Title of article
On site calibration for new fluorescence detectors of the telescope array experiment
Author/Authors
Tokuno، نويسنده , , H. and Murano، نويسنده , , Y. and Kawana، نويسنده , , S. and Tameda، نويسنده , , Y. and Taketa، نويسنده , , A. and Ikeda، نويسنده , , D. and Udo، نويسنده , , S. and Ogio، نويسنده , , Mary S. and Fukushima، نويسنده , , M. and Azuma، نويسنده , , Sven R. and Fukuda، نويسنده , , M. and Inoue، نويسنده , , N. and Kadota، نويسنده , , K. and Kakimoto، نويسنده , , F. and Sagawa، نويسنده , , H. and Sakurai، نويسنده , , Quentin N. and Shibata، نويسنده , , T. and T، نويسنده ,
Pages
8
From page
364
To page
371
Abstract
The Telescope Array experiment is searching for the origin of ultra-high energy cosmic rays using a ground array of particle detectors and three fluorescence telescope stations. The precise calibration of the fluorescence detectors is important for small systematic errors in shower reconstruction. This paper details the process of calibrating cameras for two of the fluorescence telescope stations. This paper provides the operational results of these camera calibrations.
Keywords
Ultra-high energy cosmic rays , Fluorescence light , Extensive air showers
Journal title
Astroparticle Physics
Record number
2024935
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