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Related papers: JEM-EUSO Science Objectives

200 papers

Mini-EUSO is a telescope launched on board the International Space Station in 2019 and currently located in the Russian section of the station. Main scientific objectives of the mission are the search for nuclearites and Strange Quark…

EUSO experiment, while monitoring the downward Earth atmosphere layers, may observe among common Ultra High Energy Cosmic Rays, UHECR, also High Energy Neutrino-Induced Showers either blazing upward to the detectors at high (PeVs) energies…

Astrophysics · Physics 2016-08-30 D. Fargion

Astrophysical Very-High-Energy (VHE, >10PeV) neutrinos deliver crucial information about the sources of Ultra-High-Energy Cosmic Rays (UHECRs), the composition of UHECRs, and neutrino/particle physics at highest energies. UHE-tau neutrinos…

Instrumentation and Methods for Astrophysics · Physics 2023-08-31 Eliza Gazda

The two main advantages of space-based observation of extreme-energy ($\gtrsim 10^{19}$~eV) cosmic-rays (EECRs) over ground-based observatories are the increased field of view, and the all-sky coverage with nearly uniform systematics of an…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Peter B. Denton , Luis A. Anchordoqui , Andreas A. Berlind , Matthew Richardson , Thomas J. Weiler

One of the main impacts of the JEM-EUSO mission will come from its unprecedented exposure. This feature creates, for the first time in the field, the possibility of studying individual UHECR sources. However, the intrinsic characteristics…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Gustavo Medina-Tanco

The Extreme Universe Space Observatory on a Super Pressure Balloon II (EUSO-SPB2) is a second generation stratospheric balloon instrument for the detection of Ultra High Energy Cosmic Rays (UHECRs, E > 1 EeV) via the fluorescence technique…

Instrumentation and Methods for Astrophysics · Physics 2022-09-21 J. Eser , A. V. Olinto , L. Wiencke

Mini-EUSO (Extreme Universe Space Observatory) is a small-scale prototype cosmic-ray detector that will measure Earth`s UV emission and other atmospheric phenomena from space. It will be placed in the International Space Station (ISS)…

Instrumentation and Methods for Astrophysics · Physics 2019-09-11 Viktoria Kungel , Mario E. Bertaina , Francesca Bisconti , Marco Casolino , Johannes Eser , Lawrence Wiencke , JEM-EUSO Collaboration

Doing astronomy with photons of energies in excess of a GeV has turned out to be extremely challenging. Efforts are underway to develop instruments that may push astronomy to wavelengths smaller than $10^{-14}$~cm by mapping the sky in high…

High Energy Physics - Phenomenology · Physics 2009-10-28 F. Halzen

The JEM-EUSO Collaboration aims at studying Ultra High Energy Cosmic Rays (UHECR) from space. To reach this goal, a series of pathfinder missions has been developed to prove the observation principle and to raise the technological readiness…

Instrumentation and Methods for Astrophysics · Physics 2020-10-30 Valentina Scotti , Giuseppe Osteria , Francesco Perfetto

EUSO--TA is a ground-based telescope installed in 2013 in the Black Rock Mesa Telescope Array (BRM-TA) site, operating with 2.5$\mu$s time resolution to observe the night sky in the UV range. The optical system contains two 1m$^2$ Fresnel…

Instrumentation and Methods for Astrophysics · Physics 2023-09-19 Zbigniew Plebaniak

The latest and most advanced effort towards a space-based optical cosmic ray detector developed within the Joint Experiment Mission for the Extreme Universe Space Observatory (JEM-EUSO) collaboration was the Extreme Universe Space…

Instrumentation and Methods for Astrophysics · Physics 2019-09-27 J. Eser , A. Olinto , L. Wiencke

JEM-EUSO is an international program for the development of space based Ultra High Cosmic Ray observatories. The program consists of a series of missions which are either under development or in the data analysis phase. The instruments…

High Energy Astrophysical Phenomena · Physics 2019-09-27 Francesco Fenu , Kenji Shinozaki , Hiroko Miyamoto , Alessandro Liberatore , Naoto Sakaki , Sergei Sharakin , Mikhail Zotov , Gabriel Chiritoi

