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Grimoire1 of the MAGIC telescopes [PDF]
12th Cosmic Ray International Seminar - CRIS 2022 12/09/2022 - 16/09/2022 Napoli, Italy, 2023 The MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov) telescopes are a system of two Cherenkov telescopes located on the Canary island of La Palma (Spain), at the Roque de Los Muchachos Observatory, and operating in stereo mode since 2009. Their design and dedicated trigger system allows to reach an energy threshold of 50 GeV, which can be lowered ...M. Manganaroopenalex +2 more sourcesThe MAGIC Telescope - prospects for GRB research [PDF]
Astronomy and Astrophysics Supplement Series, 1999 The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) Telescope collaboration is constructing a large Cherenkov telescope (17 m diameter) for the exploration of the gamma-ray energy regime above 10 GeV with high sensitivity. One of the highlights in the science program of this future observatory are the plans for fast follow-up observations of of ...D. Petryopenalex +3 more sourcesTechnical Performance of the MAGIC Telescopes [PDF]
, 2009 The MAGIC-I telescope is the largest single-dish Imaging Atmospheric Cherenkov telescope in the world. A second telescope, MAGIC-II, will operate in coincidence with MAGIC-I in stereoscopic mode. MAGIC-II is a clone of MAGIC-I, but with a number of significant improvements, namely a highly pixelized camera with a wider trigger area, improved optical ...J. Cortina, F. Göebel, Thomas Schweizer +5 more sourcesGRB Observations with the MAGIC Telescopes [PDF]
, 2009 Contribution to the 31st ICRC, Lodz, Poland, July ...M. Garczarczyk, M. Gaug, A. Antonelli, D. Bastieri, J. Becerra González, S. Covino, A. La Barbera, A. Carosi, N. Galante, F. Longo, V. Scapin, S. Spiro +11 moreopenalex +3 more sourcesProtons Spectrum from MAGIC Telescopes data [PDF]
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021), 2021 Imaging Atmospheric Cherenkov telescopes (IACTs) are designed to detect cosmic gamma rays. As a by-product, IACTs detect Cherenkov flashes generated by millions of hadronic air showers every night. We present the proton energy spectrum from several hundred GeV to several hundred TeV, retrieved from the hadron induced showers detected by the MAGIC ...Temnikov, Petar, VERGUILOV, Vassil, Maneva, Galina, Mirzoyan, Razmik, Baack, Dominik, Acciari, Victor A., Ansoldi, Stefano, Antonelli, Lucio Angelo, Arbet Engels, Axel, Artero, Manuel, Asano, Katsuaki, Babić, Ana, Baquero, Andrés, Barres de Almeida, Ulisses, Barrio, Juan Abel, Batković, Ivana, Becerra González, Josefa, Bednarek, Wlodek, Bellizzi, Lorenzo, Bernardini, Elisa, Bernardos, Maria-Isabel, Berti, Alessio, Besenrieder, Jürgen, Bhattacharyya, Wrijupan, Bigongiari, Ciro, Biland, Adrian, Blanch, Oscar, Bökenkamp, Hendrik, Bonnoli, Giacomo, Bošnjak, Željka, Busetto, Giovanni, Carosi, Roberto, Ceribella, Giovanni, Cerruti, Matteo, Chai, Yating, Chilingarian, Ashot Agassi, Cikota, Stefan, Colak, Sidika Merve, Colombo, Eduardo, Contreras, Jose Luis, Cortina, Juan, Covino, Stefano, D'Amico, Giacomo, D'Elia, Valerio, Da Vela, Paolo, Dazzi, Francesco, De