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Comparison of the resolving power (for point sources)
of the high resolution spectrometers on the X-ray telescopes
CHANDRA, XMM-NEWTON, and SODART. For XMM, curves are shown
for the RGS2 only, the better one of the two grating sets.
To avoid confusion, the CHANDRA-LEG curves are shown in the
low-energy region only (<0.4 keV), although they can be used
in the whole energy region (<10 keV). The dotted parts of the
SODART curves indicate energy regions, where the Bragg
spectrometer can still work, but its efficiency drops down
due to a very large or very small Bragg angle.
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