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Fig. 2.
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X-ray spectrum of IGR J17511-3057 as observed by XMM-Newton on 2025 March 4 with EPIC-pn (blue), EPIC-MOS1 (orange), and EPIC-MOS2 (green), along with the best-fitting model constant * TBabs * (thComp*bbodyrad) (see Table 1). The bottom panel displays the residuals from the fit.
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