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Design and production of the DESI fibre cables

Schmoll, J; Besuner, R; Bramall, D; Brooks, D; Edelstein, J; Jelinsky, P; Levi, M; ... Schlegel, D; + view all (2018) Design and production of the DESI fibre cables. In: Ground-based and Airborne Instrumentation for Astronomy VII. SPIE Green open access

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Abstract

The Dark Energy Spectroscopic Instrument (DESI) is under construction to measure the expansion history of the Universe using the Baryonic Acoustic Oscillation technique. The spectra of 35 million galaxies and quasars over 14000 sq deg will be measured during the life of the experiment. A new prime focus corrector for the KPNO Mayall telescope will deliver light to 5000 fibre optic positioners. The fibres in turn feed 10 broad-band spectrographs. We will describe the design and production progress on the fibre cables, strain relief system and preparation of the slit end. In contrast to former projects, the larger scale of production required for DESI requires teaming up with industry to find a solution to reduce the time scale of production as well as to minimise the stress on the optical fibres.

Type: Proceedings paper
Title: Design and production of the DESI fibre cables
Event: SPIE Astronomical Telescopes + Instrumentation, 2018, Austin, Texas, United States
ISBN-13: 9781510619579
Open access status: An open access version is available from UCL Discovery
DOI: 10.1117/12.2312140
Publisher version: https://doi.org/10.1117/12.2312140
Language: English
Additional information: This is the published version of record. For information on re-use, please refer to the publisher’s terms and conditions.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/10060420
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