Fig. 9
Detail of the RGS1 (black) and RGS2 (red) spectra in low-flux state around the N VII α absorption line, modeled by the TMAP atmosphere model 008 (dashed curve). The excess in the data left by the atmosphere model could be due either to N VI β line blueshifted by ~1300 km s-1, or to N VII α line redshifted by around ~500 km s-1.
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