Angelis, Alessandro, De Lotto, Barbara, Delfino, Manuel, Delgado, Jordi, Delgado Mendez, Carlos, Depaoli, Davide, Di Pierro, Federico, Di Venere, Leonardo, Do Souto Espiñeira, Elia, Dominis Prester, Dijana, Donini, Alice, Dorner, Daniela, Doro, Michele, Elsaesser, Dominik, Fallah Ramazani, Vandad, Fattorini, Alicia, Fonseca, Maria Victoria, Font, Lluis, Fruck, Christian, Fukami, Satoshi, Fukazawa, Yasushi, García López, Ramon J., Garczarczyk, Markus, Gasparyan, Sargis, Gaug, Markus, Giglietto, Nicola, Giordano, Francesco, Gliwny, Pawel, Godinović, Nikola, Green, David, Green, Jarred Gershon, Hadasch, Daniela, Hahn, Alexander, Heckmann, Lea, Herrera, Javier, Hoang, John, Hrupec, Dario, Hütten, Moritz, Inada, Tomohiro, Ishio, Kazuma, Iwamura, Yuki, Jiménez Martínez, Irene, Jormanainen, Jenni, Jouvin, Léa, Karjalainen, Marie, Kerszberg, Daniel, Kobayashi, Yukiho, Kubo, Hidetoshi, Kushida, Junko, Lamastra, Alessandra, LELAS, Damir, Leone, Francesco, Lindfors, Elina, Linhoff, Lena, Lombardi, Saverio, Longo, Francesco, López-Coto, Rubén, López-Moya, Marcos, López-Oramas, Alicia, Loporchio, Serena, Machado de Oliveira Fraga, Bernardo, Maggio, Camilla, Majumdar, Pratik, MAKARIEV, Martin, Mallamaci, Manuela, Manganaro, Marina, Mannheim, Karl, Maraschi, Laura, Mariotti, Mosè, Martínez, Manel, Mazin, Daniel, Menchiari, Stefano, Mender, Simone, Mićanović, Saša, Miceli, Davide, Miener, Tjark, Miranda, Jose Miguel, Molina, Edgar, Moralejo, Abelardo, Morcuende, Daniel, Moreno, Victoria, Moretti, Elena, Nakamori, Takeshi, Nava, Lara, Neustroev, Vitaly, Nigro, Cosimo, Nilsson, Kari, Nishijima, Kyoshi, Noda, Koji, Nozaki, Seiya, Ohtani, Yoshiki, Oka, Tomohiko, Otero-Santos, Jorge, Paiano, Simona, Palatiello, Michele, Paneque, David, Paoletti, Riccardo, Paredes, Josep M., Pavletić, Lovro, Peñil, Pablo, Persic, Massimo, Pihet, Marine, Prada Moroni, Pier Giorgio, Prandini, Elisa, Priyadarshi, Chaitanya, Puljak, Ivica, Rhode, Wolfgang, Ribó, Marc, Rico, Javier, Righi, Chiara, Rugliancich, Andrea, Sahakyan, Narek, Saito, Takayuki, Sakurai, Shunsuke, Satalecka, Konstancja, Saturni, Francesco Gabriele, Schleicher, Bernd, Schmidt, Kevin, Schweizer, Thomas, Sitarek, Julian, Šnidarić, Iva, Sobczyńska, Dorota, Spolon, Alessia, Stamerra, Antonio, Strišković, Jelena, Strom, Derek, Strzys, Marcel, Suda, Yusuke, Surić, Tihomir, Takahashi, Mitsunari, Takeishi, Ryuji, Tavecchio, Fabrizio, Terzić, Tomislav, Teshima, Masahiro, Tosti, Luca, Truzzi, Stefano, Tutone, Antonio, Ubach, Santiago, van Scherpenberg, Juliane, Vanzo, Gaia, VAZQUEZ ACOSTA, Monica, Ventura, Sofia, Vigorito, Carlo Francesco, Vitale, Vincenzo, Vovk, Ievgen, Will, Martin, Wunderlich, Carolin, Yamamoto, Tokonatsu, Zarić, Darko +194 moreopenaire +4 more sourcesIntensity interferometry with the MAGIC telescopes [PDF]
