DeBreuck        
  MRC 2025$-$218       20:27:59.49   -21:40:56.9 4.8       56               2.9, 1.2            -30        AN129                     
  MG 2037$-$0011       20:37:13.40   -00:10:58.0 8.4       22               0.3, 0.2            36         AN129                     
  MRC 2104$-$242       21:06:58.10   -24:05:11.0 4.8       28               1.6, 0.6            56         AN129                     
  4C 23.56             21:07:14.28    23:31:41.2 8.4       25               0.2, 0.2            -34        AC379                     
  NVSSJ2135$-$3337     21:35:10.48   -33:37:04.4 4.8       28               1.3, 1.0            30         AN129                     
  MG 2144$+$1928       21:44:07.52    19:29:14.8 8.4       66               0.2, 0.2            -8         AS446                     
  TN J2254$+$1857      22:54:53.71    18:57:04.6 4.9       17               0.4, 0.4            -73        AN129                     
  MRC 2308$+$0336      23:03:19.62    03:04:25.1 5.0       36               0.5, 0.4            40         AB375                     
  TXS 2353$-$003       23:55:35.90   -00:02:48.0 4.8       19               0.4, 0.4            -21        AN129                     
  TXS 2353$-$003       23:55:35.90   -00:02:48.0 8.4       17               0.3, 0.3            40         AN129                     
  ------------------ ------------- ------------- --------- ---------------- ------------------- ---------- --------- --------------- --

3C 48 was used as a primary calibrator to set the flux scale, and secondary calibrators located within $\approx 10^\circ$ of the target source were observed every $20-30$ min for phase calibration. These data were all reduced using standard techniques within [ AIPS]{}. Sources were self-calibrated first in phase, and then in amplitude and phase, to improve the final image quality. Final images were made using a ROBUST$=0$ antenna weighting as a compromise between angular resolution and sensitivity.

Already existing, non-proprietary VLA observations of our sources were obtained from the 