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The NuSTAR Extragalactic Surveys: X Ray Spectroscopic Analysis of the Bright Hard band Selected Sample

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Figure

Figure 1. Total and individual sensitivity curves as a function of the hard-band flux for the surveys included in our sample
Figure 2. Left panel: net counts in the full (3–24 keV) energy band from a 30″ aperture vs
Figure 3. Left panel: 3 –24keV net counts vs. photon index for the NuSTAR- NuSTAR-only joint fit derived using a power-law model (black dots)
Figure 4. Examples of broadband spectra for four sources with best- fit baseline models (solid lines)
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