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Fig. 3
XMM-Newton/RGS1 spectra of V5116 Sgr in high (blue) and low (red) flux periods in March 2007, and Chandra LETG/HRC-S excluding the flares (green), obtained in August 2007. The count-rate of the high-flux period of the RGS1 data has been downscaled by a factor of eight for ease of comparison.
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