Table 3
Parameters of the luminosity functions.
| Sample | Mod. | log L1 | log L2 | log Lb | log Φb | log K | α | β |
|
|
||||||||
| F-NLS1 | PL | 40.25 | 42.75 | − | − | −1.91 ± 5.90 | −1.17 ± 0.14 ± 0.48 | − |
| F-NLS1* | PL | 40.25 | 42.75 | − | − | −1.60 ± 5.90 | −1.18 ± 0.14 ± 0.48 | − |
| HERG | PL | 39.75 | 42.25 | − | − | 20.96 ± 5.68 | −1.71 ± 0.14 ± 0.41 | − |
| FSRQ | BPL | 42.25 | 43.75 | 43.32 ± 0.47 | −53.10 ± 1.34 | − | 1.61 ± 0.98 | 4.33 ± 2.00 |
Notes. The LF of F-NLS1s is showed in two different ways: with or without 1 source with unknown spectral index. The former is indicated with an asterisk. Columns: (1) sample; (2) function used for the best-fit. PL for power law, BPL for broken power law; (3) logarithm of minimum luminosity bin (erg s-1); (4) logarithm of maximum luminosity bin (erg s-1); (5) logarithm of luminosity break (erg s-1); (6) logarithm of the luminosity function at the break (Mpc-3); (7) coefficient of the power law; (8) slope of the power law (slope below the break for broken power law). The second error is that evaluated via Monte Carlo method; (9) slope above the break (for broken power law only).
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