$\begin{figure} \par\includegraphics[width=8cm,clip]{3967fig4.eps} \end{figure}$ Figure 4: Examples of multiple objects being unambiguous optical counterparts: a galaxy group ( top left), a close galaxy group ( top right), a close galaxy pair ( bottom left), and a "merger'' ( bottom right).
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{3967fig5.eps} \end{figure}$ Figure 5: The DSS2(red)-ROSAT positional differences for 3202 selected optical counterparts in fractions of the ROSAT error radius.
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{3967fig1.eps} \end{figure}$	Figure 1: Distribution of the ROSAT FSC positional errors for 2791 sources of interest.
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$\begin{figure} \par\includegraphics[width=7.5cm,clip]{3967fig2.eps} \end{figure}$	Figure 2: Some sample HQS low-dispersion spectra for the main types of objects.
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$\begin{figure} \par\includegraphics[width=7cm,clip]{3967fig3.eps} \end{figure}$	Figure 3: The DSS2(red)-MAPS positional differences for 2341 objects in common.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{3967fig4.eps} \end{figure}$	Figure 4: Examples of multiple objects being unambiguous optical counterparts: a galaxy group ( top left), a close galaxy group ( top right), a close galaxy pair ( bottom left), and a "merger'' ( bottom right).
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$\begin{figure} \par\includegraphics[width=7.5cm,clip]{3967fig5.eps} \end{figure}$	Figure 5: The DSS2(red)-ROSAT positional differences for 3202 selected optical counterparts in fractions of the ROSAT error radius.
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$\begin{figure} \par\includegraphics[width=7cm,clip]{3967fig6.eps} \end{figure}$	Figure 6: MAPS color-magnitude diagram for point-like objects ( top) and galaxies ( bottom).
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$\begin{figure} \par\includegraphics[width=7cm,clip]{3967fig7.eps} \end{figure}$	Figure 7: Distribution of the MAPS O magnitudes for point-like objects and galaxies.
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