Fig. 8.

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Corner plot for source ID 00030, best fit with a partial covering absorber. Here, the first instance of log(nH) is the host galaxy absorber column density (in units of ×1022 cm−2), log(norm) is the power law normalisation, PhoIndex is the photon index of the power law, the second instance of log(nH) is the partial covering absorber column density (×1022 cm−2), CvrFrac is the covering fraction of the absorber, and norm is the relative renormalisation of the background model with respect to the source model, which is in agreement with 1.
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