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Fig. 3
XMM-Newton RGS1/RGS2 spectrum of E0102 from a combination of 23 observations (top). The bright lines of O and Ne dominate the flux in this band. Same as top figure except with a logarithmic Y axis to emphasize the continuum and the weakest lines (bottom). Fe L emission is absent in this spectrum.
This figure is made of several images, please see below:
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