$\begin{figure} \par\includegraphics[width=7.6cm,clip]{3841fig1.eps}\end{figure}$ Figure 1: R light curve of BL Cam observed on October 13, 2003 at Château-Renard Observatory. $\Delta R$ means magnitude differences variable minus comparison star.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{3841fig2.ps}\end{figure}$ Figure 2: Power spectra of BL Cam corresponding to the 1999 data set collected by Zhou et al. (2001). Panels: 1) residuals after removing f₀, 2f₀ and 3f₀, 2) same after removing f₀-f₃, 3) same after removing f₀-f₅ and 4) same after removing f₀-f₇.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{3841fig4.eps}\end{figure}$ Figure 4: O-C diagram for BL Cam. Bottom: O-C values (dots) together with the synthetic curve (solid line) using the parameters of the binary system given in Table 9. Top: residuals from the fitting.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{3841fig1.eps}\end{figure}$	Figure 1: R light curve of BL Cam observed on October 13, 2003 at Château-Renard Observatory. $\Delta R$ means magnitude differences variable minus comparison star.
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$\begin{figure} \par\includegraphics[width=7.3cm,clip]{3841fig2.ps}\end{figure}$	Figure 2: Power spectra of BL Cam corresponding to the 1999 data set collected by Zhou et al. (2001). Panels: 1) residuals after removing f₀, 2f₀ and 3f₀, 2) same after removing f₀-f₃, 3) same after removing f₀-f₅ and 4) same after removing f₀-f₇.
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$\begin{figure} \par\includegraphics[width=7.6cm,clip]{3841fig3.eps}\end{figure}$	Figure 3: O-C diagram for BL Cam using the ephemeris of Zhou et al. (1999, Eq. (2)).
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$\begin{figure} \par\includegraphics[width=7.6cm,clip]{3841fig4.eps}\end{figure}$	Figure 4: O-C diagram for BL Cam. Bottom: O-C values (dots) together with the synthetic curve (solid line) using the parameters of the binary system given in Table 9. Top: residuals from the fitting.
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