D. Nakajima
Max Planck Society
2 Papers
11 Citations
D. Nakajima is an academic researcher from Max Planck Society. The author has contributed to research in topics: Cherenkov Telescope Array & Telescope. The author has an hindex of 2, co-authored 2 publications.
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Papers
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Mirror Development for the Cherenkov Telescope Array
A. Förster,T. Armstrong,H. Baba,J. Bähr,A. Bonardi,Giacomo Bonnoli,Pierre Brun,Rodolfo Canestrari,P. M. Chadwick,M. Chikawa,P. H. Carton,V. de Souza,J. Dipold,Michele Doro,Dominique Durand,Michal Dyrda,Enrico Giro,J.F. Glicenstein,Y. Hanabata,M. Hayashida,M. Hrabovski,C. Jeanney,M. Kagaya,Hideaki Katagiri,Luigi Lessio,Dusan Mandat,Mosè Mariotti,C. Medina,Jerzy Michalowski,P. Micolon,D. Nakajima,Jacek Niemiec,A. Nozato,M. Palatka,G. Pareschi,Miroslav Pech,B. Peyaud,G. Pühlhofer,M. Rataj,G. Rodeghiero,G. Rojas,Julien Rousselle,R. Sakonaka,Petr Schovanek,Karol Seweryn,C. Schultz,S. Shu,F. Stinzing,Marek Stodulski,Masahiro Teshima,Masahiro Teshima,P. Travniczek,C. van Eldik,V. Vassiliev,Ł. Wiśniewski,A. Wörnlein,Tatsuo Yoshida +56 more
TL;DR: The Cherenkov Telescope Array (CTA) is a planned observatory for very-high energy gamma-ray astronomy as discussed by the authors, which will consist of several tens of telescopes of different sizes, with a total mirror area of up to 10,000 square meters.
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The large size telescope of the Cherenkov Telescope Array
G. Ambrosi,Y. Awane,H. Baba,Aya Bamba,M. Barcelo,U. Barres de Almeida,Juan Abel Barrio,O. Blanch Bigas,J. Boix,L. Brunetti,E. Carmona,E. Chabanne,M. Chikawa,R. Colin,Juan Cortina,Jose Luis Contreras,Francesco Dazzi,A. De Angelis,G. Deleglise,C. Delgado,C. Díaz,A. Fiasson,David Fink,N. Fouque,Lluis Freixas,Christian Fruck,A. Gadola,Ricardo Garcia,David Gascon,N. Geffroy,Nicola Giglietto,Francesco Giordano,F. Grañena,S. Gunji,Rika Hagiwara,N. Hamer,Y. Hanabata,Tarek M. Hassan,K. Hatanaka,Kouichi Hirotani,Susumu Inoue,Yoshiyuki Inoue,Kunihito Ioka,C. Jablonski,M. Kagaya,Hideaki Katagiri,T. Kishimoto,K. Kodani,Kazunori Kohri,Yusuke Konno,S. Koyama,Hidetoshi Kubo,J. Kushida,Giovanni Lamanna,T. Le Flour,E. Lorenz,R. Rebolo Lopez,M. López-Moya,Pratik Majumdar,A. Manalaysay,Mosè Mariotti,G. Martinez,Miriam Lucio Martinez,Daniel Mazin,Jose Miguel Miranda,R. Mirzoyan,I. Monteiro,Abelardo Moralejo,Kohta Murase,Shigehiro Nagataki,D. Nakajima,Takeshi Nakamori,K. Nishijima,Koji Noda,A. Nozato,Yutaka Ohira,Masatoshi Ohishi,Hideyuki Ohoka,Akira Okumura,Reiko Orito,J. L. Panazol,D. Paneque,R. Paoletti,J. M. Paredes,G. Pauletta,S. Podkladkin,J. Prast,R. Rando,O. Reimann,Marc Ribó,S. Rosier-Lees,K. Saito,Takashi Saito,Y. Saito,N. Sakaki,R. Sakonaka,Andreu Sanuy,H. Sasaki,Makoto Sawada,V. Scalzotto,S. Schultz,T. Schweizer,T. Shibata,S. Shu,Javier Sieiro,Victor Stamatescu,S. Steiner,U. Straumann,R. Sugawara,H. Tajima,Hajime Takami,S. Tanaka,Manabu Tanaka,Luis Ángel Tejedor,Yukikatsu Terada,Masahiro Teshima,Masahiro Teshima,Tomonori Totani,H. Ueno,K. Umehara,A. Vollhardt,Robert Wagner,H. Wetteskind,Tokonatsu Yamamoto,Ryo Yamazaki,A. Yoshida,Tatsuo Yoshida,Takanori Yoshikoshi +127 more
TL;DR: The Cherenkov Telescope Array (CTA) project as discussed by the authors aims to implement the world's largest next generation of Very High Energy gamma-ray Imaging Atmospheric Cherankov Telescopes devoted to the observation from a few tens of GeV to more than 100 TeV. The sensitivity at the lowest energy range will be dominated by four Large Size Telescopes, located at the center of each array and designed to achieve observations of high red-shift objects with the threshold energy of 20 GeV.