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Are most low-luminosity active galactic nuclei really obscured?

Hopkins, Philip F. and Hickox, Ryan and Quataert, Eliot and Hernquist, Lars (2009) Are most low-luminosity active galactic nuclei really obscured? Monthly Notices of the Royal Astronomical Society, 398 (1). pp. 333-349. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20200521-163329824

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Abstract

At low Eddington ratios (ṁ), two effects make it more difficult to detect certain active galactic nuclei (AGN) given a particular set of selection methods. First, even allowing for fixed accretion physics, at low ṁ AGN become less luminous relative to their hosts, diluting their emission; the magnitude of the dilution depends on host properties and, therefore, on luminosity and redshift. Secondly, low-forumla systems are expected and observed to transition to a radiatively inefficient state, which changes the spectral energy distribution (SED) shape and dramatically decreases the luminosity at optical through infrared (IR) wavelengths. The effects of dilution are unavoidable, while the precise changes in accretion physics at low ṁ are somewhat uncertain, but potentially very important for our understanding of AGN. These effects will have different implications for samples with different selection criteria, and generically lead to differences in the AGN populations recovered in observed samples, even at fixed bolometric luminosity and after correction for obscuration. Although the true Eddington ratio distribution may depend strongly on mass/luminosity, this will be seen only in surveys robust to dilution and radiative inefficiency, such as X-ray or narrow-line samples; by contrast, selection effects imply that AGN in optical samples will have uniformly high Eddington ratios, with little dependence on luminosity, even at low L_(bol) where the median ‘true’ ṁ ≲ 0.01. These same selection effects also imply that different selection criteria pick out systems with different hosts: as a result, the clustering of low-luminosity optical/IR sources will be weaker than that of X-ray sources, and optical/IR Seyferts will reside in more disc-dominated galaxies, while X-ray-selected Seyferts will be preferentially in early-type systems. Taken together, these effects can naturally explain longstanding, apparently contradictory claims in the literature regarding AGN Eddington ratio distributions, host populations and clustering. Finally, we show that if current observed Eddington ratio distributions are correct, a large fraction of low-luminosity AGN currently classified as ‘obscured’ are in fact radiatively diluted and/or radiatively inefficient, not obscured by gas or dust. This is equally true if X-ray hardness is used as a proxy for obscuration, since radiatively inefficient SEDs near ṁ ~ 0.01 are characteristically X-ray hard. These effects can explain most of the claimed luminosity/redshift dependence in the ‘obscured’ AGN population, with the true obscured fraction as low as ∼20 per cent.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1111/j.1365-2966.2009.15136.xDOIArticle
https://arxiv.org/abs/0901.2936arXivDiscussion Paper
ORCID:
AuthorORCID
Hopkins, Philip F.0000-0003-3729-1684
Hickox, Ryan0000-0003-1468-9526
Quataert, Eliot0000-0001-9185-5044
Hernquist, Lars0000-0001-6950-1629
Additional Information:© 2009 The Authors. Journal compilation © 2009 RAS. Accepted 2009 May 25. Received 2009 May 19; in original form 2009 January 18. We thank Paul Martini and Smita Mathur for helpful discussions. We also thank the anonymous referee for valuable comments and suggestions. This work was supported in part by NSF grants ACI 96-19019, AST 00-71019, AST 02-06299 and AST 03-07690, and NASA ATP grants NAG5-12140, NAG5-13292 and NAG5-13381. Support for PFH was provided by the Miller Institute for Basic Research in Science, University of California Berkeley. EQ is supported in part by NASA grant NNG06GI68G and the David and Lucile Packard Foundation.
Funders:
Funding AgencyGrant Number
NSFACI 96-19019
NSFAST 00-71019
NSFAST 02-06299
NSFAST 03-07690
NASANAG5-12140
NASANAG5-13292
NASANAG5-13381
Miller Institute for Basic Research in ScienceUNSPECIFIED
NASANNG06GI68G
David and Lucile Packard FoundationUNSPECIFIED
Subject Keywords:galaxies: active, galaxies: evolution, quasars: general, cosmology: theory
Issue or Number:1
Record Number:CaltechAUTHORS:20200521-163329824
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200521-163329824
Official Citation:Philip F. Hopkins, Ryan Hickox, Eliot Quataert, Lars Hernquist, Are most low-luminosity active galactic nuclei really obscured?, Monthly Notices of the Royal Astronomical Society, Volume 398, Issue 1, September 2009, Pages 333–349, https://doi.org/10.1111/j.1365-2966.2009.15136.x
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:103391
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:22 May 2020 18:30
Last Modified:22 May 2020 18:30

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