6 results on '"Helo, J.C."'
Search Results
2. Scalar-mediated double beta decay and LHC
- Author
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Gonzalez, L., Helo, J.C., Hirsch, M., and Kovalenko, S.G.
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- 2016
- Full Text
- View/download PDF
3. SND@LHC: The Scattering and Neutrino Detector at the LHC
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Acampora, G., Ahdida, C., Albanese, R., Albrecht, C., Alexandrov, A., Andreini, M., Anokhina, A., Auberson, N., Baldanza, C., Battilana, C., Bay, A., Bernard, F., Bestmann, P., Betancourt, C., Blanco, A., Bogomilov, M., Bonacorsi, D., Bonivento, W.M., Bordalo, P., Boyarsky, A., Breglio, G., Buonaura, A., Buontempo, S., Cafaro, V.D., Callignon, M., Camporesi, T., Campanelli, M., Canale, V., Cassese, F., Castro, A., Centanni, D., Cepeda Godoy, S.A., Cerutti, F., Charitonidis, N., Chernyavskiy, M., Choi, K.-Y., Cholak, S., Cicero, V., Cindolo, F., Climescu, M., Conaboy, A.P., Congedo, L., Crespo, O., Cristinziani, M., Crupano, A., Dallavalle, G.M., D'Ambrosio, N., De Carvalho Saraiva, J., De Bryas Dexmiers D'Archiac, P.T., De Lellis, G., de Magistris, M., De Roeck, A., De Rújula, A., De Serio, M., De Simone, D., Dedenko, L., Di Crescenzo, A., Di Giulio, L., Dolmatov, A., Dreyfus, L., Durhan, O., Fabbri, F., Fasanella, D., Fedotovs, F., Ferrillo, M., Ferro-Luzzi, M., Fienga, F., Fini, R.A., Fiorillo, A., Fonte, P., Fresa, R., Frei, R., Funk, W., Galati, G., Galkin, V., Garay Walls, F., Garcia Alia, R., Gerbershagen, A., Giordano, V., Golovatiuk, A., Golutvin, A., Gorshenkov, M., Graverini, E., Grenard, J.-L., Guler, A.M., Gulyaeva, V., Haefeli, G.J., Helo, J.C., Herwijnen, E.van, Iengo, P., Ilieva, S., Infantino, A., Irace, A., Iuliano, A., Jacobsson, R., Jacquart, M., Kamiscioglu, C., Khalikov, E., Kim, Y.G., Kim, S.H., Komatsu, M., Konovalova, N., Kovalenko, S., Krasilnikova, I., Kuleshov, S., Lacker, H.M., Lantwin, O., Lasagni Manghi, F., Lauria, A., Lee, K.S., Lee, K.Y., Leonardo, N., Liz Vargas, M.P., Lo Meo, S., Lemettais, C., Loschiavo, V.P., Lopes, L., Lussi, B., Marcellini, S., Margiotta, A., Magnan, A., Maier, R., Maietta, M., Malinin, A., Marrazzo, V.R., Maurer, Y., Managadze, A.K., Mascellani, A., Miano, A., Mikulenko, A., Minelli, F., Montanari, A., Montesi, M.C., Naka, T., Navarria, F.L., Ogawa, S., Okateva, N., Owtscharenko, N., Ovchynnikov, M., Park, B.D., Passeggio, G., Pastore, A., Patel, M., Patrizii, L., Perrotta, A., Petrov, A., Podgrudkov, D., Polini, A., Polukhina, N., Prota, A., Queiroz, F., Quercia, A., Ramos, S., Ratnikov, F., Reghunath, A., Riccio, M., Rodrigues Cavalcante, A.B., Roganova, T., Rovelli, T., Ruchayskiy, O., Ruf, T., Sabate Gilarte, M., Sanchez Galan, F., Santos Diaz, P., Schaffner, M., Schneider, O., Sekhniaidze, G., Serra, N., Shchedrina, T., Shchutska, L., Shevchenko, V., Shibuya, H., Shirobokov, S., Shmanin, E., Simone, S., Siroli, G.P., Sito, L., Sirri, G., Schmidt, J., Soares, G., Sohn, J.Y., Soto Sandoval, O.J., Spurio, M., Starkov, N., Tastet, J.L., Timiryasov, I., Tioukov, V., Tosi, N., Trippl, C., Ulloa Poblete, P.A., Ursov, E., Ustyuzhanin, A., Vankova-Kirilova, G., Vendeuvre, C., Visone, C., Vollhardt, A., Wanke, R., Yoon, C.S., Zamora Saa, J., Zaffaroni, E., and Zick, H.J.
- Subjects
Physics - Instrumentation and Detectors ,hep-ex ,Detectors and Experimental Techniques ,physics.ins-det ,Particle Physics - Experiment ,High Energy Physics - Experiment - Abstract
SND@LHC is a compact and stand-alone experiment designed to perform measurements with neutrinos produced at the LHC in the pseudo-rapidity region of ${7.2 < \eta < 8.4}$. The experiment is located 480 m downstream of the ATLAS interaction point, in the TI18 tunnel. The detector is composed of a hybrid system based on an 830 kg target made of tungsten plates, interleaved with emulsion and electronic trackers, also acting as an electromagnetic calorimeter, and followed by a hadronic calorimeter and a muon identification system. The detector is able to distinguish interactions of all three neutrino flavours, which allows probing the physics of heavy flavour production at the LHC in the very forward region. This region is of particular interest for future circular colliders and for very high energy astrophysical neutrino experiments. The detector is also able to search for the scattering of Feebly Interacting Particles. In its first phase, the detector will operate throughout LHC Run 3 and collect a total of 250 $\text{fb}^{-1}$., Comment: 57 pages. To be published in JINST
- Published
- 2022
4. Long-range contributions to double beta decay revisited
- Author
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Helo, J.C., Hirsch, M., and Ota, T.
