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Fig. 5.
XMM-Newton PN spectra and best-fit model of IGR J16320–4751 in two extreme cases. Left panel: background-subtracted X-ray spectra of ObsID 401. Right panel: background-subtracted X-ray spectra of ObsID 701. Lower panels: fitting residuals. Errors are at 1-σ (68%) confidence levels, and χ 2 statistics are used.
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