Table 1.
Physical properties of AGNs with dust continuum size measurements.
| Name | Redshift | Rd (RM) | Ref. | Rd (OI) | Ref. | RBLR | FWHM | log λLλ(5100 Å) | Ref. | log MBH | log λEdd |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (ld) | (ld) | (ld) | (km s−1) | (erg s−1) | (M⊙) | ||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
| Mrk 335 | 0.0258 | 167.5 ± 6.0 | 1 | 185 ± 49 | 2 | 14.0 ± 4.0 | 1707 ± 79 | 43.8 | 3 | 6.90 ± 0.13 | −0.29 |
| UGC 545 | 0.0612 | ... | ... | 707 ± 77 | 4 | 37.2 ± 4.7 | 1131 ± 37 | 44.5 | 5 | 6.97 ± 0.06 | 0.39 |
| Mrk 590 (a)(b) | 0.0264 | 33.5 ± 4.2 | 1 | ... | ... | 25.6 ± 5.9 | 2716 ± 202 | 43.5 | 3 | 7.57 ± 0.12 | −1.21 |
| 3C 120 | 0.0330 | 94.4 ± 5.5 | 6 | 379 ± 85 | 2 | 26.2 ± 7.7 | 2472 ± 729 | 44.0 | 3 | 7.49 ± 0.29 | −0.64 |
| H0507+164 | 0.0179 | 35 ± 11 | 7 | ... | ... | 3.0 ± 1.2 | 4062 ± 247 | 42.6 | 8 | 6.99 ± 0.18 | −1.57 |
| Akn 120 | 0.0327 | 138 ± 18 | 1 | 387 ± 77 | 4 | 39.5 ± 8.2 | 6077 ± 147 | 43.9 | 3 | 8.45 ± 0.09 | −1.73 |
| MCG+08-11-011 | 0.0205 | 72.7 ± 1.6 | 1 | ... | ... | 15.7 ± 0.5 | 4139 ± 207 | 43.3 | 3 | 7.72 ± 0.05 | −1.54 |
| Mrk 6 (a) | 0.0195 | ... | ... | 214 ± 60 | 9 | 18.5 ± 2.5 | 5457 ± 16 | 43.6 | 10 | 8.03 ± 0.06 | −1.55 |
| Mrk 79 | 0.0222 | 67.7 ± 4.8 | 1 | ... | ... | 15.6 ± 5.0 | 4793 ± 145 | 43.7 | 3 | 7.84 ± 0.14 | −1.31 |
| PG 0844+349 | 0.0640 | 99 ± 11 | 1 | ... | ... | 32.3 ± 13.6 | 2694 ± 58 | 44.2 | 3 | 7.66 ± 0.18 | −0.59 |
| Mrk 110 | 0.0353 | 116.6 ± 6.3 | 1 | ... | ... | 25.6 ± 8.1 | 1634 ± 83 | 43.7 | 3 | 7.13 ± 0.14 | −0.61 |
| PG 0953+414 | 0.2341 | 566 ± 44 | 1 | ... | ... | 150.1 ± 22.1 | 3071 ± 27 | 45.2 | 3 | 8.44 ± 0.06 | −0.40 |
| NGC 3227 | 0.0038 | 14.37 ± 0.70 | 1 | 45.0 ± 7.2 | 4 | 3.8 ± 0.8 | 4112 ± 206 | 42.2 | 3 | 7.10 ± 0.10 | −2.00 |
| NGC 3516 (a) | 0.0088 | 72.7 ± 4.6 | 1 | ... | ... | 11.7 ± 1.3 | 5384 ± 269 | 42.8 | 3 | 7.82 ± 0.06 | −2.18 |
| NGC 3783 | 0.0097 | 76.3 ± 14.1 | 11 | 131 ± 20 | 2 | 9.6 ± 0.7 | 4486 ± 35 | 43.0 | 12 | 7.58 ± 0.03 | −1.70 |
| NGC 4051 | 0.0023 | 16.30 ± 0.57 | 1 | 38.1 ± 6.0 | 13 | 2.1 ± 0.8 | 1076 ± 277 | 41.9 | 3 | 5.68 ± 0.28 | −0.92 |
| NGC 4151 (a) | 0.0033 | 46.11 ± 0.44 | 1 | 44.1 ± 8.3 (c) | 9 | 6.6 ± 1.0 | 6371 ± 150 | 42.1 | 3 | 7.72 ± 0.07 | −2.77 |
| 3C 273 | 0.1583 | 409 ± 41 | 14 | 675 ± 126 | 2 | 146.8 ± 10.2 | 3314 ± 59 | 45.9 | 3 | 8.50 ± 0.03 | 0.28 |
