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Fig. 6.
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XMM-Newton EPIC-pn+MOS2 (top), Chandra ACIS-S X1 (middle), and X2 (bottom) observations of Haro 11, along with the spectral models constant × phabs × (diskbb + zpowerlw) and constant × phabs × (zbbody + zpowerlw) (in red) fitted to the XMM-Newton and Chandra data, respectively.
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