Table 6: Results of the fit of $F_{{\rm Peak}}$ vs. $F_{{\rm Tot}}$ for the CWSR sources indicating that an extended component is visible at 20 cm.
Frequency band $\alpha$ $\beta$
L (20 cm) 0.94 0.02
L (20 cm) * 0.96 0.01
C (6 cm) 0.99 -0.03
X (3.6 cm) 1.00 -0.06
* Fit without MS0922.9+7459.


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