Search for Extreme Energy Cosmic Rays with the TUS orbital telescope and comparison with ESAF

• Published in: EPJ Web of conferences Vol. 210; p. 6006
• Main Authors: Bertaina, Mario, Castellina, Antonella, Cremonini, Roberto, Fenu, Francesco, Klimov, Pavel, Salsi, Anthony, Sharakin, Sergey, Shinozaki, Kenji, Zotov, Mikhail
• Format: Journal Article Conference Proceeding
• Language: English
• Published: Les Ulis EDP Sciences 2019
• Subjects: Computer simulation; Cosmic rays; Ultraviolet detectors
• ISSN: 2100-014X; 2101-6275; 2100-014X
• DOI: 10.1051/epjconf/201921006006

The Tracking Ultraviolet Setup (TUS) detector was launched on April 28, 2016 as a part of the scientific payload of the Lomonosov satellite. TUS is a pathfinder mission for future space-based observation of Extreme-Energy Cosmic Rays (EECRs, E > 5x10 19 eV) with experiments such as K-EUSO. TUS data offer the opportunity to develop strategies in the analysis and reconstruction of the events which will be essential for future space-based missions. During its operation, TUS has detected about 80 thousand events which have been subject to an offline analysis to select among them those that satisfy basic temporal and spatial criteria of EECRs. A few events passed this first screening. In order to perform a deeper analysis of such candidates, a dedicated version of ESAF (EUSO Simulation and Analysis Framework) code as well as a detailed modelling of TUS optics and detector are being developed.