Table 2: Synthesis results.
LINERs PL (%) I (%) II (%) III (%) IV (%) V (%) log age (yr) Metallicity $(Z_\odot)$
NGC 315 7 2 <1 <1 <1 92 9.79 1.29
NGC 1052 <1 <1 <1 <1 11 89 10.03 1.53
NGC 2768 <1 <1 <1 <1 37 63 9.79 2.07
NGC 2832 <1 <1 <1 <1 <1 99 10.11 1.29
NGC 3193 9 <1 <1 <1 <1 91 9.72 1.12
NGC 3226 <1 <1 <1 <1 72 28 9.79 1.00
NGC 3379 <1 <1 <1 <1 <1 99 10.11 1.68
NGC 3608 2 <1 <1 <1 <1 98 10.05 1.23
NGC 4261 <1 <1 <1 <1 5 95 10.06 1.49
NGC 4278 <1 1 <1 <1 <1 99 10.07 1.75
NGC 4374 <1 <1 2 <1 90 8 9.18 2.46
NGC 4486 <1 2 1 <1 <1 96 9.99 0.86
NGC 4494 <1 <1 7 <1 11 83 9.80 1.25
NGC 4589 <1 <1 11 <1 1 88 9.76 2.50
NGC 4636 <1 <1 <1 <1 <1 99 10.04 1.00
NGC 5077 <1 4 <1 <1 <1 96 9.96 1.74
NGC 5322 <1 <1 12 <1 <1 88 9.75 2.50
NGC 5813 <1 <1 <1 <1 <1 99 10.11 1.36
NGC 5982 1 <1 <1 <1 <1 98 9.98 0.99
NGC 7626 <1 <1 <1 <1 <1 99 10.11 1.25
average 1.0 0.4 1.7 <1 11 86 9.91 1.52
rms 2.5 1.0 3.6 <1 25 24 0.22 0.51
Inactive Es   I (%) II (%) III (%) IV (%) V (%) log age (yr) Metallicity $(Z_\odot)$
NGC 221   1 <1 4 94 <1 9.33 1.88
NGC 821   <1 <1 <1 <1 99 10.10 1.18
NGC 2634   1 <1 <1 1 98 10.07 1.28
NGC 3348   <1 4 <1 <1 96 10.01 2.50
NGC 3377   <1 8 <1 11 82 9.34 2.49
NGC 3610   <1 7 <1 56 37 9.36 2.40
NGC 3613   <1 3 <1 24 73 9.80 1.57
NGC 3640   <1 <1 <1 30 70 9.82 1.45
NGC 4291   4 2 <1 29 65 9.70 2.42
NGC 4339   <1 3 <1 1 95 9.96 1.59
NGC 4365   <1 12 <1 <1 88 9.75 1.28
NGC 4406   2 <1 <1 <1 98 10.04 0.94
NGC 4473   <1 <1 <1 29 71 9.85 1.49
NGC 4478   <1 <1 <1 99 <1 9.66 0.90
NGC 4564   3 <1 <1 <1 97 10.00 1.10
NGC 4621   2 <1 <1 <1 98 10.03 1.18
NGC 4648   <1 <1 <1 <1 99 10.11 1.23
NGC 4649   <1 <1 <1 3 96 10.03 0.95
NGC 4660   <1 5 <1 15 80 9.76 1.23
NGC 4914   <1 8 <5 87 <1 9.45 2.43
NGC 5557   <1 <1 <1 1 99 10.08 1.06
NGC 5576   2 6 <1 25 66 9.62 1.52
NGC 5638   <1 <1 <1 <1 99 10.11 1.16
NGC 5831   <1 <1 <1 <1 99 10.11 1.22
NGC 7619   <1 <1 <1 <1 99 10.11 1.24
average   0.6 2.3 0.4 20 76 9.85 1.51
rms   1.1 3.4 1.3 31 32 0.26 0.53
Columns (2)-(7) list the fractional contribution to the total flux by the PL and by stellar populations I, II, III, IV, and V, respectively. Contributions less than 1% are listed as upper limits. Column (8) gives the mean stellar age, and Col. (9) gives the mean metallicity. The last two rows show the average value and rms of each column.

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