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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.

Online Databases

Wavelength and Redshift Dependence of Bulge/total light Ratios in Galaxies
J. Schulz, U. Fritze & K. J. Fricke; A&A 398, 89 (2003)
Spectral and Photometric Evolution of Young Stellar Populations:
The Impact of Gaseous emission at Various Metallicities

P. Anders & U. Fritze; A&A 401, 1063 (2003)
(includes update of "Spectral & Photometric Evolution of Simple Stellar Populations at Various Metallicities" by Schulz et al.)
Chemically consistent evolution of galaxies:
II. Spectrophotometric evolution from zero to high redshift

J. Bicker, U. Fritze, C. S. Möller, K. J. Fricke; A&A 413, 37 (2004)
Accurate photometry of extended spherically symmetric sources
P. Anders, M. Gieles, R. de Grijs; A&A 451, 375 (2006)
GALEV SSP models for star clusters in tidal fields
P. Anders, H. J. G. L. M. Lamers & H. Baumgardt; A&A 502, 817 (2009)
Galaxies to the redshift desert and beyond - I. Chemically consistent galaxy modelling
Galaxies to the redshift desert and beyond - II. Comparison to observations
R. Kotulla, submitted to MNRAS
The data will be made available on this webpage once the paper has been accepted.

Older and superseded data

Spectral & Photometric Evolution of Simple Stellar Populations at Various Metallicities
J. Schulz, U. Fritze, C. S. Möller & K. J. Fricke; A&A 392, 1 (2002)
IMPORTANT: Superseded by Anders & Fritze (2003) - please use these newer models instead.