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Galaxy Evolutionary Synthesis Models
help you understand your data on star clusters and galaxies from the early universe until today in terms of their relevant physical and chemical properties and their evolutionary state.
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Star Formation, Chemical Enrichment and Mass Assembly Histories of Galaxies: The Observational Cosmology Approach
Star Formation, Chemical Enrichment and Mass Assembly Histories of Galaxies: The Astro-Archaeological Approach
Young Star Cluster Systems: Star Formation vs. Star Cluster Formation, violent vs normal SF
Pixel-by-pixel analysis of starburst galaxies
Tidal Dwarf Galaxies
Galaxy tranformations in clusters
QSO Absorption Lines, Attenuation and the Cosmic Baryon Content
Cosmo-chemical Evolution of Galaxies
Resolved stellar populations vs. integrated light: Accuracies and limitations in the recovery of Star Formation Histories
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Data - data.galev.org
Spectral & Photometric Evolution of Simple Stellar Populations at Various Metall
Wavelength and Redshift Dependence of Bulge/total light Ratios in Galaxies
Spectral and Photometric Evolution of Young Stellar Populations: The Impact of Gaseous emission at Various Metallicities
Chemically consistent evolution of galaxies: II. Spectrophotometric evolution from zero to high redshift
Accurate photometry of extended spherically symmetric sources
Analysing Globular Cluster observations Models and analysis tools for Lick/IDS indices
Galaxies to the redshift desert and beyond I. Chemically consistent galaxy modelling
Publications
GALEV overview and summary
Star clusters
Undisturbed galaxies
Galaxy transformation, interacting galaxies, mergers and starburst
High-Redshift galaxies
Technical papers