SHARP is positioned to deliver the first statistical census of ultra-compact dual AGN, bridging kpc-scale pairs to sub-pc binary MBHs that emit gravitational waves.
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4 Pith papers cite this work. Polarity classification is still indexing.
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Spectral monitoring indicates NGC 3786's changing-look AGN transition results from torus covering factor variations driven by Eddington ratio and accretion mode changes.
A modified asymmetric broad line region model shows that time-evolving single-BH configurations do not contaminate algorithms searching for massive black hole binaries in multi-epoch spectroscopic data.
Expanded sample yields marginal evidence that f correlates with log10(FWHM/σ) of the broad Hβ line, consistent with earlier results and potentially enabling empirical f estimates.
citing papers explorer
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A new era for Dual AGN science with SHARP
SHARP is positioned to deliver the first statistical census of ultra-compact dual AGN, bridging kpc-scale pairs to sub-pc binary MBHs that emit gravitational waves.
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The Changing-look Phenomenon Accompanied by an Accretion Mode Transition in NGC 3786
Spectral monitoring indicates NGC 3786's changing-look AGN transition results from torus covering factor variations driven by Eddington ratio and accretion mode changes.
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Can a time evolving, asymmetric broad line region mimic a massive black hole binary?
A modified asymmetric broad line region model shows that time-evolving single-BH configurations do not contaminate algorithms searching for massive black hole binaries in multi-epoch spectroscopic data.
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Can BLR line profile shape improve single-epoch black hole mass estimates?
Expanded sample yields marginal evidence that f correlates with log10(FWHM/σ) of the broad Hβ line, consistent with earlier results and potentially enabling empirical f estimates.