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$\begin{figure} \par\includegraphics[height=12.04cm,width=9cm,clip]{fig1.eps}\end{figure}$ Figure 1: (x, y) measurement errors with respect to to magnitude, for 3 distinct ranges of sky background magnitude. The errors were computed from Gaussian image profile model fits. In the top, all magnitude ranges are displayed. The error-magnitude relation displays a typical distribution, with the increase at the faint magnitude end depending on the sky transparency, as revealed by the 3 sky background magnitude regimes present in our observations.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{fig2.eps} % \end{figure}$ Figure 2: Optical minus radio position offsets with respect to RA and Dec for the 59 northern ICRF sources listed in Table 1.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{fig2.eps} % \end{figure}$	Figure 2: Optical minus radio position offsets with respect to RA and Dec for the 59 northern ICRF sources listed in Table 1.
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