9 July 1998 Novel telescope-mounted spectral calibration source for the CFHT
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Abstract
At the Canada-France-Hawaii Telescope (CFHT) recent gains in Spectrographic capability has pointed out the need for a telescope-mounted Spectral Calibration Source that has three features: (1) A precise simulated pupil image, (2) Emission lines from .36 microns to 2.5 microns, (3) High throughput in the infrared. This paper describes the CFHT f/8 focus and then describes the Spectrographs and the Spectral Calibration Source (SCS) that use this focus.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Barney L. Magrath, Barney L. Magrath, Robin Arsenault, Robin Arsenault, Gregory A. Barrick, Gregory A. Barrick, Pierre Martin, Pierre Martin, Bernt Grundseth, Bernt Grundseth, Jeff Ward, Jeff Ward, Dan Wilcox, Dan Wilcox, Sue Ann Healey, Sue Ann Healey, Wiley Knight, Wiley Knight, } "Novel telescope-mounted spectral calibration source for the CFHT", Proc. SPIE 3355, Optical Astronomical Instrumentation, (9 July 1998); doi: 10.1117/12.316844; https://doi.org/10.1117/12.316844
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