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Fig. 5

image

a) NuSTAR count rate spectrum of IRAS F00183–7111 in the 3–20 keV band. The three solid-line histograms plotted along the spectral data show best-fit models of the absorbed power-law (black, APL in Table 2) and the reflection spectrum computed by xillver (red, IREFL) and the ionized absorption spectrum (blue, IABS2). All the models are folded through the detector response; b) data/model ratio for the APL model in (a); c) for IREFL (open squares) and IABS2 models (filled circles); and d) three models shown above, without response folding and plotted in flux units.

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