All Figures

$\begin{figure} \par\includegraphics[angle=180,width=12.2cm,clip]{0009fg1.eps}\end{figure}$ Figure 1: Plot of the fields used in this survey. Fields shaded in dark were used, fields shaded in light were available, but could not be used either because of a short epoch difference between the ESO and UK plates or because they contained too few bright stars to calculate the full relative astrometry. Unshaded fields below Dec = $-20^{\circ }$ could not be used because they are too close to the Galactic plane or cover the Magellanic clouds.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=7.7cm,clip]{0009fg2.eps}\end{figure}$ Figure 2: Histogram of the epoch differences between the ESO and UK R-band plates for all of the fields used in the survey.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=7cm,clip]{0009fg3.eps}\end{figure}$ Figure 3: Equal area plot of all objects in the catalogue.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=7.7cm,clip]{0009fg4.eps}\end{figure}$ Figure 4: Cumulative number of stars in this survey as a function of their proper motions. The offset straight line has a slope of -3. Error bars are $\surd$ N $_{{\rm C}}$ .
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=7.9cm,clip]{0009fg5.eps}\end{figure}$ Figure 5: Histogram of the fractional error on proper motion ( $\sigma _\mu$ / $\mu$ ) for all entries in the catalogue.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=7.7cm,clip]{0009fg6.eps}\end{figure}$ Figure 6: Number of high proper motion stars per 1.5 magnitudes in R for the Northern POSS areas of the NLTT: Solid line - this catalogue, dashed line - NLTT.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=7.7cm,clip]{0009fg7.eps}\end{figure}$ Figure 7: Number of high proper motion stars per 1.5 magnitudes in R for the Southern BPM areas of the NLTT: Solid line - this catalogue, dashed line - NLTT.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=7.7cm,clip]{0009fg8.eps}\end{figure}$ Figure 8: Number of high proper motion stars per 1.5 magnitudes in R for -32.5 $^{\circ }$ $\leq$ Dec $\leq$ -17.5 $^{\circ }$ and $\mid$ b $\mid$ $\geq$ 40 $^{\circ }$ : Solid line - this catalogue, dashed line - NLTT.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=7.6cm,clip]{0009fg9.eps}\end{figure}$ Figure 9: Plot of $K_{{\rm S}}$ (2MASS) against $R_{{\rm ESO}}-K_{{\rm S}}$ for all stars with $K_{{\rm S}}$ magnitudes. Vertical solid lines indicate the $R_{{\rm ESO}}-K_{{\rm S}}$ limits for the stellar types indicated. The horizontal dashed line indicates the SNR = 5 limit for the 2MASS $K_{{\rm S}}$ magnitude, the diagonal dashed line indicates the R= 19.5 mag cutoff of our catalogue. Large points are stars with $\mu$ $\geq$ 1.0 $\hbox {$^{\prime \prime }$ }$ ${\rm yr}^{-1}$ . The square indicates the position of the benchmark brown dwarf LP 944-20 (Tinney 1998).
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=14.1cm,clip]{0009fg10.eps}\end{figure}$ Figure 10: Plot of reduced proper motion, H_B, against $B-K_{{\rm S}}$ for all stars in the survey with B and $K_{{\rm S}}$ magnitudes. The lines showing the different regions of the plot are for guidance only.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=7.7cm,clip]{0009fg2.eps}\end{figure}$	Figure 2: Histogram of the epoch differences between the ESO and UK R-band plates for all of the fields used in the survey.
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$\begin{figure} \par\includegraphics[angle=270,width=7cm,clip]{0009fg3.eps}\end{figure}$	Figure 3: Equal area plot of all objects in the catalogue.
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$\begin{figure} \par\includegraphics[angle=270,width=7.7cm,clip]{0009fg4.eps}\end{figure}$	Figure 4: Cumulative number of stars in this survey as a function of their proper motions. The offset straight line has a slope of -3. Error bars are $\surd$ N $_{{\rm C}}$ .
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$\begin{figure} \par\includegraphics[angle=270,width=7.9cm,clip]{0009fg5.eps}\end{figure}$	Figure 5: Histogram of the fractional error on proper motion ( $\sigma _\mu$ / $\mu$ ) for all entries in the catalogue.
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$\begin{figure} \par\includegraphics[angle=270,width=7.7cm,clip]{0009fg6.eps}\end{figure}$	Figure 6: Number of high proper motion stars per 1.5 magnitudes in R for the Northern POSS areas of the NLTT: Solid line - this catalogue, dashed line - NLTT.
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$\begin{figure} \par\includegraphics[angle=270,width=7.7cm,clip]{0009fg7.eps}\end{figure}$	Figure 7: Number of high proper motion stars per 1.5 magnitudes in R for the Southern BPM areas of the NLTT: Solid line - this catalogue, dashed line - NLTT.
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$\begin{figure} \par\includegraphics[angle=270,width=7.7cm,clip]{0009fg8.eps}\end{figure}$	Figure 8: Number of high proper motion stars per 1.5 magnitudes in R for -32.5 $^{\circ }$ $\leq$ Dec $\leq$ -17.5 $^{\circ }$ and $\mid$ b $\mid$ $\geq$ 40 $^{\circ }$ : Solid line - this catalogue, dashed line - NLTT.
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$\begin{figure} \par\includegraphics[angle=270,width=14.1cm,clip]{0009fg10.eps}\end{figure}$	Figure 10: Plot of reduced proper motion, H_B, against $B-K_{{\rm S}}$ for all stars in the survey with B and $K_{{\rm S}}$ magnitudes. The lines showing the different regions of the plot are for guidance only.
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