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The 4 Ms Chandra deep field south number counts apportioned by source class: pervasive active galactic nuclei and the ascent of normal galaxies

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Figure

Figure 1. Detection probability as a function of intrinsic 0.5–2 keV flux for point sources located on axis (dashed curve) and ≈8  off axis (solid curve).
Figure 2. Effective solid angle A(S) vs. intrinsic flux limit S for the SB (dotted curve), HB (short-dashed curve), UHB (dash-dotted curve), and FB (solid curve)
Figure 3. 0.5–2 keV flux probability distributions for two AGNs in the X11 catalog with no-source-detection probabilities (provided by AE) of ≈10 −45 (solid curve) and ≈0.003 (dashed curve)
Figure 4. Observed-frame 0.5–8 keV luminosity vs. redshift for AGNs (blue triangles) and normal galaxies (red squares)
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