Table 3: Results of the VLA observations in 2002.
Source name Radio position $S_{\rm 20~cm}$ $S_{\rm 6~cm}$ $S_{\rm 3.5~cm}$ $\alpha^{\rm 20~cm}_{\rm 6~cm}$ $\alpha^{\rm 6~cm}_{\rm 3.5~cm}$
  (ICRS) (mJy) (mJy) (mJy)    
HD 135743 $\rm 15^h17^m$21 $.\!\!^{\rm s}$193 $\pm$ 0 $.\!\!^{\rm s}$001 $5.57\pm0.15$ $8.33\pm0.09$ $6.87\pm0.11$ $+0.74\pm0.05$ $-0.35\pm0.04$
  $-19^{\circ}00^{\prime}$59 $.\!\!^{\prime\prime}$26 $\pm$ 0 $.\!\!^{\prime\prime}$01          
CD-2412231 $\rm 15^h41^m$31 $.\!\!^{\rm s}$209 $\pm$ 0 $.\!\!^{\rm s}$004 $\leq$1.16 $1.17\pm0.06$ $0.74\pm0.02$ $\geq$+0.0 $-0.8\pm0.1$
  $-25^{\circ}20^{\prime}$36 $.\!\!^{\prime\prime}$49 $\pm$ 0 $.\!\!^{\prime\prime}$05          
HD 220338 $\rm 23^h23^m$01 $.\!\!^{\rm s}$17 $\pm$ 0 $.\!\!^{\rm s}$01 $\leq$0.83 $0.27\pm0.04$ $0.36\pm0.03$ $\geq$-1.3 $+0.5\pm0.3$
  $-06^{\circ}35^{\prime}$43 $.\!\!^{\prime\prime}$8 $\pm$ 0 $.\!\!^{\prime\prime}$1          


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