Table E.1.
Sources plotted in Fig. 9.
Group | Name | λEdd | v (c) | Refs. |
---|---|---|---|---|
NGC4151 | 0.05 ± 0.01 | 0.106 ± 0.007 | A | |
IC4329A | 0.08 ± 0.03 | 0.098 ± 0.004 | ||
Mrk509 | 0.09 ± 0.01 | 0.173 ± 0.004 | A | |
Mrk509 | 0.14 ± 0.01 | 0.138 ± 0.004 | A | |
ARK120 | 0.17 ± 0.02 | 0.29 ± 0.02 | A | |
Mrk79 | 0.08 ± 0.01 | 0.092 ± 0.004 | B | |
NGC4051 | 0.07 ± 0.01 | 0.04 ± 0.02 | B | |
Mrk766 | 0.19 ± 0.02 | 0.082 ± 0.006 | C | |
1 | Mrk766 | 0.30 ± 0.03 | 0.088 ± 0.002 | C |
Mrk841 | 0.02 ± 0.00 | 0.06 ± 0.02 | D | |
1H0419−577 | 0.24 ± 0.04 | 0.079 ± 0.007 | E | |
Mrk290 | 0.19 ± 0.02 | 0.16 ± 0.02 | B | |
Mrk205 | 0.16 ± 0.10 | 0.100 ± 0.004 | F | |
PG1211+143 | 0.17 ± 0.03 | 0.151 ± 0.003 | D | |
MCG-5-23-16 | 0.09 ± 0.02 | 0.116 ± 0.004 | G | |
NGC4507 | 0.79 ± 0.54 | 0.20 ± 0.02 | ||
3C111 | 0.02 ± 0.01 | 0.07 ± 0.04 | H | |
3C3903 | 0.09 ± 0.02 | 0.145 ± 0.007 | A | |
4C+74.26 | 0.04 ± 0.00 | 0.18 ± 0.03 | ||
2 | ESO103-G035 | 0.13 ± 0.03 | 0.06 ± 0.03 | |
MR2251−178 | 0.16 ± 0.03 | 0.137 ± 0.008 | ||
Mrk279 | 0.03 ± 0.00 | 0.220 ± 0.006 | B | |
NGC5506 | 0.28 ± 0.05 | 0.246 ± 0.006 | I | |
SQJ2127 | 0.16 ± 0.00 | 0.231 ± 0.006 | ||
Mrk231 | 0.17 ± 0.03 | 0.067 ± 0.008 | L,M | |
PDS456 | 0.46 ± 0.15 | 0.25 ± 0.01 | N | |
Iras 11119 | 0.65 ± 0.19 | 0.26 ± 0.01 | L,O | |
3 | IZwicky1 | 0.85 ± 0.17 | 0.27 ± 0.01 | P |
Iras 05189 | 1.30 ± 0.27 | 0.110 ± 0.010 | Q,R | |
PG1448 | 0.76 ± 0.077 | 0.150 ± 0.008 | S | |
APM08279 | 0.40 ± 0.30 | 0.36 ± 0.02 | T,U | |
MCG-03-58-007 | 0.20 ± 0.07 | 0.20 ± 0.01 | V |
Notes. From left to right, columns indicate the number of the group, the source name, λEdd, the UFO velocity vout (in units of c) and the additional references for each source. Group 1: UFO vout and black hole mass M from Tombesi et al. (2012), Lbol from Fiore et al. (2017). Group 2: values from Gofford et al. (2015). For both groups, M, Lbol have been updated (where possible) with recent values from the literature, see reference column. Group 3: individual sources, see reference column.
References. A: Peterson et al. (2004), B: Ricci et al. (2017a), C: Bentz & Manne-Nicholas (2018), D: Vestergaard & Peterson (2006), E: Tilton & Shull (2013), F: Kelly & Bechtold (2007), G: Caglar et al. (2020), H: Chatterjee et al. (2011), I: Ricci et al. (2017b), L: Nardini & Zubovas (2018), M: Feruglio et al. (2015), N: Nardini et al. (2015), Bischetti et al. (2019), O: Tombesi et al. (2015), P: Reeves & Braito (2019), Q: Smith et al. (2019), R: Onori et al. (2017), S: Laurenti et al. (2021), T: Chartas et al. (2009), U: Saturni et al. (2018), V: Braito et al. (2018).
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