Author/Authors :
Bernlِhr، نويسنده , , K and Carrol، نويسنده , , O and Cornils، نويسنده , , R and Elfahem، نويسنده , , S and Espigat، نويسنده , , P and Gillessen، نويسنده , , S and Heinzelmann، نويسنده , , G and Hermann، نويسنده , , G and Hofmann، نويسنده , , W and Horns، نويسنده , , D and Jung، نويسنده , , I and Kankanyan، نويسنده , , R and Katona، نويسنده , , A and Khelifi، نويسنده , , B and Krawczynski، نويسنده , , H and Panter، نويسنده , , M and Punch، نويسنده , , M and Rayner، نويسنده , , S and Rowell، نويسنده , , G and Tluczykont، نويسنده , , M and van Staa، نويسنده , , R، نويسنده ,
Abstract :
H.E.S.S.––the high energy stereoscopic system––is a new system of large imaging atmospheric Cherenkov telescopes, with about 100 m2 mirror area for each of four telescopes, and photomultiplier cameras with a large field of view (5°) and small pixels (0.16°). The dish and reflector are designed to provide good imaging properties over the full field of view, combined with mechanical stability. The paper describes the design criteria and specifications of the system, and the individual components––dish, mirrors, and Winston cones––as well as their characteristics. The optical performance of the telescope as a whole is the subject of a companion paper.
