Paper
9 July 2008 The Southern African Large Telescope (SALT) calibration system
D. A. H. Buckley, J. Brink, N. S. Loaring, A. Swat, H. L. Worters
Author Affiliations +
Abstract
This paper presents details of the instrument calibration system employed on the SALT. It is designed to inject light into the Spherical Aberration Corrector at about the position of the primary mirror caustic, thereby simulating the same degree of vignetting as experienced by celestial objects. A light-shaping diffuser screen, coupled with Fresnel lenses, modifies the beam to increase efficiency and attempt to illuminate the detectors in the same manner as a uniform sky. Light is conveyed by means of liquid light guides from either QTH flat field lamps or a choice of hollow cathode (CuAr, ThAr) and penray (Ar, Hg, Xe, Ne) lamps, used for wavelength calibration. Changing entrance pupil effects are accounted for by employing a moving exit pupil baffle, which can simulate the pupil geometry of a specific track.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
D. A. H. Buckley, J. Brink, N. S. Loaring, A. Swat, and H. L. Worters "The Southern African Large Telescope (SALT) calibration system", Proc. SPIE 7014, Ground-based and Airborne Instrumentation for Astronomy II, 70146H (9 July 2008); https://doi.org/10.1117/12.790385
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KEYWORDS
Calibration

Lamps

Mirrors

Waveguides

Diffusers

Telescopes

Vignetting

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