| Autor: |
Green, K, Elmer, E, Maltby, D T, Almaini, O, Merrifield, M, Hartley, W G |
| Předmět: |
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| Zdroj: |
Monthly Notices of the Royal Astronomical Society; Jun2024, Vol. 531 Issue 2, p2551-2562, 12p |
| Abstrakt: |
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 Active Galactic Nuclei (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 (|$\gt 10^{9}\rm \, {\rm M}_{\odot }$|), while X-ray detection primarily identifies AGN in galaxies of higher mass (|$\gt 10^{10}\rm \, {\rm M}_{\odot }$|). We conclude that long-term near-infrared variability provides an important new tool for obtaining more complete samples of AGN in deep survey fields. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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