Paper
30 September 2004 A multi-object double spectrograph for the Large Binocular Telescope
Darren L. DePoy, Bruce Atwood, Stanley Ralph Belville, David Frederick Brewer, Paul L. Byard, Mark Derwent, Jennifer L. Marshall, Jerry Allan Mason, C. Morgan, Thomas P. O'Brien, Patrick S. Osmer, Daniel Patrick Pappalardo, Richard W. Pogge, David Paul Steinbrecher, Edward J. Teiga, David Hal Weinberg
Author Affiliations +
Abstract
We are building a Multi-Object Double Spectrograph for the Large Binocular Telescope. The instrument is designed to have high throughput from 320 to 1000 nm, spectral resolutions of 1,000-10,000, and multi-object capability over a 6 arcminute field. The design incorporates a dichroic and splits the science beam into a blue and a red channel, each of which can illuminate an 8,192 pixel long detector (with 15 micron pixels) with good image quality. The highly modular design can hold up to three gratings and an imaging flat and a selection of filters in each channel, all of which are quickly accessible; this allows for substantial observing flexibility. Progress on the construction of the instrument and future plans will be described.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Darren L. DePoy, Bruce Atwood, Stanley Ralph Belville, David Frederick Brewer, Paul L. Byard, Mark Derwent, Jennifer L. Marshall, Jerry Allan Mason, C. Morgan, Thomas P. O'Brien, Patrick S. Osmer, Daniel Patrick Pappalardo, Richard W. Pogge, David Paul Steinbrecher, Edward J. Teiga, and David Hal Weinberg "A multi-object double spectrograph for the Large Binocular Telescope", Proc. SPIE 5492, Ground-based Instrumentation for Astronomy, (30 September 2004); https://doi.org/10.1117/12.552275
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Cited by 7 scholarly publications.
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KEYWORDS
Cameras

Collimators

Astronomical imaging

Spectrographs

Computer aided design

Optical design

Telescopes

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