All Figures

$\begin{figure} \par\includegraphics[angle=-90,width=7.8cm,clip]{0128fg01.eps}\hs... ...ce*{3mm} \includegraphics[angle=-90,width=7.8cm,clip]{0128fg08.eps} \end{figure}$ Figure 1: Best fit models and residuals for all the sources of the sample. See the notes on individual objects for details.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.9cm,clip]{0128fg09.eps}\pa... ...ce*{3mm} \includegraphics[angle=-90,width=7.9cm,clip]{0128fg10.eps} \end{figure}$ Figure 2: ESO198-G24: EPIC pn spectra around the iron line energy for the two segments of the simultaneous observation. In addition to the 6.4 keV neutral iron line, note the presence of the feature around 6 keV only in the second half of the observation (see text for details).
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.6cm,clip]{0128fg11.eps} \end{figure}$ Figure 3: IC 4329A: the Chandra HEG spectrum around the iron line.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.7cm,clip]{0128fg12.eps}\hs... ...ce*{3mm} \includegraphics[angle=-90,width=7.7cm,clip]{0128fg19.eps} \end{figure}$ Figure 4: Best fit models and residuals around the iron line energy for all the sources of the sample. Note that the spectra are corrected for the redshift of the sources. See the notes on individual objects for details.
Open with DEXTER

In the text