X-ray Observations of Luminous Dusty Quasars at z > 2
arXiv:1910.00602 · doi:10.1093/mnras/staa1220
Abstract
We present new X-ray observations of luminous heavily dust-reddened quasars (HRQs) selected from infrared sky surveys. HRQs appear to be a dominant population at high redshifts and the highest luminosities, and may be associated with a transitional "blowout" phase of black hole and galaxy co-evolution models. Despite this, their high-energy properties have been poorly known. We use the overall sample of objects with XMM-Newton coverage to study the high-energy properties of HRQs at erg/s and . For the seven sources with strong X-ray detections, we perform spectral analyses. These find a median X-ray luminosity of erg/s, comparable to the most powerful X-ray quasars known. The gas column densities are - cm, in agreement with the amount of dust extinction observed. The dust to gas ratios are sub-Galactic, but are higher than found in local AGN. The intrinsic X-ray luminosities of HRQs are weak compared to the mid-infrared () and bolometric luminosities (), in agreement with findings for other luminous quasar samples. For instance, the X-ray to bolometric corrections range from -. The moderate absorption levels and accretion rates close to the Eddington limit () are in agreement with a quasar blowout phase. Indeed, we find that the HRQs lie in the forbidden region of the - plane, and therefore that radiation pressure feedback on the dusty interstellar medium may be driving a phase of blowout that has been ongoing for a few years. The wider properties, including [OIII] narrow-line region kinematics, broadly agree with this interpretation.
arXiv commentIn press. Accepted for publication in MNRAS
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