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Table 4.
Median values and their 25th and 75th percentiles for the SFR, M*, sSFR, Dn4000, Hδ, and λsBHAR of the different AGN populations examined in our study.
| AGN population | log [SFR (M⊙ yr−1)] | log [M*(M⊙)] | log sSFR (Gyr−1) | Dn4000 | Hδ | log λsBHAR |
|---|---|---|---|---|---|---|
| Sy2 | –0.49 [–0.92, –0.03] | 10.64 [10.41, 10.84] | –2.15 [–2.52, –1.75] | 1.51 [1.39, 1.66] | 0.35 [–1.15, 1.71] | –2.57 [–3.08, –2.26] |
| Composite | –0.54 [–0.85, –0.08] | 10.62 [10.42, 10.90] | –2.13 [–2.58, –1.92] | 1.62 [1.50, 1.73] | 0.50 [–0.77, 1.15] | –3.21 [–3.61, –2.78] |
| LINERS | –0.87 [–1.32, –0.36] | 10.81 [10.56, 11.02] | –2.59 [–3.07, –2.15] | 1.71 [1.53, 1.84] | –0.35 [–1.65, 1.45] | –3.28 [–3.69, –2.80] |
| CT | 0.25 [–0.41, 0.76] | 10.66 [10.49, 10.83] | –1.39 [–2.04, –1.08] | 1.32 [1.18, 1.43] | 1.69 [–0.44, 2.76] | –1.82 [–2.10, –1.60] |
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