All Figures

$\begin{figure} \par\includegraphics[width=7.75cm,clip]{6660fig1.eps}\end{figure}$ Figure 1: Multiwavelength light curve of the GRB 050408 afterglow in the observer frame. The lines show the best fit of a fireball model with one energy injection (at 2.9 days) seen off-axis (see text for details). Our observations are plotted with filled symbols, while the ones obtained from the literature are represented by empty ones, this convention is used for all the figures.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{6660fig2.eps}\end{figure}$ Figure 2: Spectral flux distribution of the afterglow 0.6 days after the burst onset in the observer frame. The different lines represent results from fitting the data to various extinction laws: Small Magellanic Cloud (SMC), Large Magellanic Cloud (LMC), Milky Way (MW) and No Extinction (NE).
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In the text

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{6660fig3.eps}\end{figure}$ Figure 3: Spectral Flux Distribution of the afterglow from radio to X-rays 0.6, 6.0 and 13.0 days after the burst in the observer frame. Several 3- $\sigma$ upper limits from radio and millimetre observations are plotted.
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In the text

$\begin{figure} \par\includegraphics[width=7.4cm,clip]{6660fig4.eps} \end{figure}$ Figure A.1: Identification chart of GRB 050408. The calibration stars and the afterglow location have been marked. The field of view is 6.0' $\times$ 6.5', North is to the top and East to the left.

In the text

$\begin{figure} \par\includegraphics[width=7.75cm,clip]{6660fig1.eps}\end{figure}$	Figure 1: Multiwavelength light curve of the GRB 050408 afterglow in the observer frame. The lines show the best fit of a fireball model with one energy injection (at 2.9 days) seen off-axis (see text for details). Our observations are plotted with filled symbols, while the ones obtained from the literature are represented by empty ones, this convention is used for all the figures.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{6660fig2.eps}\end{figure}$	Figure 2: Spectral flux distribution of the afterglow 0.6 days after the burst onset in the observer frame. The different lines represent results from fitting the data to various extinction laws: Small Magellanic Cloud (SMC), Large Magellanic Cloud (LMC), Milky Way (MW) and No Extinction (NE).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{6660fig3.eps}\end{figure}$	Figure 3: Spectral Flux Distribution of the afterglow from radio to X-rays 0.6, 6.0 and 13.0 days after the burst in the observer frame. Several 3- $\sigma$ upper limits from radio and millimetre observations are plotted.
Open with DEXTER