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Proceedings Paper

The Maunakea Spectroscopic Explorer: throughput optimization
Author(s): Nicolas Flagey; Shan Mignot; Kei Szeto; Alan McConnachie; Rick Murowinski
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Paper Abstract

The Maunakea Spectroscopic Explorer (MSE) will obtain millions of optical to near-infrared spectra, at low (R~2,500) to high (R~40,000) spectral resolution, via a highly multiplexed (~3000) fiber-fed system. Key science programs for MSE (black hole reverberation mapping, stellar population analysis at high redshift, subkm/ s velocity accuracy for stellar astrophysics) will target faint Galactic and extra-galactic targets (typical visual magnitudes up to 24). MSE will thus need to achieve the highest throughput possible over the 360 to 1800 nm wavelength range. Here we discuss building an optimized throughput budget in terms of performance allocation and technical solutions to steer the concept design studies.

Paper Details

Date Published: 9 August 2016
PDF: 15 pages
Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 99089C (9 August 2016); doi: 10.1117/12.2231238
Show Author Affiliations
Nicolas Flagey, Canada-France-Hawaii Telescope (United States)
Shan Mignot, GEPI, Observatoire de Paris, PSL Research Univ., CNRS, Univ. Paris Diderot (France)
Kei Szeto, Canada-France-Hawaii Telescope (United States)
Alan McConnachie, Canada-France-Hawaii Telescope (United States)
Rick Murowinski, Canada-France-Hawaii Telescope (United States)


Published in SPIE Proceedings Vol. 9908:
Ground-based and Airborne Instrumentation for Astronomy VI
Christopher J. Evans; Luc Simard; Hideki Takami, Editor(s)

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