All Figures

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{figuras/2898fig1.ps}\protect \end{figure}$ Figure 1: Reference stars in the surroundings of the GRB 021004 location (bracketed into tick marks). The depicted field of view is $4.3' \times 4.0'$ .
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In the text

$\begin{figure} \par {\hspace*{2mm}\includegraphics[width=7.8cm,clip]{figuras/289... ...ps} } {\includegraphics[width=7.65cm,clip]{figuras/2898fg2b.ps} }\end{figure}$ Figure 2: a) Optical and NIR light curves of GRB 021004 for the first $\sim$ 500 days after the event. The different bands have been intentionally separated for clarity. Our observations are marked with filled symbols while published data are represented with void ones (see text for references). b) Millimetre light curves for the first $\sim$ 35 days, obtained at PdB.
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In the text

$\begin{figure} \par {\includegraphics[width=12.3cm,clip]{figuras/2898fig3.eps} }\end{figure}$ Figure 3: Multiband light curves from radio to X-rays (for the time interval 0.01-250 days after the burst onset) fitted with the multiple energy injection model. Seven energy injection episodes (see Table 5), indicated by vertical lines, can account for the observed behaviour. The visible and NIR observations are corrected for extinction and the U-band also for Lyman- $\alpha$ blanketing.
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In the text

$\begin{figure} \par {\includegraphics[width=8.8cm]{figuras/2898fig4.ps} }\end{figure}$ Figure 4: Evolution of the GRB 021004 afterglow SFDs at 0.8 (diamonds), 6 (triangles) and 60 days (squares) after the burst.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm]{figuras/2898fig5.ps}\protect \end{figure}$ Figure 5: A fit to the photometric points of the GRB 021004 host galaxy yielding a starburst galaxy template. The H-band limit of 21.5 magnitude ( $\sim$ $2.7~\mu$ Jy) is not plotted. The filled points are our observations while the open ones are obtained from the fit of the galaxy. The flux density is represented in logarithmic scale.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{figuras/2898fig1.ps}\protect \end{figure}$	Figure 1: Reference stars in the surroundings of the GRB 021004 location (bracketed into tick marks). The depicted field of view is $4.3' \times 4.0'$ .
Open with DEXTER

$\begin{figure} \par {\hspace*{2mm}\includegraphics[width=7.8cm,clip]{figuras/289... ...ps} } {\includegraphics[width=7.65cm,clip]{figuras/2898fg2b.ps} }\end{figure}$	Figure 2: a) Optical and NIR light curves of GRB 021004 for the first $\sim$ 500 days after the event. The different bands have been intentionally separated for clarity. Our observations are marked with filled symbols while published data are represented with void ones (see text for references). b) Millimetre light curves for the first $\sim$ 35 days, obtained at PdB.
Open with DEXTER

$\begin{figure} \par {\includegraphics[width=12.3cm,clip]{figuras/2898fig3.eps} }\end{figure}$	Figure 3: Multiband light curves from radio to X-rays (for the time interval 0.01-250 days after the burst onset) fitted with the multiple energy injection model. Seven energy injection episodes (see Table 5), indicated by vertical lines, can account for the observed behaviour. The visible and NIR observations are corrected for extinction and the U-band also for Lyman- $\alpha$ blanketing.
Open with DEXTER

$\begin{figure} \par {\includegraphics[width=8.8cm]{figuras/2898fig4.ps} }\end{figure}$	Figure 4: Evolution of the GRB 021004 afterglow SFDs at 0.8 (diamonds), 6 (triangles) and 60 days (squares) after the burst.
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$\begin{figure} \par\includegraphics[width=8.8cm]{figuras/2898fig5.ps}\protect \end{figure}$	Figure 5: A fit to the photometric points of the GRB 021004 host galaxy yielding a starburst galaxy template. The H-band limit of 21.5 magnitude ( $\sim$ $2.7~\mu$ Jy) is not plotted. The filled points are our observations while the open ones are obtained from the fit of the galaxy. The flux density is represented in logarithmic scale.
Open with DEXTER