Zobrazeno 1 - 10
of 88
pro vyhledávání: '"Salamida, Francesco"'
Autor:
Salamida, Francesco
Publikováno v:
PoS(ICRC2023)016
The Pierre Auger Observatory is a unique facility designed to study ultra-high energy cosmic rays, with energies up to 10$^{20}$ eV and beyond. The Observatory is located in Argentina and comprises more than 1600 water Cherenkov detectors spread over
Externí odkaz:
http://arxiv.org/abs/2312.14673
Autor:
Bradfield, Fraser, Albury, Justin, Bellido, Jose, Chytka, Ladislav, Farmer, John, Fujii, Toshihiro, Hamal, Petr, Horvath, Pavel, Hrabovsky, Miroslav, Jilek, Vlastimil, Kmec, Jakub, Kvita, Jiri, Malacari, Max, Mandat, Dusan, Mastrodicasa, Massimo, Matthews, John N., Michal, Stanislav, Nagasawa, Hiromu, Namba, Hiroki, Nozka, Libor, Palatka, Miroslav, Pech, Miroslav, Privitera, Paolo, Sakurai, Shunsuke, Salamida, Francesco, Schovanek, Petr, Smida, Radomir, Stanik, Daniel, Svozilikova, Zuzana, Taketa, Akimichi, Terauchi, Kenta, Thomas, Stan B., Travnicek, Petr, Vacula, Martin
Publikováno v:
PoS(ICRC2023)303
The Fluorescence detector Array of Single-pixel Telescopes (FAST) is one of several proposed designs for a next-generation cosmic-ray detector. Such detectors will require enormous collecting areas whilst also needing to remain cost-efficient. To mee
Externí odkaz:
http://arxiv.org/abs/2308.11989
Autor:
Sakurai, Shunsuke, Albury, Justin, Bellido, Jose, Bradfield, Fraser, Chytka, Ladislav, Farmer, John, Fujii, Toshihiro, Hamal, Petr, Horvath, Pavel, Hrabovsky, Miroslav, Jilek, Vlastimil, Kmec, Jakub, Kvita, Jiri, Malacari, Max, Mandat, Dusan, Mastrodicasa, Massimo, Matthews, John N., Michal, Stanislav, Nagasawa, Hiromu, Namba, Hiroki, Nozka, Libor, Palatka, Miroslav, Pech, Miroslav, Privitera, Paolo, Salamida, Francesco, Schovanek, Petr, Smida, Radomir, Stanik, Daniel, Svozilikova, Zuzana, Taketa, Akimichi, Terauch, Kenta, Thomas, Stan B., Travnicek, Petr, Vacula, Martin
Publikováno v:
PoS(ICRC2023)302
Ultra-high energy cosmic rays (UHECRs), whose energy are beyond $10^{18}~\mathrm{eV}$, are the most energetic particles we have ever detected. The latest results seem to indicate a heavier composition at the highest energies, complicating the search
Externí odkaz:
http://arxiv.org/abs/2308.11988
Autor:
Fujii, Toshihiro, Albury, Justin, Bellido, Jose, Chytka, Ladislav, Farmer, John, Hamal, Petr, Horvath, Pavel, Hrabovsky, Miroslav, Kubo, Hidetoshi, Kvita, Jiri, Malacari, Max, Mandat, Dusan, Mastrodicasa, Massimo, Matthews, John, Michal, Stanislav, Ni, Xiaochen, Nozaki, Seiya, Nozka, Libor, Oka, Tomohiko, Palatka, Miroslav, Pech, Miroslav, Privitera, Paolo, Schovanek, Petr, Salamida, Francesco, Smida, Radomir, Thomas, Stan, Taketa, Akimichi, Terauchi, Kenta, Travnicek, Petr, Vacula, Martin, Yoo, Seokhyun
Publikováno v:
PoS (ICRC2021) 402 (2021)
The origin and nature of ultra-high-energy cosmic rays (UHECRs) remain an open question in astroparticle physics. Motivated by the need for an unprecedented aperture for further advancements, the Fluorescence detector Array of Single-pixel Telescopes
Externí odkaz:
http://arxiv.org/abs/2107.02949
Autor:
Cummings, Austin, Aloisio, Roberto, Bertaina, Mario, Bisconti, Francesca, Fenu, Francesco, Salamida, Francesco
Publikováno v:
PoS(ICRC2019)862
Many proposed and upcoming experiments seek to observe signals from upward going air showers initiated by tau leptons resulting from neutrino interactions inside the Earth. To save calculation time, event estimations for these observation methods are
Externí odkaz:
http://arxiv.org/abs/1910.01021
Autor:
Cummings, Austin, Aloisio, Roberto, Bertaina, Mario, Bisconti, Francesca, Fenu, Francesco, Salamida, Francesco
Publikováno v:
PoS(ICRC2019)861
The ANITA collaboration has recently announced the supposed observation of two upward going cosmic ray showers at earth emergence angles $27^{\circ}$ and $35^{\circ}$ with reconstructed energy $\sim$0.6~EeV. Upward air showers (UAS) are expected from
Externí odkaz:
http://arxiv.org/abs/1910.00992
