The DAQ system support to the AIV activities of the ASTRI camera proposed for the Cherenkov Telescope Array

0552783 - FZÚ 2022 RIV US eng C - Konferenční příspěvek (zahraniční konf.)
Conforti, V. … celkem 8 autorů
The DAQ system support to the AIV activities of the ASTRI camera proposed for the Cherenkov Telescope Array.
Proceedings of SPIE. Vol. 10707. Bellingham: SPIE, 2018 - (Guzman, J.; Ibsen, J.), s. 1-12, č. článku 1070724. ISBN 9781510619678. ISSN 0277-786X. E-ISSN 1996-756X.
[SPIE Astronomical Telescopes + Instrumentation 2018, Software and Cyberinfrastructure for Astronomy /5./. Austin, Texas (US), 10.06.2018-13.06.2018]
Výzkumná infrastruktura: CTA-CZ - 90046
Klíčová slova: data acquisition * camera server * bulk data
Obor OECD: Particles and field physics
https://doi.org/10.1117/12.2312131

The Cherenkov Telescope Array (CTA), the next generation ground-based observatory for very high-energy gamma rays, is being built and will be operated by an international consortium. Two arrays will be located in the northern and southern hemispheres. Each telescope array will operate different numbers and types of telescopes. The Italian National Institute for Astrophysics (INAF) is leading the ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) project in the framework of the small size class of telescopes (SST). A first goal of the ASTRI project is the realization of an end-to-end prototype in dual-mirror configuration (SST-2M). The ASTRI camera focal plane is composed of a matrix of silicon photo-multiplier sensors managed by innovative front-end and back-end electronics.
Trvalý link: http://hdl.handle.net/11104/0327881