The Array Data Acquisition System software architecture of the ASTRI Mini-Array Project

Autor(es):Mostrar menos -

Conforti, Vito ; Gianotti, Fulvio ; Pastore, Valerio ; Trifoglio, Massimo ; Bulgarelli, Andrea A. ; Addis, Antonio ; Baroncelli, Leonardo ; Capalbi, Milvia ; Fioretti, Valentina ; Parmiggiani, Nicolo ; Sangiorgi, Pierluca ; Corpora, Mattia ; Catalano, Osvaldo ; Costa, Alessandro ; Incardona, Federico ; Russo, F. ; ASTRI Project ; Ibsen, J ; Chiozzi, G

• Tipo de documento: Artigo Científico
• Fonte: SOFTWARE AND CYBERINFRASTRUCTURE FOR ASTRONOMY VII; v. 12189, p. 9-pg., 2022-01-01.

Resumo

The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Project was born as a collaborative international effort led by the Italian National Institute for Astrophysics (INAF) to design and realize an end-to-end prototype of the Small-Sized Telescope (SST) of the Cherenkov Telescope Array (CTA) in a dual-mirror configuration (2M). The prototype, named ASTRI-Horn, has been operational since 2014 at the INAF observing station located on Mt. Etna (Italy). The ASTRI Project is now building the ASTRI Mini-Array consisting of nine ASTRI-Horn-like telescopes to be installed and operated at the Teide Observatory (Spain). The ASTRI software is aimed at supporting the Assembly Integration and Verification (AIV), and the operations of the ASTRI Mini-Array. The Array Data Acquisition System (ADAS) includes all hardware, software and communication infrastructure required to gather the bulk data of the Cherenkov Cameras and the Intensity Interferometers installed on the telescopes, and make these data available to the Online Observation Quality System (OOQS) for the on-site quick look, and to the Data Processing System (DPS) for the off-site scientific pipeline. This contribution presents the ADAS software architecture according to the use cases and requirement specifications, with particular emphasis on the interfaces with the Back End Electronics (BEE) of the instruments, the array central control, the OOQS, and the DPS. (AU)

• Processo FAPESP: 13/10559-5 - Investigação de fenômenos de altas energias e plasmas astrofísicos: teoria, simulações numéricas, observações e desenvolvimento de instrumentação para o Cherenkov Telescope Array (CTA)
• Beneficiário: Elisabete Maria de Gouveia Dal Pino
• Modalidade de apoio: Auxílio à Pesquisa - Projetos Especiais