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The Cherenkov Telescope Array (CTA) will be the major global observatory for VHE gamma-ray astronomy over the next decade and beyond. It will be an explorer of the extreme universe, with a broad scientific potential: from understanding the…

High Energy Astrophysical Phenomena · Physics 2019-07-22 Ulisses Barres de Almeida

The Cherenkov Telescope Array (CTA) will be the next-generation gamma-ray observatory, investigating gamma-ray and cosmic ray astrophysics at energies from 20 GeV to more than 300 TeV. The observatory, consisting of large arrays of imaging…

High Energy Astrophysical Phenomena · Physics 2018-01-22 The CTA Consortium

The Cherenkov Telescope Array (CTA) is planned to be the next generation ground based observatory for very high energy (VHE) gamma-ray astronomy. Gamma-rays provide a powerful insight into the non-thermal universe and hopefully a unique…

Instrumentation and Methods for Astrophysics · Physics 2016-06-28 Ciro Bigongiari

The Cherenkov Telescope Array (CTA) will be the next generation of ground based gamma-ray telescopes allowing us to study very high energy phenomena in the Universe. CTA aims to gain about a factor of ten in sensitivity compared to current…

High Energy Astrophysical Phenomena · Physics 2017-05-23 S. Mangano

The Cherenkov Telescope Array (CTA) is a project for a next-generation observatory for very high energy (GeV-TeV) ground-based gamma-ray astronomy, currently in its design phase, and foreseen to be operative a few years from now. Several…

The Cherenkov Telescope Array (CTA) is the major ground-based gamma-ray observatory planned for the next decade and beyond. Consisting of two large atmospheric Cherenkov telescope arrays (one in the southern hemisphere and one in the…

High Energy Astrophysical Phenomena · Physics 2019-06-12 The CTA Consortium , represented by Rene A. Ong

The Cherenkov Telescope Array (CTA) is the next generation high-energy gamma-ray observatory. It will improve the sensitivity of current instruments up to an order of magnitude, while providing energy coverage for photons from 20 GeV to at…

High Energy Astrophysical Phenomena · Physics 2019-07-18 Fabian Schüssler

The Cherenkov Telescope Array (CTA) is the next generation ground-based observatory for gamma-ray astronomy at very-high energies. It will be capable of detecting gamma rays in the energy range from 20 GeV to more than 300 TeV with…

Instrumentation and Methods for Astrophysics · Physics 2019-07-22 Daniel Mazin

The Cherenkov Telescope Array (CTA), the new-generation ground-based observatory for $\gamma$-ray astronomy, provides unique capabilities to address significant open questions in astrophysics, cosmology, and fundamental physics. We study…

