Modeling, Systems Engineering, and Project Management for Astronomy IX 2020
DOI: 10.1117/12.2562305
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Fibre links for the WEAVE instrument: the making of

Abstract: The WEAVE instrument nearing completion for the William Herschel Telescope is a fiber-fed spectrograph operating in three different modes. Two comprise deployable fibers at the prime focus for point-like objects and small integral field units (IFU), the third is a large IFU placed at the center of the field. Three distinct fiber systems support these modes and route the photons to the spectrograph located on the Nasmyth platform 33m away: the first features 960+940 fibers and is duplicated to allow configuring… Show more

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“…To optimise the use of the detector spatially, all optical fibres need to be ordered linearly at the interface to the spectrograph. This is achieved by grouping the ends of the fibres into numbered metal casings called slitlets, which was completed prior to the fibres arriving at Oxford [10] . It is also important that the ordering of the fibres is recorded to match the spectra to the correct object.…”
Section: Slit Assemblymentioning
confidence: 99%
“…To optimise the use of the detector spatially, all optical fibres need to be ordered linearly at the interface to the spectrograph. This is achieved by grouping the ends of the fibres into numbered metal casings called slitlets, which was completed prior to the fibres arriving at Oxford [10] . It is also important that the ordering of the fibres is recorded to match the spectra to the correct object.…”
Section: Slit Assemblymentioning
confidence: 99%