Mini-EUSO is a UV telescope that will look downwards to the Earth's atmosphere onboard the International Space Station. With the design of the ultra-high energy cosmic ray fluorescence detectors belonging to the JEM-EUSO program, it will…

Mini-EUSO is the first space-borne detector of the JEM-EUSO (Joint Exploratory Missions for Extreme Universe Space Observatory) program, operating on the International Space Station (ISS) since October 2019. Designed to search for…

Instrumentation and Methods for Astrophysics · Physics 2026-01-19 Matteo Battisti

The Global Cosmic-ray Observatory (GCOS) is a proposed large-scale observatory for studying ultra-high-energy cosmic particles, including ultra-high-energy cosmic rays (UHECRs), photons, and neutrinos. Its primary goal is to characterise…

High Energy Astrophysical Phenomena · Physics 2023-10-02 Rafael Alves Batista

The Extreme Universe Space Observatory on a Super Pressure Balloon 1 (EUSO-SPB1) was launched in 2017 April from Wanaka, New Zealand. The plan of this mission of opportunity on a NASA super pressure balloon test flight was to circle the…

Instrumentation and Methods for Astrophysics · Physics 2024-01-15 EUSO Collaboration , G. Abdellaoui , S. Abe , J. H. Adams. , D. Allard , G. Alonso , L. Anchordoqui , A. Anzalone , E. Arnone , K. Asano , R. Attallah , H. Attoui , M. Ave Pernas , R. Bachmann , S. Bacholle , M. Bagheri , M. Bakiri , J. Baláz , D. Barghini , S. Bartocci , M. Battisti , J. Bayer , B. Beldjilali , T. Belenguer , N. Belkhalfa , R. Bellotti , A. A. Belov , K. Benmessai , M. Bertaina , P. F. Bertone , P. L. Biermann , F. Bisconti , C. Blaksley , N. Blanc , S. Blin-Bondil , P. Bobik , M. Bogomilov , K. Bolmgren , E. Bozzo , S. Briz , A. Bruno , K. S. Caballero , F. Cafagna , G. Cambié , D. Campana , J. N. Capdevielle , F. Capel , A. Caramete , L. Caramete , R. Caruso , M. Casolino , C. Cassardo , A. Castellina , O. Catalano , A. Cellino , K. Černý , M. Chikawa , G. Chiritoi , M. J. Christl , R. Colalillo , L. Conti , G. Cotto , H. J. Crawford , R. Cremonini , A. Creusot , A. Cummings , A. de Castro Gónzalez , C. de la Taille , L. del Peral , J. Desiato , A. Diaz Damian , R. Diesing , P. Dinaucourt , A. Djakonow , T. Djemil , A. Ebersoldt , T. Ebisuzaki , J. Eser , F. Fenu , S. Fernández-González , S. Ferrarese , G. Filippatos , W. Finch , C. Fornaro , M. Fouka , A. Franceschi , S. Franchini , C. Fuglesang , T. Fujii , M. Fukushima , P. Galeotti , E. García-Ortega , D. Gardiol , G. K. Garipov , E. Gascón , E. Gazda , J. Genci , A. Golzio , P. Gorodetzky , R. Gregg , A. Green , F. Guarino , C. Guépin , A. Guzmán , Y. Hachisu , A. Haungs , T. Heigbes , J. Hernández Carretero , L. Hulett , D. Ikeda , N. Inoue , S. Inoue , F. Isgrò , Y. Itow , T. Jammer , S. Jeong , J. Jochum , E. Joven , E. G. Judd , A. Jung , F. Kajino , T. Kajino , S. Kalli , I. Kaneko , M. Kasztelan , K. Katahira , K. Kawai , Y. Kawasaki , A. Kedadra , H. Khales , B. A. Khrenov , Jeong-Sook Kim , Soon-Wook Kim , M. Kleifges , P. A. Klimov , I. Kreykenbohm , J. F. Krizmanic , K. Królik , V. Kungel , Y. Kurihara , A. Kusenko , E. Kuznetsov , H. Lahmar , F. Lakhdari , J. Licandro , L. López Campano , F. López Martínez , S. Mackovjak , M. Mahdi , D. Mandát , M. Manfrin , L. Marcelli , J. L. Marcos , W. Marszał , Y. Martín , O. Martinez , K. Mase , M. Mastafa , J. N. Matthews , N. Mebarki , G. Medina-Tanco , A. Menshikov , A. Merino , M. Mese , J. Meseguer , S. S. Meyer , J. Mimouni , H. Miyamoto , Y. Mizumoto , A. Monaco , J. A. Morales de los Ríos , J. M. Nachtman , S. Nagataki , S. Naitamor , T. Napolitano , A. Neronov , K. Nomoto , T. Nonaka , T. Ogawa , S. Ogio , H. Ohmori , A. V. Olinto , Y. Onel , G. Osteria , A. N. Otte , A. Pagliaro , W. Painter , M. I. Panasyuk , B. Panico , E. Parizot , I. H. Park , B. Pastircak , T. Paul , M. Pech , I. Pérez-Grande , F. Perfetto , T. Peter , P. Picozza , S. Pindado , L. W. Piotrowski , S. Piraino , Z. Plebaniak , A. Pollini , E. M. Popescu , R. Prevete , G. Prévôt , H. Prieto , M. Przybylak , G. Puehlhofer , M. Putis , P. Reardon , M. H. Reno , M. Reyes , M. Ricci , M. D. Rodríguez Frías , O. F. Romero Matamala , F. Ronga , M. D. Sabau , G. Saccá , H. Sagawa , Z. Sahnoune , A. Saito , N. Sakaki , H. Salazar , J. L. Sánchez , J. C. Sanchez Balanzar , A. Santangelo , A. Sanz-Andrés , O. A. Saprykin , F. Sarazin , M. Sato , A. Scagliola , T. Schanz , H. Schieler , P. Schovánek , V. Scotti , M. Serra , S. A. Sharakin , H. M. Shimizu , K. Shinozaki , J. F. Soriano , A. Sotgiu , I. Stan , I. Strharský , N. Sugiyama , D. Supanitsky , M. Suzuki , J. Szabelski , N. Tajima , T. Tajima , Y. Takahashi , M. Takeda , Y. Takizawa , M. C. Talai , Y. Tameda , C. Tenzer , S. B. Thomas , O. Tibolla , L. G. Tkachev , T. Tomida , N. Tone , S. Toscano , M. Traïche , Y. Tsunesada , K. Tsuno , S. Turriziani , Y. Uchihori , J. F. Valdés-Galicia , P. Vallania , L. Valore , G. Vankova-Kirilova , T. M. Venters , C. Vigorito , L. Villaseñor , B. Vlcek , P. von Ballmoos , M. Vrabel , S. Wada , J. Watanabe , J. Watts. , R. Weigand Muñoz , A. Weindl , L. Wiencke , M. Wille , J. Wilms , T. Yamamoto , J. Yang , H. Yano , I. V. Yashin , D. Yonetoku , S. Yoshida , R. Young , I. S. Zgura , M. Yu. Zotov , A. Zuccaro Marchi

The TUS observatory was the first orbital detector aimed at the detection of ultra-high energy cosmic rays (UHECRs). It was launched on April 28, 2016, from the Vostochny cosmodrome in Russia and operated until December 2017. It collected…

High Energy Astrophysical Phenomena · Physics 2021-12-22 Francesco Fenu , Kenji Shinozaki , Mikhail Zotov , Mario Bertaina , Antonella Castellina , Alberto Cellino , Pavel Klimov

The possibility of directly detecting Ultra-high energy (UHE from now on) WIMPs are considered by the WIMPs interaction with the nuclei in the air. Since neutrinos dominate the events from the spherical crown near JEM-EUSO, all the events…

High Energy Astrophysical Phenomena · Physics 2019-10-11 Ye Xu

Mini-EUSO is a telescope observing the Earth in the ultraviolet band (290-430 nm) since 2019, through a nadir-facing UV-transparent window in the Russian Zvezda module of the International Space Station. The main camera has an optical…

Instrumentation and Methods for Astrophysics · Physics 2023-09-22 Laura Marcelli