Table B.1: The radio and optical properties of objects in the southern/equatorial sample of GPS galaxies.
IAU Other Radio position $m_{R_{\rm C}}$ z $S_{\rm 2.7~GHz}$ $\nu_{\rm peak}$ $S_{\rm peak}$ Ref. Ref. Comm.
name name (J2000) (mag)   (Jy) (GHz) (Jy) mR z  
J0022+0014 4C+00.02 00 22 25.48 +00 14 56.0 18.10 $\pm$ 0.20 0.305 1.94 0.6 3.1 3 3 A
J0108-1201 B0105-122 01 08 13.20 -12 00 50.3 22.39 $\pm$ 0.06 1.539 0.52 1.0 0.9 2 1  
J0206-3024 B0204-306 02 06 43.26 -30 24 58.2 21.00 $\pm$ 0.50   0.58 0.5 0.9 14    
J0210+0419 B0208+040 02 10 44.52 +04 19 35.4 $K_{\rm s}$ 18.3 $\pm$ 0.2   0.56 0.4 1.3 1    
J0210-2213 B0207-224 02 10 10.05 -22 13 36.6 23.52 $\pm$ 0.13 1.491 0.86 1.5 1.1 2 1  
J0242-2132 B0240-217 02 42 35.87 -21 32 26.2 17.10 $\pm$ 0.50 0.314 0.97 1.0 1.3 14 12  
J0323+0534 4C+05.14 03 23 20.27 +05 34 11.9 19.20 $\pm$ 0.50   1.60 0.4 7.1 14    
J0401-2921 B0359-294 04 01 21.50 -29 21 26.1 21.00 $\pm$ 0.20 0.656 0.58 0.4 1.0 1 1  
J0407-3924 B0405-395 04 07 34.43 -39 24 47.2 20.40 $\pm$ 0.50 0.474 0.52 0.4 1.4 14 1  
J0407-2757 B0405-280 04 07 57.94 -27 57 05.1 21.14 $\pm$ 0.04 0.728 0.93 1.5 1.4 2 1  
J0433-0229 4C-02.17 04 33 54.90 -02 29 56.0 19.10 $\pm$ 0.50 0.530 1.04 0.4 3.0 14 1  
J0441-3340 B0439-337 04 41 33.80 -33 40 03.6 22.50 $\pm$ 0.40   0.88 1.5 1.2 1    
J0457-0848 B0454-088 04 57 20.24 -08 49 05.2 20.30 $\pm$ 0.50 0.516 0.58 0.4 1.0 14 1  
J0503+0203 B0500+019 05 03 21.20 +02 03 04.6 i21.0 $\pm$ 0.20 0.583 2.46 2.5 2.5 5 5 A
J0943-0819 B0941-080 09 43 36.86 -08 19 32.0 17.50 $\pm$ 0.20 0.228 1.73 0.4 4.2 10 11 A
J0913+1454 B0910+151 09 13 35.00 +14 54 20.1 22.90 $\pm$ 0.50   0.54 0.6 1.1 1    
J1044-2712 B1042-269 10 44 37.63 -27 12 18.6 22.80 $\pm$ 0.40   0.55 1.5 0.8 1    
J1057+0012 B1054+004 10 57 15.78 +00 12 03.7 22.30 $\pm$ 0.30   0.58 0.4 1.6 1    
J1109+1043 B1107+109 11 09 46.04 +10 43 43.4 22.60 $\pm$ 0.30   0.80 0.5 2.4 1    
J1110-1858 B1107-187 11 10 00.45 -18 58 49.2 19.60 $\pm$ 0.20 0.497 0.65 1.0 0.9 9 13  
J1120+1420 4C+14.41 11 20 27.81 +14 20 55.0 20.10 $\pm$ 0.10 0.362 1.50 0.4 3.7 5 5 A
J1122-2742 B1120-274 11 22 56.41 -27 42 48.2 23.00 $\pm$ 0.50   0.74 1.4 0.8 1    
J1135-0021 4C-00.45 11 35 12.96 -00 21 19.5 21.90 $\pm$ 0.40 0.975 0.76 0.4 2.9 1 1  
J1203+0414 B1200+045 12 03 21.95 +04 14 17.7 18.80 $\pm$ 0.50 1.221 0.52 0.4 1.4 14 1 E
J1345-3015 B1343-300 13 45 51.52 -30 15 04.1 21.20 $\pm$ 0.20 1.132 0.56 0.4 2.5 1 1  
J1347+1217 4C+12.50 13 47 33.36 +12 17 24.2 15.20 $\pm$ 0.20 0.122 3.88 0.4 8.8 3 3 A
J1350-2204 B1347-218 13 50 14.33 -22 04 43.7 20.93 $\pm$ 0.05 0.700 0.72 0.4 1.4 2 1  
J1352+0232 B1349+027 13 52 30.68 +02 32 47.7 20.00 $\pm$ 0.50 0.607 0.78 0.4 2.0 14 1  
