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The High Redshift Population of Field Galaxies

Published online by Cambridge University Press:  25 May 2016

David C. Koo
David C. Koo*
Affiliation:
UCO/Lick Observatory, University of California, Santa Cruz, CA 95064, USA

Abstract

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In principle, observations of the high redshift population of field galaxies should provide powerful probes of interactions and mergers. As initial examples of such explorations, we highlight recent results from the DEEP program that take advantage of Keck and HST, including median redshifts for samples fainter than I ~ 22, morphologies and colors to z ~ 1, and especially the nature of z ~ 3 galaxies in the Hubble Deep Field. Although tantalizing, the results will need much larger samples to be confirmed and better quantified.

Type
Deep Fields & Evolution
Information
Symposium - International Astronomical Union , Volume 186: Galaxy Interactions at High and Low Redshift , 1999 , pp. 423 - 429
Copyright
Copyright © Kluwer 1999 

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