Translator Disclaimer
Paper
21 March 1997 Gemini instrumentation program overview
Author Affiliations +
Proceedings Volume 2871, Optical Telescopes of Today and Tomorrow; (1997) https://doi.org/10.1117/12.268993
Event: Optical Telescopes of Today and Tomorrow, 1996, Landskrona/Hven, Sweden
Abstract
Exploiting instrument platforms like the current generation of 8 - 10 m class telescopes represents a new era in instrument design, construction, handling, and use. Gemini's instruments are no exception to this revolution. For example, since at least 50% of Gemini's observing time will be queue scheduled, Cassegrain-mounted instruments will effectively remain on- line, ready to be called into service for typically months at a time with minimal delay to match observing programs with changing conditions. Furthermore, effective instrument emissivities of less than 1% will be needed to take advantage of the very low emissivity of the telescopes. Here we report on the technical status of the phase I instruments, describe attention being given to the total system performance of the telescopes and instruments, and list some of the considerations going into the phase II instrument program.
© (1997) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Douglas A. Simons, Fred C. Gillett, and Richard J. McGonegal "Gemini instrumentation program overview", Proc. SPIE 2871, Optical Telescopes of Today and Tomorrow, (21 March 1997); https://doi.org/10.1117/12.268993
PROCEEDINGS
12 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

The WSO: a world-class observatory for the ultraviolet
Proceedings of SPIE (February 24 2003)
The International Ultraviolet Explorer
Proceedings of SPIE (November 09 1981)
Gemini instrument program
Proceedings of SPIE (August 16 2000)

Back to Top