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BAT AGN spectroscopic survey - XV: the high frequency radio cores of ultra-hard X-ray selected AGN

Smith, Krista Lynne and Mushotzky, Richard F. and Koss, Michael and Trakhtenbrot, Benny and Ricci, Claudio and Wong, O. Ivy and Bauer, Franz E. and Ricci, Federica and Vogel, Stuart and Stern, Daniel and Powell, Meredith C. and Urry, C. Meg and Harrison, Fiona and Mejía-Restrepo, Julián Esteban and Oh, Kyuseok and Baek, Junhyun and Chung, Aeree (2020) BAT AGN spectroscopic survey - XV: the high frequency radio cores of ultra-hard X-ray selected AGN. Monthly Notices of the Royal Astronomical Society, 492 (3). pp. 4216-4234. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20200326-150430295

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Abstract

We have conducted 22 GHz radio imaging at 1 arcsec resolution of 100 low-redshift AGN selected at 14–195 keV by the Swift-BAT. We find a radio core detection fraction of 96 per cent, much higher than lower frequency radio surveys. Of the 96 radio-detected AGN, 55 have compact morphologies, 30 have morphologies consistent with nuclear star formation, and 11 have sub-kpc to kpc-scale jets. We find that the total radio power does not distinguish between nuclear star formation and jets as the origin of the radio emission. For 87 objects, we use optical spectroscopy to test whether AGN physical parameters are distinct between radio morphological types. We find that X-ray luminosities tend to be higher if the 22 GHz morphology is jet-like, but find no significant difference in other physical parameters. We find that the relationship between the X-ray and core radio luminosities is consistent with the L_R/L_X ∼ 10⁻⁵ of coronally active stars. We further find that the canonical fundamental planes of black hole activity systematically overpredict our radio luminosities, particularly for objects with star formation morphologies.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/stz3608DOIArticle
https://arxiv.org/abs/2001.00877arXivDiscussion Paper
ORCID:
AuthorORCID
Smith, Krista Lynne0000-0001-5785-7038
Mushotzky, Richard F.0000-0002-7962-5446
Koss, Michael0000-0002-7998-9581
Trakhtenbrot, Benny0000-0002-3683-7297
Ricci, Claudio0000-0001-5231-2645
Bauer, Franz E.0000-0002-8686-8737
Ricci, Federica0000-0001-5742-5980
Stern, Daniel0000-0003-2686-9241
Powell, Meredith C.0000-0003-2284-8603
Urry, C. Meg0000-0002-0745-9792
Harrison, Fiona0000-0003-2992-8024
Mejía-Restrepo, Julián Esteban0000-0001-8450-7463
Oh, Kyuseok0000-0002-5037-951X
Additional Information:© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model). Received: 09 August 2019; Revision received: 12 December 2019; Accepted: 17 December 2019; Published: 03 January 2020. Support for KLS was provided by the National Aeronautics and Space Administration through Einstein Postdoctoral Fellowship Award Number PF7-180168, issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under contract NAS8-03060. CR acknowledges the Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT) + Programa de Atraccion e Insercion de Capital Humano Avanzado (PAI) Convocatoria Nacional subvencion a instalacion en la academia convocatoria año 2017 PAI77170080. KO is an International Research Fellow of the Japan Society for the Promotion of Science (JSPS) (ID:P17321). FR acknowledges support from Fondo Nacional de Desarrollo Cientifico y Tecnologico (FONDECYT) Postdoctorado 3180506; FR and FEB acknowledge support from CONICYT project Basal AFB-170002.
Group:Astronomy Department
Funders:
Funding AgencyGrant Number
NASA Einstein FellowshipPF7-180168
NASANAS8-03060
Comisión Nacional de Investigación Científica y Tecnológica (CONICYT)2017 PAI77170080
Japan Society for the Promotion of Science (JSPS)UNSPECIFIED
Fondo Nacional de Desarrollo Científico y Tecnológico (FONDECYT)3180506
BASAL-CATAAFB-170002
Subject Keywords:galaxies: active, galaxies: nuclei, galaxies: Seyfert, radio continuum: galaxies
Issue or Number:3
Record Number:CaltechAUTHORS:20200326-150430295
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200326-150430295
Official Citation:Krista Lynne Smith, Richard F Mushotzky, Michael Koss, Benny Trakhtenbrot, Claudio Ricci, O Ivy Wong, Franz E Bauer, Federica Ricci, Stuart Vogel, Daniel Stern, Meredith C Powell, C Meg Urry, Fiona Harrison, Julian Mejia-Restrepo, Kyuseok Oh, Junhyun Baek, Aeree Chung, BAT AGN spectroscopic survey - XV: the high frequency radio cores of ultra-hard X-ray selected AGN, Monthly Notices of the Royal Astronomical Society, Volume 492, Issue 3, March 2020, Pages 4216–4234, https://doi.org/10.1093/mnras/stz3608
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:102131
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:27 Mar 2020 02:54
Last Modified:27 Mar 2020 02:54

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