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UV camera conceptual designs for TMT Fiber WFOS
Author(s): L. Gilles; D. Shafer; B. Delabre
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Paper Abstract

This paper discusses refractive, reflective and catadioptric designs for the Thirty Meter Telescope Fiber Wide Field Optical Spectrograph (WFOS) instrument concept. Custom macros were written to evaluate performance at the detector plane with the grating at the pupil as a function of fiber position in the pseudo-slit and wavelength, and a tolerance analysis has been performed for each design based on best engineering practices to assess performance robustness against opto-mechanical errors. The catadioptric camera appears to provide the best compromise in this regard.

Paper Details

Date Published: 13 July 2018
PDF: 22 pages
Proc. SPIE 10702, Ground-based and Airborne Instrumentation for Astronomy VII, 10702AD (13 July 2018); doi: 10.1117/12.2315618
Show Author Affiliations
L. Gilles, Thirty Meter Telescope International Observatory LLC (United States)
D. Shafer, David Shafer Optical Design (United States)
B. Delabre, European Southern Observatory (Germany)


Published in SPIE Proceedings Vol. 10702:
Ground-based and Airborne Instrumentation for Astronomy VII
Christopher J. Evans; Luc Simard; Hideki Takami, Editor(s)

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