- Published
- 2016
- Full Text
- View/download PDF
5. Searching for long-lived particles beyond the Standard Model at the Large Hadron Collider
- Author
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Alimena, J. Beacham, J. Borsato, M. Cheng, Y. Vidal, X.C. Cottin, G. Curtin, D. De Roeck, A. Desai, N. Evans, J.A. Knapen, S. Kraml, S. Lessa, A. Liu, Z. Mehlhase, S. Ramsey-Musolf, M.J. Russell, H. Shelton, J. Shuve, B. Verducci, M. Zurita, J. Adams, T. Adersberger, M. Alpigiani, C. Apresyan, A. Bainbridge, R.J. Batozskaya, V. Beauchesne, H. Benato, L. Berlendis, S. Bhal, E. Blekman, F. Borovilou, C. Boyd, J. Brau, B.P. Bryngemark, L. Buchmueller, O. Buschmann, M. Buttinger, W. Campanelli, M. Cesarotti, C. Chen, C. Cheng, H.-C. Cheong, S. Citron, M. Coccaro, A. Coco, V. Conte, E. Cormier, F. Corpe, L.D. Craig, N. Cui, Y. Dall'occo, E. Dallapiccola, C. Darwish, M.R. Davoli, A. Cosa, A.D. De Simone, A. Rose, L.D. Deppisch, F.F. Dey, B. Diamond, M.D. Dienes, K.R. Dildick, S. Döbrich, B. Drewes, M. Eich, M. Elsawy, M. Valle, A.E.D. Facini, G. Farina, M. Feng, J.L. Fischer, O. Flaecher, H.U. Foldenauer, P. Freytsis, M. Fuks, B. Galon, I. Gershtein, Y. Giagu, S. Giammanco, A. Gligorov, V.V. Golling, T. Grancagnolo, S. Gustavino, G. Haas, A. Hahn, K. Hajer, J. Hammad, A. Heinrich, L. Heisig, J. Helo, J.C. Hesketh, G. Hill, C.S. Hirsch, M. Hohlmann, M. Holmes, T. Hulsbergen, W. Huth, J. Ilten, P. Jacques, T. Jayatilaka, B. Jeng, G.-Y. Johns, K.A. Kaji, T. Kasieczka, G. Kats, Y. Kazana, M. Keller, H. Khlopov, M.Y. Kling, F. Kolberg, T.R. Kostiuk, I. Kuwertz, E.S. Kvam, A. Landsberg, G. Lanfranchi, G. Lara, I. Ledovskoy, A. Linthorne, D. Liu, J. Longarini, I. Lowette, S. Lubatti, H. Lutz, M. Luo, J. Mamuzić, J. Marinangeli, M. Mariotti, A. Marlow, D. McCullough, M. McDermott, K. Mermod, P. Milstead, D. Mishra-Sharma, S. Mitsou, V.A. Berlingen, J.M. Moortgat, F. Morandini, A. Morris, A.P. Morse, D.M. Mrenna, S. Nachman, B. Nemevsek, M. Nesti, F. Ohm, C. Pascoli, S. Pedro, K. Pena, C. Rodriguez, K.J.P. Piedra, J. Pinfold, J.L. Policicchio, A. Popara, G. Prisciandaro, J. Proffitt, M. Rauco, G. Redi, F. Reece, M. Hall, A.R. Sfar, H.R. Renner, S. Robinson, D. Roepe, A. Ronzani, M. Salvioni, E. Santra, A. Sawada, R. Scholtz, J. Schuster, P. Schwaller, P. Sebastiani, C. Sekmen, S. Selvaggi, M. Si, W. Soffi, L. Stolarski, D. Stuart, D. Iii, J.S. Sung, K. Taylor, W. Templ, S. Thomas, B. Torró-Pastor, E. Trocino, D. Trojanowski, S. Trovato, M. Tsai, Y. Tully, C.G. Vámi, T.Á. Vasquez, J.C. Sierra, C.V. Vellidis, K. Vermassen, B. Vit, M. Walker, D.G.E. Wang, X.-P. Watts, G. Xie, S. Yexley, M. Young, C. Yu, J.-H. Zalewski, P. Zhang, Y.
- Subjects
Physics::Instrumentation and Detectors - Abstract
Particles beyond the Standard Model (SM) can generically have lifetimes that are long compared to SM particles at the weak scale. When produced at experiments such as the Large Hadron Collider (LHC) at CERN, these long-lived particles (LLPs) can decay far from the interaction vertex of the primary proton-proton collision. Such LLP signatures are distinct from those of promptly decaying particles that are targeted by the majority of searches for new physics at the LHC, often requiring customized techniques to identify, for example, significantly displaced decay vertices, tracks with atypical properties, and short track segments. Given their non-standard nature, a comprehensive overview of LLP signatures at the LHC is beneficial to ensure that possible avenues of the discovery of new physics are not overlooked. Here we report on the joint work of a community of theorists and experimentalists with the ATLAS, CMS, and LHCb experiments-as well as those working on dedicated experiments such as MoEDAL, milliQan, MATHUSLA, CODEX-b, and FASER-to survey the current state of LLP searches at the LHC, and to chart a path for the development of LLP searches into the future, both in the upcoming Run 3 and at the high-luminosity LHC. The work is organized around the current and future potential capabilities of LHC experiments to generally discover new LLPs, and takes a signature-based approach to surveying classes of models that give rise to LLPs rather than emphasizing any particular theory motivation. We develop a set of simplified models; assess the coverage of current searches; document known, often unexpected backgrounds; explore the capabilities of proposed detector upgrades; provide recommendations for the presentation of search results; and look towards the newest frontiers, namely high-multiplicity 'dark showers', highlighting opportunities for expanding the LHC reach for these signals. © 2020 The Author(s). Published by IOP Publishing Ltd.
