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The Array Control and Data Acquisition System of the Cherenkov Telescope Array

Authors :
Oya, Igor
Antolini, Ermete
Füßling, Matthias
Hinton, J
Mitchell, Alison
Schlenstedt, Stefan
Baroncelli, Leonardo
Bulgarelli, Andrea
Conforti, Vito
Parmiggiani, Nicolò
Borkowski, J
Carosi, Alessandro
Jacquemier, Jean
Maurin, Gilles
Colomé, J.
Hoischen, Clemens
Lebout, Dylan
Lyard, Etienne
Walter, Roland
Melkumyan, David
Mosshammer, K.
Sadeh, Iftach
Schmidt, Thomas
Wegner, Peter
Schwanke, Ullrich
Schwarz, Joseph
Tosti, Giacomo
Laboratoire d'Annecy de Physique des Particules (LAPP)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)
Deutsches Elektronen-Synchrotron [Zeuthen] (DESY)
Helmholtz-Gemeinschaft = Helmholtz Association
Therenkov Telescope Array Observatory gGmbH [Heidelberg] (CTAO gGmbH)
INAF - Osservatorio Astronomico di Bologna (OABO)
Istituto Nazionale di Astrofisica (INAF)
Copernicus Astronomical Center of the Polish Academy of Sciences (CAMK)
Polish Academy of Sciences (PAN)
Institute for Space Studies of Catalonia [Barcelona] (IEEC-CSIC)
Universität Potsdam
Interacting with Large Data (ILDA)
Laboratoire de Recherche en Informatique (LRI)
Université Paris-Sud - Paris 11 (UP11)-CentraleSupélec-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-CentraleSupélec-Centre National de la Recherche Scientifique (CNRS)-Inria Saclay - Ile de France
Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria)
Université de Genève (UNIGE)
Humboldt University of Berlin
INAF - Osservatorio Astronomico di Brera (OAB)
Università degli Studi di Perugia (UNIPG)
Helmholtz-Gemeinschaft
AstroParticule et Cosmologie (APC (UMR_7164))
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules)
Institut für Physik
Humboldt Universität zu Berlin
University of Potsdam = Universität Potsdam
Université de Genève = University of Geneva (UNIGE)
Humboldt University Of Berlin
Università degli Studi di Perugia = University of Perugia (UNIPG)
Source :
17th International Conference on Accelerator and Large Experimental Physics Control Systems, 17th International Conference on Accelerator and Large Experimental Physics Control Systems, Oct 2019, New York, United States. pp.WEMPR005, ⟨10.18429/JACoW-ICALEPCS2019-WEMPR005⟩, ICALEPCS 2019-17th Biennial International Conference on Accelerator and Large Experimental Physics Control Systems, ICALEPCS 2019-17th Biennial International Conference on Accelerator and Large Experimental Physics Control Systems, Oct 2019, New York, NY, United States. ⟨10.18429/JACoW-ICALEPCS2019-WEMPR005⟩, ICALEPCS 2019-17th Biennial International Conference on Accelerator and Large Experimental Physics Control Systems, Oct 2019, New York, NY, United States
Publication Year :
2019
Publisher :
HAL CCSD, 2019.

Abstract

The Cherenkov Telescope Array (CTA) project is the initiative to build the next-generation gamma-ray observatory. With more than 100 telescopes planned to be deployed in two sites, CTA is one of the largest astronomical facilities under construction. The Array Control and Data Acquisition (ACADA) system will be the central element of on-site CTA Observatory operations. The mission of the ACADA system is to manage and optimize the telescope array operations at each of the CTA sites. To that end, ACADA will provide all necessary means for the efficient execution of observations, and for the handling of the several Gb/s generated by each individual CTA telescope. The ACADA system will contain a real-time analysis pipeline, dedicated to the automatic generation of science alert candidates based on the inspection of data being acquired. These science alerts, together with external alerts arriving from other scientific installations, will permit ACADA to modify ongoing observations at sub-minute timescales in order to study high-impact scientific transient phenomena. This contribution describes the challenges, architecture, design principles, and development status of the ACADA system.<br />Proceedings of the 17th International Conference on Accelerator and Large Experimental Physics Control Systems, ICALEPCS2019, New York, NY, USA

Details

Language :
English
Database :
OpenAIRE
Journal :
17th International Conference on Accelerator and Large Experimental Physics Control Systems, 17th International Conference on Accelerator and Large Experimental Physics Control Systems, Oct 2019, New York, United States. pp.WEMPR005, ⟨10.18429/JACoW-ICALEPCS2019-WEMPR005⟩, ICALEPCS 2019-17th Biennial International Conference on Accelerator and Large Experimental Physics Control Systems, ICALEPCS 2019-17th Biennial International Conference on Accelerator and Large Experimental Physics Control Systems, Oct 2019, New York, NY, United States. ⟨10.18429/JACoW-ICALEPCS2019-WEMPR005⟩, ICALEPCS 2019-17th Biennial International Conference on Accelerator and Large Experimental Physics Control Systems, Oct 2019, New York, NY, United States
Accession number :
edsair.doi.dedup.....7435432d2b643b43496a898e4ea41ba4