论文信息 - On site calibration for new fluorescence detectors of the telescope array experiment

On site calibration for new fluorescence detectors of the telescope array experiment

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.

[1] K. Greisen. End to the cosmic ray spectrum , 1966 .

[2] Robert O. Reid,et al. The cosmic ray energy spectrum above 4*1017 eV as measured by the Haverah Park array , 1991 .

[3] H. Shimizu,et al. Energy determination in the Akeno Giant Air Shower Array experiment , 2002, astro-ph/0209422.

[4] J. Linsley. Thickness of the particle swarm in cosmic-ray air showers , 1986 .

[5] G. G. Stokes. "J." , 1890, The New Yale Book of Quotations.

[6] Masaaki Kobayashi,et al. YAlO3: Ce-Am light pulsers as a gain monitor for undoped CsI detectors in a magnetic field , 1994 .

[7] M. Teshima,et al. Energy spectrum of primary cosmic rays above 1017.0 eV determined from extensive air shower experiments at Akeno , 1992 .

[8] M. Teshima,et al. The cosmic ray energy spectrum above 3 × 1018 eV measured by the Akeno Giant Air Shower Array , 1995 .

[9] N. T. Thao,et al. Observation of the suppression of the flux of cosmic rays above 4 x 10 (19) eV. , 2008, Physical review letters.

[10] Tomohiro Matsuda,et al. Telescope Array Experiment , 2019, EPJ Web of Conferences.

[11] J. Ulrichs,et al. The cosmic-ray energy spectrum above 1017 eV , 1986 .

[12] J. R. Thomas,et al. First observation of the Greisen-Zatsepin-Kuzmin suppression. , 2008, Physical review letters.

[13] J. W. Elbert,et al. The Cosmic ray energy spectrum observed by the Fly's Eye , 1994 .