Paper
1 May 1989 Design Of The Keck Observatory Alignment Camera
Gary A. Chanan
Author Affiliations +
Proceedings Volume 1036, Precision Instrument Design; (1989) https://doi.org/10.1117/12.950971
Event: SPIE Advanced Processing Technologies for Optical and Electronic Devices (colocated wth OPTCON), 1988, Santa Clara, CA, United States
Abstract
The alignment camera for the Keck Observatory uses a modified Shack-Hartmann test to phase the 36 segments of the primary mirror. The camera also has the capability to do direct imaging (and therefore image stacking), and to perform simple image quality measurements on individual segments. In this paper we motivate several of the design considerations for the alignment camera and describe the overall design.
© (1989) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gary A. Chanan "Design Of The Keck Observatory Alignment Camera", Proc. SPIE 1036, Precision Instrument Design, (1 May 1989); https://doi.org/10.1117/12.950971
Lens.org Logo
CITATIONS
Cited by 21 scholarly publications and 2 patents.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Cameras

Sensors

Image segmentation

Image stacking

Mirrors

Prisms

Collimators

RELATED CONTENT

Design of the Gemini near-infrared spectrograph
Proceedings of SPIE (June 29 2006)
The optical design of the X-shooter for the VLT
Proceedings of SPIE (June 30 2006)
Optical design of PANORAMIX II, the OMM wide field VIS...
Proceedings of SPIE (September 30 2004)
The CCAT 25m diameter submillimeter-wave telescope
Proceedings of SPIE (September 27 2012)
Optical design of the Southern African Large Telescope
Proceedings of SPIE (February 04 2003)

Back to Top