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Table 4:

The values of the radio spectral index  $\alpha _{\rm r}$, the peak frequency  $\nu _{\rm s}$, the corresponding $\nu_{\rm s}~S(\nu_{\rm s})$ in 10-12 erg cm-2 s-1 and the curvature parameter b characterising VLBL candidates.
      Faint state       High state    
Source $\alpha _{\rm r}$  Log $\nu _{\rm s}$ $\nu_{\rm s}~S(\nu_{\rm s})$ b $\alpha _{\rm r}$ Log $\nu _{\rm s}$ $\nu_{\rm s}~S(\nu_{\rm s})$ b $\Gamma$
BZB J0753+5352  -0.60 13.13 3.21 0.17 -0.60 13.02 10.7 0.20 1.74 $\pm$ 0.15
BZB J0818+4222  -0.29 13.15 3.93 0.21 -0.06 12.75 9.68 0.19 1.42 $\pm$ 0.11
BZB J0823+2223  0.42 12.89 1.18 0.16 0.36 12.88 2.35 0.17 1.80 $\pm$ 0.34
BZB J0832+4913  0.11 12.89 2.61 0.25 0.02 13.06 12.5 0.23  
BZB J0929+8612  -0.34 12.81 7.55 0.30 -0.61 12.93 28.3 0.32  
BZB J1223+8040  0.11 12.97 2.58 0.20 - - - -  
BZB J1927+6117 -0.17 12.79 8.52 0.28 - - - -  
BZB J2009+7229  0.07 13.10 1.06 0.12 0.07 12.99 2.57 0.15 1.96 $\pm$ 0.33

Notes. Faint and high state are distinguished. Where available, the values of the photon index $\Gamma$ of a power law fit to Swift X-ray data are reported.


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