Fig. 3.
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Spectrum of the rise (ObsID 4201960102), peak (ObsID 4201960113), and decline (ObsID 4201960150) of the outburst of EXO 2030+375 and their best fit with the bbody+pl model in blue, yellow, and red respectively. The lower panels show the residuals for fits with an absorbed power law with an iron Kα line emission and with an additional black body or partial covering component.
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