Fig. 10.
Multiwavelength fit of our unified clumpy geometry to data of NGC 1365. Infrared photometry on the left overlayed with two CLUMPY fit solutions, and spectra from three NuSTAR observations are shown on the right with UXCLUMPY fits. Insets show parameter probability distributions for each fitted dataset in corresponding colours. The infrared fit solution shown in brown is overall compatible with the X-ray fits (blue, green, orange).
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