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The Cherenkov Telescope Array (CTA) will be the next generation ground based observatory in very high energy gamma ray astronomy. The facility will achieve a wide energy coverage, starting from a threshold of a few tens of GeV up to…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 M. K. Daniel , M. Gaug , P. Majumdar

The Cherenkov Telescope Array (CTA) is an international initiative to build the next generation ground-based very-high-energy gamma-ray observatory. Full sky coverage will be assured by two arrays, one located on each of the northern and…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Maria Concetta Maccarone , Dan Parsons , Markus Gaug , Raquel de los Reyes

The Cherenkov Telescope Array (CTA) will present the next leap forward in gamma-ray astronomy, pushing beyond the present energy frontier to probe beyond 300 TeV. This capability is provided by the 70 Small Sized Telescopes (SSTs). The SSTs…

Instrumentation and Methods for Astrophysics · Physics 2019-07-23 Jason John Watson , Justus Zorn

The Cherenkov Telescope Array (CTA) is the next major ground-based observatory for gamma-ray astronomy. With CTA gamma-ray sources will be studied in the very-high energy gamma-ray range of a few tens of GeV to 100 TeV with up to ten times…

Instrumentation and Methods for Astrophysics · Physics 2014-08-05 Kevin J. Meagher

The Cherenkov Telescope Array (CTA) will be the largest ground-based observatory operating in the very-high-energy gamma-ray (20 GeV - 300 TeV) range. It will be based on more than one hundred telescopes, located at two sites (northern and…

Instrumentation and Methods for Astrophysics · Physics 2018-01-22 Maria Concetta Maccarone

The Cherenkov Telescope Array Observatory (CTAO) is a next-generation facility for ground-based very high energy gamma ray astronomy. CTAO will be operated as an open observatory. With two sites, in the northern and southern hemispheres,…

Instrumentation and Methods for Astrophysics · Physics 2023-05-23 Werner Hofmann , Roberta Zanin

The Small Size Telescope with Single Mirror (SST-1M) is one of the proposed types of Small Size Telescopes (SST) for the Cherenkov Telescope Array (CTA). About 70 SST telescopes will be part the CTA southern array which will also include…

The Cherenkov Telescope Array (CTA) is a planned observatory for very-high energy gamma-ray astronomy. It will consist of several tens of telescopes of different sizes, with a total mirror area of up to 10,000 square meters. Most mirrors of…

The Cherenkov Telescopes Array (CTA) is planned to be an Observatory for very high energy gamma ray astronomy and will consist of several tens of telescopes which account for a reflective surface of more than 10000 m$^2$. The mirrors of…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 M. C. Medina , B. Garcia , J. Maya , A. Mancilla , J. J. Larrarte , E. Rasztocky , M. Benitez , J. Dipold , M. Platino

The Cherenkov Telescope Array (CTA) is the next generation very high energy gamma-ray observatory covering the 20 GeV - 300 TeV energy range with unprecedented sensitivity, angular and energy resolution. With a site in each hemisphere, CTA…

The pointing capability of a telescope in the Cherenkov Telescope Array (CTA) is a crucial aspect in the calibration of the instrument. It describes how a position in the sky is transformed to the focal plane of the telescope and allows…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Domenico Tiziani , Markus Garczarczyk , Louise Oakes , Ullrich Schwanke , Christopher van Eldik

The Cherenkov Telescope Array (CTA) observatory will be deployed over two sites in the two hemispheres. Both sites will be equipped with four Large Size Telescopes (LSTs), which are crucial to achieve the science goals of CTA in the 20-200…

Instrumentation and Methods for Astrophysics · Physics 2017-08-09 D. Mazin , J. Cortina , M. Teshima , the CTA Consortium

