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Near-IR integral field spectroscopy with adaptive optics

Abstract:
Integral field spectroscopy, in conjunction with adaptive optics systems, has the unique potential of providing spectra at spatial resolutions close to the diffraction limit of the telescope. We present first results from integral field spectroscopy in conjunction with an adaptive optics system, achieving diffraction limited images and spectra at the Calar Alto 3.5 meter telescope. SINFONI, an adaptive optics assisted integral field spectrometer currently being built for the VLT, is one of the few adaptive optics optimized integral field instruments. We present a brief summary of its features, together with a brief description of the image slicer employed in SINFONI.
Publication status:
Published

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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


Journal:
IMAGING THE UNIVERSE IN THREE DIMENSIONS: ASTROPHYSICS WITH ADVANCED MULTI-WAVELENGTH IMAGING DEVICES More from this journal
Volume:
195
Pages:
206-215
Publication date:
2000-01-01
Event title:
International Conference on Imaging the Universe in 3 Dimensions
ISBN:
1583810226


Keywords:
Pubs id:
pubs:5499
UUID:
uuid:0d9ec9c0-821b-48e7-a519-998e999f8988
Local pid:
pubs:5499
Source identifiers:
5499
Deposit date:
2012-12-19
ARK identifier:

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