- Published
- 2020
6. Science with the Cherenkov Telescope Array
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Cascone, E., Valore, L., Vallania, P., Valentino, M., Vagnetti, F., Vagelli, V., Umana, G., Tsujimoto, S., Pujadas, I., Trifoglio, M., Trichard, C., Travnicek, P., Tovmassian, G., Tothill, N., Tosti, G., Torresi, E., Torres, D., Tornikoski, M., Tonev, D., Tomastik, J., Tokanai, F., Peixoto, C., Tluczykont, M., Tibaldo, L., Tian, W., Thoudam, S., Testa, V., Teshima, M., Terzic, T., Terrier, R., Terada, Y., Temnikov, P., Tejedor, L., Tayabaly, K., Tavernet, J., Tavecchio, F., Tavani, M., Tajima, H., Tagliaferri, G., Supanitsky, A., Suomijarvi, T., Straumann, U., Stratta, G., Stolarczyk, T., Stephan, M., Stefanik, S., Stawarz, Ł., Starling, R., Stanič, S., Stamerra, A., Sol, H., Slowikowska, A., Sliusar, V., Sitarek, J., Sironi, G., Sillanpää, A., Siejkowski, H., Sidoli, L., Shellard, R., Shalchi, A., Servillat, M., Sergijenko, O., Semikoz, D., Seitenzahl, I., Scuderi, S., Sciacca, E., Schwanke, U., Schussler, F., Schulz, A., Schovanek, P., Schoorlemmer, H., Schneider, M., Schlenstedt, S., Schioppa, E., Saturni, F., Satalecka, K., Sarkar, S., Santander, M., Sano, H., Sanguillon, M., Sangiorgi, P., Sandoval, A., Sandaker, H., Sánchez-Conde, M., Salina, G., Sakurai, S., Sakaki, N., Saito, T., Safi-Harb, S., Sadeh, I., Rulten, C., Rugliancich, A., Rudak, B., Rowell, G., Rovero, A., Rosado, J., Romeo, G., Romano, P., Rojas, G., Vázquez, J., Fernandez, G., Rodriguez, J., Rizi, V., Rivoire, S., Riquelme, M., Rieger, F., Rico, J., Richtler, T., Ribó, M., Ribeiro, D., Rhode, W., Rezaeian, A., Renaud, M., Reisenegger, A., Reimer, A., Reimer, O., Razzaque, S., Rainò, S., Quirrenbach, A., Queiroz, F., Pürckhauer, S., Punch, M., Pühlhofer, G., Prouza, M., Prokoph, H., Prokhorov, D., Principe, G., Prast, J., Prandini, E., Pozo, D., Polo, M., Pohl, M., Pita, S., Pisarski, A., Piano, G., Pfeifer, M., Peyaud, B., Petruk, O., Petrucci, P., Petrashyk, A., Persic, M., Perri, M., Pedaletti, G., Pech, M., PeEr, A., Parsons, R., Pareschi, G., Paredes, J., Naito, T., Nagayoshi, T., Nagataki, S., Nagai, A., Murase, K., Muraishi, H., Murach, T., Mundell, C., Mukherjee, R., Moulin, E., Morselli, A., Morris, P., Morlino, G., Mori, K., Morcuende-Parrilla, D., Moralejo, A., Montaruli, T., Mohrmann, L., Mohammed, M., Moderski, R., Mizuno, T., Mitchell, A., Mirzoyan, R., Mirabal, N., Minaya, I., Meyer, M., Mereghetti, S., Melandri, A., Medina, C., Mazin, D., Maxted, N., Maurin, G., Masuda, S., Masetti, N., Martínez, G., Martínez, M., Martin, P., Martí, J., Markoff, S., Marín, J., Marcowith, A., Mangano, S., Manganaro, M., Maneva, G., Mandat, D., Malaguti, G., Majumdar, P., Maier, G., Maccarone, M., Lyard, E., Luque-Escamilla, P., Lucarelli, F., Lu, C., López-Coto, R., López, M., Longo, F., Lombardi, S., Lohse, T., Lindfors, E., Limon, M., Lico, R., Lenain, J., De Oliveira, M., Lefaucheur, J., Lees, J., Leach, S., Blanc, O., Lapington, J., Lang, R., Lamanna, G., La Palombara, N., Kushida, J., Kuroda, H., Mezek, G., Kubo, H., Krauß, F., Krause, M., Kraus, M., Kosack, K., Komin, N., Kohri, K., Koch, B., Knödlseder, J., Knapp, J., Kisaka, S., Kimura, S., Kimeswenger, S., Kieda, D., Khélifi, B., Kazanas, D., Kawanaka, N., Katz, U., Katagiri, H., Karkar, S., Kaaret, P., Jurysek, J., Jung-Richardt, I., Jean, P., Jankowsky, D., Janecek, P., Jamrozy, M., Iwamura, Y., Ishio, K., Iori, M., Ioka, K., Iocco, F., Inoue, Y., Inoue, T., Inoue, S., Inome, Y., Inada, T., Iarlori, M., Hütten, M., Humensky, T., Hrupec, D., Hrabovsky, M., Hovatta, T., Horvath, P., Horns, D., Hörandel, J., Horan, D., Holder, J., Hofmann, W., Hnatyk, B., Hinton, J., Hermann, G., Helo, J., Heller, M., Hayashida, M., Hayashi, K., Hassan, T., Hardcastle, M., Hara, S., Hadasch, D., Gunji, S., Griffiths, S., Greenshaw, T., Green, A., Granot, J., Grandi, P., Graham, J., Götz, D., González, J., González, M., Gómez-Vargas, G., Goldoni, P., Godinovic, N., Gnatyk, R., Glicenstein, J., Giuliani, A., Giroletti, M., Giro, E., Giordano, F., Giommi, P., Giglietto, N., Giavitto, G., Gerard, L., Gaug, M., Gasparetto, T., Gaskins, J., Garczarczyk, M., López, R., Garcia, B., Gallant, Y., Gadola, A., Gabici, S., Füßling, M., Funk, S., Fukazawa, Y., Fujita, Y., Fruck, C., Coromina, L., Fortson, L., Fornasa, M., Fontaine, G., Fioretti, V., Filipovic, M., Fesquet, M., Ferrand, G., Fernández-Barral, A., Fernandez-Alonso, M., Fegan, S., Fedorova, E., Fasola, G., Farnier, C., Falcone, A., Falceta-Goncalves, D., Fairbairn, M., Evoli, C., Espinoza, C., Ernenwein, J., Elsässer, D., Ekoume, T., Einecke, S., Egberts, K., Eckner, C., Ebr, J., Dwarkadas, V., Dubus, G., Dravins, D., Drass, H., Doro, M., Dorner, D., Prester, D., Domínguez, A., Djannati-Ataï, A., Diebold, S., Dib, C., Díaz, C., Di Venere, L., Di Pierro, F., Di Girolamo, T., Della Volpe, D., Delgado, C., Del