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…

Instrumentation and Methods for Astrophysics · Physics 2019-02-27 The Cherenkov Telescope Array Consortium , : , B. S. Acharya , I. Agudo , I. Al Samarai , R. Alfaro , J. Alfaro , C. Alispach , R. Alves Batista , J. -P. Amans , E. Amato , G. Ambrosi , E. Antolini , L. A. Antonelli , C. Aramo , M. Araya , T. Armstrong , F. Arqueros , L. Arrabito , K. Asano , M. Ashley , M. Backes , C. Balazs , M. Balbo , O. Ballester , J. Ballet , A. Bamba , M. Barkov , U. Barres de Almeida , J. A. Barrio , D. Bastieri , Y. Becherini , A. Belfiore , W. Benbow , D. Berge , E. Bernardini , M. G. Bernardini , M. Bernardos , K. Bernlöhr , B. Bertucci , B. Biasuzzi , C. Bigongiari , A. Biland , E. Bissaldi , J. Biteau , O. Blanch , J. Blazek , C. Boisson , J. Bolmont , G. Bonanno , A. Bonardi , C. Bonavolontà , G. Bonnoli , Z. Bosnjak , M. Böttcher , C. Braiding , J. Bregeon , A. Brill , A. M. Brown , P. Brun , G. Brunetti , T. Buanes , J. Buckley , V. Bugaev , R. Bühler , A. Bulgarelli , T. Bulik , M. Burton , A. Burtovoi , G. Busetto , R. Canestrari , M. Capalbi , F. Capitanio , A. Caproni , P. Caraveo , V. Cárdenas , C. Carlile , R. Carosi , E. Carquín , J. Carr , S. Casanova , E. Cascone , F. Catalani , O. Catalano , D. Cauz , M. Cerruti , P. Chadwick , S. Chaty , R. C. G. Chaves , A. Chen , X. Chen , M. Chernyakova , M. Chikawa , A. Christov , J. Chudoba , M. Cieślar , V. Coco , S. Colafrancesco , P. Colin , V. Conforti , V. Connaughton , J. Conrad , J. L. Contreras , J. Cortina , A. Costa , H. Costantini , G. Cotter , S. Covino , R. Crocker , J. Cuadra , O. Cuevas , P. Cumani , A. D'Aì , F. D'Ammando , P. D'Avanzo , D. D'Urso , M. Daniel , I. Davids , B. Dawson , F. Dazzi , A. De Angelis , R. de Cássia dos Anjos , G. De Cesare , A. De Franco , E. M. de Gouveia Dal Pino , I. de la Calle , R. de los Reyes Lopez , B. De Lotto , A. De Luca , M. De Lucia , M. de Naurois , E. de Oña Wilhelmi , F. De Palma , F. De Persio , V. de Souza , C. Deil , M. Del Santo , C. Delgado , D. della Volpe , T. Di Girolamo , F. Di Pierro , L. Di Venere , C. Díaz , C. Dib , S. Diebold , A. Djannati-Ataï , A. Domínguez , D. Dominis Prester , D. Dorner , M. Doro , H. Drass , D. Dravins , G. Dubus , V. V. Dwarkadas , J. Ebr , C. Eckner , K. Egberts , S. Einecke , T. R. N. Ekoume , D. Elsässer , J. -P. Ernenwein , C. Espinoza , C. Evoli , M. Fairbairn , D. Falceta-Goncalves , A. Falcone , C. Farnier , G. Fasola , E. Fedorova , S. Fegan , M. Fernandez-Alonso , A. Fernández-Barral , G. Ferrand , M. Fesquet , M. Filipovic , V. Fioretti , G. Fontaine , M. Fornasa , L. Fortson , L. Freixas Coromina , C. Fruck , Y. Fujita , Y. Fukazawa , S. Funk , M. Füßling , S. Gabici , A. Gadola , Y. Gallant , B. Garcia , R. Garcia López , M. Garczarczyk , J. Gaskins , T. Gasparetto , M. Gaug , L. Gerard , G. Giavitto , N. Giglietto , P. Giommi , F. Giordano , E. Giro , M. Giroletti , A. Giuliani , J. -F. Glicenstein , R. Gnatyk , N. Godinovic , P. Goldoni , G. Gómez-Vargas , M. M. González , J. M. González , D. Götz , J. Graham , P. Grandi , J. Granot , A. J. Green , T. Greenshaw , S. Griffiths , S. Gunji , D. Hadasch , S. Hara , M. J. Hardcastle , T. Hassan , K. Hayashi , M. Hayashida , M. Heller , J. C. Helo , G. Hermann , J. Hinton , B. Hnatyk , W. Hofmann , J. Holder , D. Horan , J. Hörandel , D. Horns , P. Horvath , T. Hovatta , M. Hrabovsky , D. Hrupec , T. B. Humensky , M. Hütten , M. Iarlori , T. Inada , Y. Inome , S. Inoue , T. Inoue , Y. Inoue , F. Iocco , K. Ioka , M. Iori , K. Ishio , Y. Iwamura , M. Jamrozy , P. Janecek , D. Jankowsky , P. Jean , I. Jung-Richardt , J. Jurysek , P. Kaaret , S. Karkar , H. Katagiri , U. Katz , N. Kawanaka , D. Kazanas , B. Khélifi , D. B. Kieda , S. Kimeswenger , S. Kimura , S. Kisaka , J. Knapp , J. Knödlseder , B. Koch , K. Kohri , N. Komin , K. Kosack , M. Kraus , M. Krause , F. Krauß , H. Kubo , G. Kukec Mezek , H. Kuroda , J. Kushida , N. La Palombara , G. Lamanna , R. G. Lang , J. Lapington , O. Le Blanc , S. Leach , J. -P. Lees , J. Lefaucheur , M. A. Leigui de Oliveira , J. -P. Lenain , R. Lico , M. Limon , E. Lindfors , T. Lohse , S. Lombardi , F. Longo , M. López , R. López-Coto , C. -C. Lu , F. Lucarelli , P. L. Luque-Escamilla , E. Lyard , M. C. Maccarone , G. Maier , P. Majumdar , G. Malaguti , D. Mandat , G. Maneva , M. Manganaro , S. Mangano , A. Marcowith , J. Marín , S. Markoff , J. Martí , P. Martin , M. Martínez , G. Martínez , N. Masetti , S. Masuda , G. Maurin , N. Maxted , D. Mazin , C. Medina , A. Melandri , S. Mereghetti , M. Meyer , I. A. Minaya , N. Mirabal , R. Mirzoyan , A. Mitchell , T. Mizuno , R. Moderski , M. Mohammed , L. Mohrmann , T. Montaruli , A. Moralejo , D. Morcuende-Parrilla , K. Mori , G. Morlino , P. Morris , A. Morselli , E. Moulin , R. Mukherjee , C. Mundell , T. Murach , H. Muraishi , K. Murase , A. Nagai , S. Nagataki , T. Nagayoshi , T. Naito , T. Nakamori , Y. Nakamura , J. Niemiec , D. Nieto , M. Nikołajuk , K. Nishijima , K. Noda , D. Nosek , B. Novosyadlyj , S. Nozaki , P. O'Brien , L. Oakes , Y. Ohira , M. Ohishi , S. Ohm , N. Okazaki , A. Okumura , R. A. Ong , M. Orienti , R. Orito , J. P. Osborne , M. Ostrowski , N. Otte , I. Oya , M. Padovani , A. Paizis , M. Palatiello , M. Palatka , R. Paoletti , J. M. Paredes , G. Pareschi , R. D. Parsons , A. Pe'er , M. Pech , G. Pedaletti , M. Perri , M. Persic , A. Petrashyk , P. Petrucci , O. Petruk , B. Peyaud , M. Pfeifer , G. Piano , A. Pisarski , S. Pita , M. Pohl , M. Polo , D. Pozo , E. Prandini , J. Prast , G. Principe , D. Prokhorov , H. Prokoph , M. Prouza , G. Pühlhofer , M. Punch , S. Pürckhauer , F. Queiroz , A. Quirrenbach , S. Rainò , S. Razzaque , O. Reimer , A. Reimer , A. Reisenegger , M. Renaud , A. H. Rezaeian , W. Rhode , D. Ribeiro , M. Ribó , T. Richtler , J. Rico , F. Rieger , M. Riquelme , S. Rivoire , V. Rizi , J. Rodriguez , G. Rodriguez Fernandez , J. J. Rodríguez Vázquez , G. Rojas , P. Romano , G. Romeo , J. Rosado , A. C. Rovero , G. Rowell , B. 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Todero Peixoto , F. Tokanai , J. Tomastik , D. Tonev , M. Tornikoski , D. F. Torres , E. Torresi , G. Tosti , N. Tothill , G. Tovmassian , P. Travnicek , C. Trichard , M. Trifoglio , I. Troyano Pujadas , S. Tsujimoto , G. Umana , V. Vagelli , F. Vagnetti , M. Valentino , P. Vallania , L. Valore , C. van Eldik , J. Vandenbroucke , G. S. Varner , G. Vasileiadis , V. Vassiliev , M. Vázquez Acosta , M. Vecchi , A. Vega , S. Vercellone , P. Veres , S. Vergani , V. Verzi , G. P. Vettolani , A. Viana , C. Vigorito , J. Villanueva , H. Voelk , A. Vollhardt , S. Vorobiov , M. Vrastil , T. Vuillaume , S. J. Wagner , R. Wagner , R. Walter , J. E. Ward , D. Warren , J. J. Watson , F. Werner , M. White , R. White , A. Wierzcholska , P. Wilcox , M. Will , D. A. Williams , R. Wischnewski , M. Wood , T. Yamamoto , R. Yamazaki , S. Yanagita , L. Yang , T. Yoshida , S. Yoshiike , T. Yoshikoshi , M. Zacharias , G. Zaharijas , L. Zampieri , F. Zandanel , R. Zanin , M. Zavrtanik , D. Zavrtanik , A. A. Zdziarski , A. Zech , H. Zechlin , V. I. Zhdanov , A. Ziegler , J. Zorn

