Presentation + Paper
29 August 2022 MOONS fibre positioning module: instrument build overview
Author Affiliations +
Abstract
MOONS (Multi-Object Optical and Near-infrared Spectrograph) is a third-generation visible and near-infrared spectrograph for the ESO Very Large Telescope, currently nearing the end of the assembly phase. The three channel spectrograph is fed via a fibre positioning module (FPM) which configures the location of 1001 fibres. The robotic fibre positioning units (FPUs) have been jointly developed by the UK Astronomy Technology Centre (UKATC) and MPS Microsystems (MPS) and provide a high-performance multiplexed focal plane with excellent transmission characteristics. An overview of the as-built mechanisms and supporting infrastructure is presented, with details on the extensive calibration process carried out. The integration process to date will be described, including a discussion of key lessons learned.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stephen Watson, Raziye Artan, David Atkinson, Steven Beard, Martin Black, Ciaran Breen, Ian Bryson, Jose Carrera, Stefane Caseiro, Lee Chapman, Stephen Chittick, William Cochrane, Miriam Colling, Oscar Gonzalez, Markus Hug, Ciaran Lawrence, Alexander Lay, David Montgomery, Yves Moser, Johannes Nix, Alan O'Brien, Phil Rees, William Taylor, and Bart Willemse "MOONS fibre positioning module: instrument build overview", Proc. SPIE 12188, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation V, 1218829 (29 August 2022); https://doi.org/10.1117/12.2627329
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Metrology

Calibration

Cameras

Resistance

Spectrographs

Computer aided design

Connectors

Back to Top