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Stellar Populations at Higher Redshifts

Published online by Cambridge University Press:  01 December 2006

Tadayuki Kodama
Tadayuki Kodama*
Affiliation:
National Astronomical Obseravtory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan email: kodama@optik.mtk.nao.ac.jp
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Abstract

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We will review some recent advances in understanding the evolution of stellar populations in galaxies at relatively higher redshifts (z ≳ 0.5). We will focus on “mass assembly”, “down-sizing” and “high-z zoo” which have been among the most major topics and have seen great observational achievements in the past few years. In particular, wide-field near-infrared surveys, large spectroscopic surveys, and the Spitzer observations at infrared wavelengths, have unveiled underlying stellar masses and dusty star formation in high-z galaxies, which have been crucial in making such recent progresses.

Keywords

galaxies: evolutiongalaxies: formationgalaxies: luminosity functionmass functiongalaxies: stellar contentgalaxies: high-redshiftgalaxies: clusters: generalcosmology: large-scale structure of universe
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 537 - 545
Copyright
Copyright © International Astronomical Union 2007

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