BASS. LIV. Physical Properties of AGN-hosting Galaxy Mergers from Multiwavelength SED Fitting

Abstract Galaxy mergers are believed to play an important role in triggering rapid supermassive black hole (SMBH) growth. As merging nuclei approach each other, the physical properties of the participating galaxies and the associated SMBH growth are expected to evolve significantly. This study measures and characterizes these physical properties throughout the merger sequence. We constructed multiwavelength spectral energy distributions (SEDs) from hard X-rays to the far-IR for a sample of 72 nearby active galactic nucleus (AGN) host galaxies. The sample comprises 64 interacting systems, including single AGN in mergers and dual AGN, with nuclear separations ≤30 kpc, as well as eight isolated active galaxies with merging features. We carefully adapted available photometric measurements at each wavelength to account for their complex morphologies and varying spatial resolutions, to perform SED fitting using CIGALE, aimed to derive critical physical properties. Our results reveal that merging galaxies hosting AGN(s) show deviations from the star-forming main sequence and a wide range of star formation rates (SFRs). Both AGN activity and star formation are significantly influenced by the merger process, but these effects are more prominent in major (mass ratios < 4:1) interactions. We find that the projected nuclear separation is not a good tracer of the merger stage. Instead, morphological classification accurately assesses the merger progression. Based on this morphological analysis, late-stage mergers exhibit elevated SFRs (5.1×), AGN luminosities (2.4×), and nuclear obscuration (2.8×) compared to earlier stages, supporting previous findings and reinforcing the link between merger-driven galaxy evolution and SMBH growth.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-11-25
DOI
https://doi.org/10.3847/1538-4357/ae0a4b
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
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article

BASS. LIV. Physical Properties of AGN-hosting Galaxy Mergers from Multiwavelength SED Fitting

Ezequiel Treister, Ignacio del Moral-Castro, M. Boquien, D. B. Sanders et al.
The Astrophysical Journal
Galaxies: Formation, Evolution, Phenomena
article

BASS. LIV. Physical Properties of AGN-hosting Galaxy Mergers from Multiwavelength SED Fitting

Ezequiel Treister, Ignacio del Moral-Castro, M. Boquien, D. B. Sanders, Kyuseok Oh, Y. Sophia Dai, Cláudio Ricci, Michael Koss, Miguel Parra Tello, F. E. Bauer, Roberto J. Assef, Matilde Signorini, K. K. Gupta, R. F. Mushotzky, Alessandro Peca, A. F. Rojas, C. M. Urry, F. Ricci, Giacomo Venturi, Marco Troncoso
article en

Abstract

Abstract Galaxy mergers are believed to play an important role in triggering rapid supermassive black hole (SMBH) growth. As merging nuclei approach each other, the physical properties of the participating galaxies and the associated SMBH growth are expected to evolve significantly. This study measures and characterizes these physical properties throughout the merger sequence. We constructed multiwavelength spectral energy distributions (SEDs) from hard X-rays to the far-IR for a sample of 72 nearby active galactic nucleus (AGN) host galaxies. The sample comprises 64 interacting systems, including single AGN in mergers and dual AGN, with nuclear separations ≤30 kpc, as well as eight isolated active galaxies with merging features. We carefully adapted available photometric measurements at each wavelength to account for their complex morphologies and varying spatial resolutions, to perform SED fitting using CIGALE, aimed to derive critical physical properties. Our results reveal that merging galaxies hosting AGN(s) show deviations from the star-forming main sequence and a wide range of star formation rates (SFRs). Both AGN activity and star formation are significantly influenced by the merger process, but these effects are more prominent in major (mass ratios < 4:1) interactions. We find that the projected nuclear separation is not a good tracer of the merger stage. Instead, morphological classification accurately assesses the merger progression. Based on this morphological analysis, late-stage mergers exhibit elevated SFRs (5.1×), AGN luminosities (2.4×), and nuclear obscuration (2.8×) compared to earlier stages, supporting previous findings and reinforcing the link between merger-driven galaxy evolution and SMBH growth.

The Astrophysical JournalVol. 994(2)
Roma Tre University (IT), Centre National de la Recherche Scientifique (FR), University of Hawaii System (US), Scuola Normale Superiore (IT), University of Liège (BE), Pontificia Universidad Católica de Chile (CL), University of Tarapacá (CL), Chinese Academy of Sciences (CN), Université Côte d'Azur (FR), Arcetri Astrophysical Observatory (IT), Korea Astronomy and Space Science Institute (KR), Ghent University (BE), Yale University (US), Observatoire de la Côte d’Azur (FR), Eureka Scientific (US), National Astronomical Observatories (CN), European Space Research and Technology Centre (NL), University of Maryland, College Park (US), Federico Santa María Technical University (CL), Universidad Diego Portales (CL)
Openalex Percentile: Top 75%
Galaxies: Formation, Evolution, Phenomena
DOIOpen Access PDFOpenAlex
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