High Energy Astrophysical Phenomena · Physics 2021-03-01 The Cherenkov Telescope Array Consortium , : , H. Abdalla , H. Abe , F. Acero , A. Acharyya , R. Adam , I. Agudo , A. Aguirre-Santaella , R. Alfaro , J. Alfaro , C. Alispach , R. Aloisio , R. Alves B , L. Amati , E. Amato , G. Ambrosi , E. O. Angüner , A. Araudo , T. Armstrong , F. Arqueros , L. Arrabito , K. Asano , Y. Ascasíbar , M. Ashley , M. Backes , C. Balazs , M. Balbo , B. Balmaverde , A. Baquero Larriva , V. Barbosa Martins , M. Barkov , L. Baroncelli , U. Barres de Almeida , J. A. Barrio , P. Batista , J. Becerra , Y. Becherini , G. Beck , J. Becker Tjus , R. Belmont , W. Benbow , E. Bernardini , A. Berti , M. Berton , B. Bertucci , V. Beshley , B. Bi , B. Biasuzzi , A. Biland , E. Bissaldi , J. Biteau , O. Blanch , F. Bocchino , C. Boisson , J. Bolmont , G. Bonanno , L. Bonneau Arbeletche , G. Bonnoli , P. Bordas , E. Bottacini , M. Böttcher , V. Bozhilov , J. Bregeon , A. Brill , A. M. Brown , P. Bruno , A. Bruno , A. Bulgarelli , M. Burton , M. Buscemi , A. Caccianiga , R. Cameron , M. Capasso , M. Caprai , A. Caproni , R. Capuzzo-Dolcetta , P. Caraveo , R. Carosi , A. Carosi , S. Casanova , E. Cascone , D. Cauz , K. Cerny , M. Cerruti , P. Chadwick , S. Chaty , A. Chen , M. Chernyakova , G. Chiaro , A. Chiavassa , L. Chytka , V. Conforti , F. Conte , J. L. Contreras , J. Coronado-Blazquez , J. Cortina , A. Costa , H. Costantini , S. Covino , P. Cristofari , O. Cuevas , F. D'Ammando , M. K. Daniel , J. Davies , F. Dazzi , A. De Angelis , M. de Bony de Lavergne , V. De Caprio , R. de Cássia dos Anjos , E. M. de Gouveia Dal Pino , B. De Lotto , D. De Martino , M. de Naurois , E. de Oña Wilhelmi , F. De Palma , V. de Souza , C. Delgado , R. Della Ceca , D. della Volpe , D. Depaoli , T. Di Girolamo , F. Di Pierro , C. Díaz , C. Díaz-Bahamondes , S. Diebold , A. Djannati-Ataï , A. Dmytriiev , A. Domínguez , A. Donini , D. Dorner , M. Doro , J. Dournaux , V. V. Dwarkadas , J. Ebr , C. Eckner , S. Einecke , T. R. N. Ekoume , D. Elsässer , G. Emery , C. Evoli , M. Fairbairn , D. Falceta-Goncalves , S. Fegan , Q. Feng , G. Ferrand , E. Fiandrini , A. Fiasson , V. Fioretti , L. Foffano , M. V. Fonseca , L. Font , G. Fontaine , F. J. Franco , L. Freixas Coromina , S. Fukami , Y. Fukazawa , Y. Fukui , D. Gaggero , G. Galanti , V. Gammaldi , E. Garcia , M. Garczarczyk , D. Gascon , M. Gaug , A. Gent , A. Ghalumyan , G. Ghirlanda , F. Gianotti , M. Giarrusso , G. Giavitto , N. Giglietto , F. Giordano , J. Glicenstein , P. Goldoni , J. M. González , K. Gourgouliatos , T. Grabarczyk , P. Grandi , J. Granot , D. Grasso , J. Green , J. Grube , O. Gueta , S. Gunji , A. Halim , M. Harvey , T. Hassan Collado , K. Hayashi , M. Heller , S. Hernández Cadena , O. Hervet , J. Hinton , N. Hiroshima , B. Hnatyk , R. Hnatyk , D. Hoffmann , W. Hofmann , J. Holder , D. Horan , J. Hörandel , P. Horvath , T. Hovatta , M. Hrabovsky , D. Hrupec , G. Hughes , M. Hütten , M. Iarlori , T. Inada , S. Inoue , A. Insolia , M. Ionica , M. Iori , M. Jacquemont , M. Jamrozy , P. Janecek , I. Jiménez Martínez , W. Jin , I. Jung-Richardt , J. Jurysek , P. Kaaret , V. Karas , S. Karkar , N. Kawanaka , D. Kerszberg , B. Khélifi , R. Kissmann , J. Knödlseder , Y. Kobayashi , K. Kohri , N. Komin , A. Kong , K. Kosack , H. Kubo , N. La Palombara , G. Lamanna , R. G. Lang , J. Lapington , P. Laporte , M. Lemoine-Goumard , J. Lenain , F. Leone , G. Leto , F. Leuschner , E. Lindfors , S. Lloyd , T. Lohse , S. Lombardi , F. Longo , A. Lopez , M. López , R. López-Coto , S. Loporchio , F. Lucarelli , P. L. Luque-Escamilla , E. Lyard , C. Maggio , A. Majczyna , M. Makariev , M. Mallamaci , D. Mandat , G. Maneva , M. Manganaro , G. Manicò , A. Marcowith , M. Marculewicz , S. Markoff , P. Marquez , J. Martí , O. Martinez , M. Martínez , G. Martínez , H. Martínez-Huerta , G. Maurin , D. Mazin , J. D. Mbarubucyeye , D. Medina Miranda , M. Meyer , S. Micanovic , T. Miener , M. Minev , J. M. Miranda , A. Mitchell , T. Mizuno , B. Mode , R. Moderski , L. Mohrmann , E. Molina , T. Montaruli , A. Moralejo , J. Morales Merino , D. Morcuende-Parrilla , A. Morselli , R. Mukherjee , C. Mundell , T. Murach , H. Muraishi , A. Nagai , T. Nakamori , R. Nemmen , J. Niemiec , D. Nieto , M. Nievas , M. Nikołajuk , K. Nishijima , K. Noda , D. Nosek , S. Nozaki , P. O'Brien , Y. Ohira , M. Ohishi , T. Oka , R. A. Ong , M. Orienti , R. Orito , M. Orlandini , E. Orlando , J. P. Osborne , M. Ostrowski , I. Oya , A. Pagliaro , M. Palatka , D. Paneque , F. R. Pantaleo , J. M. Paredes , N. Parmiggiani , B. Patricelli , L. Pavletić , A. Pe'er , M. Pech , M. Pecimotika , M. Peresano , M. Persic , O. Petruk , K. Pfrang , P. Piatteli , E. Pietropaolo , R. Pillera , B. Pilszyk , D. Pimentel , F. Pintore , S. Pita , M. Pohl , V. Poireau , M. Polo , R. R. Prado , J. Prast , G. Principe , N. Produit , H. Prokoph , M. Prouza , H. Przybilski , E. Pueschel , G. Pühlhofer , M. L. Pumo , M. Punch , F. Queiroz , A. Quirrenbach , R. Rando , S. Razzaque , E. Rebert , S. Recchia , P. Reichherzer , O. Reimer , A. Reimer , Y. Renier , T. Reposeur , W. Rhode , D. Ribeiro , M. Ribó , T. Richtler , J. Rico , F. Rieger , V. Rizi , J. Rodriguez , G. Rodriguez Fernandez , J. C. Rodriguez Ramirez , J. J. Rodríguez Vázquez , P. Romano , G. Romeo , M. Roncadelli , J. Rosado , A. Rosales de Leon , G. Rowell , B. Rudak , W. Rujopakarn , F. Russo , I. Sadeh , L. Saha , T. Saito , F. Salesa Greus , D. Sanchez , M. Sánchez-Conde , P. Sangiorgi , H. Sano , M. Santander , E. M. Santos , A. Sanuy , S. Sarkar , F. G. Saturni , U. Sawangwit , A. Scherer , B. Schleicher , P. Schovanek , F. Schussler , U. Schwanke , E. Sciacca , S. Scuderi , M. Seglar Arroyo , O. Sergijenko , M. Servillat , K. Seweryn , A. Shalchi , P. Sharma , R. C. Shellard , H. Siejkowski , A. Sinha , V. Sliusar , A. Slowikowska , A. Sokolenko , H. Sol , A. Specovius , S. Spencer , D. Spiga , A. Stamerra , S. Stanič , R. Starling , T. Stolarczyk , U. Straumann , J. Strišković , Y. Suda , P. Świerk , G. Tagliaferri , H. Takahashi , M. Takahashi , F. Tavecchio , L. Taylor , L. A. Tejedor , P. Temnikov , R. Terrier , T. Terzic , V. Testa , W. Tian , L. Tibaldo , D. Tonev , D. F. Torres , E. Torresi , L. Tosti , N. Tothill , G. Tovmassian , P. Travnicek , S. Truzzi , F. Tuossenel , G. Umana , M. Vacula , V. Vagelli , M. Valentino , B. Vallage , P. Vallania , C. van Eldik , G. S. Varner , V. Vassiliev , M. Vázquez Acosta , M. Vecchi , J. Veh , S. Vercellone , S. Vergani , V. Verguilov , G. P. Vettolani , A. Viana , C. F. Vigorito , V. Vitale , S. Vorobiov , I. Vovk , T. Vuillaume , S. J. Wagner , R. Walter , J. Watson , M. White , R. White , R. Wiemann , A. Wierzcholska , M. Will , D. A. Williams , R. Wischnewski , A. Wolter , R. Yamazaki , S. Yanagita , L. Yang , T. Yoshikoshi , M. Zacharias , G. Zaharijas , D. Zaric , M. Zavrtanik , D. Zavrtanik , A. Zech , H. Zechlin , V. I. Zhdanov , M. Živec

