The METIS instrument control system
Abstract
METIS, the Mid-infrared ELT Imager and Spectrograph, will be one of the first-generation ELT instruments. It has an Instrument Control System (ICS) that allows the instrument to operate in various observing modes, using a multitude of mostly cryogenic mechanisms such as filter wheels, linear stages (e.g. to move mirrors and masks), a derotator, piezo mechanisms for high-speed or high-accuracy displacements (e.g. for pupil stabilization, for adaptive optics field selection and modulation, ...), a chopper, and so on. Thermal and vacuum control of the cryostat on the other hand is handled by a dedicated PLC-based system and is not described in this paper. The ICS is built using the ESO ELT instrument framework, which provides the basic building blocks to control the mechanisms, along with the interface to the telescope and its services, from the low-level pointing and tracking system, the real-time Single Conjugate Adaptive Optics (SCAO) system, to the high-level sequencer-based observing system. In this paper we provide an overview of the ICS electronics, the low-level software running on a Beckhoff PLC, and finally the high-level software running on a Linux workstation. As a detailed description of the entire system is out of scope of the paper, we focus instead on the general design, implementation and testing principles. We show how a fast real-time network (EtherCAT) and off-the-shelf industrial I/O, together with the services provided by the ELT instrument framework, can meet the requirements of ELT instruments, and how they can offer an elegant solution to technically demanding problems such as the high-speed synchronization between a chopper and a detector controller. Finally, we demonstrate how a modular electronics design, a flexible software architecture, and a strong focus on simulation can alleviate some of the organizational challenges of building, integrating and testing an ICS of a complex instrument, which subsystems are developed by institutes in different locations.
Authors 26
-
Affiliation as printed
KU Leuven (Belgium)
-
Affiliation as printed
KU Leuven (Belgium)
-
Affiliation as printed
KU Leuven (Belgium)
-
Affiliation as printed
KU Leuven (Belgium)
-
Affiliation as printed
KU Leuven (Belgium)
-
Affiliation as printed
KU Leuven (Belgium)
-
Affiliation as printed
KU Leuven (Belgium)
-
Affiliation as printed
KU Leuven (Belgium)
-
Affiliation as printed
KU Leuven (Belgium)
-
Affiliation as printed
European Southern Observatory (Germany)
-
Affiliation as printed
European Southern Observatory (Germany)
-
Affiliation as printed
European Southern Observatory (Germany)
-
Affiliation as printed
CENTRA (Portugal)
-
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Affiliation as printed
CEA (France)
-
Max Planck Institute for Astronomy
Affiliation as printed
Max-Planck-Institut für Astronomie (Germany)
-
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Affiliation as printed
CEA (France)
-
Affiliation as printed
Univ. zu Köln (Germany)
-
Max Planck Institute for Astronomy
Affiliation as printed
Max-Planck-Institut für Astronomie (Germany)
-
Netherlands Institute for Radio Astronomy
Affiliation as printed
ASTRON (Netherlands)
-
Netherlands Institute for Radio Astronomy
Affiliation as printed
ASTRON (Netherlands)
-
Max Planck Institute for Astronomy
Affiliation as printed
Max-Planck-Institut für Astronomie (Germany)
-
UK Astronomy Technology Centre
Affiliation as printed
UK Astronomy Technology Ctr. (United Kingdom)
-
Affiliation as printed
Leiden Univ. (Netherlands)
-
Max Planck Institute for Astronomy
Affiliation as printed
Max-Planck-Institut für Astronomie (Germany)
-
Affiliation as printed
KU Leuven (Belgium)
Cited by 1 stored of 1
1 result
No patents citing this paper on Lens.org (checked 2026-10-11).
References 4
-
W6842438210details pending0citations
-
W6869628091details pending0citations
-
W6870925361details pending0citations
-
W6872206541details pending0citations
4 results