Speaker
Oleg Kalashev
(INR RAS)
Description
We present updated results of the search for the ultra-high energy photons with primary energies greater than 1 EeV. The data of the Telescope Array Surface Detector collected over 12 years are used in this work. The method is based on the machine learning classifier, which trains on both the reconstructed composition-sensitive parameters of the event and the calibrated waveform signals at each triggered station of the Surface Detector.
Keywords
ultra high energy cosmic rays; GZK photons;Telescope Array; Surface Detector
Subcategory | Experimental Results |
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Collaboration | Telescope Array |
Primary authors
Oleg Kalashev
(INR RAS)
Dr
Grigory Rubtsov
(INR RAS)