The Cherenkov Telescope Array (CTA) \cite{CTA:2010} will be the successor to current Imaging Atmospheric Cherenkov Telescopes (IACT) like H.E.S.S., MAGIC and VERITAS. CTA will improve in sensitivity by about an order of magnitude compared…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 E. Birsin , J. Colomé , D. Hoffmann , H. Koeppel , G. Lamanna , T. Le Flour , A. Lopatin , E. Lyard , D. Melkumyan , I. Oya , J-L. Panazol , S. Schlenstedt , T. Schmidt , U. Schwanke , R. Walter , P. Wegner

The Cherenkov Telescope Array (CTA) will be the next generation ground-based gamma-ray observatory. CTA consists of different telescope types of which the largest ones (Large-Sized Telescopes, LSTs) cover the lower energy range, between 20…

Instrumentation and Methods for Astrophysics · Physics 2023-07-13 D. Depaoli , A. Chiavassa , D. Corti , F. Di Pierro , M. Mariotti , R. Rando

The Cherenkov Telescope Array (CTA) is the the next generation facility of imaging atmospheric Cherenkov telescopes; two sites will cover both hemispheres. CTA will reach unprecedented sensitivity, energy and angular resolution in…

The Cherenkov Telescope Array (CTA) is a major ground-based observatory proposed for gamma-ray astronomy. CTA is envisioned to consist of two large arrays of atmospheric Cherenkov telescopes for the study of sources of high-energy gamma…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 R. A. Ong , T. Aune , J. Hall

The Cherenkov Telescope Array (CTA) project, led by an international collaboration of institutes, aims to create the world's largest next generation observatory for Very High Energy (VHE) gamma-ray astronomy. It will be devoted to…

Instrumentation and Methods for Astrophysics · Physics 2019-09-26 A. Dmytriiev , L. Dangeon , G. Fasola , H. Sol , A. Zech , J. Gironnet , O. Le Blanc , J. P. Amans , G. Buchholtz , J. L. Dournaux , F. de Frondat , D. Horville , J. M. Huet , I. Jégouzo , P. Laporte

The Cherenkov Telescope Array (CTA) is a project for the construction of a next generation VHE gamma ray observatory with full sky coverage. Its aim is improving by about one order of magnitude the sensitivity of the existing installations,…

Instrumentation and Methods for Astrophysics · Physics 2011-11-10 The CTA Consortium

The Cherenkov Telescope Array (CTA) is the next generation of ground-based gamma-ray observatory. The observatory will consist of two arrays, one located in the southern hemisphere (Paranal,Chile) and the other in the northern hemisphere…

Instrumentation and Methods for Astrophysics · Physics 2020-12-17 Victor Barbosa Martins , Markus Garczarczyk