J1352+1107 4C+11.46 13 52 56.37 +11 07 07.7 21.00 $\pm$ 0.20 0.891 0.78 0.4 3.6 1 1  
J1447-3409 B1444-339 14 47 19.69 -34 09 16.2 21.00 $\pm$ 0.10 0.851 0.50 0.5 1.0 14 1  
J1506-0919 B1503-091 15 06 03.05 -09 19 12.5 19.70 $\pm$ 0.50 1.486 0.87 0.6 1.6 14 1 E
J1521+0430 4C+04.51 15 21 14.51 +04 30 20.0 22.10 $\pm$ 0.11 1.296 2.30 1.0 5.4 7 11 A
J1543-0757 B1540-077 15 43 01.69 -07 57 03.6 17.40 $\pm$ 0.10 0.172 1.21 0.4 1.7 6 6 C
J1546+0026 B1543+005 15 46 09.50 +00 26 24.6 20.10 $\pm$ 0.20 0.556 1.24 0.6 2.2 3 6 C
J1548-1213 B1545-120 15 48 12.97 -12 13 31.8 21.88 $\pm$ 0.13 0.883 1.45 0.4 3.7 2 2  
J1556-0622 4C-06.43 15 56 13.99 -06 22 37.8 22.20 $\pm$ 0.13 (1.195) 0.77 0.4 2.4 2 1  
J1600-0037 B1557-004 16 00 00.91 -00 37 23.3 -   0.54 1.0 1.2 2   D
J1604-2223 B1601-222 16 04 01.45 -22 23 41.3 18.75 $\pm$ 0.10 0.141 0.57 0.6 1.0 6 2  
J1640+1220 4C+12.60 16 40 47.96 +12 20 02.1 21.36 $\pm$ 0.20 1.150 1.48 0.4 3.7 2 2  
J1648+0242 4C+02.43 16 48 31.79 +02 42 46.0 22.10 $\pm$ 0.30 0.824 0.61 0.4 3.4 1 1  
J1734+0926 B1732+094 17 34 58.38 +09 26 57.8 20.80 $\pm$ 0.10 0.735 1.08 1.0 1.1 6 1 B
J2011-0644 B2008-068 20 11 14.22 -06 44 03.6 21.18 $\pm$ 0.04 0.547 2.09 1.4 2.6 2 2 A
J2058+0540 4C+05.78 20 58 28.84 +05 42 50.7 23.40 $\pm$ 0.30 1.381 0.65 0.4 3.1 8 8  
J2123-0112 B2121-014 21 23 39.12 -01 12 34.3 23.30 $\pm$ 0.10 1.158 0.64 0.4 2.0 4 3  
J2130+0502 B2128+048 21 30 32.88 +05 02 17.5 22.21 $\pm$ 0.07 0.990 3.12 1.0 4.8 2 11 A
J2151+0552 B2149+056 21 51 37.88 +05 52 13.0 20.20 $\pm$ 0.20 0.740 1.01 5.0 1.2 4 11 A, E
J2212+0152 4C+01.69 22 12 37.97 +01 52 51.7 i22.0 $\pm$ 0.20 1.126 1.80 0.4 4.6 5 1 A
J2325-0344 B2322-040 23 25 10.23 -03 44 46.7 23.50 $\pm$ 0.20 1.509 0.91 1.4 1.2 10 1 B
J2339-0604 4C-06.76 23 37 11.95 -06 04 12.4 22.91 $\pm$ 0.20 1.227 0.80 0.4 3.8 2 1  
Comments: (A) also in the sample of >1 Jy GPS sources from Stanghellini et al. (1998); (B) also in the sample of de Vries et al. (1997); (C) also in the sample of de Vries et al. (2000); (D) near a bright star, no magnitude; (E) radio source is optically identified with a quasar; will be excluded from the sample.
References: (1) this paper; (2) Snellen et al. (2002); (3) Snellen et al. (1996a); (4) O'Dea et al. (1990); (5) de Vries et al. (1995); (6) de Vries et al. (2000); (7) Biretta et al. (1985); (8) Stern et al. (1999); (9) Fugmann et al. (1988); (10) Stanghellini et al. (1993); (11) Stanghellini et al. (1998); (12) Otrupcek & Wright (1991); (13) Drinkwater et al. (1997); (14) Digitized Sky Survey II; APM catalogue (Irwin et al. 1994); SuperCosmos Sky Surveys (Hambly et al. 2001).

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