$\begin{figure} \par\resizebox{8.2cm}{!}{\rotatebox{-90}{\includegraphics{6014f00... ...\resizebox{8.2cm}{!}{\rotatebox{-90}{\includegraphics{6014f002.ps}}}\end{figure}$ Figure 1: Two representative low resolution spectra obtained at Byurakan Observatory. In the upper panel, the object is FBS 0826+185, a cool N-type star with R=11.5, B-R=4.6, J-K=1.68 and b=+30 $^{\circ }$ . In the lower panel, the object is FBS 1043+213, a warm C star with R=11.2, B-R=2.3, J-K=0.88 and b = +61 $^{\circ }$ .
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.2cm,clip]{6014f007.eps}\\ [2mm] \includegraphics[angle=-90,width=7.2cm,clip]{6014f008.eps}\end{figure}$ Figure 4: Colour-colour diagrams with J-H vs. H-K (from 2MASS photometry). Lower panel: HES sources. Upper panel: FBS sources. In both panels, the dotted lines correspond to J-K = 1 and J-K = 2.
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In the text

$\begin{figure} \par\resizebox{7.8cm}{!}{\rotatebox{-90}{\includegraphics{6014f010.eps}}}\end{figure}$ Figure 6: Proper motions of 402 HES objects, with $\mu_{\alpha} \cos~(\delta)$ in abscissa and $\mu _{\delta }$ in ordinates. Circles with an overplotted cross correspond to cases where $\mu$ is larger than 30 mas yr^-1 and where the motion in $\alpha$ or $\delta$ is detected with at least a 3 $\sigma$ quality.
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In the text

$\begin{figure} \par\resizebox{8.2cm}{!}{\rotatebox{-90}{\includegraphics{6014f00... ...\resizebox{8.2cm}{!}{\rotatebox{-90}{\includegraphics{6014f002.ps}}}\end{figure}$	Figure 1: Two representative low resolution spectra obtained at Byurakan Observatory. In the upper panel, the object is FBS 0826+185, a cool N-type star with R=11.5, B-R=4.6, J-K=1.68 and b=+30 $^{\circ }$ . In the lower panel, the object is FBS 1043+213, a warm C star with R=11.2, B-R=2.3, J-K=0.88 and b = +61 $^{\circ }$ .
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$\begin{figure} \par\resizebox{7.5cm}{!}{\rotatebox{-90}{\includegraphics{6014f00... ...resizebox{7.5cm}{!}{\rotatebox{-90}{\includegraphics{6014f004.eps}}}\end{figure}$	Figure 2: Plots of the R-band magnitude as a function of the B-R colour index. Upper panel: FBS objects from Paper I and this paper. Lower panel: HES objects.
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$\begin{figure} \par\includegraphics[angle=-90,width=7.2cm,clip]{6014f005.eps}\\ [2mm] \includegraphics[angle=-90,width=7.2cm,clip]{6014f006.eps}\end{figure}$	Figure 3: Colour-magnitude diagrams K vs. J-K. Lower panel: HES sources. Upper panel : FBS sources. In both panels, the limits J-K = 1 and K=10 are overplotted (see text).
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$\begin{figure} \par\includegraphics[angle=-90,width=7.2cm,clip]{6014f007.eps}\\ [2mm] \includegraphics[angle=-90,width=7.2cm,clip]{6014f008.eps}\end{figure}$	Figure 4: Colour-colour diagrams with J-H vs. H-K (from 2MASS photometry). Lower panel: HES sources. Upper panel: FBS sources. In both panels, the dotted lines correspond to J-K = 1 and J-K = 2.
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$\begin{figure} \par\includegraphics[angle=-90,width=7.7cm,clip]{6014f009.ps}\end{figure}$	Figure 5: Difference between J(DENIS) and J(2MASS) plotted as a function of the J-K colour index of 2MASS.
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$\begin{figure} \par\resizebox{7.8cm}{!}{\rotatebox{-90}{\includegraphics{6014f010.eps}}}\end{figure}$	Figure 6: Proper motions of 402 HES objects, with $\mu_{\alpha} \cos~(\delta)$ in abscissa and $\mu _{\delta }$ in ordinates. Circles with an overplotted cross correspond to cases where $\mu$ is larger than 30 mas yr^-1 and where the motion in $\alpha$ or $\delta$ is detected with at least a 3 $\sigma$ quality.
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