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DESI commissioning instrument metrology

Coles, RA; Brooks, D; Derwent, M; Martini, P; O'Brien, T; Ross, A; Tie, SS; (2018) DESI commissioning instrument metrology. In: Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation III. 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 Baryon 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 fiber optic positioners. The fibers in turn feed ten broad-band spectrographs. We will describe the methods and results for the commissioning instrument metrology program. The primary goals of this program are to calculate the transformations and further develop the systems that will place fibers within 5μm RMS of the target positions. We will use the commissioning instrument metrology program to measure the absolute three axis Cartesian coordinates of the five CCDs and 22 illuminated fiducials on the commissioning instrument.

Type: Proceedings paper
Title: DESI commissioning instrument metrology
Event: SPIE Astronomical Telescopes + Instrumentation, 2018, Austin, Texas, United States
ISBN-13: 9781510619654
Open access status: An open access version is available from UCL Discovery
DOI: 10.1117/12.2312592
Publisher version: https://doi.org/10.1117/12.2312592
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/10060418
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