XMM Users' Handbook


next up previous contents
Next: Count rate conversion from Up: RGS specific proposal submission Previous: RGS spectral quality

   
RGS flux to count rate conversion

Figs. 63-65 provide RGS flux to count rate conversion factors for a variety of standard spectral models. Families of curves for various values of the foreground absorbing column density, NH, are plotted. Fluxes and count rates are calculated for the 0.3-2.0 keV band; fluxes are unabsorbed values. All calculations are performed for the -1. grating order.


  
Figure 63: RGS flux to count rate conversion factors for various power law spectra and different values for the absorbing column density, NH. All numbers were obtained for the -1. grating order only.
\begin{figure}
\begin{center}
\leavevmode
\epsfig{width=0.6\hsize, angle=270, file=figs/rgsfluxtocr_pl.eps}
\end{center} \end{figure}


  
Figure 64: RGS flux to count rate conversion factors for various black body spectra and different values for the absorbing column density, NH. All numbers were obtained for the -1. grating order only.
\begin{figure}
\begin{center}
\leavevmode
\epsfig{width=0.6\hsize, angle=270, file=figs/rgsfluxtocr_bb.eps}
\end{center} \end{figure}


  
Figure 65: RGS flux to count rate conversion factors for various Mekal thermal plasma spectra and different values for the absorbing column density, NH. All numbers were obtained for the -1. grating order only.
\begin{figure}
\begin{center}
\leavevmode
\epsfig{width=0.6\hsize, angle=270, file=figs/rgsfluxtocr_rs.eps}
\end{center} \end{figure}


next up previous contents
Next: Count rate conversion from Up: RGS specific proposal submission Previous: RGS spectral quality
European Space Agency - XMM Science Operations Centre