Table 2
Properties of the AGNs in our sample used in the paper.
Objecta | Apertureb | Fgal c | Referenced | FWHMe | RBLRf | Fmax/Fming | Referenceh | JD(div)i | Fcnt(div)j |
blue/red | Hβ/Hα | Hβ/Hα | Hβ/Hα | 2 400 000+ | |||||
|
|||||||||
NGC 4151 | 2.0′′ × 6.0′′ | 6.00 | 1 | 6110/4650 | 5/6 | 4.8/3.1 | 1 | 51 283 | 46.2 |
NGC 5548 | 5.0′′ × 7.5′′ | 3.06 | 2,3 | 6300 | 49/27 | 4.9/3.5 | 8 | 51 702 | 4.41 |
3C 390.3 | 2.0′′ × 6.0′′ | 0.46 | 4 | 11 900/11 000 | 96/120 | 4.7/3.4 | 9 | 52 327 | 0.74 |
Arp 102B | 2.5′′ × 6.0′′ | 1.13/1.21 | 5 | 15 900/14 300 | 15/21 | 3.0/2.4 | 5 | 55 367 | 0.38 |
Ark 564 | 2.5′′ × 6.0′′ | 2.40 / 0.99 | 6 | 960/800 | 4/5 | 1.6/1.5 | 10 | 53 505 | 2.55 |
E1821+643 | 2.0′′ × 6.0′′ | 0.29 | 7 | 5610 | 120 | 1.4 | 7 | 53 683 | 10.35 |
Notes.Columns:
modified Julian date dividing period 1 and 2 of different levels of activity and the corresponding continuum flux at 5100 Å in units of 10-15 erg cm-2 s-1 Å -1.
Reference. (1) Shapovalova et al. (2008); (2,3) Peterson et al. (1995, 2002); (4) Sergeev et al. (2002); (5) Shapovalova et al. (2013); (6) Shemmer et al. (2001); (7) Shapovalova et al. (2016); (8) Shapovalova et al. (2004); (9) Shapovalova et al. (2010b); (10) Shapovalova et al. (2012).
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