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arXiv · 0807.3774

The MagE Spectrograph

J. L. Marshall·Scott Burles·Ian B. Thompson·Stephen A. Shectman·Bruce C. Bigelow·Gregory Burley·Christoph Birk·Jorge Estrada·Patricio Jones·Matthew Smith·Vince Kowal·Jerson Castillo·Robert Storts·Greg Ortiz
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Abstract

The Magellan Echellette (MagE) spectrograph is a single-object optical echellette spectrograph for the Magellan Clay telescope. MagE has been designed to have high throughput in the blue; the peak throughput is 22% at 5600 A including the telescope. The wavelength coverage includes the entire optical window (3100 A - 1 micron). The spectral resolution for a 1" slit is R~4100. MagE is a very simple spectrograph with only four moving parts, prism cross-dispersion, and a vacuum Schmidt camera. The instrument saw first light in November 2007 and is now routinely taking science observations.

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J. L. Marshall, Scott Burles, Ian B. Thompson, Stephen A. Shectman, Bruce C. Bigelow, Gregory Burley, Christoph Birk, Jorge Estrada, Patricio Jones, Matthew Smith, Vince Kowal, Jerson Castillo, Robert Storts, Greg Ortiz. 2008-07-24. The MagE Spectrograph. https://doi.org/10.1117/12.789972

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