Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[angle=90,width=8.1cm,clip]{0507fig1.ps} \end{figure}$ Figure 1: Periodogram of the Sierra Nevada data. The highest peak corresponds to 3.04 cycles per day or approximately 7.89 h.
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In the text

$\begin{figure} \par\includegraphics[width=8.3cm,height=8.6cm,clip,angle=90]{0507... ...degraphics[width=8.3cm,height=8.6cm,clip,angle=90]{0507fig3.ps} \par\end{figure}$ Figure 2: Left: lightcurve of 2002 TX₃₀₀ phased to a rotation period of 7.89762 h. The bottom plot corresponds to the raw Sierra Nevada data, with different symbols for the different dates of observation. A sinusoidal fit has been superimposed. The upper plot corresponds to the median of the Sierra Nevada data, in small phase bins. The middle plot shows the median of the Sierra Nevada data (triangles) as well as the NOT data (diamonds) and the CFHT data (squares). Right: same but for a rotation period of 15.7942 h.
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In the text

$\begin{figure} \par\includegraphics[width=8.3cm,height=8.8cm,clip,angle=90,]{0507fig4.ps} \end{figure}$ Figure 3: BVRI magnitudes obtained from CFHT data. Asterisks represent the B data, diamonds correspond to V, triangles correspond to R data and squares correspond to I data.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=8.1cm,clip]{0507fig1.ps} \end{figure}$	Figure 1: Periodogram of the Sierra Nevada data. The highest peak corresponds to 3.04 cycles per day or approximately 7.89 h.
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$\begin{figure} \par\includegraphics[width=8.3cm,height=8.8cm,clip,angle=90,]{0507fig4.ps} \end{figure}$	Figure 3: BVRI magnitudes obtained from CFHT data. Asterisks represent the B data, diamonds correspond to V, triangles correspond to R data and squares correspond to I data.
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