Table 5: Other sources of interest. Sources for which no reference is given are those from the ATCA program with spectra that are inverted, but which do not meet our criteria for inclusion as GPS candidates. The spectral index, $\alpha $, is that determined between 4.8 and 8.4 GHz from the ATCA monitoring (Tingay et al. 2003b). Parameters are the same as for previous tables.

Source
B1950 Refs. a Type z S4.8 m4.8 p4.8 $\alpha $  Flag
          (Jy)   (%)    

J0106-4034
0104-408   Q 0.584 3.56 0.06 1.34 (1.4) 0.57 c
J0457-2324 0454-234 T01 Q 1.003 2.04 0.15 1.44 (3.5) 0.23 l
J0538-4405 0537-441 T01 BL 0.894 3.48 0.30 1.28 (1.0) 0.15 l
J1035-2011 1032-199   Q 2.198 1.01 0.11 3.03 (4.1) 0.52 l
J1058-8003 1057-797 T01 Q ... 2.03 0.20 3.14   0.16 c
J1337-1257 1334-127 T01 Q 0.539 3.55 0.24 3.34   0.41 l
J1419-1928 1417-192 T03 G 0.120 0.47 0.07 2.44   -0.03 e
J1743-0350 1741-038   Q 1.054 4.43 0.11 0.96 (1.2) 0.29 c
J1751+0939 1749+096   BL 0.322 2.41 0.28 1.41 (6.1) 0.61 c
J1957-3845 1954-388 T01 Q 0.626 3.21 0.26 3.09 (1.0) 0.05 c
J2123+0535 2121+053   Q 1.878 0.95 0.32 1.17 (2.5) 0.54 c
J2131-1207 2128-123 T01 Q 0.499 2.55 0.04 1.20 (0.6) 0.09 c
J2148+0657 2145+067 T01 Q 0.990 6.33 0.05 <0.5    (1.0) 0.25 c
J2239-5701 2236-572   EF ... 0.72 0.05 4.39   0.24 c
J2258-2758 2255-282 T01 Q 0.926 3.37 0.10 0.92   0.89 l
J2358-1020 2355-106   Q 1.626 1.11 0.34 2.84   -0.18 c

$\textstyle \parbox{13.5cm}{
$^{{a}}$\space References:
T01 = \cite{tor01};
T03 = \cite{tay03}.}$


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