![\begin{figure}
\par\includegraphics[width=7.5cm,clip]{Gl071_f1.eps}
\end{figure}](/articles/aa/full/2005/09/aagl071/img14.gif) |
Figure 1:
The WSRT 1.4 GHz contour map superimposed upon an HST F702W image
of the region of sky associated with SMM J16359+6612. Radio
emission from all three lensed images (SMM-A, SMM-B and SMM-C) is
detected by the WSRT. The boxes represent the SCUBA source
positions. Radio emission from three other SCUBA sources in the
field (including the highly magnified arclet #289,
SMM J16359+66118) are also boxed. Contours are
drawn at -3, 3, 5, 10, 20 and 40 times the 1-
noise level of 15 microJy/beam. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=7.5cm,clip]{Gl071_f2.eps}
\end{figure}](/articles/aa/full/2005/09/aagl071/img17.gif) |
Figure 2:
The VLA 8.2 GHz contour map superimposed upon an HST F702W image
of the region of sky associated with SMM J16359+6612F702W. Radio
emission from all three lensed images is detected by the WSRT.
The boxes represent the SCUBA source positions. Radio emission
from the highly magnified arclet (#289), SMM J16359+66118 is also
detected. Contours are drawn at -3, 3, 4, 7 and 10 times the
1-
noise level of 6 microJy/beam. |
| Open with DEXTER | |
In the text