Poster + Paper
13 December 2020 Performance of the Dark Energy Spectroscopic Instrument (DESI) focal plane
Parker Fagrelius, Yutong Duan, Kevin Fanning, Klaus Honscheid, Steven Kent, Paul Martini, Claire Poppett, David Rabinowitz, Michael Schubnell, Joseph Silber, David Brooks, Todd Claybaugh, Peter Doel, Enrique Gaztañaga, Michael Levi, Christophe Magneville, Francisco Prada, Greg Tarlé
Author Affiliations +
Conference Poster
Abstract
The recently commissioned Dark Energy Spectroscopic Instrument (DESI) will measure the expansion history of the Universe using the Baryon Acoustic Oscillation technique. The spectra of 35 million galaxies and quasars over 14,000 sq deg will be measured during the life of the experiment. A new prime focus corrector for the KPNO Mayall telescope delivers light to 5,000 fiber optic positioners which in turn feed ten broad-band spectro- graphs. The DESI focal plane subsystem contains the fiber optic positioners and guide and focus cameras, which enable the alignment of fibers with astronomical targets. This paper describes the performance of the installed instrument.
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Parker Fagrelius, Yutong Duan, Kevin Fanning, Klaus Honscheid, Steven Kent, Paul Martini, Claire Poppett, David Rabinowitz, Michael Schubnell, Joseph Silber, David Brooks, Todd Claybaugh, Peter Doel, Enrique Gaztañaga, Michael Levi, Christophe Magneville, Francisco Prada, and Greg Tarlé "Performance of the Dark Energy Spectroscopic Instrument (DESI) focal plane", Proc. SPIE 11447, Ground-based and Airborne Instrumentation for Astronomy VIII, 114478K (13 December 2020); https://doi.org/10.1117/12.2561631
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Cited by 1 scholarly publication.
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KEYWORDS
Spectroscopes

Fiber optics

Robots

Astronomy

Baryon acoustic oscillations

Cameras

Galactic astronomy

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