Technical and scientific performance of the prototype Schwarzschild-Couder Telescope for CTA

Autor: Mirco Caprai, Olivier Hervet, Robert Halliday, Giovanni Pareschi, Qi Feng, Massimo Capasso, Richard G. Bose, Peter Y. Yu, Daniel Nieto, Luca Tosti, L. P. Taylor, Hiroyasu Tajima, Samuel A. Mognet, Maria Ionica, Wystan Benbow, David Kieda, Julien Rousselle, Francesca R. Pantaleo, Corbin Covault, Massimo Valentino, Vincenzo Masone, Leonardo Di Venere, Rodolfo Canestrari, Massimiliano Bitossi, Andrea Rugliancich, Gagik Tovmassian, Jamie Holder, D. Ross, Leonardo Stiaccini, Enrico Giro, Emanuale Fiandrini, Riccardo Paoletti, Pedro I. Batista, Giovanni Ambrosi, Valerio Vagelli, Carla Aramo, Richard White, Simone Incardona, Federico Di Pierro, Anthony M. Brown, Francesco Giordano, Nicola Giglietto, A. Zink, Ruo-Yu Shang, K. Meagher, Jason J. Watson, J. H. Buckley, N. Otte, B. A. W. Mode, Bruna Bertucci, Thomas Meures, Marcos Santander, Michelangelo Ambrosio, Vladimir V. Vassiliev, Luca Riitano, Reshmi Mukherjee, Stephen Fegan, W. Jin, Alfonso Boiano, Colin B. Adams, Akira Okumura, Justin Vanderbrouke, Carmela Bonavolontà, Giovanni Tripodo, Manel Errando, David A. Williams, A. Brill, E. Roache, D. Ribeiro, Giovanni Marsella, Francesco Licciulli, Elisa Pueschel, Elisabetta Bissaldi, Davide Depaoli, Thomas B. Humensky, Amy Furniss, Serena Loporchio, Alasdair E. Gent

The Cherenkov Telescope Array (CTA) is the next-generation ground-based observatory for very-high-energy gamma rays. One candidate design for CTA's medium-sized telescopes consists of the Schwarzschild-Couder Telescope (SCT), featuring innovative dua

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http://hdl.handle.net/11391/1502966