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We present the results of a program of optical and near-infrared spectroscopic follow-up of candidate active galactic nuclei (AGNs) selected in the mid-infrared. This survey selects both normal and obscured AGNs closely matched in luminosity across a wide range, from Seyfert galaxies with bolometric luminosities L bol ∼ 1010 L to highly luminous quasars (L bol ∼ 1014 L ), all with redshifts ranging from 0 to 4.3. Samples of candidate AGNs were selected with mid-infrared color cuts at several different 24 μm flux density limits to ensure a range of luminosities at a given redshift. The survey consists of 786 candidate AGNs and quasars, of which 672 have spectroscopic redshifts and classifications. Of these, 137 (20%) are type 1 AGNs with blue continua, 294 (44%) are type 2 objects with extinctions AV ≳ 5 toward their AGNs, 96 (14%) are AGNs with lower extinctions (AV ∼ 1), and 145 (22%) have redshifts, but no clear signs of AGN activity in their spectra. Of the survey objects 50% have L bol > 1012 L , in the quasar regime. We present composite spectra for type 2 quasars and objects with no signs of AGN activity in their spectra. We also discuss the mid-infrared - emission-line luminosity correlation and present the results of cross correlations with serendipitous X-ray and radio sources. The results show that: (1) obscured objects dominate the overall AGN population, (2) mid-infrared selected AGN candidates exist which lack AGN signatures in their optical spectra but have AGN-like X-ray or radio counterparts, and (3) X-ray and optical classifications of obscured and unobscured AGNs often differ. © 2013. The American Astronomical Society. All rights reserved.
Author(s): Lacy M, Ridgway SE, Gates EL, Nielsen DM, Petric AO, Sajina A, Urrutia T, Cox Drews S, Harrison C, Seymour N, Storrie-Lombardi LJ
Publication type: Article
Publication status: Published
Journal: Astrophysical Journal. Supplement Series
Year: 2013
Volume: 208
Issue: 2
Online publication date: 27/09/2013
ISSN (print): 0067-0049
ISSN (electronic): 1538-4365
Publisher: Institute of Physics Publishing
URL: https://doi.org/10.1088/0067-0049/208/2/24
DOI: 10.1088/0067-0049/208/2/24
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