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Proceedings Paper

ATLAS: a Cassegrain spectrograph based on volume phase holographic gratings
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Paper Abstract

We are proposing a new spectrograph (ATLAS) which would revolutionize intermediate-dispersion observations at the AAT. Based on the new technology of volume phase holographic gratings, and using transmission optics, ATLAS offers high throughput and a wide field. It will be ideally situated to extensive surveys of faint objects. It has been designed with a collimated beam diameter of 150 mm, giving resolution (lambda) /(delta) (lambda) up to nearly 10,000 with a 1.5 arcsecond slit and good efficiency. It will be a dual-beam instrument, to maximize observing speed and allow optimized optical coatings to be used. The project is working towards its concept design review which will occur during 2000.

Paper Details

Date Published: 27 March 2000
PDF: 9 pages
Proc. SPIE 4008, Optical and IR Telescope Instrumentation and Detectors, (27 March 2000); doi: 10.1117/12.395472
Show Author Affiliations
J. Gordon Robertson, Anglo-Australian Observatory and Univ. of Sydney (Australia)
Keith Taylor, Anglo-Australian Observatory (United States)
Ivan K. Baldry, Anglo-Australian Observatory (Australia)
Peter R. Gillingham, Anglo-Australian Observatory (Australia)
Samuel Charles Barden, National Optical Astronomy Observatories (United States)


Published in SPIE Proceedings Vol. 4008:
Optical and IR Telescope Instrumentation and Detectors
Masanori Iye; Alan F. M. Moorwood, Editor(s)

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