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Presentation . 2026
License: CC BY
Data sources: Datacite
ZENODO
Presentation . 2026
License: CC BY
Data sources: Datacite
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Host Galaxy properties of highly accreting SMBH in the local Universe

descriptionPublicationkeyboard_double_arrow_right Presentation 27 Feb 2026Publisher:Zenodo
Authors: Rojas Lilayú, Alejandra;

doi: 10.5281/zenodo.18804967 , 10.5281/zenodo.18804968

Host Galaxy properties of highly accreting SMBH in the local Universe

Abstract

An open question in extragalactic astronomy is the extent to which Active Galactic Nuclei (AGN) affect the evolution of their host galaxies. Host galaxy properties of AGN, such as star formation rate and stellar mass, are key parameters for studying the role of AGN in galaxy evolution. However, disentangling the infrared emission from AGN and star-forming components is a challenging task that requires comparing advanced spectral energy distribution (SED) models.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
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