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The Cherenkov Telescopes Array (CTA) is planned as the future instrument for very-high-energy (VHE) gamma-ray astronomy with a wide energy range of four orders of magnitude and an improvement in sensitivity compared to current instruments…

The Next-Generation Atmospheric Cherenkov Telescope Array (NG-ACTA) is proposed as a prospective infrastructure for very high energy (VHE) gamma-ray astronomy, consisting of a mixed-aperture array of 88 telescopes with a maximum array…

High Energy Astrophysical Phenomena · Physics 2026-03-23 Jiancheng Wang , Jirong Mao

The Cherenkov Telescope Array (CTA) is expected to become the by far largest and most sensitive observatory for very-high-energy gamma rays in the energy range from 20 GeV to more than 300 TeV. CTA will be capable of detecting gamma rays…

Instrumentation and Methods for Astrophysics · Physics 2019-07-19 G. Maier , L. Arrabito , K. Bernlöhr , J. Bregeon , P. Cumani , T. Hassan , J. Hinton , A. Moralejo

The Cherenkov Telescope Array (CTA) is an international next-generation ground-based gamma-ray observatory. CTA will be implemented as southern and northern hemisphere arrays of tens of small, medium and large-sized imaging Cherenkov…

The Cherenkov Telescope Array (CTA) is the next generation facility of Imaging Atmospheric Cherenkov Telescopes. It will reach unprecedented sensitivity and energy resolution in very-high-energy gamma-ray astronomy. CTA will detect…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 M. Doro , M. Daniel , R. de los Reyes , M. Gaug , M. C. Maccarone

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

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

Observations of astrophysical transients have brought many novel discoveries and provided new insights into physical processes at work under extreme conditions in the Universe. Multi-wavelength and multi-messenger observations of variable…

Instrumentation and Methods for Astrophysics · Physics 2022-10-19 C. Hoischen , M. Füßling , S. Ohm , A. Balzer , H. Ashkar , K. Bernlöhr , P. Hofverberg , T. L. Holch , T. Murach , H. Prokoph , F. Schüssler , S. J. Zhu , D. Berge , K. Egberts , C. Stegmann

High energy gamma-ray astronomy is a newly emerging and very successful branch of astronomy and astrophysics. Exciting results have been obtained by the current generation Cherenkov telescope systems such as H.E.S.S., MAGIC, VERITAS and…

Astrophysics · Physics 2019-08-14 G. Hermann , W. Hofmann , T. Schweizer , M. Teshima

I provide an incomplete inventory of the astronomical variability that will be found by next-generation time-domain astronomical surveys. These phenomena span the distance range from near-Earth satellites to the farthest Gamma Ray Bursts.…

Astrophysics · Physics 2009-11-13 Andrew C. Becker

A wide variety of Galactic sources show transient emission at soft and hard X-ray energies: low- and high-mass X-ray binaries containing compact objects, isolated neutron stars exhibiting extreme variability as magnetars as well as…

High Energy Astrophysical Phenomena · Physics 2025-05-29 Cherenkov Telescope Array Observatory Consortium

The next generation of ground-based gamma-ray observatories, such as e.g. CTA, will consist of about 50-100 telescopes, and cameras with in total ~100000 to ~200000 channels. The telescopes of the core array will cover and effective area of…

Astrophysics · Physics 2009-11-13 G. Hermann , C. Bauer , C. Foehr , W. Hofmann , T. Kihm , F. Koeck

The current generation of Cherenkov telescopes is mainly limited in their gamma-ray energy and flux reconstruction by uncertainties in the determination of atmospheric parameters. The Cherenkov Telescope Array (CTA) aims to provide…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 M. Doro , M. Gaug , O. Blanch , LL. Font , D. Garrido , A. Lopez-Oramas , M. Martinez

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

Two of the Key Science Projects of the Cherenkov Telescope Array (CTA) consist in performing a deep survey of the Galactic and Extragalactic sky, providing an unbiased view of the Universe at energies above tens of GeV. To optimize the time…

Instrumentation and Methods for Astrophysics · Physics 2019-07-19 A. Donini , T. Gasparetto , J. Bregeon , F. Di Pierro , F. Longo , G. Maier , A. Moralejo , T. Vuillaume

The Cherenkov Telescope Array (CTA) will be an instrument covering a wide energy range in very-high-energy (VHE) gamma rays. CTA will include several types of telescopes, in order to optimize the performance over the whole energy range.…

The galactic and extragalactic surveys are two of the main proposed legacy projects of the Cherenkov Telescope Array (CTA), providing an unbiased view of the Universe at energies above tens of GeV. Considering Cherenkov telescopes' limited…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Lucie Gérard

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 the future ground-based gamma-ray observatory and will be composed of two arrays of imaging atmospheric Cherenkov telescopes (IACTs) located in the Northern and Southern hemispheres respectively. The…

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