JeTCAF model-fitted 0.4−75.0 keV spectra for all four epochs of NGC 1365 during XMM-Newton and NuSTAR era. Here, panels a–d corresponds to epochs A to D. The different Gaussian lines are used for emission/excess at different energy ranges, including at ∼6.4 keV. The model fits show the absorption line and spectral shape change in each epoch, along with a P Cygni profile in the FeK band.