Paper
13 February 2003 Science at mid-infrared wavelengths with large telescopes
Author Affiliations +
Abstract
For background-limited observations such as those at mid-infrared wavelengths, an increase in telescope aperture not only improves the angular resolution (as it does at all wavelengths) but also leads to very large increases in sensitivity because of the reduced background within the diffraction-limited point spread function. In this presentation we look at the magnitude of that increase for several different operational modes of mid-infrared instrumentation, and we consider some of the implications for science on the current generation of 8-10 meter telescopes.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Charles M. Telesco, David Ciardi, and Chris C. Packham "Science at mid-infrared wavelengths with large telescopes", Proc. SPIE 4834, Discoveries and Research Prospects from 6- to 10-Meter-Class Telescopes II, (13 February 2003); https://doi.org/10.1117/12.460956
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KEYWORDS
Mid-IR

Stars

Telescopes

Space telescopes

Coronagraphy

Spatial resolution

Gemini Observatory

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