Table 5.
Summary of stellar populations by galaxy class with uncertainties from jack-knifing as described in the text.
| class | xy | xyi | xio | xo | μy | μyi | μio | μo | |
|---|---|---|---|---|---|---|---|---|---|
| [%] | [%] | [%] | [%] | [%] | [%] | [%] | [%] | ||
| AGN | 4.53 ± 1.24 | 0.64 ± 0.64 | 21.32 ± 6.37 | 73.49 ± 6.62 | 0.07 ± 0.02 | 0.04 ± 0.04 | 6.91 ± 2.61 | 93.00 ± 2.62 | |
| SF | 4.18 ± 1.43 | 6.52 ± 4.57 | 30.98 ± 8.56 | 58.32 ± 14.03 | 0.08 ± 0.05 | 2.62 ± 2.21 | 20.67 ± 13.33 | 76.65 ± 15.58 | |
| non-SF | 0.53 ± 0.34 | 0.86 ± 0.85 | 15.00 ± 4.29 | 83.61 ± 4.70 | 0.00 ± 0.00 | 0.13 ± 0.12 | 5.17 ± 1.71 | 94.71 ± 1.79 |
Notes. Quoted are the fractional contributions to the light (mass) in percent in the four designated bins: young xy (μy), young-intermediate xyi (μyi), intermediate-old xio (μio), and old xo (μo). They are defined by their boundaries of log (age/yr) = 7.5, 8.5, and 9.5.
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