Software design for the control system for Small-Size Telescopes with single-mirror of the Cherenkov Telescope Array
PBN-AR
Instytucja
Wydział Informatyki, Elektroniki i Telekomunikacji (Akademia Górniczo-Hutnicza im. Stanisława Staszica w Krakowie)
Informacje podstawowe
Główny język publikacji
EN
Czasopismo
PoS Proceedings of Science
ISSN
EISSN
1824-8039
Wydawca
Sissa (Trieste): Proceedings of Science (PoS)
DOI
Rok publikacji
2015
Numer zeszytu
1033
Strony od-do
1--7
Numer tomu
30
Identyfikator DOI
Liczba arkuszy
0.5
Autorzy
(liczba autorów: 53)
Pozostali autorzy
+ 51
Streszczenia
Język
EN
Treść
The Small-Size Telescope with single-mirror (SST-1M) is a 4 m Davies-Cotton telescope and is among the proposed telescope designs for the Cherenkov Telescope Array (CTA). It is conceived to provide the high-energy (> few TeV) coverage. The SST-1M contains proven technology for the telescope structure and innovative electronics and photosensors for the camera. Its design is meant to be simple, low-budget and easy-to-build industrially. Each device subsystem of an SST-1M telescope is made visible to CTA through a dedicated industrial standard server. The software is being developed in collaboration with the CTA Medium-Size Telescopes to ensure compatibility and uniformity of the array control. Early operations of the SST-1M prototype will be performed with a subset of the CTA central array control system based on the Alma Common Software (ACS). The triggered event data are time stamped, formatted and finally transmitted to the CTA data acquisition. The software system developed to control the devices of an SST-1M telescope is described, as well as the interface between the telescope abstraction to the CTA central control and the data acquisition system.
Cechy publikacji
original article
peer-reviewed
Inne
System-identifier
idp:093419