A UV prime-focus spectrograph for the CFHT

Astronomy and Astrophysics – Astronomy

Scientific paper

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Ultraviolet Astronomy, Ultraviolet Spectrometers, Charge Coupled Devices, Elliptical Galaxies, Gratings (Spectra), Quasars, Seyfert Galaxies

Scientific paper

The UV prime spectrograph at the Canada-France-Hawaii Telescope is the first instrument to be designed with an aspherized diffraction grating. This technique leads to all reflective Schmidt designs with a very small amount of optical surfaces and fast aperture ratio. A thin backside illuminated RCA CCD is now used as the detector. Since the detector is at the focus of an f/1 mounting, within the optical path, a minicryostat (5 cm×5 cm×3 cm) was designed to minimize the central obscuration. This paper describes this new instrument, its performances and some examples of applications.

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