Résumé
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.
| langue originale | Anglais |
|---|---|
| Pages (de - à) | 182-195 |
| Nombre de pages | 14 |
| journal | Astroparticle Physics |
| Volume | 28 |
| Numéro de publication | 2 |
| Les DOIs | |
| état | Publié - 1 oct. 2007 |
| Modification externe | Oui |
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