Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{Gc191_f1.eps} \end{figure}$ Figure 1: I-band image of the field of HG 031203. North is up, east to the left; the image is 2 $^\prime$ on a side. The positions of the host galaxy and of the comparison stars are noted. Blooming from a bright star, (outside this image) is visible as a N-S streak and a ring caused by reflection is evident just to the southeast of HG 031203.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Gc191_f2.eps} \end{figure}$ Figure 2: The I-band lightcurve of HG 031203 (uncorrected for extinction). The characteristic supernova "bump'' is apparent. The reddened ( A_I = 2.14 mag) and scaled (-0.55 mag) intrinsic lightcurve of SN1998bw, with the flux of the galaxy ( $I_{\rm host} = 19.27$ ) added, is plotted for comparison, starting at the time of the XRF (solid line) and starting two days prior to the XRF (scaled by -0.6 mag, dashed line). The brightened SN1998bw lightcurve is quite an accurate template for the data.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{Gc191_f1.eps} \end{figure}$	Figure 1: I-band image of the field of HG 031203. North is up, east to the left; the image is 2 $^\prime$ on a side. The positions of the host galaxy and of the comparison stars are noted. Blooming from a bright star, (outside this image) is visible as a N-S streak and a ring caused by reflection is evident just to the southeast of HG 031203.
Open with DEXTER