Title of article :
G-APDs in Cherenkov astronomy: The FACT camera
Author/Authors :
Krنhenbühl، نويسنده , , T. and Anderhub، نويسنده , , H. and Backes، نويسنده , , M. and Biland، نويسنده , , A. and Boller، نويسنده , , A. and Braun، نويسنده , , I. and Bretz، نويسنده , , T. and Commichau، نويسنده , , V. and Djambazov، نويسنده , , L. and Dorner، نويسنده , , D. and Farnier، نويسنده , , C. and Gendotti، نويسنده , , A. and Grimm، نويسنده , , O. and von Gunten، نويسنده , , H. F. Hildebrand، نويسنده , , D. and Horisberge، نويسنده ,
Pages :
4
From page :
96
To page :
99
Abstract :
Geiger-mode avalanche photodiodes (G-APD, SiPM) are a much discussed alternative to photomultiplier tubes in Cherenkov astronomy. The First G-APD Cherenkov Telescope (FACT) collaboration builds a camera based on a hexagonal array of 1440 G-APDs and has now finalized its construction phase. A light-collecting solid PMMA cone is glued to each G-APD to eliminate dead space between the G-APDs by increasing the active area, and to restrict the light collection angle of the sensor to the reflector area in order to reduce the amount of background light. The processing of the signals is integrated in the camera and includes the digitization using the domino ring sampling chip DRS4.
Keywords :
Cherenkov telescope , Geiger-mode avalanche photodiode , Gamma-ray astronomy
Journal title :
Astroparticle Physics
Record number :
2020055
Link To Document :
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