![\begin{figure}
\par\includegraphics[width=7.5cm,clip]{5456fig1.eps}
\end{figure}](/articles/aa/full/2006/35/aa5456-06/img22.gif) |
Figure 1:
Upper panel: the RXTE/PCA light curve of Swift J1922.7-1716
in the 3-15 keV energy band observed from 53 664.37 to 53 664.44 MJD.
Lower panel: the power density spectrum in
form. The best fit Lorentzian models are also shown. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[angle=-90,width=8cm,clip]{5456fig2.ps}
\end{figure}](/articles/aa/full/2006/35/aa5456-06/img90.gif) |
Figure 2: The unfolded spectrum of Swift J1922.7-1716 fitted with an absorbed disc blackbody, DBB, plus COMPTT model. The data points correspond to the two XRT (0.5-7 keV), the PCA (4-22 keV), and the ISGRI (20-100 keV) spectra, respectively. The DBB model is shown by a dotted curve, the dashed curve gives the COMPTT model, while the total spectrum is shown by a solid curve. The lower panel presents the residuals between the data and the model. |
| Open with DEXTER | |
In the text