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Table 2.
Weighted median values of SFR, M*, and λsBHAR for obscured and unobscured AGN.
| NH = 1023 cm−2 |
NH = 1022 cm−2 | |||
|---|---|---|---|---|
| Unobscured | Obscured | Unobscured | Obscured | |
| Number of AGN | 1115 | 34 | 965 | 130 |
| log SFR | 0.82 | 0.57 | 0.93 | 0.67 |
| p-value (SFR) | 0.10 | 0.26 | ||
| log M* | 10.86 | 10.95 | 10.85 | 10.97 |
| p-value (M*) | 0.02 | 0.007 | ||
| log λsBHAR | −1.60 | −1.71 | −1.52 | −1.73 |
| p-value (λsBHAR) | 0.00006 | 0.0003 | ||
Notes. We used different NH thresholds for the source classification. The number of sources and the p-values yielded by applying KS tests are also presented.
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