Design and development of the Supervisor software component for the ASTRI Mini-Array Cherenkov Camera

Corpora, M.; Grillo, A.; Sangiorgi, Pierluca; Capalbi, M.; Catalano, O.; Sottile, G.; Tosti, G.; Bulgarelli, A.; Lucarelli, F.; Parmiggiani, N.; Schwarz, Joseph; Russo, Federico; Conforti, Vito; Scuderi, S.

doi:10.1117/12.2629350

Cited by 1 publication

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“…Control systems are used to control, monitor, and manage alarms and the status of the telescopes (telescope control system, 24 , 25 developed by INAF based on the ASTRI-Horn experience), of the assemblies used to characterize the atmosphere (atmosphere characterization control system), and of the calibration system (array calibration control system);…”

Section: General Software Architecturementioning

confidence: 99%

“…(a) Control systems are used to control, monitor, and manage alarms and the status of the telescopes (telescope control system, 24,25 developed by INAF based on the ASTRI-Horn experience), of the assemblies used to characterize the atmosphere (atmosphere characterization control system), and of the calibration system (array calibration control system); (b) Collectors, to monitor and determine alarms and the status of environmental devices (environmental monitoring system collector), of the ICT system 15 (on-site ICT system collector), of the power system (power management system collector), of the safe and security system (safety and security system collector), and the telescope service cabinets (telescope service cabinet collector, one for each telescope);…”

Section: Supervisory Control and Data Acquisition Systemmentioning

confidence: 99%

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Software architecture and development approach for the ASTRI Mini-Array project at the Teide Observatory

Bulgarelli,

Lucarelli,

Tosti

et al. 2024

J. Astron. Telesc. Instrum. Syst.

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The Astrophysics with Italian Replicating Technology Mirrors (ASTRI) Mini-Array is an international collaboration led by the Italian National Institute for Astrophysics (INAF) and devoted to imaging atmospheric Cherenkov light for very-high γ-ray astrophysics, detection of cosmic-rays, and stellar Hambury-Brown intensity interferometry. The project is deploying an array of nine dual-mirror aplanatic imaging atmospheric Cherenkov telescopes of 4-m class at the Teide Observatory on Tenerife in the Canary Islands. Based on SiPM sensors, the focal plane camera covers an unprecedented field of view of 10.5 deg in diameter. The array is most sensitive to γ-ray radiation above 1 up to 200 TeV, with an angular resolution of 3 arcmin, better than the current particle arrays, such as LHAASO and HAWC.

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Section: General Software Architecturementioning

confidence: 99%