All Figures

$\begin{figure} \par\includegraphics[width=14.15cm,clip]{0423fig1.eps}\end{figure}$ Figure 1: Angular distance to the core vs. time elapsed since 1998.0. The plots show the change in angular separation with time of source features for which we have measured an angular velocity from observations at three or more epochs. The lines are linear fits to the data, the slope representing the proper motion, $\mu$ , tabulated in Table 4.
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{0423fi2a.eps}\par\includegra... ...ip]{0423fi2b.eps}\par\includegraphics[width=6cm,clip]{0423fi2c.eps} \end{figure}$ Figure 2: VLBA images of QSO 0153+744 on 27 July 1999 (1999.57), 15 June 2000 (2000.46), and 28 December 2000 (2000.99). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{0423fi3a.eps}\par\includegra... ...ip]{0423fi3b.eps}\par\includegraphics[width=6cm,clip]{0423fi3c.eps} \end{figure}$ Figure 3: VLBA images of QSO 0153+744 on 27 July 1999 (1999.57), 15 June 2000 (2000.46), and 28 December 2000 (2000.99). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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In the text

$\begin{figure} \par\includegraphics[height=5.7cm,width=6cm,clip]{0423fi4a.eps}\par\includegraphics[height=5.7cm,width=6cm,clip]{0423fi4b.eps} \end{figure}$ Figure 4: VLBA images of QSO 0212+735, from observations on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). Axes are relative $\alpha$ and $\delta$ in mas. See Table 1 for contour levels, synthesized beam size ( bottom left in the figure), and peak flux densities. See Table 2 for component parametrization.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=6.3cm,clip]{0423fi5a.eps}\hspace... ...s}\hspace*{4mm} \includegraphics[width=6.3cm,clip]{0423fi5d.eps} }\end{figure}$ Figure 5: VLBA images of BL 0454+844 from observations on 19 July 1999 (1999.55), 27 July 1999 (1999.57), 15 June 2000 (2000.46), and 4 March 2001 (2001.17). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{0423fi6a.eps}\par\includegraphics[width=6cm,clip]{0423fi6b.eps}\end{figure}$ Figure 6: VLBA images of QSO 0615+820 from observations on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). Axes are relative $\alpha$ and $\delta$ in mas. See Table 1 for contour levels, synthesized beam sizes ( bottom left in the maps), and peak flux densities. See Table 2 for component parametrization.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=6.3cm,clip]{0423fi7a.eps}\hspace... ...\hspace*{4mm} \includegraphics[width=6.3cm,clip]{0423fi7d.eps} }\end{figure}$ Figure 7: VLBA images of BL 0716+714 from observations on 19 July 1999 (1999.55), 27 July 1999 (1999.57), 15 June 2000 (2000.46), and 4 March 2001 (2001.17). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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In the text

$\begin{figure} \par\includegraphics[width=6.7cm,clip]{0423fi8a.eps}\par\includeg... ...ip]{0423fi8b.eps} \includegraphics[width=6.7cm,clip]{0423fi8c.eps} \end{figure}$ Figure 8: VLBA images of QSO 0836+710 from observations on 20 March 1998 (1998.22), 27 July 1999 (1999.57), and 15 June 2000 (2000.46). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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In the text

$\begin{figure} \par\includegraphics[height=5.8cm,width=6cm,clip]{0423fi9a.eps}\par\includegraphics[height=5.8cm,width=6cm,clip]{0423fi9b.eps} \end{figure}$ Figure 9: VLBA images of QSO 1039+811 from observations on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). Axes are relative $\alpha$ and $\delta$ in mas. See Table 1 for contour levels, synthesized beam sizes ( bottom left in the figure), and peak flux densities. See Table 2 for component parametrization.
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In the text

