Fig. D.3.
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Absorbed power-law (tbabs*ztabs*zpowerlaw, top row) and double blackbody (tbabs*(zbbody+zbbody), bottom row) model fits to the convolved XMM spectra (XMM1, left column; XMM2, middle; XMM3, right). The preferred model fit for XMM1 and XMM3 is the dual black body model, whereas it is the absorbed power-law model for XMM2. XMM1, XMM2 and XMM3 were obtained at 36, 196, and 393 days after optical peak.
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