$\begin{figure} \includegraphics[width=8.8cm,clip]{figure1.eps} \end{figure}$ Figure 1: Receiver stability. Over a period of 24 hours of integration, the noise keeps decreasing steadily.
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In the text

$\begin{figure} \includegraphics[angle=270,width=8.8cm,clip]{odin_11_f2.eps} \end{figure}$ Figure 2: O₂ spectra with unscaled C¹⁸O spectra. The noise peaks at source velocity are 1.5 $\sigma$ (L134N) and 2.5 $\sigma$ (Orion A). The horizontal axis is LSR velocity in km s^-1, the vertical axis, $T_{\rm A}$ in K (uncorrected for beam efficiency).
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=7cm,clip]{odin_11_f3.eps} \end{figure}$ Figure 3: The SWAS and Odin beams towards $\rho$ Oph A. The dashed circle represents the SWAS central beam, not taken into account in their detection (Goldsmith et al. 2002).
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In the text

$\begin{figure} \includegraphics[angle=270,width=8.8cm,clip]{odin_11_f4.eps} \end{figure}$ Figure 4: Smoothed $\rho$ Oph A O₂ spectrum, with the signal expected at 119 GHz from the SWAS O₂ column density estimate superimposed. Axes are the same as in Fig. 2.
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In the text

$\begin{figure} \includegraphics[width=8.8cm,clip]{figure1.eps} \end{figure}$	Figure 1: Receiver stability. Over a period of 24 hours of integration, the noise keeps decreasing steadily.
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$\begin{figure} \includegraphics[angle=270,width=8.8cm,clip]{odin_11_f2.eps} \end{figure}$	Figure 2: O₂ spectra with unscaled C¹⁸O spectra. The noise peaks at source velocity are 1.5 $\sigma$ (L134N) and 2.5 $\sigma$ (Orion A). The horizontal axis is LSR velocity in km s^-1, the vertical axis, $T_{\rm A}$ in K (uncorrected for beam efficiency).
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$\begin{figure} \par\includegraphics[angle=270,width=7cm,clip]{odin_11_f3.eps} \end{figure}$	Figure 3: The SWAS and Odin beams towards $\rho$ Oph A. The dashed circle represents the SWAS central beam, not taken into account in their detection (Goldsmith et al. 2002).
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$\begin{figure} \includegraphics[angle=270,width=8.8cm,clip]{odin_11_f4.eps} \end{figure}$	Figure 4: Smoothed $\rho$ Oph A O₂ spectrum, with the signal expected at 119 GHz from the SWAS O₂ column density estimate superimposed. Axes are the same as in Fig. 2.
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