$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics{ms3755f1.ps}}\end{figure}$ Figure 1: Comparison of the V magnitudes and B-V colors derived here with the photometry of Olszewski et al. (1987). The comparison is in the sense of this work minus Olszewski et al. (1987).
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In the text

$\begin{figure} \par\resizebox{13cm}{!}{\includegraphics{ms3755f2.ps}}\end{figure}$ Figure 2: The (B-V,V) color-magnitude diagram for Lindsay 1 + field stars within $210\hbox {$^{\prime \prime }$ }$ (left panel). The field CMD (right panel) is based on all stars in the area with the same radius outside the cluster.
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In the text

$\begin{figure} \par\resizebox{13cm}{!}{\includegraphics{ms3755f3.ps}} \end{figure}$ Figure 3: The (B-V, V) and (V-I, I) CMDs for Lindsay 1. Candidate AGB stars are represented by filled circles. (B-V, V) and (V-I, I) ridgelines are also shown.
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In the text

$\begin{figure} \par\resizebox{8cm}{!}{\includegraphics{ms3755f6.ps}} \end{figure}$ Figure 6: The observed differential (top) and integrated (bottom) luminosity function for the Lindsay 1 RGB.
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In the text

$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics{ms3755f1.ps}}\end{figure}$	Figure 1: Comparison of the V magnitudes and B-V colors derived here with the photometry of Olszewski et al. (1987). The comparison is in the sense of this work minus Olszewski et al. (1987).
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$\begin{figure} \par\resizebox{13cm}{!}{\includegraphics{ms3755f2.ps}}\end{figure}$	Figure 2: The (B-V,V) color-magnitude diagram for Lindsay 1 + field stars within $210\hbox {$^{\prime \prime }$ }$ (left panel). The field CMD (right panel) is based on all stars in the area with the same radius outside the cluster.
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$\begin{figure} \par\resizebox{13cm}{!}{\includegraphics{ms3755f3.ps}} \end{figure}$	Figure 3: The (B-V, V) and (V-I, I) CMDs for Lindsay 1. Candidate AGB stars are represented by filled circles. (B-V, V) and (V-I, I) ridgelines are also shown.
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$\begin{figure} \par\resizebox{8cm}{!}{\includegraphics{ms3755f4.ps}} \end{figure}$	Figure 4: The (U-V, U) CMD for Lindsay 1. Candidate AGB stars are presented with filled circles.
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$\begin{figure} \par\resizebox{8.5cm}{!}{\includegraphics{ms3755f5.ps}} \end{figure}$	Figure 5: The (J-K, K) and (V-K, K) CMDs for the brightest RGB stars in Lindsay 1.
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$\begin{figure} \par\resizebox{8cm}{!}{\includegraphics{ms3755f6.ps}} \end{figure}$	Figure 6: The observed differential (top) and integrated (bottom) luminosity function for the Lindsay 1 RGB.
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