Table 3
Average FIR emission offsets between AGNs and non-AGNs over all mass bins.
| Average offsets | ||||||
| GOODS | COSMOS | |||||
|
|
||||||
| z | Total sample | Low-LX | High-LX | Total sample | Low-LX | High-LX |
|
|
||||||
| 0.5–0.8 | 0.41 ± 0.04 | 0.29 ± 0.06 | ... | 0.44 ± 0.06 | 0.21 ± 0.05 | 0.81 ± 0.07 |
| 0.8–1.5 | 0.60 ± 0.06 | 0.56 ± 0.06 | ... | 0.44 ± 0.10 | 0.50 ± 0.09 | 0.45 ± 0.04 |
| 1.5–2.5 | −0.06 ± 0.05 | −0.01 ± 0.06 | ... | 0.37 ± 0.04 | 0.02 ± 0.07 | 0.42 ± 0.04 |
| 0.5–2.5 | 0.32 ± 0.03 | 0.28 ± 0.10 | ... | 0.42 ± 0.04 | 0.24 ± 0.04 | 0.56 ± 0.03 |
Notes. The different rows correspond to different redshift bins, while the columns correspond to the entire sample, the low- and the high-LX luminosity ones. Average logarithmic offsets were computed as linear averages of the differences between the logarithmic FIR luminosities. Uncertainties were computed by summing in quadrature the logarithmic error bars on νLν(60 μm). Upper limits were not considered in the average computation. Bins with less than three sources were discarded.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.