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Fig. 1.


Examples of the jet detection. Left panel: C-band image of J0933+6106 (RA = 09h33m104, Dec = +61d06m46s) (top) and its azimuthal flux density distribution within the 3.5σ circular area (bottom). Right panel: similar plots for J1005+2403 (RA = 10h05m079, Dec = +24d03m38s). The red lines indicate the determined PAjet. The solid black line shows the azimuthal brightness distribution for the source, and five gray lines show the same value calculated in random positions within 40 mas from the source. Both images are from the VLBA Imaging and Polarimetry Survey (VIPS, Helmboldt et al. 2007).

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