28 September 1999 DEIMOS camera assembly
Author Affiliations +
DEIMOS is a large multi-object spectrography with an imaging mode that is being built for the W. M. Keck 2 Telescope. The camera contains nine lens elements in five groups. The overall length of the camera and detector assembly is 0.67 meters, and the largest element is 0.33 meters in diameter. Typical centration and spacing tolerances are at the level of 25 microns. We describe the error budget, the design of the lens-supporting structure, and the assembly procedures.
© (1999) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Terry S. Mast, Sandra M. Faber, Vernon Wallace, Jeffrey P. Lewis, David F. Hilyard, "DEIMOS camera assembly", Proc. SPIE 3786, Optomechanical Engineering and Vibration Control, (28 September 1999); doi: 10.1117/12.363832; https://doi.org/10.1117/12.363832


Optical design of a red-sensitive spectrograph
Proceedings of SPIE (September 24 2012)
The performance of TripleSpec at Palomar
Proceedings of SPIE (July 09 2008)
A wide field reflector for the detection of high energy...
Proceedings of SPIE (January 30 2004)
Calibration database for the Hubble Space Telescope
Proceedings of SPIE (November 01 1993)
Evolution of the HST proposal selection process
Proceedings of SPIE (July 25 2000)

Back to Top