![\begin{figure}
\par\includegraphics[width=6cm,clip]{Fd302_f1.ps}
\end{figure}](/articles/aa/full/2003/30/aafd302/img12.gif) |
Figure 1:
A  arcsec2 section of the STIS/CL image around
the host galaxy of GRB 011211 (Jakobsson et al. 2003b). North is up and
East is to the left. The GRB went off in the faint, southern part of the
object (position marked with a cross). The contours show the Ly emission based on our narrow band observations. The Ly emission
weighted centroid of the galaxy is close to the northern knot seen in the
STIS image. |
| Open with DEXTER | |
In the text
 |
Figure 2:
Left panel:
calculated colour-colour diagram based on Bruzual &
Charlot (1993) model galaxy spectra.
The filled squares are 0<z<0.6 galaxies with ages from a
few to 15 Gyr and the open triangles are
0.3<z< 3.0 galaxies
with ages from a few Myr to 1 Gyr. The dotted box contains all these
calculated galaxy colours. The full-drawn line corresponds to
objects having the same broad-band colours, but various amounts of
absorption (upper part) or emission (lower part) in the narrow-band filter.
Middle panel:
colour-colour diagram for all objects in the GRB field. The
squares with error-bars indicate objects detected at S/N>5 in the
narrow-band image. As expected, most objects have colours consistent
with being in the dotted box. However, a number of objects, including
the GRB 011211 host, are seen in the lower left part of the diagram.
Right panel: the colours of the seven LEGO candidates which are
selected to have
 .
|
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=13.4cm,clip]{Fd302_f5.eps}
\end{figure}](/articles/aa/full/2003/30/aafd302/img16.gif) |
Figure 3:
 arcsec2 sections around each of the seven LEGO candidates from the narrow band (top row), B-band (middle row) and R-band
(bottom row). North is up and East is to the left. The host galaxy is
number six named S1211_6. |
| Open with DEXTER | |
In the text