A new deconvolution algorithm separates AGN host galaxies from central point sources via smoothness, sparsity, and a pixel-wise product balance constraint, achieving HST-comparable resolution on Subaru HSC data.
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Recovers individual f virial factors from dynamical modeling plus RM data and reports evidence for correlation of log f with black hole mass plus marginal links to BLR thickness, inclination, and line shape.
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A New PSF Deconvolution Algorithm: Simultaneous Spatial Resolution Enhancement and Point Source Removal for Morphological Analysis of AGN Host Galaxies
A new deconvolution algorithm separates AGN host galaxies from central point sources via smoothness, sparsity, and a pixel-wise product balance constraint, achieving HST-comparable resolution on Subaru HSC data.
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What Does the Virial Coefficient of the \Hb Broad-Line Region Depend On?
Recovers individual f virial factors from dynamical modeling plus RM data and reports evidence for correlation of log f with black hole mass plus marginal links to BLR thickness, inclination, and line shape.