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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 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

Neural networks as well as other methods of machine learning (ML) are known to be highly efficient in different classification tasks, including classification of images and videos. Mini- EUSO is a wide-field-of-view imaging telescope that…

TUS (Tracking Ultraviolet Set-up) is the world's first orbital detector of ultra-high-energy cosmic rays (UHECRs). It was launched into orbit on 28th April 2016 as a part of the scientific payload of the Lomonosov satellite. The main aim of…

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 flux of ultra-high energy (UHE) cosmic rays (CRs) depends on the cosmic distribution of their sources. Data from CR observations are yet inconclusive about their exact location or distribution, but provide a measure for the average…

Cosmology and Nongalactic Astrophysics · Physics 2013-06-06 Markus Ahlers , Luis A. Anchordoqui , Angela V. Olinto , Thomas C. Paul , Andrew M. Taylor

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

EUSO-TA is a ground-based florescence detector built to validate the design of an ultra-high energy cosmic ray fluorescence detector to be operated in space. EUSO-TA detected the first air shower events with the technology developed within…

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 second generation of the Extreme Universe Space Observatory on a Super Pressure Balloon (EUSO-SPB2) is a balloon instrument that searched for ultra high energy cosmic rays (UHECRs) with energies above 1 EeV and very high energy…

Instrumentation and Methods for Astrophysics · Physics 2023-10-16 Rebecca Diesing , Stephan S. Meyer , Johannes Eser , Alexa Bukowski , Alex Miller , Jake Apfel , Gerard Beck , Angela V. Olinto

JEM-EUSO is a mission to study ultra-high-energy cosmic rays (UHECRs) by measuring the fluorescence light from giant air showers at the altitude of the International Space Station. In the tilted mode, JEM-EUSO will become very sensitive to…

High Energy Astrophysical Phenomena · Physics 2009-08-05 Katsuaki Asano , Kenji Shinozaki , Masahiro Teshima

EUSO-Balloon is a pathfinder mission for the Extreme Universe Space Observatory onboard the Japanese Experiment Module (JEM-EUSO). It was launched on the moonless night of the 25$^{th}$ of August 2014 from Timmins, Canada. The flight ended…

Instrumentation and Methods for Astrophysics · Physics 2018-08-09 G. Abdellaoui , S. Abe , J. H. Adams , A. Ahriche , D. Allard , L. Allen , G. Alonso , L. Anchordoqui , A. Anzalone , Y. Arai , K. Asano , R. Attallah , H. Attoui , M. Ave Pernas , S. Bacholle , M. Bakiri , P. Baragatti , P. Barrillon , S. Bartocci , J. Bayer , B. Beldjilali , T. Belenguer , N. Belkhalfa , R. Bellotti , A. Belov , K. Belov , K. Benmessai , M. Bertaina , P. L. Biermann , S. Biktemerova , F. Bisconti , N. Blanc , J. Błȩcki , S. Blin-Bondil , P. Bobik , M. Bogomilov , E. Bozzo , A. Bruno , K. S. Caballero , F. Cafagna , D. Campana , J-N. Capdevielle , F. Capel , A. Caramete , L. Caramete , P. Carlson , R. Caruso , M. Casolino , C. Cassardo , A. Castellina , C. Catalano O. Catalano , A. Cellino , M. Chikawa , G. Chiritoi , M. J. Christl , V. Connaughton , L. Conti , G. Cordero , G. Cotto , H. J. Crawford , R. Cremonini , S. Csorna , A. Cummings , S. Dagoret-Campagne , C. De Donato , C. de la Taille , C. De Santis , L. del Peral , M. Di Martino , A. Diaz Damian , T. Djemil , I. Dutan , A. Ebersoldt , T. Ebisuzaki , R. Engel , J. Eser , F. Fenu , S. Fernández-González , J. Fernández-Soriano , S. Ferrarese , M. Flamini , C. Fornaro , M. Fouka , A. Franceschi , S. Franchini , C. Fuglesang , T. Fujii , J. Fujimoto , M. Fukushima , P. Galeotti , E. García-Ortega , G. Garipov , E. Gascón , J. Genci , G. Giraudo , C. González Alvarado , P. Gorodetzky , R. Greg , F. Guarino , A. Guzmán , Y. Hachisu , M. Haiduc , B. Harlov , A. Haungs , J. Hernández Carretero , W. Hidber Cruz , D. Ikeda , N. Inoue , S. Inoue , F. Isgrò , Y. Itow , T. Jammer , S. Jeong , E. Joven , E. G. Judd , A. Jung , J. Jochum , F. Kajino , T. Kajino , S. Kalli , I. Kaneko , Y. Karadzhov , J. Karczmarczyk , K. Katahira , K. Kawai , Y. Kawasaki , A. Kedadra , H. Khales , B. A. Khrenov , Jeong-Sook Kim , Soon-Wook Kim , M. Kleifges , P. A. Klimov , D. Kolev , H. Krantz , I. Kreykenbohm , K. Kudela , Y. Kurihara , A. Kusenko , E. Kuznetsov , A. La Barbera , C. Lachaud , H. Lahmar , F. Lakhdari , R. Larson , O. Larsson , J. Lee , J. Licandro , L. López Campano , M. C. Maccarone , S. Mackovjak , M. Mahdi , D. Maravilla , L. Marcelli , J. L. Marcos , A. Marini , W. Marszał , K. Martens , Y. Martín , O. Martinez , M. Martucci , G. Masciantonio , K. Mase , M. Mastafa , R. Matev , J. N. Matthews , N. Mebarki , G. Medina-Tanco , M. A. Mendoza , A. Menshikov , A. Merino , J. Meseguer , S. S. Meyer , J. Mimouni , H. Miyamoto , Y. Mizumoto , A. Monaco , J. A. Morales de los Ríos , C. Moretto S. Nagataki , S. Naitamor , T. Napolitano , W. Naslund , R. Nava , A. Neronov , K. Nomoto , T. Nonaka , T. Ogawa , S. Ogio , H. Ohmori , A. V. Olinto , P. Orleański , G. Osteria , A. Pagliaro , W. Painter , M. I. Panasyuk , B. Panico , G. Pasqualino , E. Parizot , I. H. Park , B. Pastircak , T. Patzak , T. Paul , I. Pérez-Grande , F. Perfetto , T. Peter , P. Picozza , S. Pindado , L. W. Piotrowski , S. Piraino , L. Placidi , Z. Plebaniak , S. Pliego , A. Pollini , Z. Polonski , E. M. Popescu , P. Prat , G. Prévôt , H. Prieto , G. Puehlhofer , M. Putis , J. Rabanal , A. A. Radu , M. Reyes , M. Rezazadeh , M. Ricci , M. D. Rodríguez Frías , M. Rodencal , F. Ronga , G. Roudil , I. Rusinov , M. Rybczyński , M. D. Sabau , G. Sáez Cano , H. Sagawa , Z. Sahnoune , A. Saito , N. Sakaki , H. Salazar , J. C. Sanchez Balanzar , J. L. Sánchez , A. Santangelo , A. Sanz-Andrés , M. Sanz Palomino , O. Saprykin , F. Sarazin , M. Sato , T. Schanz , H. Schieler , V. Scotti , S. Selmane , D. Semikoz , M. Serra , S. Sharakin , H. M. Shimizu , K. Shinozaki , T. Shirahama , B. Spataro , I. Stan , T. Sugiyama , D. Supanitsky , M. Suzuki , B. Szabelska , J. Szabelski , N. Tajima , T. Tajima , Y. Takahashi , H. Takami , M. Takeda , Y. Takizawa , M. C. Talai , C. Tenzer , S. B. Thomas , O. Tibolla , L. Tkachev , H. Tokuno , T. Tomida , N. Tone , S. Toscano , M. Traïche , R. Tsenov , Y. Tsunesada , K. Tsuno , J. Tubbs , S. Turriziani , Y. Uchihori , O. Vaduvescu , J. F. Valdés-Galicia , P. Vallania , G. Vankova , C. Vigorito , L. Villaseñor , B. Vlcek , P. von Ballmoos , M. Vrabel , S. Wada , J. Watanabe , J. Watts , M. Weber , R. Weigand Muñoz , A. Weindl , L. Wiencke , M. Wille , J. Wilms , Z. Włodarczyk , T. Yamamoto , J. Yang , H. Yano , I. V. Yashin , D. Yonetoku , S. Yoshida , R. Young , I. S Zgura , M. Yu. Zotov , A. Zuccaro Marchi

