16 November 1982 Cooled Grating Array Spectrometer For 0.6-5 μm
Author Affiliations +
Abstract
A grating spectrometer, designed to illuminate an array of 122 InSb photodiodes with minimum aberrations and maximum speed, has been constructed. The instrument will be used on the 5 meter Hale telescope at Palomar Observatory, and is easily adaptable to telescopes of various focal ratios. A resolving power of 100-1000 can be obtained at wavelengths between 0.6 pm and 5 pm with remotely interchangeable gratings. The spectrometer is sufficiently compact to fit on the 8-inch work surface of a commercially available dewar, and uses simple on-axis spherical and paraboloidal optical elements. The camera mirror produces an f/2.5 beam which, with the 0.2 mm detectors, allows a 3" focal-plane aperture on the 5 meter telescope. All rays fall within a 100 μm blur circle at all points along the array. Distortions have been corrected with a tilted field flattening lens in front of the detector.
© (1982) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
J. E. Nordholt, J. E. Nordholt, J. H. Lacy, J. H. Lacy, } "Cooled Grating Array Spectrometer For 0.6-5 μm", Proc. SPIE 0331, Instrumentation in Astronomy IV, (16 November 1982); doi: 10.1117/12.933453; https://doi.org/10.1117/12.933453
PROCEEDINGS
4 PAGES


SHARE
Back to Top