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Table 2.

Fitted brightness distribution model parameters, calculated core brightness temperatures, and monochromatic radio powers for J0906+6930 and J2102+6015 from the combined 5-epoch VLBI data at 2.3 and 8.6 GHz.

Source ν GHz Component S mJy r mas ϕ̥ θmaj mas θmin mas ψ̥ Tb 1011 K P 1027 WHz−1
J0906+6930 2.3 0 107.5 ± 16.1 0 0 1.42 ± 0.05 0.67 ± 0.03 171 1.76 ± 0.28 4.8 ± 0.7
1 10.8 ± 1.6 2.46 ± 0.08 137 ± 2 1.93 ± 0.16
8.6 0 79.9 ± 12.0 0 0 0.38 ± 0.01 0.08 ± 0.01 43 2.81 ± 0.45 3.6 ± 0.5
1 29.1 ± 4.4 0.74 ± 0.01 224 ± 1 0.14 ± 0.02
2 6.6 ± 1.0 1.26 ± 0.02 184 ± 1 0.36 ± 0.05
J2102+6015 2.3 0 304.7 ± 45.7 0 0 4.26 ± 0.18 2.56 ± 0.08 101 0.36 ± 0.06 27.3 ± 4.1
8.6 0 95.8 ± 14.4 0 0 0.44 ± 0.02 0.46 ± 0.07 8.6 ± 1.3
1 35.5 ± 5.3 0.62 ± 0.02 260 ± 2 0.75 ± 0.05
2 26.0 ± 3.9 0.53 ± 0.02 95 ± 2 0.58 ± 0.03
3 1.1 ± 0.2 10.13 ± 0.03 270 ± 1 <0.2

Notes. Column 2 – observing frequency, Col. 4 – flux density, Col. 5 – radius from the central component, Col. 6 – position angle, Col. 7 – elliptical Gaussian component major axis or circular Gaussian component diameter (FWHM), Col. 8 – elliptical Gaussian component minor axis (FWHM), Col. 9 – elliptical Gaussian component major axis position angle; position angles are measured from north through east, Col. 10 – brightness temperature, Col. 11 – monochromatic radio power at the given frequency in the rest frame of the source.

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