Observing ultra-high energy cosmic rays (UHECR) and very high energy (VHE) neutrinos from space is a promising way to measure their extremely low fluxes by significantly increasing the observed volume. The Extreme Universe Space Observatory…

High Energy Astrophysical Phenomena · Physics 2023-09-01 Johannes Eser , Angela V. Olinto , Lawrence Wiencke

EUSO-TA is a ground-based experiment, placed at Black Rock Mesa of the Telescope Array site as a part of the JEM-EUSO (Joint Experiment Missions for the Extreme Universe Space Observatory) program. The UV fluorescence imaging telescope with…

Instrumentation and Methods for Astrophysics · Physics 2021-12-21 Z. Plebaniak , M. Przybylak , D. Barghini , M. Bertaina , F. Bisconti , M. Casolino , D. Gardiol , R. Lipiec , L. W. Piotrowski , K. Shinozaki , J. Szabelski

The TurLab facility is a laboratory, equipped with a 5 m diameter and 1 m depth rotating tank, located in the Physics Department of the University of Turin. Originally, it was mainly built to study systems of different scales where rotation…

In 2016, the NASA Juno spacecraft will initiate its one-year mission around Jupiter and become the first probe to explore the polar regions of Jupiter. The HST UV instruments (STIS and ACS) can greatly contribute to the success of the Juno…

The Joint Experiment Missions for Extreme Universe Observatory comprises a collection of complementary missions dedicated to pioneering technologies and techniques for a future space-based multi-messenger observatory which will have…

Instrumentation and Methods for Astrophysics · Physics 2023-10-10 Thomas C. Paul

The Tracking Ultraviolet Set-up (TUS) is the world's first orbital imaging detector of Ultra High Energy Cosmic Rays (UHECR) and it operated in 2016-2017 as part of the scientific equipment of the Lomonosov satellite. The TUS was developed…

Instrumentation and Methods for Astrophysics · Physics 2021-08-11 S. Sharakin , O. I. Ruiz Hernandez

The Extreme Universe Space Observatory on a Super Pressure Balloon (EUSO-SPB1) is the second balloon pathfinder of the JEM-EUSO collaboration. It is a nadir pointing UV telescope which aims at observing Ultra High Energy Cosmic Rays (UHECR)…

Instrumentation and Methods for Astrophysics · Physics 2019-09-19 Abraham Diaz Damian