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The Desi Spectrograph System and Production

Edelstein, J; Jelinsky, P; Levi, M; Tarle, G; Brooks, D; (2018) The Desi Spectrograph System and Production. In: Proceedings of the Ground-based and Airborne Instrumentation for Astronomy VII: 107027G (2018). SPIE: Austin, Texas, USA. Green open access

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Abstract

The Dark Energy Spectroscopic Instrument (DESI) is a project in construction to measure the expansion history of the Universe using the Baryon Acoustic Oscillation technique. The spectra of 35 million galaxies and quasars over 14,000 square degrees will be measured during the life of the experiment. A new prime focus corrector for the KPNO Mayall telescope will deliver light to 5000 fiber optic positioners. The fibers in turn feed ten broad-band spectrographs covering a 360 - 980 nm passband with a spectral resolution (λ/Δλ) between 1500 and 4000. The spectrograph uses two dichroic beam splitters to separate the flux among three spectral cameras, each with a volume phase holographic grating and lens system that focuses onto a charge coupled device detector. We describe the spectrograph, its system requirements, design and construction.

Type: Proceedings paper
Title: The Desi Spectrograph System and Production
Event: SPIE Astronomical Telescopes + Instrumentation, 2018
ISBN-13: 9781510619579
Open access status: An open access version is available from UCL Discovery
DOI: 10.1117/12.2311821
Publisher version: https://doi.org/10.1117/12.2311821
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: DESI, dark energy, multi-object spectrograph, Mayall telescope
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/10060428
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