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Allen, L.; Baragatti, P.; Belz, J.W.; Blecki, J.; Blin-Bondil, S.; Caballero, K.S.; Cafagna, F.; Campana, D.; Capdevielle, J-N.; Capel, F.; Caramete, A.; Carlson, P.; Caruso, R.; Cassardo, C.; Cellino, A.; Chiritoi, G.; Cordero, G.; Csorna, S.; del Peral, L.; Di Martino, M.; Ebisuzaki, T.; Ferrarese, S.; Fouka, M.; Franceschi, A.; Franchini, S.; Fujimoto, J.; Galeotti, P.; García-Ortega, E.; Gascón, E.; Genci, J.; Giraudo, G.; González Alvarado, C.; Greg, R.; Hachisu, Y.; Harlov, B.; Inoue, S.; Jung, A.; Jochum, J.; Karczmarczyk, J.; Kawai, K.; Kudela, K.; Kusenko, A.; Larsson, O.; Licandro, J.; López Campano, L.; Maccarone, M.C.; Mahdi, M.; Maravilla, D.; Marcelli, L.; Marcos, J.L.; Marszal, W.; Martín, Y.; Mebarki, N.; Mendoza, M.A.; Menshikov, A.; Mizumoto, Y.; Nagataki, S.; Naitamor, S.; Napolitano, T.; Nomoto, K.; Painter, W.; Panasyuk, M.I.; Parizot, E.; Pérez-Grande, I.; Perfetto, F.; Peter, T.; Piotrowski, L.W.; Popescu, E.M.; Prieto, H.; Putis, M.; Rabanal, J.; Rybczyński, M.; Saito, A.; Sakaki, N.; Sánchez, J.L.; Sanz-Andrés, A.; Saprykin, O.; Scotti, V.; Selmane, S.; Semikoz, D.; Serra, M.; Sugiyama, T.; Szabelski, J.; Tajima, T.; Takizawa, Y.; Tameda, Y.; Tibolla, O.; Tone, N.; Tsenov, R.; Tsunesada, Y.; Tubbs, J.; Uchihori, Y.; Vaduvescu, O.; Vankova, G.; Vigorito, C.; von Ballmoos, P.; Wada, S.; Watanabe, J.; Weber, M.; Young, R.
Astroparticle physics, 11/2018, Letnik: 102Journal Article
EUSO-TA is a ground-based telescope, installed at the Telescope Array (TA) site in Black Rock Mesa, Utah, USA. This is the first detector to successfully use a Fresnel lens based optical system and multi-anode photomultipliers (64 channels per tube, 2304 channels encompassing a 10.6° × 10.6° field of view) for detection of Ultra High Energy Cosmic Rays (UHECR). The telescope is located in front of one of the fluorescence detectors of the TA experiment. Since its installation in 2013, the detector has observed several ultra-high energy cosmic ray events and, in addition, meteors. The limiting magnitude of 5.5 on summed frames ( ∼ 3 ms) has been established. Measurements of the UV night sky emission in different conditions and moon phases and positions have been completed. The performed observations serve as a proof of concept for the future application of this detector technology.
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Dostop do baze podatkov JCR je dovoljen samo uporabnikom iz Slovenije. Vaš trenutni IP-naslov ni na seznamu dovoljenih za dostop, zato je potrebna avtentikacija z ustreznim računom AAI.
Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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Povezave do osebnih bibliografij avtorjev | Povezave do podatkov o raziskovalcih v sistemu SICRIS |
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Vir: Osebne bibliografije
in: SICRIS
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