English
Related papers

Related papers: The next generation Cherenkov Telescope Array obse…

200 papers

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…

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 an atmospheric Cherenkov observatory that will image the cosmos in very-high-energy gamma rays. CTA will study the highest-energy particle accelerators in the Universe and potentially confirm the…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 J. Vandenbroucke

The Cherenkov Telescope Array (CTA) is the next generation very high energy gamma-ray observatory. It will consist of three classes of telescopes, of large, medium and small sizes. The small telescopes, of 4 m diameter, will be dedicated to…

The next-generation ground-based gamma-ray Cherenkov Telescope Array Observatory (CTAO) will consist of imaging atmospheric Cherenkov telescopes (IACTs) of three different sizes distributed in two sites. The Large-Sized Telescopes will…

High Energy Astrophysical Phenomena · Physics 2023-09-21 Daniel Morcuende , Rubén López-Coto , Abelardo Moralejo , Seiya Nozaki , Thomas Vuillaume

The Cherenkov Telescope Array (CTA) will be the next generation gamma-ray observatory, which will consist of three kinds of telescopes of different sizes. Among those, the Large Size Telescope (LST) will be the most sensitive in the low…

Instrumentation and Methods for Astrophysics · Physics 2021-08-23 Y. Ohtani , A. Berti , D. Depaoli , F. Di Pierro , D. Green , L. Heckmann , M. Hütten , T. Inada , R. López-Coto , E. Medina , A. Moralejo , D. Morcuende , G. Pirola , M. Strzys , Y. Suda , I. Vovk

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

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 Cherenkov Telescope Array (CTA) will be the first ground-based observatory for gamma-ray astronomy. With more than a hundred of 4th generation of Imaging Atmospheric Cherenkov Telescopes (IACTs) distributed in two large arrays, CTA will…

Instrumentation and Methods for Astrophysics · Physics 2019-09-05 Thomas Tavernier , Jean-François Glicenstein , François Brun

The Cherenkov Telescope Array (CTA) will be the next generation observatory employing different types of Cherenkov telescopes for the detection of particle showers initiated by very-high-energy gamma rays. A good knowledge of the Earth's…

Instrumentation and Methods for Astrophysics · Physics 2018-01-22 Stanislav Stefanik , Raquel de los Reyes , Dalibor Nosek

The Cherenkov Telescope Array (CTA) is the next-generation ground-based observatory for very-high energy gamma-ray astronomy. CTA will have unparalleled sensitivity and angular resolution and will detect gamma-ray sources nearly 100 times…

Instrumentation and Methods for Astrophysics · Physics 2022-09-07 Leslie Taylor

We present studies for optimizing the next generation of ground-based imaging atmospheric Cherenkov telescopes (IACTs). Results focus on mid-sized telescopes (MSTs) for CTA, detecting very high energy gamma rays in the energy range from a…

Instrumentation and Methods for Astrophysics · Physics 2015-07-15 M. Wood , T. Jogler , J. Dumm , S. Funk

The Gamma-ray Cherenkov Telescope (GCT) is one of the Small Size Telescopes (SSTs) proposed for the Cherenkov Telescope Array (CTA) aimed at the 1 TeV to 300 TeV energy range. GCT will be equipped with a Compact High-Energy Camera (CHEC)…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Richard White , Harm Schoorlemmer

The Cherenkov Telescope Array (CTA) is an international project for a next-generation ground-based gamma-ray observatory. CTA, conceived as an array of tens of imaging atmospheric Cherenkov telescopes, comprising small, medium and…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 D. Nieto , S. Griffiths , B. Humensky , P. Kaaret , M. Limon , I. Mognet , A. Peck , A. Petrashyk , D. Ribeiro , J. Rousselle , B. Stevenson , V. Vassiliev , P. Yu

The Cherenkov Telescope Array (CTA) is a ground-based $\gamma$-ray observatory that will observe the full sky in the energy range from 20 GeV to 100 TeV from facilities in both hemispheres. It is proposed to consist of more than 100…

Instrumentation and Methods for Astrophysics · Physics 2015-09-08 Ramin Marx , Raquel de los Reyes

We provide an updated assessment of the power of the Cherenkov Telescope Array (CTA) to search for thermally produced dark matter at the TeV scale, via the associated gamma-ray signal from pair-annihilating dark matter particles in the…

