scholarly journals Development and characterization of Near-UV sensitive Silicon Photomultipliers for the Schwarzschild-Couder Telescope prototype for the Cherenkov Telescope Array

2017 ◽  
Author(s):  
Emanuele Fiandrini ◽  
Giovanni Ambrosi ◽  
Michelangelo Ambrosio ◽  
Carla Aramo ◽  
Bruna Bertucci ◽  
...  
2019 ◽  
Vol 209 ◽  
pp. 01001
Author(s):  
Salvatore Scuderi

The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) program was born as a collaborative international effort led by the Italian National Institute for Astrophysics (INAF) to design and realize, within the Cherenkov Telescope Array (CTA) framework, an end-to-end prototype of the Small-Sized Telescope (SST) in a dual-mirror configuration (2M). While the activities concerning the characterization of the prototype are under completion, the program entered a new phase. With the final aim of contributing at the production of the SST telescopes for the CTAO Southern site, we started the development of nine telescopes based on the evolution of the ASTRI prototype design to work as pathfinder for the CTAO. Furthermore, together with the CHEC (Compact High Energy Camera) collaboration, the ASTRI team presented a proposal, that will be evaluated with other proposals, to deliver to CTAO the complete set of SST telescopes.


2019 ◽  
Vol 209 ◽  
pp. 01049
Author(s):  
G. Ambrosi ◽  
M. Ambrosio ◽  
C. Aramo ◽  
B. Bertucci ◽  
E. Bissaldi ◽  
...  

Silicon Photomultipliers (SiPMs) are excellent devices to detect the faint and short Cherenkov light emitted in high energy atmospheric showers, and therefore suitable for use in imaging air Cherenkov Telescopes. The high density Near Ultraviolet Violet SiPMs (NUV-HD3) produced by Fondazione Bruno Kessler (FBK) in collaboration with INFN were used to equip optical modules for a possible upgrade of the Schwarzschild-Couder Telescope camera prototype, in the framework of the Cherenkov Telescope Array project. SiPMs are 6×6 mm2 devices based on 40×40 μm2 microcells optimized for photo-detection at the NUV wavelengths. More than 40 optical modules, each composed by a 4×4 array of SiPMs, were assembled. In this contribution we report on the development and on the assembly of the optical modules, their validation and integration in the camera.


2016 ◽  
Vol 128 (961) ◽  
pp. 035004 ◽  
Author(s):  
Gagik Tovmassian ◽  
Mercedes-Stephania Hernandez ◽  
Jose Luis Ochoa ◽  
Jean-Pierre Ernenwein ◽  
Dusan Mandat ◽  
...  

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