$\begin{figure} \par\includegraphics[width=8.5cm,clip]{7535fig1.eps}\end{figure}$ Figure 1: A part of the observed spectrum towards Orion KL after 31 h of on-source integration. The noise level is $\sigma =2.7$ mK. The expected position of one of the vinyl acetylene lines is marked (C₂H₃ CCH), as well as identifications of other detected lines.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{7535fig1.eps}\end{figure}$	Figure 1: A part of the observed spectrum towards Orion KL after 31 h of on-source integration. The noise level is $\sigma =2.7$ mK. The expected position of one of the vinyl acetylene lines is marked (C₂H₃ CCH), as well as identifications of other detected lines.
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