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Fig. 3.

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Data-to-model ratio of the fit above 3 keV with the REFLKERR relativistic reflection model, using a primary Comptonisation continuum shape and assuming a slab geometry for the hot corona. Black: 2019 XMM-Newton/pn; dark grey: 2019 NuSTAR; blue: 2020 XMM-Newton/pn; light blue: 2020 NuSTAR; orange: 2017 NuSTAR.

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