9 August 2016 Fiber system design for the Dark Energy Spectroscopic Instrument (DESI)
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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 40 million galaxies 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 Fiber Systems design with specific emphasis on novel approaches and essential elements that lead to exceptional performance.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Claire Poppett, Claire Poppett, Ray Sharples, Ray Sharples, Jerry Edelstein, Jerry Edelstein, Jürgen Schmoll, Jürgen Schmoll, David Bramall, David Bramall, Parker Fagrelius, Parker Fagrelius, "Fiber system design for the Dark Energy Spectroscopic Instrument (DESI)", Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 99089A (9 August 2016); doi: 10.1117/12.2234553; https://doi.org/10.1117/12.2234553

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