$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics{bul24_1609_Ks_54276.492... ...\resizebox{8.8cm}{!}{\includegraphics{bul39_5385_Ks_54276.57204.ps}}\end{figure}$ Figure 2: The difference between SOFI instrumental magnitude and 2MASS magnitude versus instrumental magnitude for a single epoch for two different objects. The symbols indicate different 1 mag bins in 2MASS magnitude.
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In the text

$\begin{figure} \par\includegraphics[width=90mm,clip]{PL_raw_RRL_paper.ps}\end{figure}$ Figure 6: The K-band PL-relation for the RR Lyrae stars in the GB. The line is a best fit excluding the outliers labelled in Table 2 which fall outside the plot. The dotted line is the fit for a fixed slope of -2.38.
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In the text

$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics{bul_sc24_1609.ps}}\par\resizebox{8.8cm}{!}{\includegraphics{bul_sc39_5385.ps}}\end{figure}$	Figure 1: Phased OGLE I-band light curves of two of the P2C. The periods of the two stars are 0.76522 (bul_sc24_1609) and 9.94431 (bul_sc39_5385) days.
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$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics{bul24_1609_Ks_54276.492... ...\resizebox{8.8cm}{!}{\includegraphics{bul39_5385_Ks_54276.57204.ps}}\end{figure}$	Figure 2: The difference between SOFI instrumental magnitude and 2MASS magnitude versus instrumental magnitude for a single epoch for two different objects. The symbols indicate different 1 mag bins in 2MASS magnitude.
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$\begin{figure} \par\mbox{\resizebox{8.8cm}{!}{\includegraphics{bul24_1609_ILC.ps}}\resizebox{8.8cm}{!}{\includegraphics{bul39_5385_ILC.ps}} } \end{figure}$	Figure 3: The K-band light curves of two P2C. The top panel shows the magnitude versus time, the bottom panel the phased light curve.
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$\begin{figure} \par\mbox{\resizebox{8.8cm}{!}{\includegraphics{RRL40_259253_ILC.ps}}\resizebox{8.8cm}{!}{\includegraphics{RRL4_207388_ILC.ps}} } \end{figure}$	Figure 4: The K-band light curves of two RR Lyrae. The top panel shows the magnitude versus time, the bottom panel the phased light curve.
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$\begin{figure} \par\includegraphics[width=90mm]{PL_raw_PAPER.ps}\end{figure}$	Figure 5: The K-band PL-relation for P2C in the GB. The line is a best fit excluding the cross.
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$\begin{figure} \par\includegraphics[width=90mm,clip]{PL_raw_RRL_paper.ps}\end{figure}$	Figure 6: The K-band PL-relation for the RR Lyrae stars in the GB. The line is a best fit excluding the outliers labelled in Table 2 which fall outside the plot. The dotted line is the fit for a fixed slope of -2.38.
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