Evolutionary Population Synthesis Models of Primeval Galaxies: a Critical Appraisal
Astrophysics
2007-05-23 v1
Abstract
A theoretical approach relying on evolutionary population synthesis models could help refining the search criteria in deep galaxy surveys on the basis of a better knowledge of the expected apparent photometric properties of high-redshift objects. The following is a brief discussion reviewing some relevant aspects of the question in order to allow a more critical appraisal to primeval galaxy recognition.
Keywords
Cite
@article{arxiv.astro-ph/9711072,
title = {Evolutionary Population Synthesis Models of Primeval Galaxies: a Critical Appraisal},
author = {Alberto Buzzoni},
journal= {arXiv preprint arXiv:astro-ph/9711072},
year = {2007}
}
Comments
6 pages + 6 PS figures, LateX, Invited paper presented at IAU Symposium No. 183, Cosmological Parameters and Evolution of the Universe, held in Kyoto, Japan (Aug 18-22, 1997) in occasion of the XXIII IAU General Assembly. Ed. K. Sato, ASP Conf. Series (in press). (see also http://www.merate.mi.astro.it/~eps/home.html)