Table 5: Summary of variability detection and radio flux densities of the monitored sources. Sources with the flag X were rejected by Londish (2003) because of high proper motion.
Source Our monitoring Londish On line plates SDSS Radio data Flag
          $F(1.4~{\rm GHz})^1$ $F(8.4~{\rm GHz})^2$  
          mJy mJy  
1002-00 no no no no     X
1026-00 no no no no     X
1036+01 no no yes no   $\le$0.1  
1045+00 no no no no     X
1053-00 no no yes no   $\le$0.1  
1055-01 no yes yes - 11    
1106+00 possibly ? no no   $\le$0.1  
1134+00 no no no no      
1139-02 no no no no      
1140-00 no no no no     X
1141-00 possibly possibly yes yes   3.6  
1145-02 no no no no     X
1145+00 no no no no      
1159-02 no no no no   0.3  
1200+00 no no no no      
1205-00 no no no no     X
1208-00 no no no no     X
1218-01 yes yes yes yes 244    
1223-01 no no yes no     X
1234-01 no possibly no no      
1254-01 no no no no      
1300-02 no no no no     X
1316-00 no no no no     X
1328+00 no no no no     X
1400+00 no no possibly no   0.3 X
1402-01 possibly possibly no no   $\le$0.1  
1409-00 no no no no     X
1410-02 no yes yes no      
1425-01 no possibly yes yes 10    
1. Flux density from NVSS.
2. Flux density from Londish et al. (2002), Londish (2003).

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