Cumulative marginalized posterior distributions of the amplitudes (left) and the spectral indices (right) of pulsars’ RNs for the dataset OneF corrupted with 0% (red), 0.3% (blue), 1% (green), 5% (pink), and 10% (orange) of outliers. The histograms, in both panels, are the sum of the normalized marginalized posteriors of the amplitudes and the spectral indices of the RN of each pulsar.