MIRADAS for the Gran Telescopio Canarias: System Overview
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2012
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SPIE-Int Soc Optical Engineering
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Eikenberry, S. S., J. G. Bennett, B. Chinn, H. V. Donoso, S. A. Eikenberry, E. Ettedgui, A. Fletcher, et al. «MIRADAS for the Gran Telescopio Canarias: system overview». En Ground-based and Airborne Instrumentation for Astronomy IV, 8446:1794-1806. SPIE, 2012. https://doi.org/10.1117/12.925686.
Abstract
The Mid-resolution InfRAreD Astronomical Spectrograph (MIRADAS, a near-infrared multi-object echelle spectrograph operating at spectral resolution R=20,000 over the 1-2.5 mu m bandpass) was selected in 2010 by the Gran Telescopio Canarias (GTC) partnership as the next-generation near-infrared spectrograph for the world's largest optical/infrared telescope, and is being developed by an international consortium. The MIRADAS consortium includes the University of Florida, Universidad de Barcelona, Universidad Complutense de Madrid, Instituto de Astrofisica de Canarias, Institut de Fisica d'Altes Energies, Institut d'Estudis Espacials de Catalunya and Universidad Nacional Autonoma de Mexico, as well as probe arm industrial partner A-V-S (Spain). In this paper, we review the overall system design for MIRADAS, as it nears Preliminary Design Review in the autumn of 2012.
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© 2012 SPIE. Conference on Ground-Based and Airborne Telescopes (4º. 2012. Amsterdam, Netherlands)