UCL Discovery
UCL home » Library Services » Electronic resources » UCL Discovery

NuSTAR and Keck Observations of Heavily Obscured Quasars Selected by WISE

Yan, W; Hickox, RC; Hainline, KN; Stern, D; Lansbury, G; Alexander, DM; Hviding, RE; ... Myers, AD; + view all (2019) NuSTAR and Keck Observations of Heavily Obscured Quasars Selected by WISE. The Astrophysical Journal , 870 (1) , Article 33. 10.3847/1538-4357/aaeed4. Green open access

[thumbnail of Yan_2019_ApJ_870_33.pdf]
Preview
Text
Yan_2019_ApJ_870_33.pdf - Published Version

Download (3MB) | Preview

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 (NH) based on the suppression of the hard X-ray emission. We estimate NH 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.

Type: Article
Title: NuSTAR and Keck Observations of Heavily Obscured Quasars Selected by WISE
Open access status: An open access version is available from UCL Discovery
DOI: 10.3847/1538-4357/aaeed4
Publisher version: https://doi.org/10.3847/1538-4357/aaeed4
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: galaxies: active; galaxies: nuclei; X-rays: galaxies
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/10091822
Downloads since deposit
0Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item