Santo, M., Deil, C., Covino, S., Cotter, G., Costantini, H., Costa, A., Cortina, J., Contreras, J., Conrad, J., Connaughton, V., Conforti, V., Colin, P., Colafrancesco, S., Coco, V., Cieślar, M., Chudoba, J., Christov, A., Chikawa, M., Chernyakova, M., Chen, X., Chen, A., Chaty, S., Chadwick, P., Cerruti, M., Cauz, D., Catalano, O., Catalani, F., Casanova, S., Carr, J., Carquín, E., Carosi, R., Carlile, C., Cárdenas, V., Caraveo, P., Caproni, A., Capitanio, F., Capalbi, M., Canestrari, R., Busetto, G., Burtovoi, A., Burton, M., Bulik, T., Bulgarelli, A., Bühler, R., Bugaev, V., Buckley, J., Buanes, T., Brunetti, G., Brun, P., Brill, A., Bregeon, J., Braiding, C., Böttcher, M., Bosnjak, Z., Bonnoli, G., Bonavolontà, C., Bonardi, A., Bonanno, G., Bolmont, J., Boisson, C., Blazek, J., Blanch, O., Biteau, J., Bissaldi, E., Biland, A., Bigongiari, C., Biasuzzi, B., Bertucci, B., Bernlöhr, K., Bernardos, M., Bernardini, E., Berge, D., Benbow, W., Belfiore, A., Becherini, Y., Bastieri, D., Barkov, M., Bamba, A., Ballet, J., Ballester, O., Balbo, M., Balazs, C., Backes, M., Ashley, M., Paoletti, R., Palatka, M., Palatiello, M., Paizis, A., Padovani, M., Oya, I., Otte, N., Ostrowski, M., Osborne, J., Orito, R., Orienti, M., Ong, R., Okumura, A., Okazaki, N., Ohm, S., Ohishi, M., Ohira, Y., Oakes, L., OBrien, P., Nozaki, S., Novosyadlyj, B., Nosek, D., Noda, K., Nishijima, K., Nikołajuk, M., Nieto, D., Niemiec, J., Nakamura, Y., Nakamori, T., Asano, K., Arrabito, L., Arqueros, F., Armstrong, T., Araya, M., Aramo, C., Antolini, E., Ambrosi, G., Amato, E., Alispach, C., Alfaro, J., Alfaro, R., Agudo, I., Zhdanov, V.I., Zdziarski, A.A., Williams, D.A., Watson, J.J., Ward, J.E., Wagner, S.J., Vettolani, G.P., Varner, G.S., Torres, D.F., Todero Peixoto, C.J., Tejedor, L.A., Tavernet, J.-P., Supanitsky, A.D., Shellard, R.C., Rovero, A.C., Vázquez, J.J., Rezaeian, A.H., Parsons, R.D., Paredes, J.M., Osborne, J.P., Ong, R.A., De Souza, V., De Persio, F., De Palma, F., Wilhelmi, E., De Naurois, M., De Lucia, M., De Luca, A., De Lotto, B., Lopez, R., De La Calle, I., Pino, E., De Franco, A., De Cesare, G., Anjos, R., De Angelis, A., Dazzi, F., Dawson, B., Davids, I., Daniel, M., DUrso, D., DAvanzo, P., DAmmando, F., DAì, A., Cumani, P., Cuevas, O., Cuadra, J., Crocker, R., Minaya, I.A., Maccarone, M.C., Luque-Escamilla, P.L., Lenain, J.-P., De Oliveira M.A., Leigui, Lees, J.-P., Lang, R.G., Kukec Mezek, G., Kieda, D.B., Humensky, T.B., De Los Reyes Lopez, R., De Gouveia Dal Pino, E.M., Contreras, J.L., Chaves, R.C., Brown, A.M., Schioppa, E.J., Saturni, F.G., Bernardini, M.G., Barrio, J.A., Barres De Almeida, U., Antonelli, L.A., Amans, J.-P., Alves Batista, R., Al Samarai, I., Acharya, B.S., Helo, J.C., Hardcastle, M.J., Green, A.J., González, J.M., González, M.M., Glicenstein, J.-F., Ernenwein, J.-P., Ekoume, T.R., Dwarkadas, V.V., Dominis Prester, D., Chaves, R., Brown, A., Bernardini, M., Barrio, J., De Almeida, U., Antonelli, L., Amans, J., Batista, R., Samarai, I., Acharya, B., Consortium, The Cherenkov, Zorn, J., Ziegler, A., Zhdanov, V., Zechlin, H., Zech, A., Zdziarski, A., Zavrtanik, D., Zavrtanik, M., Zanin, R., Zandanel, F., Zampieri, L., Zaharijas, G., Zacharias, M., Yoshikoshi, T., Yoshiike, S., Yoshida, T., Yang, L., Yanagita, S., Yamazaki, R., Yamamoto, T., Wood, M., Wischnewski, R., Williams, D., Will, M., Wilcox, P., Wierzcholska, A., White, R., White, M., Werner, F., Watson, J., Warren, D., Ward, J., Walter, R., Wagner, R., Wagner, S., Vuillaume, T., Vrastil, M., Vorobiov, S., Vollhardt, A., Voelk, H., Villanueva, J., Vigorito, C., Viana, A., Vettolani, G., Verzi, V., Vergani, S., Veres, P., Vercellone, S., Vega, A., Vecchi, M., Acosta, M., Vassiliev, V., Vasileiadis, G., Varner, G., Vandenbroucke, J., Van Eldik, C., Cherenkov Telescope Array Consortium, The, Acharya, B. S., Agudo, I., Al Samarai, I., Alfaro, R., Alfaro, J., Alispach, C., Alves Batista, R., Amans, J. -P., Amato, E., Ambrosi, G., Antolini, E., Antonelli, L. A., Aramo, C., Araya, M., Armstrong, T., Arqueros, F., Arrabito, L., Asano, K., Ashley, M., Backes, M., Balazs, C., Balbo, M., Ballester, O., Ballet, J., Bamba, A., Barkov, M., Barres de Almeida, U., Barrio, J. A., Bastieri, D., Becherini, Y., Belfiore, A., Benbow, W., Berge, D., Bernardini, E., Bernardini, M. G., Bernardos, M., Bernlöhr, K., Bertucci, B., Biasuzzi, B., Bigongiari, C., Biland, A., Bissaldi, E., Biteau, J., Blanch, O., Blazek, J., Boisson, C., Bolmont, J., Bonanno, G., Bonardi, A., Bonavolontà, C., Bonnoli, G., Bosnjak, Z., Böttcher, M., Braiding, C., Bregeon, J., Brill, A., Brown, A. M., Brun, P., Brunetti, G., Buanes, T., Buckley, J., Bugaev, V., Bühler, R., Bulgarelli, A., Bulik, T., Burton, M., Burtovoi, A., Busetto, G., Canestrari, R., Capalbi, M., Capitanio, F., Caproni, A., Caraveo, P., Cárdenas, V., Carlile, C., Carosi, R., Carquín, E., Carr, J., Casanova, S., Cascone, E., Catalani, F., Catalano, O., Cauz, D., Cerruti, M., Chadwick, P., Chaty, S., Chaves, R. C. G., Chen, A., Chen, X., Chernyakova, M., Chikawa, M., Christov, A., Chudoba, J., Cieślar, M., Coco, V., Colafrancesco, S., Colin, P., Conforti, V., Connaughton, V., Conrad, J., Contreras, J. L., Cortina, J., Costa, A., Costantini, H., Cotter, G., Covino, S., Crocker, R., Cuadra, J., Cuevas, O., Cumani, P., D'Aì, A., D'Ammando, F., D'Avanzo, P., D'Urso, D., Daniel, M., Davids, I., Dawson, B., Dazzi, F., De