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XZ: Deriving redshifts from X ray spectra of obscured AGN

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Fig. 3. Corner plot showing the parameter space over photon index, col- col-umn density, and redshift for the heavily obscured AGN R65 (blue) and the mildly obscured AGN R4 (gray), see Fig
Table 2. Redshift catalogue of CDF-S sources with IG≥1 bit (excerpt).
Fig. 5. Comparison of XZ and specz for constrained cases (IG ≥ 2). The filled circles show the median of the XZ probability distribution while the error bars correspond to 1σ-equivalent quantiles and color-coded by the median of the obscuration level
Figure 13 shows an example of the multiple solution issue, R447. While the photoz = 0.74 ± 0.01 and specz = 0.735 agree, the XZ (nominally 1.48 +0.08 −0.87 ) has two solutions, with the less  prob-able solution covering the same range as the photoz and spe
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