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Table 1.

Sample sources from Berton et al. (2016).

SDSS Name RA Dec z Scale MBH> logL1.4 AGN type
(J2000.0) (J2000.0) (kpc/″) (M) W Hz−1
SDSS J002833.42+005510.9 00:28:33.423 +00:55:10.98 0.10429 1.975 8.94 24.77 2
SDSS J075756.71+395936.0 07:57:56.693 +39:59:36.00 0.06578 1.303 7.13 24.00 2
SDSS J084856.57+013647.8 08:48:56.574 +01:36:47.82 0.34987 5.088 7.05 25.54 Int
SDSS J092607.99+074526.6 09:26:08.003 +07:45:26.64 0.44169 5.868 7.28 26.05 Int
SDSS J094525.90+352103.5 09:45:25.888 +35:21:03.48 0.20777 3.505 7.23 25.24 Int
SDSS J114311.01+053516.1 11:43:11.030 +05:35:16.09 0.49694 6.264 8.84 26.26 Int
SDSS J115727.61+431806.3 11:57:27.605 +43:18:06.33 0.23012 3.790 7.68 25.58 Int
SDSS J140416.35+411748.7 14:04:16.366 +41:17:48.83 0.36042 5.187 7.96 25.96 2
SDSS J140942.44+360415.8 14:09:42.461 +36:04:15.98 0.14864 2.676 8.24 24.91 Int
SDSS J164311.34+315618.4 16:43:11.343 +31:56:18.40 0.58668 6.808 7.44 26.20 Int

Notes. Columns: (1) Complete name; (2) Right ascension in h:m:s; (3) Declination in d:m:s; (4) Redshift; (5) Scale calculated considering the Hubble constant to 67.8 km s−1 Mpc−1, a flat Universe with the matter density parameter ΣM = 0.308 and the vacuum density parameter Σvac = 0.692; (6) Logarithm of the black hole mass in M from Berton et al. (2016); (7) Log of the radio luminosity at 1.4 GHz from Kunert-Bajraszewska et al. (2010); and (8) AGN type visually determined from the SDSS spectra: type 2 or intermediate (Int).

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