Table 5
The parameters derived for the quasars from VLBI imaging.
| Source name | Complete VLBI flux density (mJy) | Main component flux density (mJy) | α | Size | T B | L | ||
| at 1.6 GHz | at 5 GHz | at 1.6 GHz | at 5 GHz | mas | 109 K | 1026 W Hz-1 | ||
|
|
||||||||
| J0813+3508 | 17.1 ± 0.9 | 7.3 ± 0.4* | 12.8 ± 0.6 | 6.8 ± 0.3* | −0.6 | 1.18 ± 0.02 | 1.5 ± 0.1 | 8.4 ± 0.4 |
| J1146+4037 | 15.5 ± 0.8 | 8.6 ± 0.4* | 15.5 ± 0.8 | 8.4 ± 0.4* | −0.5 | 0.74 ± 0.01 | 4.5 ± 0.3 | 10.7 ± 0.5 |
| J1242+5422 | 17.7 ± 0.9 | 9.7 ± 0.5 | 17.1 ± 0.9 | 9.4 ± 0.5 | −0.5 | 0.67 ± 0.01 | 5.9 ± 0.5 | 9.0 ± 0.5 |
| J1611+0844 | 13.0 ± 0.8 | 12.9 ± 0.6 | 13.0 ± 0.8 | 12.4 ± 0.6 | −0.0 | 0.85 ± 0.01 | 4.7 ± 0.3 | 4.6 ± 0.2 |
| J1659+2101 | 29.3 ± 1.5 | 10.6 ± 0.7 | 19.7 ± 1.0 | 10.6 ± 0.7 | −0.6 | 3.07 ± 0.12 | 0.3 ± 0.04 | 12.3 ± 0.8 |
Notes. Column 1 – source name; Col. 2-3 – complete VLBI flux density at 1.6 GHz and 5 GHz (mJy); Col. 4–5 – main component VLBI flux density at 1.6 GHz and 5 GHz (mJy); Col. 6 – two-point spectral index of the main component; Col. 7 – fitted circular Gaussian diameter (FWHM) for the main component at 5 GHz (mas); Col. 8 – rest-frame brightness temperature at 5 GHz (109 K); Col. 9 – rest-frame monochromatic 5-GHz luminosity (1026 W Hz-1). The VLBI flux density calibration uncertainties are assumed as 5%. The statistical errors of the fitted model parameters are estimated according to Fomalont (1999).
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