Paper
30 September 2004 A prime focus camera for the Discovery Channel Telescope
Author Affiliations +
Abstract
The Discovery Channel Telescope (DCT) is a 4.2 meter telescope that will provide a two degree diameter well-corrected field of view at prime focus with wavelength coverage across the groundbased ultraviolet and optical range. The design of the telescope and the prime focus corrector are described in other papers at this conference. The prime focus of the DCT will be occupied by a CCD camera similar in scope to the SAO Megacam for the MMT, the CFHT MegaCam, and the Kepler focal plane, but with differences in detail. It will be used for a variety of planetary science and astrophysics observing programs, the most demanding technically being searches for near-Earth and Kuiper Belt objects. This paper describes the design requirements, major systems issues, current design, and expected performance of the prime focus camera for the DCT.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Edward W. Dunham and Thomas A. Sebring "A prime focus camera for the Discovery Channel Telescope", Proc. SPIE 5492, Ground-based Instrumentation for Astronomy, (30 September 2004); https://doi.org/10.1117/12.552230
Lens.org Logo
CITATIONS
Cited by 3 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Charge-coupled devices

Telescopes

Cameras

Wavefront sensors

Camera shutters

CCD cameras

Control systems

RELATED CONTENT

The Zwicky transient facility observing system
Proceedings of SPIE (July 14 2014)
On-sky performance of the SDSS-V wide field corrector
Proceedings of SPIE (August 29 2022)
The Zwicky Transient Facility Camera
Proceedings of SPIE (August 09 2016)
Design of the CFH12K 12K x 8K CCD mosaic...
Proceedings of SPIE (August 16 2000)
INT prime focus mosaic camera
Proceedings of SPIE (March 25 1996)
LBC the prime focus optical imagers at the LBT...
Proceedings of SPIE (March 07 2003)

Back to Top