Table 4
Detailed comparison between AGNs and non-AGNs by separately considering PACS detected and undetected sources.
| GOODS | COSMOS | |||||
| z | (1) | (2) | (3) | (1) | (2) | (3) |
|
|
||||||
| Total sample | ||||||
|
|
||||||
| 0.5–0.8 | 77% | 0.28 ± 0.04 | 3.87 ± 1.00 | 64% | 0.43 ± 0.06 | 2.27 ± 1.00 |
| 0.8–1.5 | 1% | 0.38 ± 0.06 | 2.02 ± 0.99 | 18% | 0.22 ± 0.06 | 3.28 ± 1.02 |
| 1.5–2.5 | 82% | −0.13 ± 0.04 | 1.76 ± 1.00 | 36% | 0.28 ± 0.04 | 10.17 ± 1.30 |
|
|
||||||
| Low-LX subsample | ||||||
|
|
||||||
| 0.5–0.8 | 76% | 0.22 ± 0.04 | 7.26 ± 1.29 | 99% | 0.23 ± 0.05 | 1.90 ± 1.03 |
| 0.8–1.5 | 1% | 0.39 ± 0.05 | 1.71 ± 0.98 | 83% | 0.17 ± 0.08 | 3.78 ± 1.06 |
| 1.5–2.5 | 59% | −0.14 ± 0.05 | 1.44 ± 1.39 | 31% | −0.08 ± 0.08 | 4.38 ± 1.41 |
Notes. Columns: (1) probability, according to a Kolmogorov Smirnov test, that the log (νLν(60 μm)) distributions of PACS detected AGNs and non-AGNs are consistent with describing the same population; (2) average offset between the stacked log (νLν(60 μm)) for PACS undetected AGNs and non-AGN; (3) ratio of PACS detection rates of AGNs and non-AGNs. The upper table refers to the low luminosity subsample (upper panel of Fig. 6), whereas the lower table represents the total sample (lower panel of Fig. 6).
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