Paper
24 September 2012 GMACS: a wide field, multi-object, moderate-resolution, optical spectrograph for the Giant Magellan Telescope
D. L. DePoy, R. Allen, R. Barkhouser, E. Boster, D. Carona, A. Harding, R. Hammond, J. L. Marshall, J. Orndorff, C. Papovich, K. Prochaska, T. Prochaska, J. P. Rheault, S. Smee, S. Shectman, S. Villanueva Jr.
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Abstract
We present a conceptual design for a moderate resolution optical spectrograph for the Giant Magellan Telescope (GMT). The spectrograph is designed to make use of the large field-of-view of the GMT and be suitable for observations of very faint objects across a wide range of optical wavelengths. We show some details of the optical and mechanical design of the instrument.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
D. L. DePoy, R. Allen, R. Barkhouser, E. Boster, D. Carona, A. Harding, R. Hammond, J. L. Marshall, J. Orndorff, C. Papovich, K. Prochaska, T. Prochaska, J. P. Rheault, S. Smee, S. Shectman, and S. Villanueva Jr. "GMACS: a wide field, multi-object, moderate-resolution, optical spectrograph for the Giant Magellan Telescope", Proc. SPIE 8446, Ground-based and Airborne Instrumentation for Astronomy IV, 84461N (24 September 2012); https://doi.org/10.1117/12.926186
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Cited by 14 scholarly publications.
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KEYWORDS
Spectrographs

Cameras

Telescopes

Astronomical imaging

Collimators

Optical design

Mirrors

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