Angelis, A., de Cássia dos Anjos, R., De Cesare, G., De Franco, A., de Gouveia Dal Pino, E. M., de la Calle, I., de los Reyes Lopez, R., De Lotto, B., De Luca, A., De Lucia, M., de Naurois, M., de Oña Wilhelmi, E., De Palma, F., De Persio, F., de Souza, V., Deil, C., Del Santo, M., Delgado, C., della Volpe, D., Di Girolamo, T., Di Pierro, F., Di Venere, L., Díaz, C., Dib, C., Diebold, S., Djannati-Ataï, A., Domínguez, A., Dominis Prester, D., Dorner, D., Doro, M., Drass, H., Dravins, D., Dubus, G., Dwarkadas, V. V., Ebr, J., Eckner, C., Egberts, K., Einecke, S., Ekoume, T. R. N., Elsässer, D., Ernenwein, J. -P., Espinoza, C., Evoli, C., Fairbairn, M., Falceta-Goncalves, D., Falcone, A., Farnier, C., Fasola, G., Fedorova, E., Fegan, S., Fernandez-Alonso, M., Fernández-Barral, A., Ferrand, G., Fesquet, M., Filipovic, M., Fioretti, V., Fontaine, G., Fornasa, M., Fortson, L., Freixas Coromina, L., Fruck, C., Fujita, Y., Fukazawa, Y., Funk, S., Füßling, M., Gabici, S., Gadola, A., Gallant, Y., Garcia, B., Garcia López, R., Garczarczyk, M., Gaskins, J., Gasparetto, T., Gaug, M., Gerard, L., Giavitto, G., Giglietto, N., Giommi, P., Giordano, F., Giro, E., Giroletti, M., Giuliani, A., Glicenstein, J. -F., Gnatyk, R., Godinovic, N., Goldoni, P., Gómez-Vargas, G., González, M. M., González, J. M., Götz, D., Graham, J., Grandi, P., Granot, J., Green, A. J., Greenshaw, T., Griffiths, S., Gunji, S., Hadasch, D., Hara, S., Hardcastle, M. J., Hassan, T., Hayashi, K., Hayashida, M., Heller, M., Helo, J. C., Hermann, G., Hinton, J., Hnatyk, B., Hofmann, W., Holder, J., Horan, D., Hörandel, J., Horns, D., Horvath, P., Hovatta, T., Hrabovsky, M., Hrupec, D., Humensky, T. B., Hütten, M., Iarlori, M., Inada, T., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Iocco, F., Ioka, K., Iori, M., Ishio, K., Iwamura, Y., Jamrozy, M., Janecek, P., Jankowsky, D., Jean, P., Jung-Richardt, I., Jurysek, J., Kaaret, P., Karkar, S., Katagiri, H., Katz, U., Kawanaka, N., Kazanas, D., Khélifi, B., Kieda, D. B., Kimeswenger, S., Kimura, S., Kisaka, S., Knapp, J., Knödlseder, J., Koch, B., Kohri, K., Komin, N., Kosack, K., Kraus, M., Krause, M., Krauß, F., Kubo, H., Kukec Mezek, G., Kuroda, H., Kushida, J., La Palombara, N., Lamanna, G., Lang, R. G., Lapington, J., Le Blanc, O., Leach, S., Lees, J. -P., Lefaucheur, J., Leigui de Oliveira, M. A., Lenain, J. -P., Lico, R., Limon, M., Lindfors, E., Lohse, T., Lombardi, S., Longo, F., López, M., López-Coto, R., Lu, C. -C., Lucarelli, F., Luque-Escamilla, P. L., Lyard, E., Maccarone, M. C., Maier, G., Majumdar, P., Malaguti, G., Mandat, D., Maneva, G., Manganaro, M., Mangano, S., Marcowith, A., Marín, J., Markoff, S., Martí, J., Martin, P., Martínez, M., Martínez, G., Masetti, N., Masuda, S., Maurin, G., Maxted, N., Mazin, D., Medina, C., Melandri, A., Mereghetti, S., Meyer, M., Minaya, I. A., Mirabal, N., Mirzoyan, R., Mitchell, A., Mizuno, T., Moderski, R., Mohammed, M., Mohrmann, L., Montaruli, T., Moralejo, A., Morcuende-Parrilla, D., Mori, K., Morlino, G., Morris, P., Morselli, A., Moulin, E., Mukherjee, R., Mundell, C., Murach, T., Muraishi, H., Murase, K., Nagai, A., Nagataki, S., Nagayoshi, T., Naito, T., Nakamori, T., Nakamura, Y., Niemiec, J., Nieto, D., Nikołajuk, M., Nishijima, K., Noda, K., Nosek, D., Novosyadlyj, B., Nozaki, S., O'Brien, P., Oakes, L., Ohira, Y., Ohishi, M., Ohm, S., Okazaki, N., Okumura, A., Ong, R. A., Orienti, M., Orito, R., Osborne, J. P., Ostrowski, M., Otte, N., Oya, I., Padovani, M., Paizis, A., Palatiello, M., Palatka, M., Paoletti, R., Paredes, J. M., Pareschi, G., Parsons, R. D., Pe'Er, A., Pech, M., Pedaletti, G., Perri, M., Persic, M., Petrashyk, A., Petrucci, P., Petruk, O., Peyaud, B., Pfeifer, M., Piano, G., Pisarski, A., Pita, S., Pohl, M., Polo, M., Pozo, D., Prandini, E., Prast, J., Principe, G., Prokhorov, D., Prokoph, H., Prouza, M., Pühlhofer, G., Punch, M., Pürckhauer, S., Queiroz, F., Quirrenbach, A., Rainò, S., Razzaque, S., Reimer, O., Reimer, A., Reisenegger, A., Renaud, M., Rezaeian, A. H., Rhode, W., Ribeiro, D., Ribó, M., Richtler, T., Rico, J., Rieger, F., Riquelme, M., Rivoire, S., Rizi, V., Rodriguez, J., Rodriguez Fernandez, G., Rodríguez