$\begin{figure} \par\includegraphics[width=8.4cm,clip]{aa4288f1.eps}\end{figure}$ Figure 1: Finding chart for the 2 stars observed in HP-1 (NTT-SUSI V image). The frame size is $2.2\times 2.2$ arcmin, and the resolution is 0.13 arcsec/px.
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In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{aa4288f2.eps}\end{figure}$ Figure 2: The NTT-SUSI V vs. V-I CMD of HP-1 with the target stars (they are almost coincident) indicated.
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In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{aa4288f1.eps}\end{figure}$	Figure 1: Finding chart for the 2 stars observed in HP-1 (NTT-SUSI V image). The frame size is $2.2\times 2.2$ arcmin, and the resolution is 0.13 arcsec/px.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{aa4288f2.eps}\end{figure}$	Figure 2: The NTT-SUSI V vs. V-I CMD of HP-1 with the target stars (they are almost coincident) indicated.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{aa4288f3.eps}\end{figure}$	Figure 3: The WFI V vs. V-I CMD of HP-1. Size of extraction is $5'\times 5'$ .
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$\begin{figure} \par\includegraphics[width=12cm,clip]{aa4288f4.ps}\end{figure}$	Figure 4: The WFI and NTT data used to establish proper motion cleaning of the field.
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$\begin{figure} \par\includegraphics[width=8.1cm,clip]{aa4288f5.eps}\end{figure}$	Figure 5: CaI 6169.044 and 6169.564 Å lines shown for the solar, Arcturus, and HP1-2 spectra.
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$\begin{figure} \par\includegraphics[width=8.2cm,clip]{aa4288f6.eps}\end{figure}$	Figure 6: CaI 6471.668 Å line shown for the solar, Arcturus, and HP1-2 spectra.
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$\begin{figure} \par\includegraphics[width=8.2cm,clip]{aa4288f7.eps}\end{figure}$	Figure 7: CaI 6499.654 Å line shown for the solar, Arcturus, and HP1-2 spectra.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{aa4288f8.eps}\end{figure}$	Figure 8: CaI 6717.687 Å line shown for the solar, Arcturus, and HP1-2 spectra.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{aa4288f9.eps}\end{figure}$	Figure 9: SiI 6237.328 Å line shown for the solar, Arcturus, and HP1-2 spectra.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{aa4288f10.eps}\end{figure}$	Figure 10: TiII 6491.58 Å line shown for the solar, Arcturus, and HP1-2 spectra.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{aa4288f11.eps}\end{figure}$	Figure 11: MgI 6318.72, 6319.24, 6319.45 Å lines shown for the solar, HP1-2 and HP1-3 spectra.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{aa4288f12.eps}\end{figure}$	Figure 12: EuII 6645.127 Å line shown for the Arcturus, HP1-2 and HP1-3 spectra.
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