Table 1.
List of sources in our sample and their relevant parameters.
| ID | Survey ID | Redshift | MBH | R | Notes |
|---|---|---|---|---|---|
| J0324+3410 | 1H 0323+342 | 0.062900 1 | 2 – 3.4 × 107 A,O,P | 318 N | Fermi detected5 |
| J0849+5108 | SBS 0846+513 | 0.584701 2 | 0.8 – 9.8 × 107 B,C,D | 1445 G | Fermi detected6 |
| J0948+0022 | PMN J0948+0022 | 0.585102 2 | 0.2 – 8.1 × 108 E,F,10 | 355 G,10 | Fermi detected7 |
| J1305+5116 | WISE J130522.75+511640.3 | 0.787552 2 | 3.2 × 108 G | 223 G | Optical spec. indicates strong outflow11 |
| J1505+0326 | PKS 1502+036 | 0.407882 2 | 0.04 – 2 × 108 G,H,5,I,11 | 1549 G | Fermi detected5 |
| J1548+3511 | HB89 1546+353 | 0.479014 2 | 7.9 × 107 G | 692 G | Evidence for past radio variability |
| J1628+4007 | RXJ16290+4007 | 0.272486 2 | 3.5 × 107 K,10 | 29 M,10 | High optical and radio variability10 |
| J1633+4718 | RXJ1633.3+4718 | 0.116030 4 | 3 × 106 J | 166G | Evidence for past radio variability |
| J1644+2619 | FBQS J1644+2619 | 0.145000 3 | 2.1 × 108 L | 447 M | Fermi detected8 |
| J1722+5654 | SDSS J172206.02+565451.6 | 0.425967 2 | 2.5 – 3.3 × 107 G,9 | 234 G,9 | Evidence for high-amplitude optical variability9 |
Notes. Columns: (1) Source identifier, (2) survey identifier, (3) redshift, (4) black hole mass, (5) radio loudness. (1) Zhou et al. (2007); (2) Hewett & Wild (2010); (3) Foschini et al. (2015); (4) Oh et al. (2015); (5) Abdo et al. (2009b); (6) D’Ammando et al. (2012); (7) Abdo et al. (2009a); (8) D’Ammando et al. (2015); (9) Komossa et al. (2006a); (10) Komossa et al. (2006b); (11) Komossa et al. (2016); (A) Landt et al. (2017); (B) Zhou et al. (2005); (C) Shen et al. (2011); (D) Paliya et al. (2016); (E) Zhou et al. (2003); (F) Abdo et al. (2009a); (G) Yuan et al. (2008); (H) Paliya & Stalin (2016); (I) Calderone et al. (2013); (J) Yuan et al. (2010); (K) Foschini et al. (2015); (L) D’Ammando et al. (2017); (M) Doi et al. (2016); (N) Foschini (2011); (O) Wang et al. (2016); (P) Kynoch et al. (2018).
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