$\begin{figure} \par\includegraphics[width=17.9cm,clip]{Hi071_f1.ps} \end{figure}$ Figure 1: R-band image of the field of GRB 050709, on 2005 Jul. 12.41 (A) and 20.42 (B). Panel C shows the result of the subtraction, evidencing a fading source coincident with the Chandra counterpart (circle). The boxes cover a region $30\hbox {$^{\prime \prime }$ }\times 20\hbox {$^{\prime \prime }$ }$ wide.
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In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{Hi071_f2.ps} \end{figure}$ Figure 2: Broad-band spectral energy distribution of the afterglow of GRB 050709 on Jul. 12.4 UT. The bow-tie shaped region represent the simultaneous X-ray spectrum taken from Chandra (Fox et al. 2005b). The dot-dashed and dotted lines indicate the extrapolation of the optical and X-ray spectra, respectively.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{Hi071_f3.ps} \end{figure}$ Figure 3: Details of the GRB 050709 host galaxy spectrum close to the H $\alpha$ and H $\beta$ lines, showing that the narrow emission emissions are superimposed on wider absorption features.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Hi071_f4.eps} \end{figure}$ Figure 4: Light curve of the GRB 050709 afterglow (points), compared to those of several SNe (R band). Zero extinction is assumed at the GRB site.
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In the text

$\begin{figure} \par\includegraphics[width=17.9cm,clip]{Hi071_f1.ps} \end{figure}$	Figure 1: R-band image of the field of GRB 050709, on 2005 Jul. 12.41 (A) and 20.42 (B). Panel C shows the result of the subtraction, evidencing a fading source coincident with the Chandra counterpart (circle). The boxes cover a region $30\hbox {$^{\prime \prime }$ }\times 20\hbox {$^{\prime \prime }$ }$ wide.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{Hi071_f2.ps} \end{figure}$	Figure 2: Broad-band spectral energy distribution of the afterglow of GRB 050709 on Jul. 12.4 UT. The bow-tie shaped region represent the simultaneous X-ray spectrum taken from Chandra (Fox et al. 2005b). The dot-dashed and dotted lines indicate the extrapolation of the optical and X-ray spectra, respectively.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{Hi071_f3.ps} \end{figure}$	Figure 3: Details of the GRB 050709 host galaxy spectrum close to the H $\alpha$ and H $\beta$ lines, showing that the narrow emission emissions are superimposed on wider absorption features.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Hi071_f4.eps} \end{figure}$	Figure 4: Light curve of the GRB 050709 afterglow (points), compared to those of several SNe (R band). Zero extinction is assumed at the GRB site.
Open with DEXTER