XMM-Newton
Users Handbook
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The wavelength scale is determined by the relative alignment of the
various instruments and their structural stability.
Fig. 67 shows the residuals of the RGS measured
versus nominal positions for certain emission lines and a set of
observations of coronal sources. Residuals from first order spectra
are indicated in the top panel. For an on-axis source, the wavelength
scale accuracy is 7 mÅ (1). This accuracy can probably be
improved in the future. It has been verified that the wavelength scale
is stable over a long timescale.
Figure 67:
Comparison of measured and laboratory wavelengths
for a number of sources and observations. Top panels show the
difference in Å between laboratory and measured wavelengths as
a function of wavelength for the first (red) and second (blue)
orders; the bottom panels show the accumulated histograms,
including a Gaussian fit.
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European Space Agency - XMM-Newton Science Operations Centre