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This article has an erratum: [https://doi.org/10.1051/0004-6361/202554514e]


Fig. 8.

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Models considered in this work to fit the optical/UV observations (red points) and XRT spectra (purple line) for days 58062 MJD (up) and 58094 MJD (bottom). The contribution of X-ray heating of the companion star is represented with a pink dotted line, the irradiated disk is plotted as a brown dashed line, the viscously heated disk is plotted with a green dash-dotted line. The xspec models bbodyrad and pegpowerlaw used to fit the XRT spectra are plotted with light blue dotted and navy blue dashed lines, respectively.

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