Paper
9 July 1998 Recent advances with WYFFOS
David L. King, Susan P. Worswick
Author Affiliations +
Abstract
WYFFOS is a bench-mounted spectrograph based on a Baranne white pupil design, located on one of the Nasmyth platforms of the William Herschel Telescope. It is fed by 126 optical fibers which are accurately positioned in the corrected one degree focal plane by the robotic positioner. AUTOFIB-2 at the prime focus of the WHT. We describe two enhancements to the normal use of WYFFOS; the provision of an 'echelle' mode of operation, and the design for a new longer focal length camera.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David L. King and Susan P. Worswick "Recent advances with WYFFOS", Proc. SPIE 3355, Optical Astronomical Instrumentation, (9 July 1998); https://doi.org/10.1117/12.316756
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Cited by 2 scholarly publications.
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KEYWORDS
Cameras

Spectrographs

Mirrors

Charge-coupled devices

CCD cameras

Sensors

Collimators

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