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ALFA and 3D: integral field spectroscopy with adaptive optics

Abstract:

One of the most important techniques for astrophysics with adaptive optics is the ability to do spectroscopy at diffraction limited scales. The extreme difficulty of positioning a faint target accurately on a very narrow slit can be avoided by using an integral field unit, which provides the added benefit of full spatial coverage. During 1998, working with ALFA and the 3D integral field spectrometer, we demonstrated the validity of this technique by extracting and distinguishing spectra from ...

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Publication status:
Published

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Publisher copy:
10.1117/12.390393

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Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Astrophysics
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Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Astrophysics
Tacconi-Garman, LE More by this author
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Volume:
4007
Pages:
952-961
Publication date:
2000-05-10
DOI:
ISSN:
0277-786X
URN:
uuid:1cbc2917-b598-4208-aa13-a7e54ce75318
Source identifiers:
6274
Local pid:
pubs:6274
ISBN:
0-8194-3632-1
Keywords:

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