Chandra stacking constraints on the contribution of 24 μm Spitzer sources to the unresolved cosmic X-ray background

We employ X-ray stacking techniques to examine the contribution from X-ray-undetected, mid-infrared-selected sources to the unresolved, hard(6-8 keV) cosmic X-ray background (CXB). We use the publicly available, 24 mu m Spitzer Space Telescope MIPS catalogs from the Great Observatories Origins Deep Survey (GOODS)-North and South fields, which are centered on the 2 Ms Chandra Deep Field-North and 1 Ms Chandra Deep Field-South, to identify bright (S-24 mu m > 80 mu Jy) mid-infrared sources that may be powered by heavily obscured AGNs. We S 1 80 24 mm measure a significant stacked X-ray signal in all of the X-ray bands examined, including, for the first time, a significant (3.2 sigma) 6-8 keV stacked X-ray signal from an individually undetected X-ray source population. We find that the X-ray-undetected MIPS sources make up approximate to 2% ( or less) of the total CXB below 6 keV, but approximate to 6% in the 6-8 keV band. The 0.5-8 keV stacked spectrum is consistent with a hard power law (Gamma = 1.44 +/- 0.007), with the spectrum hardening at higher X- ray energies. Our findings show that these bright MIPS sources do contain obscured AGNs, but are not the primary source of the unresolved similar to 40% of 6-8 keV CXB. Our study rules out obscured, luminous quasars as a significant source of the remaining unresolved CXB and suggests that it most likely arises from a large population of obscured, high-redshift (z greater than or similar to 1), Seyfert-luminosity AGNs.