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Machine Learning for the EUSO-SPB2 Fluorescence Telescope Data Analysis
Colorado School of Mines, Golden, CO, USA.
KTH, School of Engineering Sciences (SCI), Physics, Particle Physics, Astrophysics and Medical Imaging.ORCID iD: 0000-0001-5456-3894
KTH, School of Engineering Sciences (SCI), Physics, Particle Physics, Astrophysics and Medical Imaging.ORCID iD: 0000-0002-0406-0962
Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Russia.
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Number of Authors: 1582024 (English)In: 38th International Cosmic Ray Conference, ICRC 2023, Sissa Medialab Srl , 2024, article id 234Conference paper, Published paper (Refereed)
Abstract [en]

The Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2) is the most advanced balloon mission undertaken by the JEM-EUSO collaboration. EUSO-SPB2 is built on the experience of previous stratosphere missions, EUSO-Balloon and EUSO-SPB, and of the Mini-EUSO space mission currently active onboard the International Space Station. EUSOSPB2 is equipped with two instruments: a fluorescence telescope aimed at registering ultra-high energy cosmic rays (UHECRs) with an energy above 2 EeV and a Cherenkov telescope built to measure direct Cherenkov emission from cosmic rays with energies above 1 PeV. The EUSO-SPB2 mission will provide pioneering observations on the path towards a space-based multi-messenger observatory. As such, a special attention was paid to the development of triggers and other software aimed at comprehensive data analysis. A whole number of methods based on machine learning (ML) and neural networks was developed during the construction of the experiment and a few others are under active development. Here we provide a brief review of the ML-based methods already implemented in the instrument and the ground software and report preliminary results on the ML-based reconstruction of UHECR parameters for the fluorescence telescope.

Place, publisher, year, edition, pages
Sissa Medialab Srl , 2024. article id 234
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-358159Scopus ID: 2-s2.0-85212282520OAI: oai:DiVA.org:kth-358159DiVA, id: diva2:1924785
Conference
38th International Cosmic Ray Conference, ICRC 2023, Nagoya, Japan, Jul 26 2023 - Aug 3 2023
Note

QC 20250114

Available from: 2025-01-07 Created: 2025-01-07 Last updated: 2025-01-14Bibliographically approved

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Bolmgren, KarlFuglesang, Christer

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