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arXiv · astro-ph/0107273

Population Synthesis and the Diagnostics of High-redshift Galaxies

Alberto Buzzoni
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Abstract

The effect of redshift on the observation of distant galaxies is briefly discussed emphasizing the possible sources of bias in the interpretation of high-z data. A general energetic criterion to assess physical self-consistency of evolutionary population synthesis models is also proposed, for a more appropriate use of this important tool to investigate distinctive properties of primeval galaxies.

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Alberto Buzzoni. 2001-07-16. Population Synthesis and the Diagnostics of High-redshift Galaxies. https://doi.org/10.1007/978-94-010-0393-3_39

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