$\begin{figure} \par\includegraphics[height=5.7cm,width=6cm,clip]{0423f10a.eps}\par\includegraphics[height=5.7cm,width=6cm,clip]{0423f10b.eps} \end{figure}$ Figure 10: VLBA images of QSO 1150+812 from observations on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). Axes are relative $\alpha$ and $\delta$ in mas. See Table 1 for contour levels, synthesized beam sizes ( bottom left in the maps), and peak flux densities. See Table 2 for component parametrization.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=6.65cm,clip]{0423f11a.eps}\hspac... ...1d.eps} } \par\includegraphics[width=6.65cm,clip]{0423f11e.eps}\par \end{figure}$ Figure 11: VLBA images of BL 1749+701 from observations on 21 May 1999 (1999.39), 27 July 1999 (1999.57), 6 November 1999 (1999.85), 15 June 2000 (2000.46), and 28 December 2000 (2000.99). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=6.3cm,clip]{0423f12a.eps}\hspace... ...\hspace*{4mm} \includegraphics[width=6.3cm,clip]{0423f12d.eps} }\end{figure}$ Figure 12: VLBA Images of QSO 1803+784 from observations on 1 November 1998 (1998.84), 27 July 1999 (1999.57), 6 November 1999 (1999.85), and 15 June 2000 (2000.46). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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In the text

$\begin{figure} \par\includegraphics[height=5.6cm,width=6cm,clip]{0423f13a.eps}\par\includegraphics[height=5.6cm,width=6cm,clip]{0423f13b.eps} \end{figure}$ Figure 13: VLBA images of QSO 1928+738 (4C 73.18) from observations on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). Axes are relative $\alpha$ and $\delta$ in mas. See Table 1 for contour levels, synthesized beam sizes ( bottom left in the maps), and peak flux densities. See Table 2 for component parametrization.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=6.3cm,clip]{0423f14a.eps}\hspace... ...s}\hspace*{4mm} \includegraphics[width=6.3cm,clip]{0423f14d.eps} }\end{figure}$ Figure 14: VLBA images of BL 2007+777 from observations on 27 July 1999 (1999.57), 6 November 1999 (1999.85), 15 June 2000 (2000.46), and 4 March 2001 (2001.17). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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In the text

