中文
相关论文

相关论文: Physics Performance of the Large-Sized Telescope p…

200 篇论文

The Cherenkov Telescope Array (CTA) will consist of two arrays of Imaging Atmospheric Cherenkov Telescopes (IACTs) at the northern and southern hemispheres. CTA will feature IACTs with mirrors of three different sizes optimized to cover…

天体物理仪器与方法 · 物理学 2019-07-25 Juan Cortina

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…

天体物理仪器与方法 · 物理学 2023-07-13 D. Depaoli , A. Chiavassa , D. Corti , F. Di Pierro , M. Mariotti , R. Rando

The Cherenkov Telescope Array (CTA) will be the world's largest and most sensitive ground-based gamma-ray observatory in the energy range from a few tens of GeV to tens of TeV. The LST-1 prototype, currently in its commissioning phase, is…

高能天体物理现象 · 物理学 2021-11-30 Jakub Juryšek , Etienne Lyard , Roland Walter

On October $10^{\rm th}$ 2018 started the commissioning of the first Large Size Telescope (LST) prototype at the Cherenkov Telescope Array (CTA) northern site at the Observatorio del Roque de los Muchachos, Canary Island of La Palma…

天体物理仪器与方法 · 物理学 2019-09-19 Michele Palatiello , Maurizio Iori , Franca Cassol , Diego Cauz , Fabio Ferrarotto

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…

天体物理仪器与方法 · 物理学 2020-04-21 Jürgen Knödlseder

The Cherenkov Telescope Array (CTA) is a future very high energy gamma-ray observatory. CTA will be comprised of small-, medium- and large-size telescopes covering an energy range from tens of GeV to hundreds of TeV and will surpass…

天体物理仪器与方法 · 物理学 2019-08-14 T. Jogler , M. D. Wood , J. Dumm

The Cherenkov Telescope Array (CTA) is a future very high energy gamma-ray observatory. CTA will be comprised of small-,medium- and large-size telescopes covering an energy range from tens of GeV to hundreds of TeV and will surpass existing…

天体物理仪器与方法 · 物理学 2019-08-14 T. Jogler , M. D. Wood , J. Dumm , A. Bouvier

The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude…

The Cherenkov Telescope Array (CTA) will use three telescope sizes to efficiently detect cosmic gamma rays in the energy range from several tens of GeV to hundreds of TeV. The Small-Sized Telescopes (SSTs) will form the largest section of…

天体物理仪器与方法 · 物理学 2021-10-28 R. White

The Cherenkov Telescope Array (CTA) is a large collaborative effort aimed at the design and operation of an observatory dedicated to the VHE gamma-ray astrophysics in the energy range 30 GeV-100 TeV, which will improve by about one order of…

天体物理仪器与方法 · 物理学 2019-08-14 Stefano Vercellone

A Large Size air Cherenkov Telescope (LST) prototype, proposed for the Cherenkov Telescope Array (CTA), is under construction at the Canary Island of La Palma (Spain) this year. The LST camera, which comprises an array of about 500…

The Cherenkov Telescope Array (CTA) is the next generation observatory for very high energy gamma rays. The capability of the array to detect gamma-rays above 10 TeV is going to be achieved with a large number of Small Size Telescopes…

天体物理仪器与方法 · 物理学 2019-08-14 Anna Barnacka , Leszek Bogacz , Mira Grudzińska , Adam Frankowski , Mateusz Janiak , Piotr Lubiński , Rafał Moderski

The Cherenkov Telescope Array (CTA) is the next-generation gamma-ray observatory with sensitivity in the energy range from 20 GeV to beyond 300 TeV. CTA is proposed to consist of two arrays of 40-100 imaging atmospheric Cherenkov…

天体物理仪器与方法 · 物理学 2019-08-14 G. Maier , L. Arrabito , K. Bernlöhr , J. Bregeon , F. Di Pierro , T. Hassan , T. Jogler , J. Hinton , A. Moralejo , M. Wood

The Large-Sized Telescopes (LSTs) of the Cherenkov Telescope Array Observatory (CTAO) will play a crucial role in the study of transient gamma-ray sources, such as gamma-ray bursts and flaring active galactic nuclei. The low energy…

天体物理仪器与方法 · 物理学 2023-09-22 Sami Caroff , Pierre Aubert , Enrique Garcia , Gilles Maurin , Vincent Pollet , Thomas Vuillaume

The Cherenkov Telescope Array (CTA) is the next generation of ground-based gamma-ray astronomy observatory that will improve the sensitivity of current generation instruments by one order of magnitude. The LST-1 is the first telescope…

