Presentation + Paper
29 August 2022 Latest developments for the Giant Magellan Telescope (GMT) control system
Author Affiliations +
Abstract
The Giant Magellan Telescope (GMT) is a complex observatory with thirty major subsystems, many low-level subsystems, components, external contracts, and interfaces. Almost all subsystems require software and controls to operate. An important goal for GMT is to have software and control subsystems that are easy to develop, test, integrate, operate, and maintain. To provide consistency across all controlled subsystems, a set of standards and a reference architecture are provided. Software components are specified using a Domain Specific Language (DSL), which enables code-generation in several languages and automatic validation of architectural conformance and interfaces. Some of the main observatory control subsystems have already been modeled using this approach, and initial implementations are currently being tested. The most advanced control subsystem is the primary mirror Device Control System (M1 DCS), which is currently under testing before the integration of the optical mirror in the test cell. This paper describes the status of the GMT control system, the main lessons learned, and the future steps in the development of the GMT control system.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Martí Pi, Marianne Cox, José M. Filgueira, Jordi Molgó, Divya Thanasekaran, William Schoenell, Hector Swett, José Soto, Chien Peng, and Chris Contaxis "Latest developments for the Giant Magellan Telescope (GMT) control system", Proc. SPIE 12189, Software and Cyberinfrastructure for Astronomy VII, 1218917 (29 August 2022); https://doi.org/10.1117/12.2630614
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KEYWORDS
Control systems

Observatories

Safety

Telescopes

Mirrors

Actuators

Interfaces

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