Fig. 3
Left: four X-ray spectra of SSS J122222 throughout the superoutburst. See text for detail. Right: upper panel: best-fit model components of the outburst spectrum SB and the brightest outburst spectrum So,high. The data are fitted with two optically-thin thermal emission components (shown by dashed and dotted lines), absorbed by a variable column density. Lower panel: residuals.
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