Details are presented of the Whipple Observatory's 10 m atmospheric Cherenkov telescope and camera, as it evolved during the period 1997 until 2006. The design of the telescope and camera's optical and electronic systems is discussed together with a detailed description of the four-stage GRANITE (Gamma-RAy New Imaging TElescope) upgrade program, undertaken during the same time period. The objective of the upgrade was to improve the telescope's sensitivity for the detection of very-high-energy gamma-rays. Results from the program are provided and are briefly discussed in the context of the design of VERITAS.
|Original language||English (US)|
|Number of pages||14|
|State||Published - Oct 2007|
Bibliographical noteFunding Information:
This research is supported by grants from the US Department of Energy, the US National Science Foundation, the Smithsonian Institution, by NSERC in Canada, by Science Foundation Ireland and by PPARC in the UK. We also acknowledge the annoynmous referee for his meticulous reading of the paper and many useful comments.
Copyright 2008 Elsevier B.V., All rights reserved.
- Atmospheric Cherenkov effect
- Gamma-ray astronomy
- Gamma-ray telescope
- Imaging atmospheric Cherenkov technique
- Imaging atmospheric Cherenkov telescope
- Whipple collaboration