Table 4.
Number of sources, the corresponding values of SFR, M*, and λsBHAR and p-values for X-ray absorbed and unabsorbed sources, in the three redshift intervals used in our analysis.
| 0.5 < z < 1.0 |
1.0 < z < 2.0 |
2.0 < z < 3.5 |
||||
|---|---|---|---|---|---|---|
| log [NH(cm−2)] | < 1023 | > 1023 | < 1023 | > 1023 | < 1023 | > 1023 |
| Number of sources | 1631 | 17 | 1130 | 80 | 406 | 48 |
| log SFR | 1.65 | 0.07 | 2.20 | 1.33 | 2.44 | 1,89 |
| p value (SFR) | 0.03 | 0.03 | 0.31 | |||
| log M* | 10.89 | 10.96 | 11.05 | 11.11 | 11.27 | 11.33 |
| p value (M*) | 0.90 | 0.90 | 0.31 | |||
| log λsBHAR | −1.27 | −1.48 | −0.89 | −0.98 | −0.76 | −0.88 |
| p value (λsBHAR) | 0.22 | 0.87 | 0.23 | |||
Notes. Weighted median values of SFR, M*, and λsBHAR are presented. Sources are classified using a threshold of log [NH(cm−2)] = 23. p-values are yielded by applying KS test.
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