\begin{table}%b1
\caption{\label{sample}The radio and optical properties of objects in the southern/equatorial sample of GPS~galaxies.}
\small%\centerline
{
\begin{tabular}{c c c c c c c c c c c c}
\hline \hline
IAU		& Other		& \multicolumn{2}{c}{Radio position}	& $m_{R_{\rm C}}$		& $z$	& $S_{\rm 2.7~GHz}$	& $\nu_{\rm peak}$	& $S_{\rm peak}$	& Ref.	& Ref.	& Comm. \\
name		& name		& \multicolumn{2}{c}{(J2000)}		& (mag)			&	& (Jy)	& (GHz)	& (Jy)	& $m_R$	& $z$	& \\
\hline
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	& \\
\hline
\end{tabular}}
\smallskip
 Comments:  (A) also in the sample of $>$1~Jy GPS~sources from Stanghellini et~al. (\cite{Stanghellini98}); (B) also in the sample of de Vries et~al. (\cite{Vries97}); (C) also in the sample of de Vries et~al. (\cite{Vries00}); (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. (\cite{Snellen02}); (3) Snellen et~al. (\cite{Snellen96a}); (4) O'Dea et~al.  (\cite{O'Dea90}); (5) de Vries et~al. (\cite{Vries95}); (6)~de~Vries et~al. (\cite{Vries00}); (7) Biretta et~al. (\cite{Biretta}); (8) Stern et~al. (\cite{Stern}); (9) Fugmann  et~al.  (\cite{Fugmann}); (10) Stanghellini et~al. (\cite{Stanghellini93}); (11) Stanghellini et~al. (\cite{Stanghellini98}); (12) Otrupcek \& Wright (\cite{Otrupcek}); (13) Drinkwater et~al. (\cite{Drinkwater}); (14) Digitized Sky Survey II; APM catalogue (Irwin et~al. \cite{Irwin}); SuperCosmos Sky Surveys (Hambly et~al. \cite{Hambly}).
\end{table}