9 August 2016 The DESI slit design: science and calibration solutions
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The Dark Energy Survey Instrument (DESI) is a 5000-fibre optical multi object spectrograph for the 4m Mayall telecope at the Kitt Peak National Observatory. Ten identical three channel spectrographs will be equipped with 500-element fibre slits. Here we focus on the architecture of the science slits and the interchangeable auxiliary slits required for calibration.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jurgen Schmoll, Jurgen Schmoll, Robert Besuner, Robert Besuner, David Bramall, David Bramall, Colin Dunlop, Colin Dunlop, Jerry Edelstein, Jerry Edelstein, Patrick Jelinsky, Patrick Jelinsky, Claire Poppett, Claire Poppett, Ray Sharples, Ray Sharples, Gordon Talbot, Gordon Talbot, "The DESI slit design: science and calibration solutions", Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 99088T (9 August 2016); doi: 10.1117/12.2233050; https://doi.org/10.1117/12.2233050


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