Vázquez, J. J., Rojas, G., Romano, P., Romeo, G., Rosado, J., Rovero, A. C., Rowell, G., Rudak, B., Rugliancich, A., Rulten, C., Sadeh, I., Safi-Harb, S., Saito, T., Sakaki, N., Sakurai, S., Salina, G., Sánchez-Conde, M., Sandaker, H., Sandoval, A., Sangiorgi, P., Sanguillon, M., Sano, H., Santander, M., Sarkar, S., Satalecka, K., Saturni, F. G., Schioppa, E. J., Schlenstedt, S., Schneider, M., Schoorlemmer, H., Schovanek, P., Schulz, A., Schussler, F., Schwanke, U., Sciacca, E., Scuderi, S., Seitenzahl, I., Semikoz, D., Sergijenko, O., Servillat, M., Shalchi, A., Shellard, R. C., Sidoli, L., Siejkowski, H., Sillanpää, A., Sironi, G., Sitarek, J., Sliusar, V., Slowikowska, A., Sol, H., Stamerra, A., Stanič, S., Starling, R., Stawarz, Ł., Stefanik, S., Stephan, M., Stolarczyk, T., Stratta, G., Straumann, U., Suomijarvi, T., Supanitsky, A. D., Tagliaferri, G., Tajima, H., Tavani, M., Tavecchio, F., Tavernet, J. -P., Tayabaly, K., Tejedor, L. A., Temnikov, P., Terada, Y., Terrier, R., Terzic, T., Teshima, M., Testa, V., Thoudam, S., Tian, W., Tibaldo, L., Tluczykont, M., Todero Peixoto, C. J., Tokanai, F., Tomastik, J., Tonev, D., Tornikoski, M., Torres, D. F., Torresi, E., Tosti, G., Tothill, N., Tovmassian, G., Travnicek, P., Trichard, C., Trifoglio, M., Troyano Pujadas, I., Tsujimoto, S., Umana, G., Vagelli, V., Vagnetti, F., Valentino, M., Vallania, P., Valore, L., van Eldik, C., Vandenbroucke, J., Varner, G. S., Vasileiadis, G., Vassiliev, V., Vázquez Acosta, M., Vecchi, M., Vega, A., Vercellone, S., Veres, P., Vergani, S., Verzi, V., Vettolani, G. P., Viana, A., Vigorito, C., Villanueva, J., Voelk, H., Vollhardt, A., Vorobiov, S., Vrastil, M., Vuillaume, T., Wagner, S. J., Wagner, R., Walter, R., Ward, J. E., Warren, D., Watson, J. J., Werner, F., White, M., White, R., Wierzcholska, A., Wilcox, P., Will, M., Williams, D. A., Wischnewski, R., Wood, M., Yamamoto, T., Yamazaki, R., Yanagita, S., Yang, L., Yoshida, T., Yoshiike, S., Yoshikoshi, T., Zacharias, M., Zaharijas, G., Zampieri, L., Zandanel, F., Zanin, R., Zavrtanik, M., Zavrtanik, D., Zdziarski, A. A., Zech, A., Zechlin, H., Zhdanov, V. I., Ziegler, A., Zorn, J., Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Département d'Astrophysique (ex SAP) (DAP), 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, Institut de Physique Nucléaire d'Orsay (IPNO), 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 de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), 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 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), 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 Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Département de Physique des Particules (ex SPP) (DPP), Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), CTA Consortium, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astrofisico di Arcetri (OAA), Istituto Nazionale di Astrofisica (INAF), Istituto Nazionale di Fisica Nucleare, Sezione di Perugia (INFN, Sezione di Perugia), Istituto Nazionale di Fisica Nucleare (INFN), Departamento de Física Atómica, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), College of Science and Engineering, Aoyama Gakuin University (AGU), 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), Instituto de Fisica Corpuscular (IFIC), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)-Universitat de València (UV), 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 de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Istituto di Radioastronomia [Bologna] (IRA), University of Naples Federico II = Università degli studi di Napoli Federico II, Max-Planck-Institut für Kernphysik (MPIK), Max-Planck-Gesellschaft, INAF - Osservatorio Astronomico di Padova (OAPD), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), ISDC Data Centre for Astrophysics, Université de Genève = University of Geneva (UNIGE), Département de Physique Nucléaire et Corpusculaire [Genève] (DPNC), Universities Space Research Association (USRA), Universidad Complutense de Madrid = Complutense University of Madrid [Madrid] (UCM), INAF - Osservatorio Astronomico di Brera (OAB), Istituto di Astrofisica Spaziale e Fisica cosmica - Roma (IASF-Roma), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Dipartimento di Fı'sica Generale dell'Università, Istituto Nazionale di Fisica Nucleare, sezione di Bari (INFN, sezione di Bari), 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, Institut für Theoretische Physik und Astrophysik [Würzburg], Julius-Maximilians-Universität Würzburg (JMU), Jodrell Bank Centre for Astrophysics (JBCA), University of Manchester [Manchester], Institut des sciences du végétal (ISV), Centre National de la Recherche Scientifique (CNRS), Institut de Física d’Altes Energies [Barcelone] (IFAE), Universitat Autònoma de Barcelona (UAB), Agenzia Spaziale Italiana (ASI), 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), Texas A&M University System, Istituto di Astrofisica Spaziale e Fisica cosmica - Bologna (IASF-Bo), Department of Natural Sciences [Ra'anana}, Open University of Israël, University of Hertfordshire [Hatfield] (UH), Deutsches Elektronen-Synchrotron [Zeuthen] (DESY), Helmholtz-Gemeinschaft = Helmholtz Association, Solar-Terrestrial Environment Laboratory [Nagoya] (STEL), Nagoya University, Laboratoire de l'Accélérateur Linéaire (LAL), Radboud University [Nijmegen], Metsähovi Radio Observatory, Aalto University, Humboldt University Of