Abstract
Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and charged cosmic-ray events are digitized and recorded. Subsequent off-line analysis of the images improves the significance of the signal to noise ratio by a factor of 10 compared with non-imaging techniques.
| Original language | English |
|---|---|
| Pages (from-to) | 173-193 |
| Number of pages | 21 |
| Journal | Experimental Astronomy |
| Volume | 1 |
| Issue number | 3 |
| DOIs | |
| State | Published - May 1990 |