| NGC 4593 | 0.0083 | 41.82 ± 0.90 | 1 | 54.8 ± 8.8 | 4 | 4.0 ± 0.8 | 5142 ± 572 | 42.6 | 3 | 7.31 ± 0.13 | −1.84 |
| MCG-6-30-15 | 0.0078 | 19.6 ± 4.9 | 15 | ... | ... | 5.7 ± 1.8 | 1947 ± 58 | 41.6 | 3 | 6.63 ± 0.14 | −2.13 |
| NGC 5548 | 0.0172 | 61.21 ± 0.30 | 1 | ... | ... | 13.9 ± 8.7 | 7256 ± 2203 | 43.3 | 3 | 8.15 ± 0.38 | −2.00 |
| Mrk 817 | 0.0313 | 92.6 ± 8.9 | 1 | ... | ... | 19.9 ± 8.3 | 5348 ± 536 | 43.7 | 3 | 8.05 ± 0.20 | −1.45 |
| PG 1613+658 | 0.1211 | 334 ± 40 | 1 | ... | ... | 40.1 ± 15.1 | 9074 ± 103 | 44.8 | 3 | 8.81 ± 0.16 | −1.19 |
| Z 229-15 | 0.0279 | 20.4 ± 5.8 | 16 | ... | ... | 3.9 ± 0.8 | 3350 ± 72 | 42.9 | 17 | 6.93 ± 0.09 | −1.18 |
| Mrk 509 | 0.0344 | 121.3 ± 1.6 | 1 | 297 ± 31 | 2 | 79.6 ± 5.8 | 3015 ± 2 | 44.2 | 3 | 8.15 ± 0.03 | −1.11 |
| NGC 7469 | 0.0163 | 85.29 ± 0.43 | 1 | ... | ... | 10.8 ± 2.4 | 4369 ± 6 | 43.5 | 3 | 7.60 ± 0.10 | −1.24 |
| NGC 1365 (a) | 0.0055 | ... | ... | 38.1 ± 4.8 | 2 | ... | 1586 ± 465 | 41.9 | 2 (f),18 | ... | ... |
| IRAS 03450+0055 | 0.0315 | 157.4 ± 5.9 | 1 | ... | ... | ... | 3098 ± 55 | 43.9 | 1,19 | ... | ... |
| IRAS 09149−6206 (d) | 0.0573 | ... | ... | 482 ± 49 | 2 | ... | 4281 ± 121 | 45.0 | 20,21 | 8.06 ± 0.25 | −0.26 |
| Mrk 1239 | 0.0199 | ... | ... | 189 ± 30 | 4 | ... | 830 ± 10 | 44.5 | 22 (f) | ... | ... |
| WPVS 48 | 0.0370 | 70.8 ± 4.6 | 23 | ... | ... | ... | 1890 ± 60 | 43.6 | 24 | ... | ... |
| Mrk 744 | 0.0091 | 19.9 ± 2.2 | 1 | ... | ... | ... | 5616 ± 129 | 41.8 | 1,21 (g) | ... | ... |
| HE 1029−1401 | 0.0858 | ... | ... | 880 ± 133 | 4 | ... | 5684 ± 284 | 44.6 | 21 | ... | ... |
| GQ Com | 0.1650 | 210 ± 40 | 25 | ... | ... | ... | 5036 ± 252 | 44.6 | 26 | ... | ... |
| Mrk 231 | 0.0422 | ... | ... | 393 ± 83 | 13 | ... | 3130 ± 156 | 45.0 | 2 (f),27 | ... | ... |
| ESO 323-G77 | 0.0150 | ... | ... | 100.0 ± 4.8 | 28 | ... | 2635 ± 132 | 43.1 | 21 | ... | ... |
| IRAS 13349+2438 | 0.1076 | ... | ... | 1096 ± 71 | 13 | ... | 1796 ± 90 | 45.0 | 29 | ... | ... |
| IC 4329A | 0.0161 | ... | ... | 178 ± 10 | 4 | ... | 6472 ± 324 | 43.2 | 21 | ... | ... |
| PGC 50427 (e) | 0.0235 | 46.7 ± 2.2 | 30 | ... | ... | ... | 3036 ± 74 | 43.1 | 30 | 7.34 ± 0.04 | −1.42 |
| PDS 456 | 0.1840 | ... | ... | 1599 ± 213 | 2 | ... | 3974 ± 764 | 46.3 | 31 | ... | ... |
| PGC 89171 | 0.0270 | ... | ... | 303 ± 36 | 4 | ... | 2644 ± 132 | 43.9 | 21 | ... | ... |
| NGC 7603 | 0.0288 | ... | ... | 332 ± 66 | 4 | ... | 6350 ± 318 | 44.4 | 21 | ... | ... |
Notes.
