PopStar I: Evolutionary synthesis models description
M. Molla, M.L. Garcia-Vargas, and A. Bressan

TL;DR
This paper introduces new evolutionary synthesis models for stellar populations across various ages and metallicities, incorporating detailed atmosphere models and nebular effects, suitable for studying high-redshift galaxies.
Contribution
The paper presents a comprehensive set of synthesis models that include nebular continuum effects and are validated against observed star cluster colours.
Findings
Models compare well with existing models at young and old ages.
Inclusion of nebular continuum significantly reddens young stellar populations.
Models reproduce observed colours of LMC star clusters.
Abstract
We present new evolutionary synthesis models for Simple Stellar Populations for a wide range of ages and metallicities. The models are based on the Padova isochrones. The core of the spectral library is provided by the medium resolution Lejeune et al. atmosphere models. These spectra are complemented by NLTE atmosphere models for hot stars that have an important impact in the stellar cluster's ionizing spectra: O, B and WR stellar spectra at the early ages, and spectra of post-AGB stars and planetary nebulae, at intermediate and old ages. At young ages, our models compare well with other existing models but we find that, the inclusion of the nebular continuum, not considered in several other models, reddens significantly the integrated colours of very young stellar populations. This is consistent with the results of spectral synthesis codes particularly devised for the study of…
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