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SWIFT: An adaptive optics assisted I/z band integral field spectrograph

Abstract:
SWIFT is an adaptive optics assisted integral field spectrograph covering the I and z astronomical bands (0.7-1.0 mu m) at a spectral resolving power R <= 5000. At its heart is an all-glass image slicer with high throughput based on a novel de-magnifying design allowing a compact instrument. SWIFT profits from two recent developments: (i) the improved ability of second generation adaptive optics systems to correct for atmospheric turbulence in SWIFTS's bandpass, and (ii) the availability of CCD array detectors with high quantum efficiency at very red wavelengths. It is a dedicated integral field spectrograph, specifically built to address a range of interesting astrophysical questions. (c) 2005 Elsevier B.V. All rights reserved.
Publication status:
Published

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Publisher copy:
10.1016/j.newar.2005.10.019

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Role:
Author


Journal:
NEW ASTRONOMY REVIEWS More from this journal
Volume:
49
Issue:
10-12
Pages:
647-654
Publication date:
2006-01-01
DOI:
ISSN:
1387-6473


Language:
English
Keywords:
Pubs id:
pubs:31007
UUID:
uuid:7ac7e702-e75f-479d-8c99-0498fb5929ee
Local pid:
pubs:31007
Source identifiers:
31007
Deposit date:
2012-12-19

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