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The High Redshift Universe with Adaptive Optics: Recent results from CFHT

1998/01/09 by D. Crampton, David Crampton, Crampton, David
Physics and Astronomy · #Adaptive optics and wavefront sensing #Astronomy and Astrophysical Research #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/9801076

4 pages latex using paspconf.sty. To appear in "The Young Universe", eds. S. D'Odorico, A. Fontana and E. Giallongo, A.S.P. Conf. Series. Related figures are available at http://www.hia.nrc.ca/science/instrumentation/optical/pueo2/pueo2.html

arxiv created 1998/01/09 · arxiv updated 2009/12/01

Abstract

The CFHT Adaptive Optics Bonnette (AOB) has been used to obtain high spatial resolution (0.1") observations of several extragalactic targets including the nuclei of nearby galaxies, high redshift galaxies, AGN, radiogalaxies, the host galaxies of quasars and gravitational lenses. Examples of these are discussed and the role of adaptive optics in exploring the high redshift universe is critically assessed in light of these results.

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