Ridgway, Susan E. and Heckman, Tim and Lacy, Mark (2004) Colors and magnitudes of quasar host galaxies at high redshift. In: The Interplay among Black Holes, Stars, and ISM in Galactic Nuclei. Proceedings of the International Astronomical Union. Vol.2004. No.Sympos. International Astronomical Union , pp. 537-538. https://resolver.caltech.edu/CaltechAUTHORS:RIDpiaus04
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Abstract
We discuss the results so far of a program to image in the rest-frame optical and near-UV the host galaxies of a sample of 5 high redshift (z ~ 2–3) radio-quiet quasars with nuclear luminosities lower than most samples studied at high z. We found that in the rest-frame optical the hosts have luminosities of about L*, comparable to the Lyman break galaxies at similar redshifts. From the rest-frame UV imaging, we can derive optical–UV colors, and find they show a great deal of variation, but may be somewhat redder and less starforming than the LBGs. We are supplementing this work at high z with study of the hosts of z ~ 1 radio-quiet quasars with similar low nuclear luminosities.
Item Type: | Book Section | ||||||
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Additional Information: | © 2004 International Astronomical Union | ||||||
Series Name: | Proceedings of the International Astronomical Union | ||||||
Issue or Number: | Sympos | ||||||
Record Number: | CaltechAUTHORS:RIDpiaus04 | ||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:RIDpiaus04 | ||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
ID Code: | 3683 | ||||||
Collection: | CaltechAUTHORS | ||||||
Deposited By: | Lindsay Cleary | ||||||
Deposited On: | 26 Jun 2006 | ||||||
Last Modified: | 02 Oct 2019 23:05 |
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