5 October 2012 NIRMOS: a wide-field near-infrared spectrograph for the Giant Magellan Telescope
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NIRMOS (Near-Infrared Multiple Object Spectrograph) is a 0.9 to 2.5 μm imager/spectrograph concept proposed for the Giant Magellan Telescope1 (GMT). Near-infrared observations will play a central role in the ELT era, allowing us to trace the birth and evolution of galaxies through the era of peak star formation. NIRMOS' large field of view, 6.5′ by 6.5′, will be unique among imaging spectrographs developed for ELTs. NIRMOS will operate in Las Campanas' superb natural seeing and is also designed to take advantage of GMT's ground-layer adaptive optics system. We describe NIRMOS' high-performance optical and mechanical design.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Daniel Fabricant, Daniel Fabricant, Robert Fata, Robert Fata, Warren R. Brown, Warren R. Brown, Brian McLeod, Brian McLeod, Mark Mueller, Mark Mueller, Thomas Gauron, Thomas Gauron, John Roll, John Roll, Henry Bergner, Henry Bergner, John Geary, John Geary, Vladimir Kradinov, Vladimir Kradinov, Tim Norton, Tim Norton, Matt Smith, Matt Smith, Joseph Zajac, Joseph Zajac, } "NIRMOS: a wide-field near-infrared spectrograph for the Giant Magellan Telescope", Proc. SPIE 8446, Ground-based and Airborne Instrumentation for Astronomy IV, 84461O (5 October 2012); doi: 10.1117/12.926262; https://doi.org/10.1117/12.926262


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