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Article overview
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ATLAS: a Cassegrain spectrograph based on volume phase holographic gratings | J.G. Robertson
; K. Taylor
; I.K. Baldry
; P.R. Gillingham
; S.C. Barden
; | Date: |
27 Jun 2000 | Subject: | astro-ph | Affiliation: | AAO and U Sydney), K. Taylor (AAO), I.K. Baldry (AAO), P.R. Gillingham (AAO) and S.C. Barden (NOAO | Abstract: | We are proposing a new spectrograph (ATLAS) which would revolutionise 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 (24’). It will be ideally suited 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 maximise observing speed and allow optimised optical coatings to be used. The project is working towards its Concept Design Review which will occur during 2000. | Source: | arXiv, astro-ph/0006378 | Services: | Forum | Review | PDF | Favorites |
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