Gamma-rays provide a powerful insight into the non-thermal universe and perhaps a unique probe for new physics beyond the standard model. Current experiments are already giving results in the physics of acceleration of cosmic rays in…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Michele Doro

The Cherenkov Telescopic Array (CTA), the next-generation ground-based gamma-ray observatory, will have unprecedented sensitivity, providing answers to open questions in gamma-ray cosmology and fundamental physics. Using simulations of…

Instrumentation and Methods for Astrophysics · Physics 2021-10-18 Ievgen Vovk , Jonathan Biteau , Humberto Martinez-Huerta , Manuel Meyer , Santiago Pita

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

Gamma-ray astronomy holds a great potential for Astrophysics, Particle Physics and Cosmology. The CTA is an inter- national initiative to build the next generation of ground-based gamma-ray observatories, which will represent a factor of…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Ulisses Barres de Almeida

The Cherenkov Telescope Array (CTA) is the observatory for ground-based gamma-ray astronomy that will shape the domain of TeV astronomy for the next decades. CTA will comprise more than 100 imaging air Cherenkov telescopes deployed on two…

Instrumentation and Methods for Astrophysics · Physics 2020-04-21 Jürgen Knödlseder

The Cherenkov Telescope Array (CTA) is a next generation ground-based very-high-energy gamma-ray observatory that will allow for observations in the >10 GeV range with unprecedented photon statistics and sensitivity. This will enable the…

High Energy Astrophysical Phenomena · Physics 2021-08-11 Alessandro Carosi , Alicia López-Oramas , Francesco Longo

Ground-based gamma-ray astronomy has experienced a major breakthrough in the last decade thanks to the advent of new generation instruments such as H.E.S.S., MAGIC, Milagro and VERITAS. A large variety of cosmic particle accelerators has…

High Energy Astrophysical Phenomena · Physics 2011-10-11 Jürgen Knödlseder

In the last decades a vaste amount of evidence for the existence of dark matter has been accumulated. At the same time, many efforts have been undertaken to try to identify what dark matter is. Indirect searches look at places in the…

Instrumentation and Methods for Astrophysics · Physics 2018-01-22 A. Morselli

The Cherenkov Telescope Array is a next generation ground-based gamma-ray observatory de- signed to detect photons in the 20 GeV to 300 TeV energy range. With a sensitivity improvement of up to one order of magnitude on the entire energy…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Roberta Zanin , Jamie Holder

The Cherenkov Telescope Array (CTA), a ground-based facility for very-high-energy (VHE) gamma-ray astronomy, will operate as an open observatory, serving a wide scientific community to explore and to study the non-thermal universe. Open…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Jürgen Knödlseder , Volker Beckmann , Catherine Boisson , Sylvie Brau-Nogué , Christoph Deil , Bruno Khélifi , Michael Mayer , Roland Walter

The Cherenkov Telescope Array (CTA) will have a unique chance of discovery for a large range of masses in Weakly Interacting Massive Particles models of dark matter. The principal target for dark matter searches with CTA is the centre of…

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