Fig. 7.
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SED fitting of NGC 6300 from X-ray to Optical-IR band, using XCIGALE: with AGN (orange line), host stellar absorption (blue dashed line) and host dust emission (red solid line) components. The X-ray fluxes are obtained from the X-ray spectral fitting presented in this work, and optical-IR fluxes are derived from photometry. The individual components are reported in the top-left part of the figure.
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