All Tables

Table 1: Ages (in units of yr), metallicities and numbering convention for the star clusters in the base.
Table 2: Empirical population synthesis results of percentage contributions from stars of all ages and metallicities to $F_{\lambda 5870}$ , for two sample galaxies. The "evolutionary paths'' favored by the analysis are highlighted (see text).
Table 3: Empirical population synthesis results of the galaxies with asymptotic (young-star) metallicities [ $Z/Z_\odot ]=-0.5$ : percentage contribution to $F_{\lambda 5870}$ .
Table 4: Empirical population synthesis results of the galaxies with asymptotic (young-star) metallicities [ $Z/Z_\odot ]= 0.0$ : percentage contribution to $F_{\lambda 5870}$ .