Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

NuSTAR and Keck observations of heavily obscured quasars selected by WISE.

Yan, Wei and Hickox, Ryan C. and Hainline, Kevin N. and Stern, Daniel and Lansbury, George and Alexander, David M. and Hviding, Raphael E. and Assef, Roberto J. and Ballantyne, David R. and Dipompeo, Michael A. and Lanz, Lauranne and Carroll, Christopher M. and Koss, Michael and Lamperti, Isabella and Civano, Francesca and Moro, Agnese Del and Gandhi, Poshak and Myers, Adam D. (2019) 'NuSTAR and Keck observations of heavily obscured quasars selected by WISE.', Astrophysical journal., 870 (1). p. 33.

Abstract

A primary aim of the ${Nuclear}\,{Spectroscopic}\,{Telescope}\,{Array}$ (NuSTAR) mission is to find and characterize heavily obscured Active Galactic Nuclei (AGNs). Based on mid-infrared photometry from the Wide-Field Infrared Survey Explorer (WISE) and optical photometry from the Sloan Digital Sky Surveys, we have selected a large population of luminous obscured AGNs (i.e., "obscured quasars"). Here we report NuSTAR observations of four WISE-selected heavily obscured quasars for which we have optical spectroscopy from the Southern African Large Telescope and W. M. Keck Observatory. Optical diagnostics confirm that all four targets are AGNs. With NuSTAR hard X-ray observations, three of the four objects are undetected, while the fourth has a marginal detection. We confirm that these objects have observed hard X-ray (10–40 keV) luminosities at or below ~1043 erg s−1. We compare X-ray and IR luminosities to obtain estimates of the hydrogen column densities (N H) based on the suppression of the hard X-ray emission. We estimate N H of these quasars to be at or larger than 1025 cm−2, confirming that WISE and optical selection can identify very heavily obscured quasars that may be missed in X-ray surveys, and they do not contribute significantly to the cosmic X-ray background. From the optical Balmer decrements, we found that our three extreme obscured targets lie in highly reddened host environments. This galactic extinction cannot adequately explain the more obscured AGNs, but it may imply a different scale of obscuration in the galaxy.

Item Type:Article
Full text:(VoR) Version of Record
Download PDF
(3803Kb)
Status:Peer-reviewed
Publisher Web site:https://doi.org/10.3847/1538-4357/aaeed4
Publisher statement:© 2019. The American Astronomical Society. All rights reserved.
Date accepted:02 November 2018
Date deposited:17 January 2019
Date of first online publication:02 January 2019
Date first made open access:17 January 2019

Save or Share this output

Export:
Export
Look up in GoogleScholar