Autor:
GERDA collaboration, Agostini, Matteo, Bakalyarov, Alexander M., Balata, Marco, Barabanov, Igor, Baudis, Laura, Bauer, Christian, Bellotti, Enrico, Belogurov, Sergej, Bettini, Alessandro, Bezrukov, Leonid, Borowicz, Dariusz, Bossio, Elisabetta, Bothe, Vikas, Brudanin, Victor, Brugnera, Riccardo, Caldwell, Allen, Cattadori, Carla, Chernogorov, Andrey, Comellato, Tommaso, D'Andrea, Valerio, Demidova, Elena V., Di Marco, Natalia, Domula, Alexander, Doroshkevich, Evgenyi, Egorov, Viacheslav, Fischer, Felix, Fomina, Maria, Gangapshev, Albert, Garfagnini, Alberto, Gooch, Chris, Grabmayr, Peter, Gurentsov, Valery, Gusev, Konstantin, Hakenmüller, Janina, Hemmer, Sabine, Hiller, Roman, Hofmann, Werner, Hult, Mikael, Inzhechik, Lev V., Csáthy, Jozsef Janicskó, Jochum, Josef, Junker, Matthias, Kazalov, Vladimir, Kermaïdic, Yoann, Kihm, Thomas, Kirpichnikov, Igor V., Klimenko, Alexander, Kneißl, Raphael, Knöpfle, Karl T., Kochetov, Oleg, Kornoukhov, Vasily N., Krause, Patrick, Kuzminov, Valery V., Laubenstein, Matthias, Lazzaro, Andrea, Lindner, Manfred, Lippi, Ivano, Lubashevskiy, Alexey, Lubsandorzhiev, Bayarto, Lutter, Guillaume, Macolino, Carla, Majorovits, Bela, Maneschg, Werner, Miloradovic, Michael, Mingazheva, Rizalina, Misiaszek, Marcin, Moseev, Pavel, Nemchenok, Igor, Panas, Krysztof, Pandola, Luciano, Pelczar, Krysztof, Pertoldi, Luigi, Piseri, Paolo, Pullia, Alberto, Ransom, Chloe, Riboldi, Stefano, Rumyantseva, Nadezda, Sada, Cinzia, Salamida, Francesco, Schönert, Stefan, Schreiner, Jochen, Schütt, Mario, Schütz, Ann-Katrin, Schulz, Oliver, Schwarz, Mario, Schwingenheuer, Bernhard, Selivanenko, Oleg, Shevchik, Egor, Shirchenko, Mark, Simgen, Hardy, Smolnikov, Anatoly, Stukov, Danila, Vanhoefer, Laura, Vasenko, Andrey A., Veresnikova, Anna, Vignoli, Chiara, von Sturm, Katharina, Wester, Thomas, Wiesinger, Christoph, Wojcik, Marcin, Yanovich, Evgeny, Zatschler, Birgit, Zhitnikov, Igor, Zhukov, Sergey V., Zinatulina, Daniya, Zschocke, Andreas, Zsigmond, Anna J., Zuber, Kai, Zuzel, Grzegorz
The GERmanium Detector Array (GERDA) experiment at the Gran Sasso underground laboratory (LNGS) of INFN is searching for neutrinoless double-beta ($0\nu\beta\beta$) decay of $^{76}$Ge. The technological challenge of GERDA is to operate in a "backgrou
Externí odkaz:
http://arxiv.org/abs/1909.02522
Autor:
Fujii, Toshihiro, Malacari, Max, Farmer, John, Albury, Justin, Bellido, Jose A., Chytka, Ladislav, Hamal, Petr, Horvath, Pavel, Hrabovsky, Miroslav, Kvita, Jiri, Mandat, Dusan, Mastrodicasa, Massimo, Matthews, John N., Michal, Stanislav, Ni, Xiaochen, Nozka, Libor, Palatka, Miroslav, Pech, Miroslav, Privitera, Paolo, Schovanek, Petr, Salamida, Francesco, Smida, Radomir, Thomas, Stan B., Travnicek, Petr, Vacula, Martin
The origin and nature of ultra-high energy cosmic rays (UHECRs) are hot topics in the astroparticle physics community. The Fluorescence detector Array of Single-pixel Telescopes (FAST) is a design for a next-generation ground-based UHECR observatory,
Externí odkaz:
http://arxiv.org/abs/1908.02904
Autor:
Gaïor, Romain, Samarai, Imen Al, Bérat, Corinne, Otano, Miguel Blanco, David, Jacques, Deligny, Oliver, Lebbolo, Hervé, Lecoz, Sandra, Letessier-Selvon, Antoine, Lhenry-Yvon, Isabelle, Mariş, Ioana C., Montanet, François, Repain, Philippe, Salamida, Francesco, Settimo, Mariangela, Stassi, Patrick, Stutz, Anne
We present the GIGAS (Gigahertz Identification of Giant Air Shower) microwave radio sensor arrays of the EASIER project (Extensive Air Shower Identification with Electron Radiometers), deployed at the site of the Pierre Auger cosmic ray observatory.
Externí odkaz:
http://arxiv.org/abs/1710.02483
Publikováno v:
PoS(ICRC2017)560
Interactions of ultra-high-energy cosmic rays with background photons set a limit to the distance cosmic rays reaching us above a certain energy can originate from, making measurements of their fluxes insensitive to properties of sources at high reds
Externí odkaz:
http://arxiv.org/abs/1707.04836