Open Access

Table 1.

Overview of the sample of JSS radio sources.

Source J2000 Alt. name id m z Scale Size L5 GHz Prec./Orb. Merger
(pc/mas) (pc) (1026W/Hz) markers marker
0019–000 J002225.42+001456.2 4C+00.02 G 18.4r 0.306 4.55 360 3.6 CTO D
0108+388 J011137.32+390628.1 G 22.0r 0.669 7.11 55 25 LST ...
0316+162 J031857.80+162832.7 CTA21 G 23.6r 0.907 7.94 2800 132 ... ...
0428+205 J043103.76+203734.3 DA138 G 19.3r 0.219 3.56 1000 3.0 LAT D
0500+019 J050321.20+020304.7 G 21.0i 0.585 6.68 95 26 S d
0710+439 J071338.16+434917.2 G 20.4r 0.518 6.29 200 15 LATO D
0941–080 J094336.94–081930.8 G 17.9r 0.228 3.67 350 1.7 LATO D
1031+567 J103507.04+562846.8 G 20.2r 0.459 5.88 470 9.4 LTO D
1117+146 J112027.81+142055.0 4C+14.41 G 20.1R 0.363 5.10 500 4.3 ... ...
1245–197 J124823.90–195918.6 Q 20.5V 1.275 8.54 1500 212 ATO d
1323+321 J132616.51+315409.5 4C+32.44 G 19.2r 0.369 5.15 450 9.9 LAT D
1345+125 J134733.36+121724.2 4C+12.50 G 15.5r 0.122 2.20 280 1.2 LS D
1358+624 J140028.65+621038.6 4C+62.22 G 19.8r 0.429 5.65 480 11 LATO D
1404+286 J140700.39+282714.7 OQ208 G 14.6r 0.077 1.46 12 0.41 LTS D
1518+047 J152114.42+043021.7 4C+04.51 G 22.6r 1.296 8.56 1400 140 ... ...
1607+268 J160913.32+264129.0 CTD93 G 20.4r 0.473 5.98 360 16 TO d
2008–068 J201114.21–064403.5 G 20.9i 0.547 6.47 200 15 TS d
2128+048 J213032.88+050217.5 G 23.3r 0.99 8.14 400 93 LCTS d
2210+016 J221237.97+015251.3 4C+01.69 G 21.7r 1.126 8.37 800 77 LCT ...
2342+821 J234403.77+822640.4 Q 20.1r 0.735 7.39 1300 31 ... ...
2352+495 J235509.46+495008.3 G 18.4R 0.238 3.79 340 2.3 LSATO D

Notes. Columns are: source name (radio sources observed with projects BS085 and BO030 are in bold), source name in J2000 coordinates, alternative name, optical identification, optical magnitude, redshift, scale, size, luminosity at 5 GHz in the rest frame, precession/orbital markers from radio images, and merger marker from optical images (see Sect. 4.1). For optical magnitudes, capital letters indicate the Johnson/Cousin photometric system, while lowercase letters indicate the Gunn photometric system.

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