZZOTTI, R. BELLOTTI, A. BERSANI, N. BEVERINI, M. BONORI, B. BOUHDAEF, M. BRESCIA, G. CACOPARDO, C. CALÌ, A. CAPONE, L. CAPONETTO, G. CARMINATI, B. CASSANO, E. CASTORINA, A. CERES, M. CIRCELLA, R. COCIMANO, R. CONIGLIONE, M. CORDELLI, M. COSTA, A. DAMICO, C. DAMATO, V. DAMATO, G. DE BONIS, G. DE ROSA, G. DE RUVO, R. DE VITA, C. DISTEFANO, E. FALCHINI, V. FLAMINIO, K. FRATINI, S. GALEOTTI, G. GIOVANETTI, A. GRIMALDI, A. GRMEK, R. HABEL, E. LEONORA, A. LONARDO, G. LONGO, D. LO PRESTI, F. LUCARELLI, L. MACCIONE, A. MARTINI, R. MASULLO, F. MAUGERI, R. MEGNA, S. MINUTOLI, M. MONGELLI, T. MONTARULI, M. MORGANTI, P. MUSICO, M. MUSUMECI, C. A. NICOLAU, A. ORLANDO, M. OSIPENKO, G. OSTERIA, R. PAPALEO, V. PAPPALARDO, C. PETTA, P. PIATTELLI, D. PIOMBO, G. RAIA, N. RANDAZZO, S. REITO, G. RICCO, G. RICCOBENE, M. RIPANI, A. ROVELLI, M. RUPPI, G. V. RUSSO, S. RUSSO, P. SAPIENZA, M. SEDITA, E. SHIROKOV, F. SIMEONE, V. SIPALA, C. SOLLIMA, F. SPEZIALE, M. TAIUTI, G. TERRENI, L. TRASATTI, S. URSO, V. VALENTE, M. VECCHI, P. VICINI, R. WISCHNEWSKI, BIAGI, SIMONE, CHIARUSI, TOMMASO, GABRIELLI, ALESSANDRO, GANDOLFI, ENZO, GIACOMELLI, GIORGIO MARIA, GIORGI, FILIPPO MARIA, MARGIOTTA, ANNARITA, SPURIO, MAURIZIO
The timing calibration is a delicate operation to perform for assuring the full functionality of a large underwater neutrino telescope. In this paper we illustrate the main features of our system for timing calibration tailored to the needs of the pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4094::53646c1e239163b508962fb52931a75e
http://hdl.handle.net/11585/126729
http://hdl.handle.net/11585/126729