Table 3: Total and polarization intensity radio images restored with a beam of 2 $^{\prime \prime }$ (see Figs. 3-6).
Source $\lambda$ Beam $\sigma $(I)* $\sigma $(Q)* $\sigma $(U)* Peak brightness Flux density Pol. flux
  (cm) ('') (mJy/beam) (mJy/beam) (mJy/beam) (mJy/beam) (mJy) (mJy)
J1712.4+6401 3.6 2.0$\times $2.0 0.015 0.018 0.017 2.8 49.5 9.5
'' 6 '' 0.019 0.020 0.020 3.5 86.0 13.0
J1713.3+6347 3.6 '' 0.014 0.016 0.016 2.3 37.0 8.0
'' 6 '' 0.018 0.020 0.020 2.4 64.5 10.5
J1713.5+6402 3.6 '' 0.014 0.017 0.018 11.6 87.0 10.0
'' 6 '' 0.021 0.024 0.022 12.7 123.5 11.5
J1715.1+6402 3.6 '' 0.014 0.017 0.015 3.5 26.0 2.0
'' 6 '' 0.016 0.020 0.021 3.5 43.5 2.0
Column 1: source; Col. 2: observation wavelength; Col. 3: beam; Cols. 4-6: rms noise of the I, Q, U images; * Note that while the I images have been obtained by averaging the two IFs in the same band, the Q and U images have been obtained for each IF separately. Here we give the values of $\sigma $(Q) and $\sigma $(U) for the frequencies 8465 MHz and 4535 MHz at 3.6 cm and 6 cm respectively. Column 7: peak brightness; Col. 8: flux density; Col. 9: polarized flux density (for the frequencies 8465 MHz and 4535 MHz at 3.6 cm and 6 cm respectively.).

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