GALAXY ISOCHRONE SYNTHESIS SPECTRAL EVOLUTION LIBRARY
(GISSEL-XXI)
Copyright © 1991-2001 G. Bruzual A. and S. Charlot. All Rights Reserved.

To build a Simple Stellar Population (SSP) Model, select the model ingredients and press the Build Model button. Enter either the model option number or select the metallicity for the desired set of tracks (highest priority to the left):

Model Option Number: Padova (2000) Z = 0.0004 Z = 0.001 Z = 0.004 Z = 0.008 Z = 0.019 Z = 0.03 Padova (1994) Z = 0.0001 Z = 0.0004 Z = 0.004 Z = 0.008 Z = 0.02 Z = 0.05 Z = 0.10 Geneva (1994) Z = 0.02

Stellar Spectra: Theoretical Model Atmospheres LCB Atlas, Revised Version LCB Atlas, Original Version LCB Atlas, Westera Revised Version Empirical Spectra (solar Z) Pickles Atlas (extended 2000) Pickles Atlas (extended 1999) Pickles Atlas (extended 1997) Pickles Atlas HiRes (extended 1997) Pickles Atlas (extended 1995) Pickles Atlas HiRes (extended 1995)

Initial Mass Function: Salpeter (1955) Scalo (1998) Kroupa et al. (1993) Scalo (1986) Miller & Scalo (1979) Kennicutt (1983) Lequeux et al. (1979) Ferrano et al. (1997) Piotto et al. (1997) Carigi et al. (1999) Upper Mass Limit: Lower Mass Limit:

Output file generic name:

Subdirectory to write output files:

Additional Output Files: Store sed's from different stellar groups Store % of total light from different stellar groups Store files from two previous options Write files required by DUST models Write files required by EMISSION LINE models Write files required by STELLAR COLLISION models Write *.seg, *.step, and *.mfd files

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Copyright © 1991-2001 G. Bruzual A. and S. Charlot. All Rights Reserved.
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