Abdellaoui G, Abe S, Adams JH, Ahriche A, Allard D, Allen L, Alonso G, Anchordoqui L, Anzalone A, Arai Y, Asano K, Attallah R, Attoui H, Ave Pernas M, Bacholle S, Bakiri M, Baragatti P, Barrillon P, Bartocci S, Bayer J, Beldjilali B, Belenguer T, Belkhalfa N, Bellotti R, Belov A, Belov K, Belz JW, Benmessai K, Bertaina M, Biermann PL, Biktemerova S, Bisconti F, Blanc N, Blecki J, Blin-Bondil S, Bobik P, Bogomilov M, Bozzo E, Bruno A, Caballero KS, Cafagna F, Campana D, Capdevielle JN, Capel F, Caramete A, Caramete L, Carlson P, Caruso R, Casolino M, Cassardo C, Castellina A, Catalano O, Cellino A, Chikawa M, Chiritoi G, Christl MJ, Connaughton V, Conti L, Cordero G, Cotto G, Crawford HJ, Cremonini R, Csorna S, Cummings A, Dagoret-Campagne S, De Donato C, De La Taille C, De Santis C, Del Peral L, Di Martino M, Djemil T, Dutan I, Ebersoldt A, Ebisuzaki T, Engel R, Eser J, Fenu F, Fernandez-Gonzalez S, Fernandez-Soriano J, Ferrarese S, Flamini M, Fornaro C, Fouka M, Franceschi A, Franchini S, Fuglesang C, Fujii T, Fujimoto J, Fukushima M, Galeotti P, Garcia-Ortega E, Garipov G, Gascon E, Genci J, Giraudo G, Gonzalez Alvarado C, Gorodetzky P, Greg R, Guarino E, Guzman A, Hachisu Y, Haiduc M, Harlov B, Haungs A, Hernandez Carretero J, Hidber Cruz W, Ikeda D, Inoue N, Inoue S, Isgro F, Itow Y, Jammer T, Jeong S, Joven E, Judd EG, Jung A, Jochum J, Kajino E, Kajino T, Kalli S, Kaneko I, Karadzhov Y, Karczmarczyk J, Katahira K, Kawai K, Kawasaki Y, Kedadra A, Khales H, Khrenov BA, Kim JS, Kim SW, Kleifges M, Klimov PA, Kolev D, Krantz H, Kreykenbohm I, Kudela K, Kurihara Y, Kusenko A, Kuznetsov E, La Barbera A, Lachaud C, Lahmar H, Lakhdari F, Larsson O, Lee J, Licandro J, Lopez Campano L, Maccarone MC, Mackovjak S, Mandi M, Maravilla D, Marcelli L, Marcos JL, Marini A, Marszal W, Martens K, Martin Y, Martinez O, Martucci M, Masciantonio G, Mase K, Mustafa M, Matev R, Matthews JN, Mebarki N, Medina-Tanco G, Mendoza MA, Menshikov A, Merino A, Meseguer J, Meyer SS, Mimouni J, Miyamoto H, Mizumoto Y, Monaco A, Morales De Los Rios JA, Nagataki S, Naitamor S, Napolitano T, Nava R, Neronov A, Nomoto K, Nonaka T, Ogawa T, Ogio S, Ohmori H, Olinto AV, Orleaniski P, Osteria G, Pagliaro A, Painter W, Panasyuk MI, Panico B, Parizot E, Park IH, Pastircak B, Patzak T, Paul T, Perez-Grande I, Perfetto F, Peter T, Picozza P, Pindado S, Piotrowski LW, Piraino S, Placidi L, Plebaniak Z, Pliego S, Pollini A, Polonski Z, Popescu EM, Prat P, Prevot G, Prieto H, Puehlhofer G, Putis M, Rabanal J, Radu AA, Reyes M, Rezazadeh M, Ricci M, Rodriguez Frias MD, Ronga F, Roudil G, Rusinov I, Rybczynski M, Sabau MD, Saez Cano G, Sagawa H, Sahnoune Z, Saito A, Sakaki N, Salazar H, Sanchez Balanzar JC, Sanchez JL, Santangelo A, Sanz-Andres A, Sanz Palomino M, Saprykin O, Sarazin F, Sato M, Schanz T, Schieler H, Scotti V, Selmane S, Semikoz D, Serra M, Sharakin S, Shimizu HM, Shin HS, Shinozaki K, Shirahama T, Sokolsky P, Spataro B, Stan I, Sugiyama T, Supanitsky D, Suzuki M, Szabelska B, Szabelski J, Tajima N, Tajima T, Takahashi Y, Takami H, Takeda M, Takizawa Y, Talai MC, Tameda Y, Tenzer C, Thomas SB, Thomson GB, Tibolla O, Tkachev L, Tokuno H, Tomida T, Tone N, Toscano S, Traiche M, Tsenov R, Tsunesada Y, Tsuno K, Tubbs J, Turriziani S, Uchihori Y, Vaduvescu O, Valdes-Galicia JF, Vallania P, Vankova G, Vigorito C, Villasenor L, Vlcek B, Von Ballmoos P, Vrabel M, Wada S, Watanabe J, Watts J, Weber M, Weigand Munoz R, Weindl A, Wiencke L, Wille M, Wilms J, Wlodarczyk Z, Yamamoto T, Yang J, Yano H, Yashin IV, Yonetoku D, Yoshida S, Young R, Zgura IS, Zotov MY, Marchi AZ (2018)
Publication Status: Published
Publication Type: Journal article
Publication year: 2018
Publisher: ELSEVIER SCIENCE BV
Book Volume: 102
Pages Range: 98-111
DOI: 10.1016/j.astropartphys.2018.05.007
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 degrees x 10.6 degrees 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 (similar to 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. (C) 2018 Elsevier B.V. All rights reserved.
APA:
Abdellaoui, G., Abe, S., Adams, J.H., Ahriche, A., Allard, D., Allen, L.,... Marchi, A.Z. (2018). EUSO-TA - First results from a ground-based EUSO telescope. Astroparticle Physics, 102, 98-111. https://dx.doi.org/10.1016/j.astropartphys.2018.05.007
MLA:
Abdellaoui, G., et al. "EUSO-TA - First results from a ground-based EUSO telescope." Astroparticle Physics 102 (2018): 98-111.
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