Mrk 590 is a changing look AGN displaying strong variability over the time of BLR and dust continuum observations (Denney et al. 2014). We do not include it in our statistical analysis.
The continuum radius of NGC 4151 reported by Kishimoto et al. (2011) is statistically consistent with the recent measurement from Kishimoto et al. (2022). We prefer the early measurements because it is close to the RM measurement.
The BLR of IRAS 09149−6206 was resolved by GRAVITY and the BH mass is derived by GRAVITY Collaboration (2020a). The λLλ(5100 Å) and FWHM of Hβ are from the BASS catalog (Koss et al. 2017).
The BH mass of PGC 50427 was measured by RM of the Hα line (Pozo Nuñez et al. 2015). We quote the λLλ(5100 Å) from Probst & Kollatschny (2020) observed close in time to Hα RM. We measure the FWHM of Hβ line from the 6dF spectrum (Jones et al. 2009).
We converted the bolometric luminosity to λLλ(5100 Å) using Eq. (A.2) of GRAVITY Collaboration (2020b).
Hβ FWHM is converted from Hα FWHM assuming FWHMHβ/FWHMHα = 1.17 (Greene & Ho 2005).
Column (1): Target name. Column (2): Redshift from NASA/IPAC Extragalactic Database (NED). Column (3): Dust continuum radius based on RM measurement. Column (4): Reference of Rd (RM). Column (5): Dust continuum radius based on OI measurement. Column (6): Reference of Rd (OI). Column (7): BLR radius based on Hβ time lag. Column (8): Hβ FWHM. Column (9): AGN optical luminosity at 5100 Å. Column (10): References of RBLR, FWHM, and λLλ(5100 Å). Column (11): BH mass derived from RBLR and FWHM from Cols. (7) and (8) assuming the virial factor f = 1. Column (12): Eddington ratio derived from λLλ(5100 Å) and BH mass from Cols. (9) and (11) with the bolometric correction factor 9 (Peterson et al. 2004).
References. (1) Minezaki et al. (2019), (2) GRAVITY Collaboration (2020b), (3) Du & Wang (2019), (4) GRAVITY Collaboration (in prep.), (5) Huang et al. (2019), (6) Ramolla et al. (2018), (7) Mandal et al. (2018), (8) Stalin et al. (2011), (9) Kishimoto et al. (2011), (10) Du et al. (2018), (11) Lira et al. (2011), (12) Bentz et al. (2021), (13) Kishimoto et al. (2009), (14) Sobrino Figaredo et al. (2020), (15) Lira et al. (2015), (16) Mandal et al. (2021a), (17) Barth et al. (2011), (18) Onori et al. (2017), (19) Rashed & Eckart (2015), (20) GRAVITY Collaboration (2020a), (21) Koss et al. (2017), (22) Pan et al. (2021), (23) Pozo Nuñez et al. (2014), (24) Probst & Kollatschny (2020), (25) Sitko et al. (1993), (26) Shangguan et al. (2018), (27) Zheng et al. (2002), (28) Leftley et al. (2021), (29) Dong et al. (2018), (30) Pozo Nuñez et al. (2015), (31) Nardini et al. (2015).
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