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Fig. 4.
Unfolded spectrum of 2SXPS J075542.5−293353 at high flux level (spectral group A) as observed by Chandra (green) and NuSTAR (other colors) together with the residuals to the best-fit model. For comparison, the spectrum of GX 304−1 as reported in Tsygankov et al. (2019b) is also shown (in gray; arbitrarily scaled).
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