Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{0924-f1.eps} \end{figure}$ Figure 1: The infrared light curve of Sagittarius A* on 3 June 2008. The data are represented by vertical red bars ( $\pm$ 1 $\sigma$ ) and a black connection line between them. Upper panel: L'-band flare events. For a better representation we added a constant value of 50 mJy to the light curve for the reference star. Lower panel: the K-band flare emission immediately following the L'-band observations. In this case no offset was added to the light curve for the reference star.
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In the text

$\begin{figure} \par\includegraphics[width=16.5cm,clip]{0924-f2.eps} \end{figure}$ Figure 2: Left: Sagittarius A* at the beginning and the peak of the APEX measurements. Right: a section of the larger map of the Galactic center. The location of Sagittarius A* is indicated by a circle. Sagittarius A* has been subtracted out as this map is used as a reference for the extended structure. The colors code the flux density in Janskys.
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{0924-f3.eps} \end{figure}$ Figure 3: The sub-mm light curve of Sagittarius A* on 3 June 2008. The data are represented by vertical red bars ( $\pm$ 1 $\sigma$ in length) and a black connection line between them.
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{APEXmodels.eps} %\end{figure}$ Figure 4: The infrared ( top) and sub-mm ( bottom) light curve of Sagittarius A*. The data are represented by vertical red bars ( $\pm$ 1 $\sigma$ ) and a black connection line between them. The dashed line represents a smoothed version of the data (after application of a 7 point sliding average for all data points exept the first). The models as described in the text and in Table 4 (blue, black, red for models A, B, C, respectively) are shown as solid lines (blue: $\sim$ 2.5 THz; black: $\sim$ 2 THz; red: $\sim$ 1 THz cutoff frequency in the source component spectra).
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{APEXmodel-B.eps} %\end{figure}$ Figure 5: Our favored model B compared to the infrared ( top) and sub-mm ( bottom) light curve of Sagittarius A*. The data are represented by vertical red bars ( $\pm$ 1 $\sigma$ ) and a black connection line between them. For furher explanation see caption of Fig. 4.
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In the text

$\begin{figure} \par\includegraphics[width=16.5cm,clip]{0924-f2.eps} \end{figure}$	Figure 2: Left: Sagittarius A* at the beginning and the peak of the APEX measurements. Right: a section of the larger map of the Galactic center. The location of Sagittarius A* is indicated by a circle. Sagittarius A* has been subtracted out as this map is used as a reference for the extended structure. The colors code the flux density in Janskys.
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$\begin{figure} \par\includegraphics[width=7.5cm,clip]{0924-f3.eps} \end{figure}$	Figure 3: The sub-mm light curve of Sagittarius A* on 3 June 2008. The data are represented by vertical red bars ( $\pm$ 1 $\sigma$ in length) and a black connection line between them.
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$\begin{figure} \par\includegraphics[width=7.5cm,clip]{APEXmodel-B.eps} %\end{figure}$	Figure 5: Our favored model B compared to the infrared ( top) and sub-mm ( bottom) light curve of Sagittarius A*. The data are represented by vertical red bars ( $\pm$ 1 $\sigma$ ) and a black connection line between them. For furher explanation see caption of Fig. 4.
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