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Fig. 2
Swift-XRT 0.3–8 keV spectral fits to the outburst (observations 1 and 2) and quiescent (observations 3–6) spectra of NSV 1436. Both spectra require two optically thin thermal components, shown dashed in outburst and dotted in quiescence. NSV 1436 is brighter and hotter in quiescence than in outburst.
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