Speaker
Oleg Kalashev
(INR RAS)
Description
A novel ultra-high-energy cosmic rays energy and arrival direction reconstruction method for Telescope Array surface detector is presented. The analysis is based on a deep convolutional neural network using detector signal time series as the input and the network is trained on a large Monte-Carlo dataset. This method is compared in terms of statistical and systematic energy and arrival direction determination errors with the standard Telescope Array surface detector event reconstruction procedure.
Keywords
ultra-high-energy cosmic rays; machine learning; event reconstruction;Telescope Array surface detector
| Subcategory | Experimental Methods & Instrumentation |
|---|---|
| Collaboration | Telescope Array |
Primary author
Oleg Kalashev
(INR RAS)
