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UV properties and evolution of high-redshift galaxies

Alberto Buzzoni
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Abstract

I assess the problem of morphological and photometric evolution of high-redshift galaxies in the ultraviolet wavelength range. My discussion will partly rely on a new set of template galaxy models, in order to infer the expected changes along the Hubble morphological sequence at the different cosmic epochs. The impact of evolution on the faint-end galaxy luminosity function at z~1 and beyond will also be evaluated and briefly discussed. See http://www.merate.mi.astro.it/~eps/home.html for more info and model retrieval.

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Alberto Buzzoni. 2002-10-07. UV properties and evolution of high-redshift galaxies. https://arxiv.org/abs/astro-ph/0210160

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