Abstract
The Track Imaging Cerenkov Experiment (TrICE) is an air Cerenkov prototype telescope designed to use multi-anode photomultipliers to achieve a high angular resolution for measuring cosmic- ray composition at TeV-PeV energies. The TrICE camera, composed of 16 Hamamatsu R8900 16-channel multi-anode photomultiplier tubes, achieves 0.086 degree angular width per pixel over 1.5 degree wide field of view. We present a description of the TrICE camera design, calibration and performance.
Original language | English (US) |
---|---|
Pages | 469-472 |
Number of pages | 4 |
State | Published - 2007 |
Event | 30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico Duration: Jul 3 2007 → Jul 11 2007 |
Other
Other | 30th International Cosmic Ray Conference, ICRC 2007 |
---|---|
Country/Territory | Mexico |
City | Merida, Yucatan |
Period | 7/3/07 → 7/11/07 |
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics