Table 4
Compilation of frequency breaks reported here and in the literature.
| Breaks reported in this study | ||||||||||
|
|
||||||||||
| Name | Ref. | Type | Satellite | Band | log(MBH) | L bol | FWHM(Hβ) | α | log(νbr) | νbr × P(νbr) |
| (km s-1) | (× 10-3) | |||||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
|
|
||||||||||
| Mrk 335 | 1 | NLSY1 | XMM | 0.2–10 | 7.34(1) | 44.69(1) | 1629 | 3.73 |
–3.76 |
2.2 ± 0.3 |
| ESO113-G10 | 1 | S1 | XMM | 0.2–10 | 44.17(7) | 2.98 |
–3.73 |
2.9 ± 0.5 | ||
| PKS0558-504 | 1 | NLSY1 | XMM | 0.2–10 | 8.48(12) | 46.74(6) | 1250* | 2.52 |
–4.60 |
16.6 ± 3.1 |
| 1H0707-495 | 1 | NLSY1 | XMM | 0.2–10 | 6.37(2) | 44.43(2) | 935 | 2.50 |
–3.82 |
24.2 ± 1.4 |
| ESO434-G40 | 1 | S1 | XMM | 0.2–10 | 6.30(3) | 44.30(3) | 2490* | 3.52 |
–4.06 |
1.0 ± 0.2 |
| NGC 3227 | 1 | S1 | XMM | 0.2–10 | 6.88(4) | 43.86(1) | 4920 | 3.44 |
–3.64 |
2.2 ± 0.3 |
| KUG1031+398 | 1 | NLSY1 | XMM | 0.2–10 | 6.60(5) | 44.82(4) | 1500 | 3.26 |
–3.44 |
1.1 ± 0.1 |
| NGC 4051 | 1 | NLSY1 | XMM | 0.2–10 | 6.13(4) | 43.56(1) | 1120 | 2.63 |
–3.52 |
25.3 ± 1.9 |
| Mrk 766 | 1 | NLSY1 | XMM | 0.2–10 | 6.57(6) | 44.08(5) | 1630 | 2.79 |
–3.70 |
7.3 ± 0.5 |
| NGC 4395 | 1 | S1 | XMM | 0.2–10 | 5.55(7) | 41.37(5) | 1500 | 2.13 |
–2.66 |
37.9 ± 1.7 |
| MCG-06-30-015 | 1 | NLSY1 | XMM | 0.2–10 | 6.71(8) | 43.85(5) | 1700 | 2.83 |
–3.75 |
6.9 ± 0.6 |
| Circinus | 1 | S2 | XMM | 0.2–10 | 6.23(14) | 43.60(8) | 1925 | 3.23 |
–3.39 |
3.3 ± 0.4 |
| NGC 5506 | 1 | NLSY1 | XMM | 0.2–10 | 7.45(9) | 44.00(5) | 1800* | 3.60 |
–3.78 |
1.9 ± 1.0 |
| NGC 6860 | 1 | S1 | XMM | 0.2–10 | 7.59(13) | 44.53(7) | 3900 | 4.56 |
–4.03 |
1.0 ± 0.2 |
| Ark564 | 1 | NLSY1 | XMM | 0.2–10 | 6.90(9) | 44.90(5) | 865 | 2.51 |
–3.46 |
6.3 ± 1.0 |
| Name | Ref. | Type | Satellite | Band | log(MBH) | Lbol | FWHM(Hβ) | α | log(νbr) | |
| (km s-1) | ||||||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | |
|
|
||||||||||
| Mrk 335 | 2 | NLSY1 | XMM | 0.2–10 | 7.34(1) | 44.69(1) | 1629 | 3.80 |
–3.77 |
|
| NGC 3227 | 3 | S1 | RXTE | 2–10 | 6.88(4) | 43.86(1) | 4920 | >1.90 | –4.59 |
|
| KUG 1031+398 | 4 | NLSY1 | XMM | 0.2–10 | 6.60(5) | 44.82(4) | 1500 | 3.40 |
–3.37 |
|
| NGC 3516 | 5 | S1 | RXTE | 2–10 | 7.50(4) | 44.29(1) | 3350 | 2.00 |
–5.70 |
|
| NGC 3783 | 5,6,7 | S1 | RXTE | 2–10 | 7.47(10) | 44.41(1) | 3570 | 1.90 |
–5.20 |
|
| NGC 4051 | 8,9,10 | NLSY1 | RXTE/XMM | 2–10 | 6.23(4) | 43.56(1) | 1120 | 2.03 |
–3.08 |
|
| NGC 4151 | 5 | S1 | RXTE | 2–10 | 7.12(10) | 43.73(1) | 5000 | 2.10 |
–5.90 |
|
| Mrk 766 | 11,12 | NLSY1 | XMM | 0.2–10 | 6.57(6) | 44.08(5) | 1630 | 2.80 |
–3.30 |
|
| 11,12 | XMM | 0.2–0.7 | 2.60 |
–3.52 |
||||||
| 11,12 | XMM | 0.7–2 | 2.70 |
–3.30 |
||||||
| 11,12 | XMM | 2–10 | 2.30 |
–3.30 |
||||||
| NGC 4395 | 13 | S1 | ASCA | 1.2–10 | 4.70(7) | 41.37(5) | 1500 | 1.78 |
–3.49 |
|
| 14 | S1 | XMM | 2–10 | 2.24 |
–2.90 |
|||||
| Fairall 9 | 5 | S1 | RXTE | 2–10 | 8.41(10) | 45.23(1) | 6270 | 2.20 |
–6.39 |
|
| MCG-06-30-015 | 15 | NLSY1 | XMM | 0.2–10 | 6.71(8) | 43.85(5) | 1700 | 2.50 |
–3.00 |
|
| 15 | XMM | 0.2–0.7 | 2.55 |
–2.89 |
||||||
| 15 | XMM | 0.7–2 | 2.30 |
–3.10 |
||||||
| 15 | XMM | 2–10 | 2.10 |
–3.00 |
||||||
| 16 | RXTE | 2–10 | 2.00 |
–4.29 |
||||||
| IC 4329A | 17 | S1 | RXTE/XMM | 3–10 | 8.34(11) | 45.52(2) | 5960 | 2.30 |
–5.60 |
|
| NGC 5506 | 3 | NLSY1 | RXTE | 2–10 | 7.45(9) | 44.00(5) | 1800* | >1.80 | –4.85 |
|
| NGC 5548 | 5 | S1 | RXTE | 2–10 | 7.64(4) | 44.83(1) | 5800 | 2.05 |
–6.22 |
|
| Ark 564 | 5,18 | NLSY1 | RXTE | 2–10 | 6.90(9) | 44.90(5) | 865 | 1.20 |
–5.80 |
|
| 19 | ASCA | 0.7–5 | 1.90 |
–2.64 |
||||||
| 19 | ASCA | 0.7–2 | 1.98 |
–2.58 |
||||||
| 19 | ASCA | 2–5 | 1.87 |
–2.77 |
||||||
| PKS 0558-504 | 20 | NLSY1 | XMM/RXTE | 2–10 | 8.48(12) | 46.74(6) | 1250* | 2.21 |
–5.17 |
|
| NGC 7469 | 21 | S1 | XMM/RXTE | 2–10 | 7.39(10) | 44.56(1) | 2650 | 1.80 |
–6.00 |
|
Notes. We refer to “S1” to all the AGN with detected broad emission lines. FWHM of Paβ is given (instead of Hβ) for sources marked with asterisks.
References. The references for the PSD fits are: 1) this work; 2) Arévalo et al. (2008); 3) Uttley & McHardy (2005); 4) Vaughan (2010); 5) Markowitz et al. (2003); 6) Arévalo et al. (2009); 7) Summons et al. (2007); 8) McHardy et al. (2004); 9) Papadakis (2004); 10) Vaughan et al. (2011); 11) Vaughan & Fabian (2003); 12) Markowitz et al. (2007); 13) Shih et al. (2003); 14) Vaughan et al. (2005); 15) Vaughan et al. (2003b); 16) McHardy et al. (2005); 17) Markowitz (2009); 18) Papadakis et al. (2002); 19) McHardy et al. (2007); 20) Papadakis et al. (2010); and 21) Markowitz (2010). The references for the bolometric luminosity are: 1) Woo & Urry (2002); 2) Zhou & Wang (2005); 3) Beckmann et al. (2003); 4) Hao et al. (2005); 5) Meyer-Hofmeister & Meyer (2011); 6) Gliozzi et al. (2010); 7) Ponti et al. (2012); and 8) Greenhill et al. (2003). The reserences for the black hole masses are: 1) Grier et al. (2012); 2) Zhou & Wang (2005); 3) Beckmann et al. (2008); 4) Denney et al. (2009); 5) Zhou & Zhao (2010); 6) Botte et al. (2005); 7) Vaughan et al. (2005); 8) McHardy et al. (2005); 9) Sobolewska & Papadakis (2009); 10) Peterson et al. (2004); 11) Markowitz (2009); 12) Gliozzi et al. (2010); 13) Ponti et al. (2012); and 14) Greenhill et al. (2003).
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