\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}