Volume 484 - 7th International Symposium on Ultra High Energy Cosmic Rays (UHECR2024) - Session Thursday
Progress in the development of the observation system for the CRAFFT project
Y. Tameda*  on behalf of the CRAFFT Collaboration
*: corresponding author
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Pre-published on: March 21, 2025
Published on: —
Abstract
In order to obtain a sufficient number of observational events to clarify the origin of ultra high energy cosmic rays, a large-scale observatory is required. Currently, next-generation detectors are being developed for this purpose. The CRAFFT project focuses on developing fluorescence detectors that can be produced and operated at low cost. In this presentation, we will report on the status of detector upgrades, the development of trigger algorithms, and the operational tests of an observation system aimed at autonomous operation.
DOI: https://doi.org/10.22323/1.484.0053
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