The Extreme Universe Observatory on a Super-Pressure Balloon II: Mission, payload, and flight

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Authors: James H. Adams, D. Allard, P. Alldredge, L Anchordoqui, A. Anzalone, M. Bagheri, Matteo Battisti, R. Bellotti, A. Belov, M Bertaina, P. F. Bertone, S. Blin-Bondil
+87 more J. Bogdan, J. Burton, F. Cafagna, R Caruso, M Casolino, K. Černý, M. J. Christl, Roberta Colalillo, H. J. Crawford, A. Creusot, A Cummings, Julianna Desiato, Rebecca Diesing, A. Di Nola, T. Ebisuzaki, Johannes Eser, Francesco Fenu, S. Ferrarese, George Filippatos, William W. Finch, F. Flaminio, Seamus Flannery, C. Fornaro, Noah Friedlander, D. Fuehne, C. Fuglesang, Srikar Gadamsetty, D. Garg, E. Gazda, Alessio Golzio, Fausto Guarino, C. Guépin, Tobias Heibges, E. G. Judd, Luke Kupari, Pavel Aleksandrovich Klimov, John Francis Krizmanic, Viktoria Kungel, E. Kuznetsov, Marco Mignone, Massimiliano Manfrin, W. Marszał, J. N. Matthews, Kameron Mehling, Marco Mese, S. S. Meyer, H Miyamoto, Alexey Murashov, J.M. Nachtman, Angela V. Olinto, Y. Onel, G. Osteria, A. Nepomuk Otte, B. Panico, E. Parizot, T. Paul, M. Pech, F. Perfetto, L. W. Piotrowski, Z. Plebaniak, Jonatan Alejandro Posligua, M. Potts, Guillaume Prévot, M. Przybylak, Patrick N. Reardon, M. H. Reno, Marco Ricci, O. F. Romero Matamala, Fred Sarazin, Petr Schovánek, V. Scotti, K. Shinozaki, Jorge Fernández Soriano, S Stephanoff, P. Sternberg, B. Stillwell, J. Szabelski, Y. Takizawa, D. Trofimov, Fredrik Unel, V. Vagelli, Laura Valore, T.M Venters, John W. Watts, Lawrence Wiencke, H. Wistrand, R. Young
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References: 61

Abstract

The Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2) is a pathfinder mission toward a space-based observatory such as the Probe of Extreme Multi-Messenger Astrophysics (POEMMA). The aim of POEMMA is the observation of Ultra High Energy Cosmic Rays (UHECRs) in order to elucidate their nature and origins and to discover ≳ 20 PeV very high energy neutrinos that originate from transient and steady astrophysical sources. EUSO-SPB2 was launched from Wānaka New Zealand on May 13th, 2023 as a NASA Balloon Program Office test flight. The mission goals included making the first near-space altitude observations of the fluorescence emission from UHECR-induced extensive air showers (EASs) and making the first direct Cherenkov light emission from PeV cosmic rays traversing Earth’s atmosphere. In addition, a Target of Opportunity program was developed for selecting and scheduling observations of potential neutrino sources as they passed just below the Earth’s limb. Although a leaky balloon forced termination over the Pacific Ocean after 37 h, data was collected to demonstrate the successful commissioning and operation of the instruments. This paper includes a description of the payload and the key instruments, pre-flight instrument characterizations in the lab and in the desert, flight operations and examples of the data collected. The flight was too short to catch a UHECR event via fluorescence, however about 10 candidate EAS events from cosmic rays were recorded via Cherenkov light.

Fields of Study & Subjects

Gamma-ray bursts and supernovae Astronomy and Astrophysical Research Astrophysics and Cosmic Phenomena

Publication details

Journal / source
Astroparticle Physics
Publisher
Elsevier BV
Volume
182
Pages
103263–103263
Publication date
22 May 2026
Language
EN