天体物理仪器与方法 · 物理学 2022-12-02 Enrique Garcia , Thomas Vuillaume , Lukas Nickel

The Cherenkov Telescope Array (CTA) is a future instrument for very-high-energy (VHE) gamma-ray astronomy that is expected to deliver an order of magnitude improvement in sensitivity over existing instruments. In order to meet the physics…

The next generation instrument for ground-based gamma-ray astronomy will be the Cherenkov Telescope Array (CTA), consisting of approximately 100 telescopes in three sizes, built on two sites with one each in the Northern and Southern Hemi-…

天体物理仪器与方法 · 物理学 2017-08-09 Louise Oakes , Markus Garczarczyk , Stephan Kaphle , Michael Mayer , Stefan Schlenstedt

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…

高能天体物理现象 · 物理学 2019-07-22 Ulisses Barres de Almeida

The Cherenkov Telescope Array (CTA) represents the next generation of ground based instruments for Very High Energy gamma-ray astronomy. It is expected to improve on the sensitivity of current instruments by an order of magnitude and…

天体物理仪器与方法 · 物理学 2019-08-14 T. Hassan , L. Arrabito , K. Bernlör , J. Bregeon , J. Hinton , T. Jogler , G. Maier , A. Moralejo , F. Di Pierro , M. Wood

Aims. LST-1, the prototype of the Large-Sized Telescope for the upcoming Cherenkov Telescope Array Observatory, is concluding its commissioning in Observatorio del Roque de los Muchachos on the island of La Palma. The proximity of LST-1…

