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Table 1

The large core shift source sample observed with the VLBA.

IAU name Alias RA (J2000) Dec (J2000) z Optical class VLBA epoch

0148 + 274 01:51:27.146174  + 27:44:41.79363 1.26 QSO 2007-03-01
0342 + 147 03:45:06.416545  + 14:53:49.55818 1.556 QSO 2007-06-01
0425 + 048 OF 42 04:27:47.570531  + 04:57:08.32555 0.5171 AGN 2007-04-30
0507 + 179 05:10:02.369133  + 18:00:41.58160 0.416 AGN 2007-05-03
0610 + 260 3C 154 06:13:50.139161  + 26:04:36.71971 0.580 QSO 2007-03-01
0839 + 187 08:42:05.094175  + 18:35:40.99050 1.272 QSO 2007-06-01
0952 + 179 09:54:56.823616  + 17:43:31.22204 1.478 QSO 2007-04-30
1004 + 141 10:07:41.498089  + 13:56:29.60070 2.707 QSO 2007-05-03
1011 + 250 10:13:53.428771  + 24:49:16.44062 1.636 QSO 2007-03-01
1049 + 215 10:51:48.789077  + 21:19:52.31374 1.300 QSO 2007-06-01
1219 + 285 W Comae 12:21:31.690524  + 28:13:58.50011 0.1612 BL Lac 2007-04-30
1406 − 076 14:08:56.481198  −07:52:26.66661 1.493 QSO 2007-05-03
1458 + 718 3C 309.1 14:59:07.583927  + 71:40:19.86646 0.904 QSO 2007-03-01
1642 + 690 16:42:07.848505  + 68:56:39.75639 0.751 QSO 2007-04-30
1655 + 077 16:58:09.011464  + 07:41:27.54034 0.621 QSO 2007-06-01
1803 + 784 18:00:45.683905  + 78:28:04.01839 0.680 QSO 2007-05-03
1830 + 285 18:32:50.185622  + 28:33:35.95514 0.594 QSO 2007-03-01
1845 + 797 3C 390.3 18:42:08.989895  + 79:46:17.12825 0.056 AGN 2007-06-01
2201 + 315 22:03:14.975788  + 31:45:38.26990 0.298 QSO 2007-04-30
2320 + 506 23:22:25.982173  + 50:57:51.96364 1.279 QSO 2007-05-03

Notes. Column 1 – IAU source name (B1950); Col. 2 – commonly used source name; Cols. 3 and 4 – VLBI position, for details see http://astrogeo.org/vlbi/solutions/rfc_2010c/ and Beasley et al. (2002), Fomalont et al. (2003), Petrov et al. (2005, 2006), Kovalev et al. (2007), Petrov et al. (2008, 2009); Cols. 5 and 6 – redshift and optical class from Véron-Cetty & Véron (2010); Col. 7 – epoch of multifrequency VLBA observations reported in this paper.

(1)

Spectroscopic redshift obtained by Afanasiev et al. (2003);

(2)

photometric redshift, see Finke et al. (2008).

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