A complete catalogue of broad-line AGNs and double-peaked emission lines from MaNGA integral-field spectroscopy of 10K galaxies: stellar population of AGNs, supermassive black holes, and dual AGNs

Fu, Youquan; Cappellari, Michele; Mao, Shude; Lu, Shengdong; Zhu, Kai; Li, Ran

doi:10.1093/mnras/stad2214

A complete catalogue of broad-line AGNs and double-peaked emission lines from MaNGA integral-field spectroscopy of 10K galaxies: stellar population of AGNs, supermassive black holes, and dual AGNs

Journal Article · Wed Jul 26 00:00:00 EDT 2023 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stad2214· OSTI ID:1994001

^[1]; ^[2]; ^[3]; ^[1]; ^[4]; ^[4]

Tsinghua Univ., Beijing (China)
Univ. of Oxford (United Kingdom)
Tsinghua Univ., Beijing (China); Chinese Academy of Sciences (CAS), Beijing (China)
Chinese Academy of Sciences (CAS), Beijing (China); Beijing Normal University (China); University of Chinese Academy of Sciences, Beijing (China)

We analyse the integral field spectroscopy data for the ≈10 000 galaxies in final data release of the MaNGA survey. We identify 188 galaxies for which the emission lines cannot be described by single Gaussian components. These galaxies can be classified into (1) 38 galaxies with broad $$\rm H\alpha$$ and [O III] $$\rm \lambda$$5007 lines, (2) 101 galaxies with broad $$\rm H\alpha$$ lines but no broad [O III] $$\rm \lambda$$5007 lines, and (3) 49 galaxies with double-peaked narrow emission lines. Most of the broad-line galaxies are classified as active galactic nuclei (AGNs) from their line ratios. The catalogue helps us further understand the AGN-galaxy coevolution through the stellar population of broad-line region host galaxies and the relation between broad lines’ properties and the host galaxies’ dynamical properties. The stellar population properties (including mass, age, and metallicity) of broad-line host galaxies suggest there is no significant difference between narrow-line Seyfert-2 galaxies and Type-1 AGNs with broad $$\rm H\alpha$$ lines. We use the broad-$$\rm H\alpha$$ line width and luminosity to estimate masses of black hole in these galaxies, and test the MBH–σe relation in Type-1 AGN host galaxies. Furthermore, we find three dual AGN candidates supported by radio images from the VLA FIRST survey. This sample may be useful for further studies on AGN activities and feedback processes.

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Research Organization:: US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)

Sponsoring Organization:: Alfred P. Sloan Foundation; National Key Research and Development Program of China; National Natural Science Foundation of China (NSFC); USDOE; USDOE Office of Science (SC)

OSTI ID:: 1994001

Alternate ID(s):: OSTI ID: 2425067

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 4 Vol. 524; ISSN 0035-8711; ISSN 1365-2966

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United States

Language:: English

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A complete catalogue of broad-line AGNs and double-peaked emission lines from MaNGA integral-field spectroscopy of 10K galaxies: stellar population of AGNs, supermassive black holes, and dual AGNs

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