天体物理仪器与方法 · 物理学 2023-12-13 H. Abe , K. Abe , S. Abe , V. A. Acciari , A. Aguasca-Cabot , I. Agudo , N. Alvarez Crespo , T. Aniello , S. Ansoldi , L. A. Antonelli , C. Aramo , A. Arbet-Engels , C. Arcaro , M. Artero , K. Asano , P. Aubert , D. Baack , A. Babić , A. Baktash , A. Bamba , A. Baquero Larriva , L. Baroncelli , U. Barres de Almeida , J. A. Barrio , I. Batković , J. Baxter , J. Becerra González , W. Bednarek , E. Bernardini , M. I. Bernardos , J. Bernete Medrano , A. Berti , J. Besenrieder , P. Bhattacharjee , N. Biederbeck , C. Bigongiari , A. Biland , E. Bissaldi , O. Blanch , G. Bonnoli , P. Bordas , Ž. Bošnjak , A. Bulgarelli , I. Burelli , L. Burmistrov , M. Buscemi , G. Busetto , A. Campoy Ordaz , M. Cardillo , S. Caroff , A. Carosi , R. Carosi , M. S. Carrasco , M. Carretero-Castrillo , F. Cassol , A. J. Castro-Tirado , D. Cauz , D. Cerasole , G. Ceribella , Y. Chai , K. Cheng , A. Chiavassa , M. Chikawa , L. Chytka , A. Cifuentes , S. Cikota , E. Colombo , J. L. Contreras , A. Cornelia , J. Cortina , H. Costantini , S. Covino , G. D'Amico , V. D'Elia , P. Da Vela , M. Dalchenko , F. Dazzi , A. De Angelis , M. de Bony de Lavergne , B. De Lotto , M. De Lucia , R. de Menezes , L. Del Peral , A. Del Popolo , G. Deleglise , M. Delfino , C. Delgado Mendez , J. Delgado Mengual , D. della Volpe , M. Dellaiera , D. Depaoli , A. De Angelis , A. Di Piano , F. Di Pierro , A. Di Pilato , R. Di Tria , L. Di Venere , R. M. Dominik , D. Dominis Prester , A. Donini , D. Dorner , M. Doro , C. Díaz , L. Eisenberger , D. Elsässer , G. Emery , J. Escudero , V. Fallah Ramazani , L. Fariña , A. Fattorini , G. Ferrara , F. Ferrarotto , A. Fiasson , L. Foffano , L. Font , L. Freixas Coromina , S. Fröse , S. Fukami , Y. Fukazawa , R. J. Garcia López , E. Garcia , M. Garczarczyk , R. J. García López , C. Gasbarra , D. Gasparrini , S. Gasparyan , M. Gaug , D. Geyer , J. G. Giesbrecht Paiva , N. Giglietto , F. Giordano , P. Gliwny , N. Godinović , R. Grau , D. Green , J. G. Green , S. Gunji , P. Günther , J. Hackfeld , D. Hadasch , A. Hahn , K. Hashiyama , T. Hassan , K. Hayashi , L. Heckmann , M. Heller , J. Herrera Llorente , K. Hirotani , D. Hoffmann , D. Horns , J. Houles , M. Hrabovsky , D. Hrupec , D. Hui , M. Hütten , M. Iarlori , R. Imazawa , T. Inada , Y. Inome , K. Ioka , M. Iori , R. Iotov , K. Ishio , M. Jacquemont , I. Jiménez Martínez , E. Jobst , J. Jormanainen , J. Jurysek , M. Kagaya , V. Karas , H. Katagiri , J. Kataoka , D. Kerszberg , G. W. Kluge , Y. Kobayashi , K. Kohri , A. Kong , P. M. Kouch , H. Kubo , J. Kushida , M. Lainez , G. Lamanna , A. Lamastra , T. Le Flour , F. Leone , E. Lindfors , L. Linhoff , M. Linhoff , S. Lombardi , F. Longo , S. Loporchio , A. Lorini , J. Lozano Bahilo , P. L. Luque-Escamilla , E. Lyard , M. Láinez Lezáun , R. López-Coto , M. López-Moya , A. López-Oramas , B. Machado de Oliveira Fraga , P. Majumdar , M. Makariev , D. Mandat , G. Maneva , M. Manganaro , S. Mangano , N. Mang , G. Manicò , K. Mannheim , M. Mariotti , P. Marquez , G. Marsella , O. Martinez , G. Martínez , M. Martínez , J. Martí , A. Mas-Aguilar , G. Maurin , D. Mazin , S. Menchiari , S. Mender , E. Mestre Guillen , S. Micanovic , D. Miceli , T. Miener , J. M. Miranda , R. Mirzoyan , T. Mizuno , S. Mićanović , M. Molero González , E. Molina , H. A. Mondal , T. Montaruli , I. Monteiro , A. Moralejo , D. Morcuende , A. Morselli , V. Moya , H. Muraishi , K. Murase , S. Nagataki , T. Nakamori , C. Nanci , A. Neronov , V. Neustroev , L. Nickel , M. Nievas Rosillo , C. Nigro , L. Nikolić , K. Nilsson , K. Nishijima , T. Njoh Ekoume , K. Noda , D. Nosek , S. Nozaki , M. Ohishi , Y. Ohtani , T. Oka , A. Okumura , R. Orito , J. Otero-Santos , S. Paiano , M. Palatiello , D. Paneque , F. R. Pantaleo , R. Paoletti , J. M. Paredes , L. Pavletić , M. Pech , M. Pecimotika , M. Peresano , M. Persic , F. Pfeiffle , E. Pietropaolo , M. Pihet , G. Pirola , C. Plard , F. Podobnik , V. Poireau , M. Polo , E. Pons , P. G. Prada Moroni , E. Prandini , J. Prast , G. Principe , C. Priyadarshi , M. Prouza , R. Rando , W. Rhode , M. Ribó , J. Rico , C. Righi , V. Rizi , G. Rodriguez Fernandez , M. D. Rodríguez Frías , N. Sahakyan , T. Saito , S. Sakurai , D. A. Sanchez , K. Satalecka , M. Sato , Y. Sato , F. G. Saturni , V. Savchenko , B. Schleicher , K. Schmidt , F. Schmuckermaier , J. L. Schubert , F. Schussler , T. Schweizer , A. Sciaccaluga , T. Siegert , R. Silvia , J. Sitarek , V. Sliusar , D. Sobczynska , A. Spolon , A. Stamerra , J. Strišković , D. Strom , M. Strzys , Y. Suda , S. Suutarinen , T. Šarić , H. Tajima , H. Takahashi , M. Takahashi , J. Takata , R. Takeishi , P. H. T. Tam , S. J. Tanaka , D. Tateishi , F. Tavecchio , P. Temnikov , Y. Terada , K. Terauchi , T. Terzić , M. Teshima , M. Tluczykont , F. Tokanai , D. F. Torres , L. Tosti , P. Travnicek , S. Truzzi , A. Tutone , S. Ubach , M. Vacula , P. Vallania , J. van Scherpenberg , M. Vazquez Acosta , S. Ventura , V. Verguilov , I. Viale , A. Vigliano , C. F. Vigorito , E. Visentin , V. Vitale , G. Voutsinas , I. Vovk , T. Vuillaume , M. Vázquez Acosta , R. Walter , Z. Wei , M. Will , T. Yamamoto , R. Yamazaki , T. Yoshida , T. Yoshikoshi , N. Zywucka