PoS - Proceedings of Science
Volume 301 - 35th International Cosmic Ray Conference (ICRC2017) - Session Cosmic-Ray Indirect. CRI-instrumentation EAS
Point Spread Function of EUSO-TA detector
Z. Plebaniak,* J. Szabelski, T. Wibig, L. Piotrowski on behalf of the JEM-EUSO Collaboration
*corresponding author
Full text: pdf
Pre-published on: August 16, 2017
Published on: August 03, 2018
Abstract
EUSO detectors are high-resolution fluorescence telescopes dedicated for measurements of ultra-high energy cosmic rays (UHECR). EUSO-TA is a experiment dedicated for testing EUSO detectors and measurements of UHECR in coincidence with Telescope Array (TA) experiment. EUSO-TA is located in front of the Black Rock Mesa (BRM) detectors of the TA experiment. During a few campaigns in 2015 and 2016 signals coming from stars, airplanes, meteors, laser shots and cosmic rays were registered. The main goal of this work is determination of Point Spread Function of EUSO detectors which plays very important role in the interpretation of registered
signal.
DOI: https://doi.org/10.22323/1.301.0460
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