XMM-Newton Users' Handbook

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Next: 3.7.1.2 Non-dispersive spectroscopy: an example Up: 3.7.1 A comparison of XMM-Newton vs. Chandra Previous: 3.7.1 A comparison of XMM-Newton vs. Chandra


3.7.1.1 Effective area for dispersive spectroscopy

Fig. 97 displays the effective area of both RGS units together (from Fig. 68), compared with different Chandra instrument combinations. In order to avoid overcrowding the figure, the combination of Chandra HRC+LETG is not shown.

Figure 97: The effective area of both RGS units combined and RGS-1 (linear scale), compared with Chandra's ACIS-S instrument with various transmission gratings. Please note that since early after the beginning of the mission CCD7 in RGS1 and CCD4 in RGS2 are inoperative (see Table 9), thus the effective area in each of the mentioned CCD energy range is reduced by a factor of 2.
\begin{figure}\begin{center} \leavevmode \epsfig{height=0.56\hsize, file=figs/xmm_vs_axaf_specarea.eps} \end{center} \end{figure}


European Space Agency - XMM-Newton Science Operations Centre