Table 3: Results of our new WSRT and archival VLA observations. The upper limits shown are 5$\sigma $ upper limits.
HD star date freq. $\lambda $ flux spectral array
number name (d/m/y) (GHz) (cm) $\mu$Jy index $\alpha $  
24912 $\xi $ Per May/Jun./95 4.9 6 $\leq$240   WSRT
    Jun./Aug./95 1.4 21 $\leq$190   WSRT
    11/Jan./99 8.4 3.6 169 $\pm$ 30 0.29 $\pm$ 0.14 VLA
    28/Nov./05 1.4 21 100 $\pm$ 18   WSRT
30614 $\alpha $ Cam 09/Oct./05 1.4 21 156 $\pm$ 12 0.57 $\pm$ 0.06 WSRT
47839 15 Mon 13/Oct./05 1.4 21 $\leq$250   WSRT
210839 $\lambda $ Cep 03/Oct./05 1.4 21 98 $\pm$ 21 0.74 $\pm$ 0.11 WSRT
214680 10 Lac 22/Sep./05 4.9 6 $\leq$95   WSRT
    21/Sep./05 1.4 21 $\leq$95   WSRT


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