9 January 1984 Two Design Approaches For High Efficiency Low Resolution Spectroscopy
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Proceedings Volume 0445, Instrumentation in Astronomy V; (1984); doi: 10.1117/12.966186
Event: 1983 Astronomy Conferences, 1983, London, United Kingdom
Abstract
In the course of a systematic analysis of various design philosophies aimed at achieving high optical throughput low resolution spectrometers for telescopes in the range of 2-4 meters, two distinct optical designs were established. The first is optimised for a telescope prime focus having a fast F/ratio, and is based on a concave grating whose aberrations are corrected by 2 or 3 off-axis lenses. The second system is a focal reducer, utilizing lenses and transmission gratings only. The use of a particular glass type having an extremely low dispersion permits excellent correction of various aberrations over a wide spectral range. Both designs provide a two-dimensionally corrected field typical of present day CCD array formats. These designs are highly suitable for long slit or field spectroscopy and offer the possibility of rapid switching to direct imaging mode.
© (1984) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Daniel Enard, Bernard Delabre, "Two Design Approaches For High Efficiency Low Resolution Spectroscopy", Proc. SPIE 0445, Instrumentation in Astronomy V, (9 January 1984); doi: 10.1117/12.966186; https://doi.org/10.1117/12.966186
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KEYWORDS
Mirrors

Cameras

Glasses

Spherical lenses

Sensors

Imaging systems

Monochromatic aberrations

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