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Table 1
Statistics of AGNs and inactive sample.
| GOODS-South + GOODS-North | ||||||
| AGN hosts | inactive galaxies | |||||
|
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| 109−1010 M⊙ | 1010−1011 M⊙ | 1011−1012 M⊙ | 109−1010 M⊙ | 1010−1011 M⊙ | 1011−1012 M⊙ | |
|
|
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| z = 0.5−0.8 | 9 (33.3%) | 34 (20.6%) | 14 (35.7%) | 49 (4.1%) | 228 (18.9%) | 59 (15.3%) |
| z = 0.8−1.5 | 19 (15.8%) | 70 (18.6%) | 49 (30.6%) | 114 (0.0%) | 458 (11.6%) | 230 (12.6%) |
| z = 1.5−2.5 | 5 (0.0%) | 59 (6.8%) | 36 (33.3%) | 34 (0.0%) | 377 (4.2%) | 168 (17.3%) |
|
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| COSMOS | ||||||
| AGN hosts | inactive galaxies | |||||
|
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| 109−1010 M⊙ | 1010−1011 M⊙ | 1011−1012 M⊙ | 109−1010 M⊙ | 1010−1011 M⊙ | 1011−1012 M⊙ | |
|
|
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| z = 0.5−0.8 | 19 (0.0%) | 75 (8.0%) | 89 (14.6%) | 114 (0.0%) | 474 (4.0%) | 507 (5.7%) |
| z = 0.8−1.5 | 15 (6.7%) | 249 (4.0%) | 245 (13.9%) | 117 (0.0%) | 1689 (1.2%) | 1071 (4.4%) |
| z = 1.5−2.5 | 3 (33.3%) | 170 (4.1%) | 187 (9.1%) | 24 (0.0%) | 1126 (0.3%) | 592 (1.9%) |
Notes. Number of AGNs and inactive galaxies in each redshift (rows) and mass (columns) bin in the different fields. Numbers in brackets show the fraction of sources fully detected by PACS (i.e. detected in the two bands used to infer νLν(60 μm) as explained in Sect. 3.2).
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