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The Oxford SWIFT integral field spectrograph - art. no. 62693L

Abstract:

We present the design of the Oxford SWIFT integral field spectrograph, a dedicated I and z band instrument (0.65 mu m - 1.0 mu m at R similar to 4000), designed to be used in conjunction with the Palomar laser guide star adaptive optics system (PALAO, and its planned upgrade PALM-3000). It builds on two recent developments (i) the improved ability of second generation adaptive optics systems to correct for atmospheric turbulence at wavelengths <= 1 mu m, and (ii) the availability of CCD ar...

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Publication status:
Published

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Publisher copy:
10.1117/12.670859

Authors


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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
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Journal:
Ground-based and Airborne Instrumentation for Astronomy, Pts 1- 3
Volume:
6269
Pages:
L2693-L2693
Publication date:
2006-01-01
Event title:
Conference on Ground-Based and Airborne Instrumentation for Astronomy
DOI:
ISSN:
0277-786X
Source identifiers:
22468
ISBN:
0819463345
Keywords:
Pubs id:
pubs:22468
UUID:
uuid:d09700e0-c105-4dd3-99c3-9b5fa4b29a4e
Local pid:
pubs:22468
Deposit date:
2012-12-19

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