Paper
5 August 2010 VISTA Telescope opto-mechanical integration
Paul Jeffers, David Henry
Author Affiliations +
Abstract
VISTA1 is an infrared survey telescope which delivers 0.5 arc second images over a 1.65 degree diameter unvignetted field of view. The project was split into separate work-packages, which after successful individual acceptance, were integrated by the project office. The main mechanical integration is the matching up of two sides of a controlled interface and should be a straightforward process. This covers the mounting of the M2 Hexapod, the installation of the M2 mirror assembly onto the M2 Hexapod, the M1 attachment to the M1 support system components and installation of the instrument mass simulator. The second stage of this integration is the mechanical alignment of the optical elements (i.e. M1 & M2) to the telescope mechanical axis. This is achieved through use of jigs and alignment equipment combined with the inbuilt adjustment in both the M2 on it's Hexapod and the manual adjustment of the M1 on its positional definers. This then leaves the telescope in a state ready to start optical commissioning using a Shack Hartman wavefront sensor. This paper deals with the mechanical integration and alignment of the telescope components up to the start of optical commissioning. There will be discussion of the build-up of information through the separate component acceptance details, to the equipment methodology, preparation and actual integration of the different systems. There will also be discussion of lessons learned.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Paul Jeffers and David Henry "VISTA Telescope opto-mechanical integration", Proc. SPIE 7733, Ground-based and Airborne Telescopes III, 77332L (5 August 2010); https://doi.org/10.1117/12.857091
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Cameras

Optical alignment

Interfaces

Mirrors

Device simulation

Infrared telescopes

RELATED CONTENT

AIV procedure for a CHEOPS demonstration model
Proceedings of SPIE (August 28 2014)
Daniel K. Inouye Solar Telescope optical alignment plan
Proceedings of SPIE (July 27 2016)
Image quality with array spectrometers
Proceedings of SPIE (June 01 1994)
Optical alignment of the LBT prime focus camera
Proceedings of SPIE (September 30 2004)

Back to Top