Table 3.
Results from the investigation of possible dependencies of the SF on MBH (top section), λE (middle section), and Lbol (bottom section) for our four samples of AGN (listed in the top row) selected via different properties and used for this part of the analysis.
| Main sample | MIR | Opt. var. | Spec. Type I | |
|---|---|---|---|---|
| MBH dependence | ||||
| log(MBH) range (MBH[M⊙]) | 4.95 to 9.65 | 6.68 to 9.47 | 4.95 to 9.65 | 7.02 to 9.65 |
| 1st quartile | 7.73 | 7.89 | 7.89 | 8.07 |
Median ( ) |
8.19 | 8.38 | 8.35 | 8.44 |
| 3rd quartile | 8.54 | 8.70 | 8.69 | 8.72 |
 slope |
0.34 ± 0.01 | 0.31 ± 0.01 | 0.32 ± 0.01 | 0.31 ± 0.01 |
| z̃ of this subset | 0.801 | 1.061 | 1.122 | 1.298 |
 slope |
0.33 ± 0.01 | 0.29 ± 0.01 | 0.34 ± 0.01 | 0.34 ± 0.01 |
| z̃ of this subset | 1.450 | 1.560 | 1.531 | 1.597 |
| λE dependence | ||||
| λE range | −2.85 to 0.09 | −2.21 to −0.09 | −2.40 to −0.14 | −2.40 to −0.14 |
| 1st quartile | −1.55 | −1.18 | −1.35 | −1.32 |
Median ( ) |
−1.17 | −0.93 | −1.05 | −1.05 |
| 3rd quartile | −0.85 | −0.70 | −0.81 | −0.79 |
 slope |
0.30 ± 0.02 | 0.38 ± 0.01 | 0.32 ± 0.02 | 0.34 ± 0.02 |
| z̃ of this subset | 0.938 | 1.195 | 1.306 | 1.345 |
 slope |
0.32 ± 0.02 | 0.22 ± 0.01 | 0.34 ± 0.01 | 0.34 ± 0.01 |
| z̃ of this subset | 1.258 | 1.531 | 1.444 | 1.550 |
| Lbol dependence | ||||
 range Lbol in erg s−1 |
40.276 to 46.676 | 45.299 to 46.676 | 42.865 to 46.676 | 44.023 to 46.676 |
| 1st quartile | 44.634 | 45.149 | 44.995 | 45.149 |
Median ( ) |
45.096 | 45.488 | 45.328 | 45.413 |
| 3rd quartile | 45.513 | 45.815 | 45.665 | 45.76s |
 slope |
0.31 ± 0.01 | 0.40 ± 0.01 | 0.41 ± 0.01 | 0.31 ± 0.01 |
| z̃ of this subset | 0.762 | 0.970 | 1.033 | 1.279 |
 slope |
0.32 ± 0.01 | 0.25 ± 0.01 | 0.31 ± 0.01 | 0.29 ± 0.01 |
| z̃ of this subset | 1.527 | 1.729 | 1.646 | 1.681 |
Notes. For each physical quantity we report the (logarithm of the) corresponding range boundaries, as well as the 1st quartile, median, and 3rd quartile values. Each sample is divided in two subsets on the basis of the (logarithm of the) median value of the physical property of interest in that sample. Each section reports, for each subset, the median redshift value and the estimated slope value for the best-fit line approximating the corresponding set of points in the linear region of the SF, with its error. We show the linear plots for each of the investigated samples of sources in Fig. 9, comparing results for each of the performed tests.
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