Berlin, The University of Tokyo (UTokyo), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Department of Physics and Astronomy [Iowa City], University of Iowa [Iowa City], Erlangen Centre for Astroparticle Physics (ECAP), Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Max-Planck-Institut für Extraterrestrische Physik (MPE), INAF- Milano, Università degli Studi di Udine - University of Udine [Italie], Dipartimento di Fisica [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Astronomical Institute Anton Pannekoek (AI PANNEKOEK), University of Amsterdam [Amsterdam] (UvA), Istituto di Astrofisica Spaziale e Fisica Cosmica - Milano (IASF-MI), NASA Goddard Space Flight Center (GSFC), Institute for Physical Research (IPR), National Academy of Sciences of the Republic of Armenia [Yerevan] (NAS RA), Dept. of Physics, University of Wisconsin-Madison, Infrared Processing and Analysis Center (IPAC), California Institute of Technology (CALTECH), KEK (High energy accelerator research organization), Department of Physics [Tokyo], Tokyo Institure of Technology, Istituto di Radioastronomia INAF, Department of Physics and Astronomy [Leicester], University of Leicester, Departament d'Astronomia i Meteorologia [Barcelona] (DAM), Universitat de Barcelona (UB), IEEC-CSIC, INAF - Osservatorio Astronomico di Trieste (OAT), DLR Institut für Physik der Atmosphäre (IPA), Deutsches Zentrum für Luft- und Raumfahrt [Oberpfaffenhofen-Wessling] (DLR), Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Centro de Ciencias de la Atmosfera [Mexico], Universidad Nacional Autónoma de México = National Autonomous University of Mexico (UNAM), Technische Universität Dortmund [Dortmund] (TU), Institut de Ciencies del Cosmos (ICCUB), International Agency for Cancer Research (IACR), School of Chemistry and Physics, University of Adelaide, Copernicus Astronomical Center of the Polish Academy of Sciences (CAMK), Polish Academy of Sciences (PAN), Centro de Ciencias Aplicadas y Desarrollo Tecnológico, University of Oxford, AGH University of Science and Technology [Krakow, PL] (AGH UST), Dipartimento di Fisica 'Giuseppe Occhialini' = Department of Physics 'Giuseppe Occhialini' [Milano-Bicocca], Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB), 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), Department of Plant Sciences [Univ California Davis] (Plant - UC Davis), University of California [Davis] (UC Davis), University of California (UC)-University of California (UC), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institute for Climate and Atmospheric Science [Leeds] (ICAS), School of Earth and Environment [Leeds] (SEE), University of Leeds-University of Leeds, Antarctic Research a European Network for Astrophysics (ARENA), Institute of Atmospheric Physics [Prague] (IAP), Czech Academy of Sciences [Prague] (CAS), University of California (UC), Laboratoire d'études en Géophysique et océanographie spatiales (LEGOS), Instituto Nacional de Técnica Aeroespacial (INTA), Lawrence Berkeley National Laboratory [Berkeley] (LBNL), Istituto Nazionale di Fisica Nucleare, Sezione di Trieste (INFN, Sezione di Trieste), Jozef Stefan Institute [Ljubljana] (IJS), Istituto di Astrofisica Spaziale e Fisica cosmica - Palermo (IASF-Pa), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS), National Institute for Nuclear Physics (INFN), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Consejo Superior de Investigaciones Científicas [Spain] (CSIC)-Universitat de València (UV), University of Naples Federico II, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), University of Geneva [Switzerland], Université de Genève (UNIGE), Complutense University of Madrid (UCM), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Bureau d'Économie Théorique et Appliquée (BETA), Institut National de la Recherche Agronomique (INRA)-Université de Strasbourg (UNISTRA)-Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut für Theoretische Physik und Astrophysik [Wurzburg], Julius-Maximilians-Universität Würzburg [Wurtzbourg, Allemagne] (JMU), Jodrell Bank Centre for Astrophysics, Universitat Autònoma de Barcelona [Barcelona] (UAB), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Helmholtz-Gemeinschaft, Radboud university [Nijmegen], Humboldt Universität zu Berlin, The University of Tokyo, Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' [Rome], National Academy of Sciences of Armenia, CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA, CALTECH, Ctr Infrared Proc & Anal, Pasadena, High Energy Accelerator Research Organization (KEK), University of Tsukuba, Universidad Nacional Autónoma de México (UNAM), University of Oxford [Oxford], Dip. di Fisica 'Occhialini' - Università degli Studi di Milano-Bicocca Piazza della Scienza, Department of Plant Sciences [Davis, CA], University of California-University of California, INAF-OAB, Czech Academy of Sciences [Prague] (ASCR), University of California, Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire