![\begin{figure}
\par\includegraphics[angle=90,width=8cm,clip]{9143fig1.ps}
\end{figure}](/articles/aa/full/2008/16/aa9143-07/img17.gif) |
Figure 1:
Finding chart for OGLE-TR-211. Size of the I-band
OGLE subframe is
 ,
North is up and East to the left. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=7.4cm,clip]{9143fig2.eps}
\end{figure}](/articles/aa/full/2008/16/aa9143-07/img20.gif) |
Figure 2: Upper panel: OGLE light curve of OGLE-TR-211, lower panel: VLT observations. The continuous line represents the best model of the transit. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=7.7cm,clip]{9143fig3.eps}
\end{figure}](/articles/aa/full/2008/16/aa9143-07/img25.gif) |
Figure 3: Upper panel: radial velocity observations for OGLE-TR-211, phased with the photometric transit ephemeris. Solid line represents the best fit assuming no eccentricity. Two periods are presented for clarity. Lower panel: bisector span values plotted as a function of phase for testing blending scenarios. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=7.9cm,clip]{9143fig4.ps}
\end{figure}](/articles/aa/full/2008/16/aa9143-07/img54.gif) |
Figure 4:
Mass-radius diagram for transiting hot Jupiters
(0.5-1.5  ). Closed symbols indicate host stars with
 K. OGLE-TR-211 is indicated by the circled dot. The lines
show the models of Guillot (2005) in two extreme cases: cold gas planet
with a
core and
 K planet without a core.
The six large planets with radius error bars above the upper models are
all strongly irradiated. |
| Open with DEXTER | |
In the text