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Increasing AGN sample completeness using long-term near-infrared variability

Green, K; Elmer, E; Maltby, D T; Almaini, O; Merrifield, M; Hartley, W G

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Authors

K Green

E Elmer

Dr. DAVID MALTBY David.Maltby@nottingham.ac.uk
Teaching Associate in Physics Andastronomy

OMAR ALMAINI omar.almaini@nottingham.ac.uk
Professor of Astrophysics

M Merrifield

W G Hartley



Abstract

In this work, we use 8 years of deep near-infrared imaging to select and study a new set of 601 active galaxies identified through long-term near-infrared (NIR) variability in the UKIDSS Ultra Deep Survey (UDS). These objects are compared to 710 X-ray bright AGN detected by the Chandra X-ray observatory. We show that infrared variability and X-ray emission select distinct sets of active galaxies, finding only a 37 per cent overlap of galaxies detected by both techniques and confirming NIR-variable AGN to be typically X-ray quiet. Examining the mass functions of the active galaxies shows that NIR variability detects AGN activity in galaxies over a significantly wider range of host stellar mass compared to X-ray detection. For example, at 𝑧 ∼ 1, variable AGN are identified among approximately 1 per cent of galaxies in a roughly flat distribution above the stellar mass completeness limit (> 109 M⊙ ), while X-ray detection primarily identifies AGN in galaxies of higher mass (> 1010 M⊙ ). We conclude that long-term near-infrared variability provides an important new tool for obtaining more complete samples of AGN in deep survey fields.

Citation

Green, K., Elmer, E., Maltby, D. T., Almaini, O., Merrifield, M., & Hartley, W. G. (2024). Increasing AGN sample completeness using long-term near-infrared variability. Monthly Notices of the Royal Astronomical Society, 531(2), 2551-2562. https://doi.org/10.1093/mnras/stae1322

Journal Article Type Article
Acceptance Date May 17, 2024
Online Publication Date May 23, 2024
Publication Date 2024-06
Deposit Date May 23, 2024
Publicly Available Date May 23, 2024
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 531
Issue 2
Pages 2551-2562
DOI https://doi.org/10.1093/mnras/stae1322
Keywords surveys, galaxies: active, galaxies: luminosity function, mass function, infrared: galaxies, X-rays: galaxies
Public URL https://nottingham-repository.worktribe.com/output/35153662
Publisher URL https://academic.oup.com/mnras/article/531/2/2551/7680582

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