Midi-Pyrénées (OMP), Observatoire de Paris - Site de Meudon (OBSPM), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Département de Physique des Particules (ex SPP) (DPhP), PSL Research University (PSL)-PSL Research University (PSL)-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)-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 Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), 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), Humboldt-Universität zu Berlin, Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome], Università degli Studi di Milano-Bicocca [Milano] (UNIMIB), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), 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, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)
- Subjects
propagation [photon] ,photon: propagation ,Cherenkov Telescope Array ,magnetic field ,01 natural sciences ,thermal ,Observatory ,formation [star] ,HESS ,site ,cluster ,ddc:522.6862 ,media_common ,pulsar ,High Energy Astrophysical Phenomena (astro-ph.HE) ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Astrophysics::Instrumentation and Methods for Astrophysics ,star: formation ,relativistic [jet] ,CERN LHC Coll ,binary [gamma ray] ,cosmic radiation [electron] ,axion-like particles ,violation ,Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena ,performance ,Astrophysics and Astronomy ,bepress|Physical Sciences and Mathematics|Physics ,media_common.quotation_subject ,Astrophysics::High Energy Astrophysical Phenomena ,burst [gamma ray] ,Higgs particle ,invariance: Lorentz ,X-ray ,ionization ,supernova ,cosmic radiation: UHE ,Lorentz [invariance] ,AGN ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,CTA ,010308 nuclear & particles physics ,Astronomy ,sensitivity ,Universe ,angular resolution ,gamma ray: VHE ,quantum gravity ,galaxy ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,HAWC ,Computer science ,VHE [gamma ray] ,feedback ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,ultraviolet ,black hole ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,cloud ,acceleration [hadron] ,neutron star ,010303 astronomy & astrophysics ,astro-ph.HE ,radio wave ,COSMIC cancer database ,imaging ,observatory ,Supernova ,annihilation ,bepress|Physical Sciences and Mathematics|Physics|Elementary Particles and Fields and String Theory ,infrared ,Particle Physics - Experiment ,accelerator ,WIMP ,Ground-based gamma-ray astronomy ,Dark matter ,UHE [cosmic radiation] ,FOS: Physical sciences ,gamma ray: burst ,GLAST ,dark matter ,jet: relativistic ,blazar ,target ,hadron: acceleration ,0103 physical sciences ,522.6862 ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,TeV gamma-ray astronomy ,hep-ex ,Gravitational wave ,background ,gravitational radiation ,electron: cosmic radiation ,gamma ray: binary ,redshift ,[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,monitoring ,Sky ,bepress|Physical Sciences and Mathematics|Astrophysics and Astronomy ,astro-ph.IM - Abstract
Singapur : WORLD SCIENTIFIC, Cherenkov Telescope Array (CTA) 211 pp. (2017). doi:10.1142/10986, The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. The scientific potential of CTA is extremely broad: from understanding the role of relativistic cosmic particles to the search for dark matter. CTA is an explorer of the extreme universe, probing environments from the immediate neighbourhood of black holes to cosmic voids on the largest scales. Covering a huge range in photon energy from 20 GeV to 300 TeV, CTA will improve on all aspects of performance with respect to current instruments. The observatory will operate arrays on sites in both hemispheres to provide full sky coverage and will hence maximize the potential for the rarest phenomena such as very nearby supernovae, gamma-ray bursts or gravitational wave transients. With 99 telescopes on the southern site and 19 telescopes on the northern site, flexible operation will be possible, with sub-arrays available for specific tasks. CTA will have important synergies with many of the new generation of major astronomical and astroparticle observatories. Multi-wavelength and multi-messenger approaches combining CTA data with those from other instruments will lead to a deeper understanding of the broad-band non-thermal properties of target sources. The CTA Observatory will be operated as an open, proposal-driven observatory, with all data available on a public archive after a pre-defined proprietary period. Scientists from institutions worldwide have combined together to form the CTA Consortium. This Consortium has prepared a proposal for a Core Programme of highly motivated observations. The programme, encompassing approximately 40% of the available observing time over the first ten years of CTA operation, is made up of individual Key Science Projects (KSPs), which are presented in this document., Published by WORLD SCIENTIFIC, Singapur
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