\begin{table}%t1 \par %\centering \par \caption{\label{t1}Jet properties of the blazars in the Mets\"ahovi-MOJAVE sample.} \begin{tabular}{lcccccccc} \hline \hline \noalign{\smallskip} IAU name & Class & $z$ & $\beta_{\rm app}$\tablefootmark{1} & $\delta_{\rm var}$ & $\Gamma$ & $\theta$ &$\theta_{\rm src}$ & LAT-det.\tablefootmark{2} \\ (B1950.0) & & & & & & (deg) & (deg) & \\ \hline \object{0003$-$066} & BL Lac & 0.347 & 0.9 & 5.1 & 2.7 & 4.0 & 20.5 & N \\ \object{0016+731} & Quasar & 1.781 & 6.7 & 7.8 & 6.9 & 7.3 & 82.0 & N \\ \object{0106+013} & Quasar & 2.099 & 26.5 & 18.2 & 28.4 & 2.9 & 111.0 & N \\ \object{0109+224} & BL Lac & 0.265 & ... & 9.1 & ... & ... & ... & Y \\ \object{0133+476} & Quasar & 0.859 & 13.0 & 20.5 & 14.4 & 2.5 & 64.8 & Y \\ \object{0202+149} & Quasar & 0.405 & 6.4 & 15.0 & 8.9 & 2.8 & 46.6 & N \\ \object{0212+735} & Quasar & 2.367 & 7.6 & 8.4 & 7.7 & 6.8 & 84.9 & N \\ \object{0234+285} & Quasar & 1.207 & 12.3 & 16.0 & 12.7 & 3.5 & 75.4 & Y \\ \object{0235+164} & BL Lac & 0.940 & ... & 23.8 & ... & ... & ... & Y \\ \object{0333+321} & Quasar & 1.259 & 12.8 & 22.0 & 14.7 & 2.3 & 60.5 & N \\ \object{0336$-$019} & Quasar & 0.852 & 22.4 & 17.2 & 23.2 & 3.2 & 104.9 & N \\ \object{0420$-$014} & Quasar & 0.915 & 7.3 & 19.7 & 11.3 & 1.9 & 41.0 & Y \\ \object{0458$-$020} & Quasar & 2.286 & 16.5 & 15.7 & 16.6 & 3.7 & 93.1 & N \\ \object{0528+134} & Quasar & 2.070 & 19.2 & 30.9 & 21.4 & 1.7 & 63.7 & Y \\ \object{0605$-$085} & Quasar & 0.872 & 16.8 & 7.5 & 22.6 & 5.7 & 131.8 & N \\ \object{0642+449} & Quasar & 3.396 & 0.8 & 10.6 & 5.4 & 0.8 & 8.3 & N \\ \object{0716+714} & BL Lac & 0.310 & 10.1 & 10.8 & 10.2 & 5.3 & 86.4 & Y \\ \object{0736+017} & Quasar & 0.191 & 14.4 & 8.5 & 16.5 & 5.9 & 119.0 & N \\ \object{0754+100} & BL Lac & 0.266 & 14.4 & 5.5 & 21.6 & 6.9 & 138.0 & N \\ \object{0804+499} & Quasar & 1.436 & 1.8 & 35.2 & 17.6 & 0.2 & 6.0 & N \\ \object{0814+425} & BL Lac & 0.245 & 1.7 & 4.6 & 2.7 & 8.6 & 42.8 & Y \\ \object{0827+243} & Quasar & 0.941 & 22.0 & 13.0 & 25.2 & 3.9 & 119.0 & N \\ \object{0836+710} & Quasar & 2.218 & 25.4 & 16.1 & 28.1 & 3.2 & 115.2 & N \\ \object{0851+202} & BL Lac & 0.306 & 5.2 & 16.8 & 9.3 & 1.9 & 34.5 & Y \\ \object{0923+392} & Quasar & 0.695 & 0.6 & 4.3 & 2.3 & 3.9 & 16.7 & N \\ \object{0945+408} & Quasar & 1.249 & 18.6 & 6.3 & 30.5 & 5.5 & 142.4 & N \\ \object{1055+018} & Quasar & 0.888 & 8.1 & 12.1 & 8.8 & 4.4 & 67.6 & Y \\ \object{1156+295} & Quasar & 0.729 & 24.9 & 28.2 & 25.1 & 2.0 & 82.9 & Y \\ \object{1222+216} & Quasar & 0.432 & 21.0 & 5.2 & 45.5 & 5.1 & 152.5 & N \\ \object{1226+023} & Quasar & 0.158 & 13.4 & 16.8 & 13.8 & 3.3 & 77.1 & Y \\ \object{1253$-$055} & Quasar & 0.536 & 20.6 & 23.8 & 20.8 & 2.4 & 81.9 & Y \\ \object{1308+326} & Quasar & 0.997 & 20.9 & 15.3 & 22.0 & 3.6 & 107.8 & Y \\ \object{1324+224} & Quasar & 1.400 & ... & 21.0 & ... & ... & ... & N \\ \object{1334$-$127} & Quasar & 0.539 & 10.3 & 8.3 & 10.6 & 6.8 & 102.6 & N \\ \object{1413+135} & BL Lac & 0.247 & 1.8 & 12.1 & 6.2 & 1.4 & 17.1 & N \\ \object{1502+106} & Quasar & 1.839 & 14.8 & 11.9 & 15.2 & 4.7 & 102.6 & Y \\ \object{1510$-$089} & Quasar & 0.360 & 20.2 & 16.5 & 20.6 & 3.4 & 101.4 & Y \\ \object{1538+149} & BL Lac & 0.605 & 8.7 & 4.3 & 11.2 & 10.6 & 128.5 & N \\ \object{1606+106} & Quasar & 1.226 & 17.9 & 24.8 & 18.9 & 2.2 & 71.8 & N \\ \object{1611+343} & Quasar & 1.397 & 5.7 & 13.6 & 8.0 & 3.0 & 45.9 & N \\ \object{1633+382} & Quasar & 1.814 & 29.5 & 21.3 & 31.1 & 2.6 & 108.4 & Y \\ \object{1637+574} & Quasar & 0.751 & 10.6 & 13.9 & 11.0 & 4.0 & 75.0 & N \\ \object{1641+399} & Quasar & 0.593 & 19.3 & 7.7 & 28.0 & 5.1 & 136.4 & N \\ \object{1730$-$130} & Quasar & 0.902 & 35.7 & 10.6 & 65.5 & 2.9 & 146.9 & N \\ \object{1739+522} & Quasar & 1.379 & ... & 26.3 & ... & ... & ... & N \\ \object{1741$-$038} & Quasar & 1.054 & ... & 19.5 & ... & ... & ... & N \\ \object{1749+096} & BL Lac & 0.322 & 6.8 & 11.9 & 8.0 & 4.2 & 60.1 & Y \\ \object{1803+784} & BL Lac & 0.684 & 9.0 & 12.1 & 9.4 & 4.5 & 73.4 & Y \\ \object{1807+698} & BL Lac & 0.051 & 0.1 & 1.1 & 1.0 & 45.3 & 50.8 & N \\ \object{1823+568} & BL Lac & 0.664 & 9.4 & 6.3 & 10.2 & 8.4 & 112.4 & N \\ \object{1828+487} & Quasar & 0.692 & 13.7 & 5.6 & 19.5 & 7.1 & 135.4 & N \\ \object{1928+738} & Quasar & 0.302 & 7.2 & 1.9 & 15.0 & 14.8 & 151.2 & N \\ \object{2121+053} & Quasar & 1.941 & 8.4 & 15.2 & 9.9 & 3.2 & 58.1 & N \\ \object{2134+004} & Quasar & 1.932 & 2.0 & 16.0 & 8.1 & 0.9 & 14.6 & N \\ \object{2136+141} & Quasar & 2.427 & 3.0 & 8.2 & 4.7 & 4.5 & 39.9 & N \\ \object{2145+067} & Quasar & 0.990 & 2.2 & 15.5 & 7.9 & 1.0 & 16.2 & N \\ \object{2200+420} & BL Lac & 0.069 & 5.0 & 7.2 & 5.4 & 7.5 & 69.7 & Y \\ \object{2201+315} & Quasar & 0.295 & 7.9 & 6.6 & 8.1 & 8.5 & 100.3 & N \\ \object{2223$-$052} & Quasar & 1.404 & 14.6 & 15.9 & 14.7 & 3.6 & 85.4 & N \\ \hline \object{2227$-$088} & Quasar & 1.562 & 8.1 & 15.8 & 10.0 & 3.0 & 54.8 & Y \\ \object{2230+114} & Quasar & 1.037 & 15.4 & 15.5 & 15.4 & 3.7 & 89.9 & Y \\ \object{2251+158} & Quasar & 0.859 & 14.2 & 32.9 & 19.5 & 1.3 & 46.7 & Y \\ \hline \end{tabular} \tablefoot{\tablefoottext{1}{Fastest non-accelerating, radial apparent speed measured in the source. The speeds differ in some cases from the speeds quoted by \citet{hov09}, partly because Hovatta et~al. used results from a preliminary kinematics analysis, and partly because we consider only non-accelerating, radially moving components in order to estimate the flow speed close to the core, where the mm-wavelength outbursts take place. Due to this, the values of $\Gamma$ and $\theta$ naturally also differ in some cases from those reported by Hovatta et al.} \tablefoottext{2} {\rm Bright} (${>}10\sigma$) LAT-detections during the first three months of science operations \citep{abd09a}.} \end{table}