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Cornils, R.; Gillessen, S.; Jung, I.; Hofmann, W.; Beilicke, M.; Bernlöhr, K.; Carrol, O.; Elfahem, S.; Heinzelmann, G.; Hermann, G.; Horns, D.; Kankanyan, R.; Katona, A.; Krawczynski, H.; Panter, M.; Rayner, S.; Rowell, G.; Tluczykont, M.; van Staa, R.
Astroparticle physics, 11/2003, Letnik: 20, Številka: 2Journal Article
Mirror facets of the high energy stereoscopic system imaging atmospheric Cherenkov telescopes are aligned using stars imaged onto the closed lid of the photomultiplier camera, viewed by a CCD camera. The alignment procedure works reliably and includes the automatic analysis of CCD images and control of the facet alignment actuators. On-axis, 80% of the reflected light is contained in a circle of less than 1 mrad diameter. The spot widens with increasing angle to the telescope axis. In accordance with simulations, the spot size has roughly doubled at an angle of 1.4° from the axis. The expected variation of spot size with elevation due to deformations of the support structure is visible, but is completely non-critical over the usual working range. Overall, the optical quality of the telescope exceeds the specifications.
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Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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Vir: Osebne bibliografije
in: SICRIS
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