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Surveys of High-Redshift QSO Hosts

Published online by Cambridge University Press:  12 April 2016

J.B. Hutchings
J.B. Hutchings*
Affiliation:
Herzberg Institute of Astrophysics, 5071 West Saanich Rd, Victoria B.C., Canada

Abstract

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Recent investigations of high-redshift QSO morphology are reviewed and compared. The PSF-removal is difficult and results are given in several different forms. The reliability of results from HST and ground-based AO are compared, and several caveats to conventional wisdom are given.

Type
Part 5. AGN Phenomena
Information
International Astronomical Union Colloquium , Volume 184: AGN Surveys , 2002 , pp. 317 - 323
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Hutchings, J.B. 1998, AJ, 116, 20 CrossRefGoogle Scholar
Hutchings, J.B. 2001, IAA workshop on QSO Hosts (astro-ph/0107157)Google Scholar
Hutchings, J.B., Saintonge, A., Schade, D., Prenette, D., 2001, AJ (submitted)Google Scholar
Lacy, M., Laurent-Muehliesen, S.A., Ridgway, S.A., Becker, R.H., White, R.L. 2001, ApJ, (astro-ph/0103087)Google Scholar