VaDAR: Varstrometry for Dual AGN Using Radio Interferometry

Binary and dual active galactic nuclei (AGNs) are an important observational tool for studying the formation and dynamical evolution of galaxies and supermassive black holes. An entirely new method for identifying possible AGN pairs makes use of the exquisite positional accuracy of Gaia to detect as...

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Main Authors: Emma Schwartzman, Tracy E. Clarke, Kristina Nyland, Nathan J. Secrest, Ryan W. Pfeifle, Henrique Schmitt, Shobita Satyapal, Barry Rothberg
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad0ed0
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author Emma Schwartzman
Tracy E. Clarke
Kristina Nyland
Nathan J. Secrest
Ryan W. Pfeifle
Henrique Schmitt
Shobita Satyapal
Barry Rothberg
author_facet Emma Schwartzman
Tracy E. Clarke
Kristina Nyland
Nathan J. Secrest
Ryan W. Pfeifle
Henrique Schmitt
Shobita Satyapal
Barry Rothberg
author_sort Emma Schwartzman
collection DOAJ
description Binary and dual active galactic nuclei (AGNs) are an important observational tool for studying the formation and dynamical evolution of galaxies and supermassive black holes. An entirely new method for identifying possible AGN pairs makes use of the exquisite positional accuracy of Gaia to detect astrometrically variable quasars, in tandem with the high spatial resolution of the Karl G. Jansky Very Large Array (VLA). We present a new pilot study of radio observations of 18 quasars (0.8 ≤ z ≤ 2.9), selected from the Sloan Digital Sky Survey DR16Q and matched with the Gaia DR3. All 18 targets are identified by their excess astrometric noise in Gaia. We targeted these 18 quasars with the VLA at 2–4 GHz ( S band) and 8–12 GHz ( X band), providing resolutions of 0.″65 and 0.″2, respectively, in order to constrain the origin of this variability. We combine these data with ancillary radio survey data and perform radio spectral modeling. The new observations are used to constrain the driver of the excess astrometric noise. We find that ∼44% of the target sample is likely to be either candidate dual AGN or gravitationally lensed quasars. Ultimately, we use this new strategy to help identify and understand this sample of astrometrically variable quasars, demonstrating the potential of this method for systematically identifying kiloparsec-scale dual quasars.
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spelling doaj.art-57c62c7aa3664bfa9a7949e5998fc42f2024-01-30T15:10:41ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-01961223310.3847/1538-4357/ad0ed0VaDAR: Varstrometry for Dual AGN Using Radio InterferometryEmma Schwartzman0https://orcid.org/0000-0002-6454-861XTracy E. Clarke1https://orcid.org/0000-0001-6812-7938Kristina Nyland2https://orcid.org/0000-0003-1991-370XNathan J. Secrest3https://orcid.org/0000-0002-4902-8077Ryan W. Pfeifle4https://orcid.org/0000-0001-8640-8522Henrique Schmitt5https://orcid.org/0000-0003-2450-3246Shobita Satyapal6https://orcid.org/0000-0003-2277-2354Barry Rothberg7https://orcid.org/0000-0003-2283-2185U.S. Naval Research Laboratory , 4555 Overlook Avenue SW, Washington, DC 20375, USA; Department of Physics and Astronomy, George Mason University , 4400 University Drive, MSN 3F3, Fairfax, VA 22030, USAU.S. Naval Research Laboratory , 4555 Overlook Avenue SW, Washington, DC 20375, USAU.S. Naval Research Laboratory , 4555 Overlook Avenue SW, Washington, DC 20375, USAU.S. Naval Observatory , 3450 Massachusetts Avenue NW, Washington, DC 20392, USAX-ray Astrophysics Laboratory, NASA Goddard Space Flight Center , Code 662, Greenbelt, MD 20771, USAU.S. Naval Research Laboratory , 4555 Overlook Avenue SW, Washington, DC 20375, USADepartment of Physics and Astronomy, George Mason University , 4400 University Drive, MSN 3F3, Fairfax, VA 22030, USADepartment of Physics and Astronomy, George Mason University , 4400 University Drive, MSN 3F3, Fairfax, VA 22030, USA; U.S. Naval Observatory , 3450 Massachusetts Avenue NW, Washington, DC 20392, USABinary and dual active galactic nuclei (AGNs) are an important observational tool for studying the formation and dynamical evolution of galaxies and supermassive black holes. An entirely new method for identifying possible AGN pairs makes use of the exquisite positional accuracy of Gaia to detect astrometrically variable quasars, in tandem with the high spatial resolution of the Karl G. Jansky Very Large Array (VLA). We present a new pilot study of radio observations of 18 quasars (0.8 ≤ z ≤ 2.9), selected from the Sloan Digital Sky Survey DR16Q and matched with the Gaia DR3. All 18 targets are identified by their excess astrometric noise in Gaia. We targeted these 18 quasars with the VLA at 2–4 GHz ( S band) and 8–12 GHz ( X band), providing resolutions of 0.″65 and 0.″2, respectively, in order to constrain the origin of this variability. We combine these data with ancillary radio survey data and perform radio spectral modeling. The new observations are used to constrain the driver of the excess astrometric noise. We find that ∼44% of the target sample is likely to be either candidate dual AGN or gravitationally lensed quasars. Ultimately, we use this new strategy to help identify and understand this sample of astrometrically variable quasars, demonstrating the potential of this method for systematically identifying kiloparsec-scale dual quasars.https://doi.org/10.3847/1538-4357/ad0ed0Radio active galactic nucleiRadio astronomyDouble quasars
spellingShingle Emma Schwartzman
Tracy E. Clarke
Kristina Nyland
Nathan J. Secrest
Ryan W. Pfeifle
Henrique Schmitt
Shobita Satyapal
Barry Rothberg
VaDAR: Varstrometry for Dual AGN Using Radio Interferometry
The Astrophysical Journal
Radio active galactic nuclei
Radio astronomy
Double quasars
title VaDAR: Varstrometry for Dual AGN Using Radio Interferometry
title_full VaDAR: Varstrometry for Dual AGN Using Radio Interferometry
title_fullStr VaDAR: Varstrometry for Dual AGN Using Radio Interferometry
title_full_unstemmed VaDAR: Varstrometry for Dual AGN Using Radio Interferometry
title_short VaDAR: Varstrometry for Dual AGN Using Radio Interferometry
title_sort vadar varstrometry for dual agn using radio interferometry
topic Radio active galactic nuclei
Radio astronomy
Double quasars
url https://doi.org/10.3847/1538-4357/ad0ed0
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