Paper
13 September 2012 Development of the single fibres and IFUs of WEAVE
Isabelle Guinouard, Piercarlo Bonifacio, Scott C. Trager, Marc A. W. Verheijen, Ian Lewis, Gavin Dalton
Author Affiliations +
Abstract
WEAVE is a new wide-field spectroscopy facility proposed for the prime focus of the 4.2m William Herschel telescope. The facility comprises a new 2 degree field of view prime focus corrector with a 1000-multiplex fibre positioner, a small number of individually deployable IFUs, and a large single IFU. The IFUs and the MOS fibres can be used to feed a dual-beam spectrograph that will provide full coverage of the majority of the visible spectrum in a single exposure at a resolution ~5000 or two 50nm-wide regions at a resolution of ~20000. This paper sums up the design of these two modes and describes the specific developments required to optimise the performances of the fibre system.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Isabelle Guinouard, Piercarlo Bonifacio, Scott C. Trager, Marc A. W. Verheijen, Ian Lewis, and Gavin Dalton "Development of the single fibres and IFUs of WEAVE", Proc. SPIE 8450, Modern Technologies in Space- and Ground-based Telescopes and Instrumentation II, 84503I (13 September 2012); https://doi.org/10.1117/12.924885
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KEYWORDS
Stars

Planets

Telescopes

Spectrographs

Molybdenum

Space telescopes

Spectroscopy

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