Only luminous and heavily obscured type 2 AGNs show high merger fractions (~0.7), unlike low-luminosity or low-obscuration ones (~0.2).
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4 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.GA 4years
2026 4verdicts
UNVERDICTED 4representative citing papers
Disc galaxies inhibit supermassive black hole growth by preserving rotational support in central gas, while mergers in ellipticals disrupt this support and enable rapid accretion.
A framework using CIGALE and GRAHSP SED fitting plus deep-learning imaging is applied to COSMOS-Web galaxies to estimate AGN fractions in the F150W band and compare methods, revealing degeneracies.
Optical spectroscopy is required to unlock the full potential of SKAO extragalactic surveys through precise redshifts, activity diagnostics, HI stacking, and large-scale structure mapping.
citing papers explorer
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Only obscured yet luminous active galactic nuclei are closely associated with galaxy mergers: Direct observational evidence from type 2 active galactic nuclei
Only luminous and heavily obscured type 2 AGNs show high merger fractions (~0.7), unlike low-luminosity or low-obscuration ones (~0.2).
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Galaxy discs regulate the growth of supermassive black holes
Disc galaxies inhibit supermassive black hole growth by preserving rotational support in central gas, while mergers in ellipticals disrupt this support and enable rapid accretion.
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Towards a consistent framework of determining active galactic nucleus contribution fraction and host galaxy properties
A framework using CIGALE and GRAHSP SED fitting plus deep-learning imaging is applied to COSMOS-Web galaxies to estimate AGN fractions in the F150W band and compare methods, revealing degeneracies.
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Unlocking the Full Potential of SKAO Extra-galactic Science with High-multiplex Optical Spectroscopy
Optical spectroscopy is required to unlock the full potential of SKAO extragalactic surveys through precise redshifts, activity diagnostics, HI stacking, and large-scale structure mapping.