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021), 2021 Due to their large mirror size, fast response to single photons, sensitivity and telescope baselines in the order of 100 m, Imaging Atmospheric Cherenkov Telescopes are ideally suited to perform intensity interferometry observations. In 2019 a test readout setup was installed in the two 17-m diameter MAGIC telescopes to allow performing interferometry ...Delgado Mendez C., Acciari V. A., Colombo E., Cortina J., Diaz C., Fink D., Fiori M., Hassan T., Jimenez-Martinez I., Lyard E., Mangano S., Mirzoyan R., Naleto G., Njoh Ekoume T., Polo M., Produit N., Rodriguez J. J., Schweizer T., Walter R., Wunderlich C., Zampieri L., Ansoldi S., Antonelli L. A., Arbet Engels A., Artero M., Asano K., Baack D., Babic A., Baquero A., Barres de Almeida U., Barrio J. A., Batkovic I., Becerra Gonzalez J., Bednarek W., Bellizzi L., Bernardini E., Bernardos M., Berti A., Besenrieder J., Bhattacharyya W., Bigongiari C., Biland A., Blanch O., Bokenkamp H., Bonnoli G., Bosnjak Z., Busetto G., Carosi R., Ceribella G., Cerruti M., Chai Y., Chilingarian A., Cikota S., Colak S. M., Contreras J. L., Covino S., D'Amico G., D'Elia V., Da Vela P., Dazzi F., De Angelis A., De Lotto B., Delfino M., Delgado J., Depaoli D., Di Pierro F., Di Venere L., Do Souto Espineira E., Dominis Prester D., Donini A., Dorner D., Doro M., Elsaesser D., Fallah Ramazani V., Fattorini A., Fonseca M. V., Font L., Fruck C., Fukami S., Fukazawa Y., Garcia Lopez R. J., Garczarczyk M., Gasparyan S., Gaug M., Giglietto N., Giordano F., Gliwny P., Godinovic N., Green J. G., Green D., Hadasch D., Hahn A., Heckmann L., Herrera J., Hoang J., Hrupec D., Hutten M., Inada T., Ishio K., Iwamura Y., Jimenez Martinez I., Jormanainen J., Jouvin L., Karjalainen M., Kerszberg D., Kobayashi Y., Kubo H., Kushida J., Lamastra A., Lelas D., Leone F., Lindfors E., Linhoff L., Lombardi S., Longo F., Lopez-Coto R., Lopez-Moya M., Lopez-Oramas A., Loporchio S., Machado de Oliveira Fraga B., Maggio C., Majumdar P., Makariev M., Mallamaci M., Maneva G., Manganaro M., Mannheim K., Maraschi L., Mariotti M., Martinez M., Mazin D., Menchiari S., Mender S., Micanovic S., Miceli D., Miener T., Miranda J. M., Molina E., Moralejo A., Morcuende D., Moreno V., Moretti E., Nakamori T., Nava L., Neustroev V., Nigro C., Nilsson K., Nishijima K., Noda K., Nozaki S., Ohtani Y., Oka T., Otero-Santos J., Paiano S., Palatiello M., Paneque D., Paoletti R., Paredes J. M., Pavletic L., Penil P., Persic M., Pihet M., Prada Moroni P. G., Prandini E., Priyadarshi C., Puljak I., Rhode W., Ribo M., Rico J., Righi C., Rugliancich A., Sahakyan N., Saito T., Sakurai S., Satalecka K., Saturni F. G., Schleicher B., Schmidt K., Sitarek J., Snidaric I., Sobczynska D., Spolon A., Stamerra A., Striskovic J., Strom D., Strzys M., Suda Y., Suric T., Takahashi M., Takeishi R., Tavecchio F., Temnikov P., Terzic T., Teshima M., Tosti L., Truzzi S., Tutone A., Ubach S., van Scherpenberg J., Vanzo G., Ventura S. +200 moreopenaire +2 more sourcesThe MAGIC telescope [PDF]
Astronomy and Geophysics, 2005 MAGIC (Major Atmospheric Gamma Imaging Cherenkov telescope) is presently the largest ground-based gamma ray telescope. MAGIC has been taking data regularly since October 2004 at the Roque de los Muchachos Observatory on the island of La Palma. In this paper the MAGIC telescope status, its performances and some preliminary results on observed gamma ray ...C. BIGONGIARI, PASCOLI, DONATELLA, MAGIC COLLABORATION +2 moreopenaire +3 more sources
