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Table B.1.

Stellar population synthesis results obtained with FIREFLY.

Name E(B-V) age ageup agelow Z Zup Zlow ages0 w0 ages1 w! ages2 w2 ages3 w3 ages4 w4 ages5 w5
MCG_Main 0.226 0.83 0.92 0.79 -0.173 -0.119 -0.314 1.000 0.485 0.602 0.242 0.301 0.227 1.041 0.045 -99.990 -99.990 -99.990 -99.990
MCG_12 0.445 0.88 0.96 0.78 -0.314 -0.173 -0.436 0.845 0.273 0.954 0.273 1.079 0.181 0.176 0.181 0.778 0.045 1.079 0.045
MCG_111112 0.000 1.08 1.09 1.01 -0.041 0.090 -0.106 1.114 0.371 1.000 0.371 1.114 0.248 1.114 0.010 -99.990 -99.990 -99.990 -99.990
MCG_1111111 0.219 1.02 1.06 0.95 -0.224 -0.045 -0.257 1.000 0.500 1.000 0.250 1.079 0.250 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990
NGC 4065_Main 0.106 0.77 0.85 0.71 0.110 0.180 -0.034 0.954 0.300 0.602 0.300 0.954 0.200 0.000 0.200 -2.046 0.001 -99.990 -99.990
NGC 4065_112 0.166 0.90 0.96 0.77 -0.163 -0.149 -0.633 1.114 0.250 1.079 0.250 -0.222 0.250 0.778 0.250 -99.990 -99.990 -99.990 -99.990
NGC 4065_1112 0.083 0.89 0.93 0.83 0.142 0.169 0.087 0.602 0.455 1.114 0.227 1.079 0.227 0.301 0.091 -99.990 -99.990 -99.990 -99.990
NGC 4104_Main 0.045 0.93 0.97 0.88 0.254 0.254 0.201 1.000 0.500 1.079 0.250 0.301 0.250 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990
NGC 4104_11 0.053 0.83 0.87 0.83 0.254 0.254 0.254 1.079 0.250 0.699 0.250 0.176 0.167 0.602 0.167 1.000 0.167 -99.990 -99.990
NGC 4104_err11 0.045 0.85 0.92 0.83 0.254 0.256 0.224 1.079 0.250 0.176 0.250 0.602 0.250 1.041 0.250 -2.046 0.001 -99.990 -99.990
NGC 4104_12 0.068 0.90 0.94 0.88 0.270 0.270 0.243 1.041 0.303 0.301 0.303 1.079 0.303 0.602 0.091 -99.990 -99.990 -99.990 -99.990
NGC 4104_2 0.008 1.11 1.11 1.08 0.135 0.135 0.128 1.114 0.495 1.114 0.495 -0.523 0.010 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990
W3_FG39_BCG 0.068 0.56 0.96 0.42 0.318 0.349 -0.041 0.602 0.909 -1.000 0.091 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990
MCG_Main 0.173 0.49 0.59 0.44 -0.317 -0.317 -0.327 0.301 0.660 0.699 0.330 1.041 0.010 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990
MCG_12 0.392 0.070 0.281 -0.018 0.156 0.156 0.113 -0.046 0.455 0.176 0.455 -0.097 0.091 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990
MCG_111112 0.000 0.35 0.72 0.22 -0.151 -0.059 -0.327 0.301 0.455 0.176 0.455 -0.046 0.045 1.114 0.045 -99.990 -99.990 -99.990 -99.990
MCG_1111111 0.219 1.01 1.05 1.01 -0.201 -0.201 -0.327 1.114 0.682 0.602 0.227 0.778 0.091 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990
NGC 4065_Main 0.113 0.32 0.58 0.32 0.047 0.210 0.047 0.301 0.909 0.477 0.091 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990
NGC 4065_112 0.121 0.42 0.46 0.38 0.089 0.111 0.076 0.477 0.364 0.477 0.364 -0.301 0.182 0.602 0.030 0.845 0.030 -0.097 0.030
NGC 4065_1112 0.045 0.99 1.03 0.99 0.272 0.276 0.263 1.041 0.792 0.699 0.198 -0.097 0.010 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990
NGC 4104_Main 0.000 1.08 1.10 1.08 0.251 0.252 0.251 1.114 0.495 1.079 0.248 1.041 0.248 -0.097 0.010 -99.990 -99.990 -99.990 -99.990
NGC 4104_11 0.030 0.98 0.98 0.97 0.241 0.241 0.233 1.114 0.500 0.845 0.167 0.301 0.167 1.000 0.167 -99.990 -99.990 -99.990 -99.990
NGC 4104_err_11 0.030 1.05 1.05 1.04 0.215 0.232 0.215 1.114 0.660 0.903 0.330 -0.097 0.010 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990
NGC 4104_12 0.075 0.97 0.97 0.95 0.347 0.349 0.347 0.778 0.495 1.114 0.495 -0.222 0.010 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990
NGC 4104_2 0.008 1.07 1.08 1.00 0.156 0.254 0.130 1.041 0.455 1.114 0.455 0.954 0.091 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990
W3_FG39_BCG 0.151 0.35 0.74 0.18 -0.133 0.047 -0.327 0.477 0.500 0.176 0.500 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990 -99.990

Notes. The first eight columns are: Galaxy name, E(B-V), age (time elapsed aBB before the mean burst), maximum age, minimum age, metallicity, maximum metallicity, minimum metallicity. Ages are in units of log(age/Gyr) and metallicities are expressed as log(Z/H), with values of -99.990 for bursts that are not needed in the fit. The next columns show the ages and weights (w) for the six single bursts. The top and bottom tables correspond to the results obtained with the MILES and STELIB libraries, respectively.

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