Paper
1 July 1990 Development and performance of a 128x128 2-um camera
Author Affiliations +
Abstract
Recent advancements in fabrication of near-infrared focal plane arrays are beginning to revolutionize near-infrared astronomy. The University of California Lick Observatory is undertaking a program to exploit these arrays by starting with a singlefilter (K band at two microns)imaging camera to be used at the Sane 3-meter telescope. The detector is a Rockwell 128x128-pixel device, sensitive from 1 to 2.5 microns and employing the NICMOS design. Camera specifications, controlling electronics, calibrations procedures, and device performance in the lab and at the telescope will be presented. Some images of astronomical targets will also be shown.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David Kirk Gilmore, David C. Koo, and Richard Charles Puetter "Development and performance of a 128x128 2-um camera", Proc. SPIE 1235, Instrumentation in Astronomy VII, (1 July 1990); https://doi.org/10.1117/12.19162
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Cameras

Astronomy

Observatories

Space telescopes

Telescopes

Astrophysics

Electronics

RELATED CONTENT

Next ELOP-Payload focal plane array
Proceedings of SPIE (October 17 2007)
INCA a light 1 to 5 µm camera...
Proceedings of SPIE (September 30 2004)
SCUBA 2 a 10,000 pixel submillimeter camera for the...
Proceedings of SPIE (July 06 2006)
Laboratory and sky testing results for the TIS H4RG 10...
Proceedings of SPIE (September 25 2007)
FORCAST: the facility mid-IR camera for SOFIA
Proceedings of SPIE (June 28 2006)

Back to Top