Evolutionary Population Synthesis Models of Primeval Galaxies: a Critical Appraisal
| dc.creator | Buzzoni, Alberto | |
| dc.date | 1997-11-07 | |
| dc.date.accessioned | 2026-07-07T02:24:57Z | |
| dc.date.available | 2026-07-07T02:24:57Z | |
| dc.description | 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. | |
| dc.description | 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) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9711072 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9711072 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11758 | |
| dc.subject | Astrophysics | |
| dc.title | Evolutionary Population Synthesis Models of Primeval Galaxies: a Critical Appraisal | |
| dc.type | text |