The NuSTAR Extragalactic Survey: Average broad-band X-ray spectral properties of the NuSTAR detected AGN
arXiv:1710.01041 · doi:10.3847/1538-4357/aa9115
Abstract
We present a study of the average X-ray spectral properties of the sources detected by the NuSTAR extragalactic survey, comprising observations of the E-CDFS, EGS and COSMOS fields. The sample includes 182 NuSTAR sources (64 detected at 8-24 keV), with 3-24 keV fluxes ranging between and erg/cm/s ( erg/cm/s) and redshifts of . We produce composite spectra from the Chandra+NuSTAR data ( keV, rest frame) for all the sources with redshift identifications (95%) and investigate the intrinsic, average spectra of the sources, divided into broad-line (BL) and narrow-line (NL) AGN, and also in different bins of X-ray column density and luminosity. The average power-law photon index for the whole sample is , flatter than typically found for AGN. While the spectral slope of BL and X-ray unabsorbed AGN is consistent with typical values (), a significant flattening is seen in NL AGN and heavily-absorbed sources ( and , respectively), likely due to the effect of absorption and to the contribution from Compton reflection to the high-energy flux (E>10 keV). We find that the typical reflection fraction in our spectra is (for ), with a tentative indication of an increase of the reflection strength with column density. While there is no significant evidence for a dependence of the photon index with X-ray luminosity in our sample, we find that decreases with luminosity, with relatively high levels of reflection () for erg/s and for erg/s AGN, assuming .
19 pages, 14 figures, 4 tables. Accepted for publication in ApJ