Table B.1.
Slopes of the power law fits obtained with different methods of fitting to data shown in Fig. 4
| quantity | cosmology only | Doppler correction | Doppler, no radio galaxies | individual sources |
|---|---|---|---|---|
| flux density Sν | −0.43 ± 0.13 | −0.01 ± 0.09 | −0.48 ± 0.11 | −0.43 ± 0.13 |
| core size θ | −0.80 ± 0.07 | −0.72 ± 0.04 | −0.77 ± 0.06 | −0.64 ± 0.05 |
| brightness temperature Tb | −0.96 ± 0.16 | −0.46 ± 0.10 | −0.93 ± 0.13 | −0.95 ± 0.13 |
Notes. Cosmology only: fits to the whole ensemble, corrected only for cosmological redshift; Doppler correction: Doppler correction applied to the data following Table B.2; Doppler, no radio galaxies: same as the previous column, but excluding radio galaxies; individual sources: Mean of fit results to individual sources with the procedure described in Section 3.1, shown as power laws in Fig. 4.
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