High Energy Astrophysical Phenomena · Physics 2021-02-02 The Cherenkov Telescope Array Consortium , : , A. Acharyya , R. Adam , C. Adams , I. Agudo , A. Aguirre-Santaella , R. Alfaro , J. Alfaro , C. Alispach , R. Aloisio , R. Alves Batista , L. Amati , G. Ambrosi , E. O. Angüner , L. A. Antonelli , C. Aramo , A. Araudo , T. Armstrong , F. Arqueros , K. Asano , Y. Ascasíbar , M. Ashley , C. Balazs , O. Ballester , A. Baquero Larriva , V. Barbosa Martins , M. Barkov , U. Barres de Almeida , J. A. Barrio , D. Bastieri , J. Becerra , G. Beck , J. Becker Tjus , W. Benbow , M. Benito , D. Berge , E. Bernardini , K. Bernlöhr , A. Berti , B. Bertucci , V. Beshley , B. Biasuzzi , A. Biland , E. Bissaldi , J. Biteau , O. Blanch , J. Blazek , F. Bocchino , C. Boisson , L. Bonneau Arbeletche , P. Bordas , Z. Bosnjak , E. Bottacini , V. Bozhilov , J. Bregeon , A. Brill , T. Bringmann , A. M. Brown , P. Brun , F. Brun , P. Bruno , A. Bulgarelli , M. Burton , A. Burtovoi , M. Buscemi , R. Cameron , M. Capasso , A. Caproni , R. Capuzzo-Dolcetta , P. Caraveo , R. Carosi , A. Carosi , S. Casanova , E. Cascone , F. Cassol , F. Catalani , D. Cauz , M. Cerruti , P. Chadwick , S. Chaty , A. Chen , M. Chernyakova , G. Chiaro , A. Chiavassa , M. Chikawa , J. Chudoba , M. Çolak , V. Conforti , R. Coniglione , F. Conte , J. L. Contreras , J. Coronado-Blazquez , A. Costa , H. Costantini , G. Cotter , P. Cristofari , A. D'Aì , F. D'Ammando , L. A. Damone , M. K. Daniel , F. Dazzi , A. De Angelis , V. De Caprio , R. de Cássia dos Anjos , E. M. de Gouveia Dal Pino , B. De Lotto , D. De Martino , E. de Oña Wilhelmi , F. De Palma , V. de Souza , C. Delgado , A. G. Delgado Giler , D. della Volpe , D. Depaoli , T. Di Girolamo , F. Di Pierro , L. Di Venere , S. Diebold , A. Dmytriiev , A. Domínguez , A. Donini , M. Doro , J. Ebr , C. Eckner , T. D. P. Edwards , T. R. N. Ekoume , D. Elsässer , C. Evoli , D. Falceta-Goncalves , E. Fedorova , S. Fegan , Q. Feng , G. Ferrand , G. Ferrara , E. Fiandrini , A. Fiasson , M. Filipovic , V. Fioretti , M. Fiori , L. Foffano , G. Fontaine , O. Fornieri , F. J. Franco , S. Fukami , Y. Fukui , D. Gaggero , G. Galaz , V. Gammaldi , E. Garcia , M. Garczarczyk , D. Gascon , A. Gent , A. Ghalumyan , F. Gianotti , M. Giarrusso , G. Giavitto , N. Giglietto , F. Giordano , A. Giuliani , J. Glicenstein , R. Gnatyk , P. Goldoni , M. M. González , K. Gourgouliatos , J. Granot , D. Grasso , J. Green , A. Grillo , O. Gueta , S. Gunji , A. Halim , T. Hassan , M. Heller , S. Hernández Cadena , N. Hiroshima , B. Hnatyk , W. Hofmann , J. Holder , D. Horan , J. Hörandel , P. Horvath , T. Hovatta , M. Hrabovsky , D. Hrupec , G. Hughes , T. B. Humensky , M. Hütten , M. Iarlori , T. Inada , S. Inoue , F. Iocco , M. Iori , M. Jamrozy , P. Janecek , W. Jin , L. Jouvin , J. Jurysek , E. Karukes , K. Katarzyński , D. Kazanas , D. Kerszberg , M. C. Kherlakian , R. Kissmann , J. Knödlseder , Y. Kobayashi , K. Kohri , N. Komin , H. Kubo , J. Kushida , G. Lamanna , J. Lapington , P. Laporte , M. A. Leigui de Oliveira , J. Lenain , F. Leone , G. Leto , E. Lindfors , T. Lohse , S. Lombardi , F. Longo , A. Lopez , M. López , R. López-Coto , S. Loporchio , P. L. Luque-Escamilla , E. Mach , C. Maggio , G. Maier , M. Mallamaci , R. Malta Nunes de Almeida , D. Mandat , M. Manganaro , S. Mangano , G. Manicò , M. Marculewicz , M. Mariotti , 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 , M. Miceli , T. Miener , M. Minev , J. M. Miranda , R. Mirzoyan , T. Mizuno , B. Mode , R. Moderski , L. Mohrmann , E. Molina , T. Montaruli , A. Moralejo , D. Morcuende-Parrilla , A. Morselli , R. Mukherjee , C. Mundell , A. Nagai , T. Nakamori , R. Nemmen , J. Niemiec , D. Nieto , M. Nikołajuk , D. Ninci , K. Noda , D. Nosek , S. Nozaki , Y. Ohira , M. Ohishi , Y. Ohtani , T. Oka , A. Okumura , R. A. Ong , M. Orienti , R. Orito , M. Orlandini , S. Orlando , E. Orlando , M. Ostrowski , I. Oya , I. Pagano , A. Pagliaro , M. Palatiello , F. R. Pantaleo , J. M. Paredes , G. Pareschi , N. Parmiggiani , B. Patricelli , L. Pavletić , A. Pe'er , M. Pecimotika , J. Pérez-Romero , M. Persic , O. Petruk , K. Pfrang , G. Piano , P. Piatteli , E. Pietropaolo , R. Pillera , B. Pilszyk , F. Pintore , M. Pohl , V. Poireau , R. R. Prado , E. Prandini , J. Prast , G. Principe , H. Prokoph , M. Prouza , H. Przybilski , G. Pühlhofer , M. L. Pumo , F. Queiroz , A. Quirrenbach , S. Rainò , R. Rando , S. Razzaque , S. Recchia , O. Reimer , A. Reisenegger , Y. Renier , W. Rhode , D. Ribeiro , M. Ribó , T. Richtler , J. Rico , F. Rieger , L. Rinchiuso , V. Rizi , J. Rodriguez , G. Rodriguez Fernandez , J. C. Rodriguez Ramirez , G. Rojas , P. Romano , G. Romeo , J. Rosado , G. Rowell , B. Rudak , F. Russo , I. Sadeh , E. Sæther Hatlen , S. Safi-Harb , F. Salesa Greus , G. Salina , D. Sanchez , M. Sánchez-Conde , P. Sangiorgi , H. Sano , M. Santander , E. M. Santos , R. Santos-Lima , A. Sanuy , S. Sarkar , F. G. Saturni , U. Sawangwit , 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 , J. Silk , C. Siqueira , V. Sliusar , A. Słowikowska , A. Sokolenko , H. Sol , S. Spencer , A. Stamerra , S. Stanič , R. Starling , T. Stolarczyk , U. Straumann , J. Strišković , Y. Suda , T. Suomijarvi , P. Świerk , F. Tavecchio , L. Taylor , L. A. Tejedor , M. Teshima , V. Testa , L. Tibaldo , C. J. Todero Peixoto , F. Tokanai , D. Tonev , G. Tosti , L. Tosti , N. Tothill , S. Truzzi , P. Travnicek , V. Vagelli , B. Vallage , P. Vallania , C. van Eldik , J. Vandenbroucke , G. S. Varner , V. Vassiliev , M. Vázquez Acosta , M. Vecchi , S. Ventura , S. Vercellone , S. Vergani , G. Verna , A. Viana , C. F. Vigorito , J. Vink , V. Vitale , S. Vorobiov , I. Vovk , T. Vuillaume , S. J. Wagner , R. Walter , J. Watson , C. Weniger , R. White , M. White , R. Wiemann , A. Wierzcholska , M. Will , D. A. Williams , R. Wischnewski , S. Yanagita , L. Yang , T. Yoshikoshi , M. Zacharias , G. Zaharijas , A. A. Zakaria , L. Zampieri , R. Zanin , D. Zaric , M. Zavrtanik , D. Zavrtanik , A. A. Zdziarski , A. Zech , H. Zechlin , V. I. Zhdanov , M. Živec

Cherenkov Telescope Array (CTA) is an upcoming instrument that will start a new generation of atmospheric Cherenkov telescopes. CTA is expected not only to provide an unprecedented sensitivity in the tens of GeV to hundreds of TeV range,…

Instrumentation and Methods for Astrophysics · Physics 2019-07-11 Julian Sitarek , Dorota Sobczyńska , Katarzyna Adamczyk , Michał Szanecki
‹ Prev 1 3 4 5 6 7 10 Next ›