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Table 1

Parameters of observed sources.

Source IVS name Right ascension Declination Optical z Scale 2FGL
J2000.0 J2000.0 class pc mas-1 member
(1) (2) (3) (4) (5) (6) (7) (8)

J0006−0623 0003−066 00  06  13.892887  −06  23  35.33545 B 0.347 4.913 ...
J0011−2612 0008−264 00  11  01.246737  −26  12  33.37719 Q 1.093 8.163 ...
J0017 + 8135 0014 + 813 00  17  08.474901  + 81  35  08.13655 Q 3.387 7.407 ...
J0019 + 7327 0016 + 731 00  19  45.786379  + 73  27  30.01753 Q 1.781 8.450 ...
J0022 + 0608 0019 + 058 00  22  32.441214  + 06  08  04.26889 B ... ... Y
J0027 + 5958 0024 + 597 00  27  03.286191  + 59  58  52.95918 U ... ... ...
J0035 + 6130 0032 + 612 00  35  25.310644  + 61  30  30.76129 U ... ... ...
J0050−0929 0048−097 00  50  41.317382  −09  29  05.21043 B ... ... Y
J0059 + 0006 0056−001 00  59  05.514929  + 00  06  51.62077 Q 0.717 7.215 ...
J0102 + 5824 0059 + 581 01  02  45.762379  +58  24  11.13659 Q 0.644a 6.902 Y

References. Columns are as follows: (1) J2000.0 IAU name; (2) IVS name (B1950.0 IAU name or alias); (3) right ascension (J2000.0) in hours, minutes, and seconds; (4) declination (J2000.0) in degrees, minutes, and seconds; (5) optical classification according to Véron-Cetty & Véron (2006), where Q is a quasar, B is a BL Lacertae object, G is an active galaxy, and U is unidentified, (6) redshift as given by Véron-Cetty & Véron (2006), the a flag indicates the redshift from Sowards-Emmerd et al. (2005), b – from Carilli et al. (1998), c – from Drake et al. (2004), d – from Afanasiev et al. (2003), e – from von Montigny et al. (1995), f – from Nilsson et al. (2008), g – from Best et al. (2003), h – from Hewitt & Burbidge (1989), k – from Snellen et al. (2002b), and l – from Snellen et al. (2002a); (7) angular scaling conversion in parsecs per milliarcsecond; (8) membership in the Fermi LAT Second Source Catalog according to Abdo et al. (2012). The coordinate positions are taken from the Radio Fundamental Catalog (http://astrogeo.org/rfc) as derived from an analysis of all VLBI observations made in absolute astrometry and geodesy mode (Beasley et al. 2002; Fomalont et al. 2003; Petrov et al. 2005, 2006; Kovalev et al. 2007; Petrov et al. 2008). Table 1 is published in its entirety at the CDS. A portion is shown here for guidance regarding its form and content.

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