Bianciotto M, Abdellaoui G, Abe S, Adams JH, Allard D, Alonso G, Anchordoqui L, Anzalone A, Arnone E, Asano K, Attallah R, Attoui H, Ave Pernas M, Bagheri M, Baláz J, Bakiri M, Barghini D, Bartocci S, Battisti M, Bayer J, Beldjilali B, Belenguer T, Belkhalfa N, Bellotti R, Belov AA, Benmessai K, Bertaina M, Bertone PF, Biermann PL, Bisconti F, Blaksley C, Blanc N, Blin-Bondil S, Bobik P, Bogomilov M, Bolmgren K, Bozzo E, Briz S, Bruno A, Caballero KS, Cafagna F, Cambié G, Campana D, Capdevielle JN, Capel F, Caramete A, Caramete L, Carlson P, Caruso R, Casolino M, Cassardo C, Castellina A, Catalano O, Cellino A, Černý K, Chikawa M, Chiritoi G, Christl MJ, Colalillo R, Conti L, Cotto G, Crawford HJ, Cremonini R, Creusot A, de Castro Gónzalez A, de la Taille C, del Peral L, Diaz Damian A, Diesing R, Dinaucourt P, Djakonow A, Djemil T, Ebersoldt A, Ebisuzaki T, Eser J, Fenu F, Fernández-González S, Ferrarese S, Filippatos G, Finch WI, Fornaro C, Fouka M, Franceschi A, Franchini S, Fuglesang C, Fujii T, Fukushima M, Galeotti P, García-Ortega E, Gardiol D, Garipov GK, Gascón E, Gazda E, Genci J, Golzio A, González Alvarado C, Gorodetzky P, Green A, Guarino F, Guépin C, Guzmán A, Hachisu Y, Haungs A, Hernández Carretero J, Hulett L, Ikeda D, Inoue N, Inoue S, Isgrò F, Itow Y, Jammer T, Jeong S, Joven E, Judd EG, Jochum J, Kajino F, Kajino T, Kalli S, Kaneko I, Karadzhov Y, Kasztelan M, Katahira K, Kawai K, Kawasaki Y, Kedadra A, Khales H, Khrenov BA, Kim JS, Kim SW, Kleifges M, Klimov PA, Kolev D, Kreykenbohm I, Krizmanic JF, Królik K, Kungel V, Kurihara Y, Kusenko A, Kuznetsov E, Lahmar H, Lakhdari F, Licandro J, López Campano L, López Martínez F, Mackovjak S, Mahdi M, Mandát D, Manfrin M, Marcelli L, Marcos JL, Marszał W, Martín Y, Martinez O, Mase K, Matev R, Matthews JN, Mebarki N, Medina-Tanco G, Menshikov A, Merino A, Mese M, Meseguer J, Meyer SS, Mimouni J, Miyamoto H, Mizumoto Y, Monaco A, Morales de los Ríos JA, Mastafa M, Nagataki S, Naitamor S, Napolitano T, Nachtman JM, Neronov A, Nomoto K, Nonaka T, Ogawa T, Ogio S, Ohmori H, Olinto AV, Onel Y, Osteria G, Otte AN, Pagliaro A, Painter W, Panasyuk MI, Panico B, Parizot E, Park IH, Pastircak B, Paul T, Pech M, Pérez-Grande I, Perfetto F, Peter T, Picozza P, Pindado S, Piotrowski LW, Piraino S, Plebaniak Z, Pollini A, Popescu EM, Prevete R, Prévôt G, Prieto H, Przybylak M, Puehlhofer G, Putis M, Reardon P, Reno MH, Reyes M, Ricci M, Rodríguez Frías MD, Romero Matamala OF, Ronga F, Sabau MD, Saccá G, Sáez Cano G, Sagawa H, Sahnoune Z, Saito A, Sakaki N, Salazar H, Sanchez Balanzar JC, Sánchez JL, Santangelo A, Sanz-Andrés A, Sanz Palomino M, Saprykin OA, Sarazin F, Sato M, Scagliola A, Schanz T, Schieler H, Schovánek P, Scotti V, Serra M, Sharakin SA, Shimizu HM, Shinozaki K, Soriano JF, Sotgiu A, Stan I, Strharský I, Sugiyama N, Supanitsky D, Suzuki M, Szabelski J, Tajima N, Tajima T, Takahashi Y, Takeda M, Takizawa Y, Talai MC, Tameda Y, Tenzer C, Thomas SB, Tibolla O, Tkachev LG, Tomida T, Tone N, Toscano S, Traïche M, Tsunesada Y, Tsuno K, Turriziani S, Uchihori Y, Vaduvescu O, Valdés-Galicia JF, Vallania P, Valore L, Vankova-Kirilova G, Venters TM, Vigorito C, Villaseñor L, Vlcek B, von Ballmoos P, Vrabel M, Wada S, Watanabe J, Watts J, Weigand Muñoz R, Weindl A, Wiencke L, Wille M, Wilms J, Winn D, Yamamoto T, Yang J, Yano H, Yashin IV, Yonetoku D, Yoshida S, Young R, Zgura IS, Zotov MY, Zuccaro Marchi A (2022)
Publication Type: Conference contribution
Publication year: 2022
Publisher: Sissa Medialab Srl
Book Volume: 395
Conference Proceedings Title: Proceedings of Science
Event location: Virtual, Berlin, DEU
K-EUSO is a planned mission of the JEM-EUSO program for the study of ultra-high energy cosmic rays (UHECR) from space, to be deployed on the International Space Station. The K-EUSO observatory consists of a UV telescope with a wide field of view, which aims at the detection of fluorescence light emitted by extensive air showers (EAS) in the atmosphere. The EAS events will be sampled with a time resolution of 1-2.5 μs to reconstruct the entire shower profile with high precision. The detector consisting of ∼ 105 independent pixels will allow a spatial resolution of ∼700 m on ground. From a 400 km altitude, K-EUSO will achieve a large and full sky exposure to sample the highest energy range of the UHECR spectrum. In this contribution, we present estimates of the performance of the observatory: an estimation of the expected exposure and triggered event rate as a function of energy and the event reconstruction performance, including resolution of arrival directions and energy of UHECRs.
APA:
Bianciotto, M., Abdellaoui, G., Abe, S., Adams, J.H., Allard, D., Alonso, G.,... Zuccaro Marchi, A. (2022). Expected performance of the K-EUSO space-based observatory. In Proceedings of Science. Virtual, Berlin, DEU: Sissa Medialab Srl.
MLA:
Bianciotto, Marta, et al. "Expected performance of the K-EUSO space-based observatory." Proceedings of the 37th International Cosmic Ray Conference, ICRC 2021, Virtual, Berlin, DEU Sissa Medialab Srl, 2022.
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