SED of the Crab Nebula obtained by processing the data set used by Aleksić et al. (2016b) with the full SkyPrism tool chain. The spectral fit is obtained via the forward folding procedure, whereas the data points are the results of the individual fits in each E_est bin. The dark blue error bars of the data points are the statistical error, and the light blue error bars indicate the uncertainties from the exposure model. The obtained results are also compared to the Crab Nebula SED from the same publication in terms of the relative flux difference (ΔF/F.)