Zobrazeno 1 - 2
of 2
pro vyhledávání: '"Fouque, Nadia"'
Autor:
Nozaki, Seiya, Awai, Kyosuke, Bamba, Aya, Barrio, Juan Abel, Bernardos, Maria Isabel, Blanch, Oscar, Boix, Joan, Cassol, Franca, Choushi, Yuki, Delgado, Carlos, Diaz, Carlos, Fouque, Nadia, Freixas, Lluis, Gliwny, Pawel, Gunji, Shunichi, Hadasch, Daniela, Hoffmann, Dirk, Houles, Julien, Inome, Yusuke, Iwamura, Yuki, Jouvin, Léa, Katagiri, Hideaki, Kawamura, Kiomei, Kerszberg, Daniel, Konno, Yusuke, Kubo, Hidetoshi, Kushida, Junko, Kobayashi, Yukiho, López-Coto, Rubén, Martinez, Gustavo, Masuda, Shu, Mazin, Daniel, Moralejo, Abelardo, Moretti, Elena, Nagayoshi, Tsutomu, Nakamori, Takeshi, Nishijima, Kyoshi, Nogami, Yuto, Nogués, Leyre, Ohoka, Hideyuki, Oka, Tomohiko, Okazaki, Nao, Okumura, Akira, Orito, Reiko, Panazol, Jean-Luc, Paoletti, Riccardo, Pio, Cristobal, Polo, Miguel, Prast, Julie, Saito, Takayuki, Sakurai, Shunsuke, Sitarek, Julian, Sunada, Yuji, Suzuki, Megumi, Takahashi, Mitsunari, Tamura, Kenji, Tanaka, Manobu, Tejedor, Luis Angel, Terada, Yukikatsu, Teshima, Masahiro, Tsukamoto, Yusuke, Yamamoto, Tokonatsu
The Cherenkov Telescope Array (CTA) is the next-generation ground-based very-high-energy gamma-ray observatory. The Large-Sized Telescope (LST) of CTA is designed to detect gamma rays between 20 GeV and a few TeV with a 23-meter diameter mirror. We h
Externí odkaz:
http://arxiv.org/abs/2203.06582
Autor:
Rando, Riccardo, Corti, Daniele, Dazzi, Francesco, De Angelis, Alessandro, Dettlaff, Antonios, Dorner, Daniela, Fink, David, Fouque, Nadia, Grundner, Felix, Haberer, Werner, Hahn, Alexander, Hermel, Richard, Korpar, Samo, Mezek, Gašper Kukec, Maier, Ronald, Manea, Christian, Mariotti, Mosè, Mazin, Daniel, Mehrez, Fatima, Mirzoyan, Razmik, Podkladkin, Sergey, Reichardt, Ignasi, Rhode, Wolfgang, Rosier, Sylvie, Schultz, Cornelia, Stella, Carlo, Teshima, Masahiro, Wetteskind, Holger, Zavrtanik, Marko
The Cherenkov Telescope Array (CTA) is the the next generation facility of imaging atmospheric Cherenkov telescopes; two sites will cover both hemispheres. CTA will reach unprecedented sensitivity, energy and angular resolution in very-high-energy ga
Externí odkaz:
http://arxiv.org/abs/1508.07120