$\begin{figure} \par\includegraphics[width=14.15cm,clip]{0423fig1.eps}\end{figure}$	Figure 1: Angular distance to the core vs. time elapsed since 1998.0. The plots show the change in angular separation with time of source features for which we have measured an angular velocity from observations at three or more epochs. The lines are linear fits to the data, the slope representing the proper motion, $\mu$ , tabulated in Table 4.
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$\begin{figure} \par\includegraphics[width=6cm,clip]{0423fi2a.eps}\par\includegra... ...ip]{0423fi2b.eps}\par\includegraphics[width=6cm,clip]{0423fi2c.eps} \end{figure}$	Figure 2: VLBA images of QSO 0153+744 on 27 July 1999 (1999.57), 15 June 2000 (2000.46), and 28 December 2000 (2000.99). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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$\begin{figure} \par\includegraphics[width=6cm,clip]{0423fi3a.eps}\par\includegra... ...ip]{0423fi3b.eps}\par\includegraphics[width=6cm,clip]{0423fi3c.eps} \end{figure}$	Figure 3: VLBA images of QSO 0153+744 on 27 July 1999 (1999.57), 15 June 2000 (2000.46), and 28 December 2000 (2000.99). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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$\begin{figure} \par\includegraphics[height=5.7cm,width=6cm,clip]{0423fi4a.eps}\par\includegraphics[height=5.7cm,width=6cm,clip]{0423fi4b.eps} \end{figure}$	Figure 4: VLBA images of QSO 0212+735, from observations on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). Axes are relative $\alpha$ and $\delta$ in mas. See Table 1 for contour levels, synthesized beam size ( bottom left in the figure), and peak flux densities. See Table 2 for component parametrization.
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$\begin{figure} \par\mbox{\includegraphics[width=6.3cm,clip]{0423fi5a.eps}\hspace... ...s}\hspace*{4mm} \includegraphics[width=6.3cm,clip]{0423fi5d.eps} }\end{figure}$	Figure 5: VLBA images of BL 0454+844 from observations on 19 July 1999 (1999.55), 27 July 1999 (1999.57), 15 June 2000 (2000.46), and 4 March 2001 (2001.17). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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$\begin{figure} \par\includegraphics[width=6cm,clip]{0423fi6a.eps}\par\includegraphics[width=6cm,clip]{0423fi6b.eps}\end{figure}$	Figure 6: VLBA images of QSO 0615+820 from observations on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). Axes are relative $\alpha$ and $\delta$ in mas. See Table 1 for contour levels, synthesized beam sizes ( bottom left in the maps), and peak flux densities. See Table 2 for component parametrization.
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$\begin{figure} \par\mbox{\includegraphics[width=6.3cm,clip]{0423fi7a.eps}\hspace... ...\hspace*{4mm} \includegraphics[width=6.3cm,clip]{0423fi7d.eps} }\end{figure}$	Figure 7: VLBA images of BL 0716+714 from observations on 19 July 1999 (1999.55), 27 July 1999 (1999.57), 15 June 2000 (2000.46), and 4 March 2001 (2001.17). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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$\begin{figure} \par\includegraphics[width=6.7cm,clip]{0423fi8a.eps}\par\includeg... ...ip]{0423fi8b.eps} \includegraphics[width=6.7cm,clip]{0423fi8c.eps} \end{figure}$	Figure 8: VLBA images of QSO 0836+710 from observations on 20 March 1998 (1998.22), 27 July 1999 (1999.57), and 15 June 2000 (2000.46). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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$\begin{figure} \par\includegraphics[height=5.8cm,width=6cm,clip]{0423fi9a.eps}\par\includegraphics[height=5.8cm,width=6cm,clip]{0423fi9b.eps} \end{figure}$	Figure 9: VLBA images of QSO 1039+811 from observations on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). Axes are relative $\alpha$ and $\delta$ in mas. See Table 1 for contour levels, synthesized beam sizes ( bottom left in the figure), and peak flux densities. See Table 2 for component parametrization.
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$\begin{figure} \par\includegraphics[height=5.7cm,width=6cm,clip]{0423f10a.eps}\par\includegraphics[height=5.7cm,width=6cm,clip]{0423f10b.eps} \end{figure}$	Figure 10: VLBA images of QSO 1150+812 from observations on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). Axes are relative $\alpha$ and $\delta$ in mas. See Table 1 for contour levels, synthesized beam sizes ( bottom left in the maps), and peak flux densities. See Table 2 for component parametrization.
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$\begin{figure} \par\mbox{\includegraphics[width=6.65cm,clip]{0423f11a.eps}\hspac... ...1d.eps} } \par\includegraphics[width=6.65cm,clip]{0423f11e.eps}\par \end{figure}$	Figure 11: VLBA images of BL 1749+701 from observations on 21 May 1999 (1999.39), 27 July 1999 (1999.57), 6 November 1999 (1999.85), 15 June 2000 (2000.46), and 28 December 2000 (2000.99). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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$\begin{figure} \par\mbox{\includegraphics[width=6.3cm,clip]{0423f12a.eps}\hspace... ...\hspace*{4mm} \includegraphics[width=6.3cm,clip]{0423f12d.eps} }\end{figure}$	Figure 12: VLBA Images of QSO 1803+784 from observations on 1 November 1998 (1998.84), 27 July 1999 (1999.57), 6 November 1999 (1999.85), and 15 June 2000 (2000.46). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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$\begin{figure} \par\includegraphics[height=5.6cm,width=6cm,clip]{0423f13a.eps}\par\includegraphics[height=5.6cm,width=6cm,clip]{0423f13b.eps} \end{figure}$	Figure 13: VLBA images of QSO 1928+738 (4C 73.18) from observations on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). Axes are relative $\alpha$ and $\delta$ in mas. See Table 1 for contour levels, synthesized beam sizes ( bottom left in the maps), and peak flux densities. See Table 2 for component parametrization.
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$\begin{figure} \par\mbox{\includegraphics[width=6.3cm,clip]{0423f14a.eps}\hspace... ...s}\hspace*{4mm} \includegraphics[width=6.3cm,clip]{0423f14d.eps} }\end{figure}$	Figure 14: VLBA images of BL 2007+777 from observations on 27 July 1999 (1999.57), 6 November 1999 (1999.85), 15 June 2000 (2000.46), and 4 March 2001 (2001.17). See Tables 1-3 for contour levels, beam sizes ( bottom left in the maps), peak flux densities, and component parametrization. Axes are relative $\alpha$ and $\delta$ in mas.
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