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We combine our dynamical modeling black hole mass measurements from the LickAGN Monitoring Project 2016 sample with measured cross-correlation time lagsand line widths to recover individual scale factors, f, used in traditionalreverberation mapping analyses. We extend our sample by including prior resultsfrom Code for AGN Reverberation and Modeling of Emission Lines (caramel)studies that have utilized our methods. Aiming to improve the precision ofblack hole mass estimates, as well as uncover any regularities in the behaviorof the broad-line region (BLR), we search for correlations between f and otherAGN/BLR parameters. We find (i) evidence for a correlation between the virialcoefficient log10(fmean,{\sigma}) and black hole mass, (ii) marginal evidencefor a similar correlation between log10(frms,{\sigma}) and black hole mass,(iii) marginal evidence for an anti-correlation of BLR disk thickness withlog10(fmean,FWHM)and log10(frms,FWHM), and (iv) marginal evidence for ananti-correlation of inclination angle with log10(fmean,FWHM),log10(frms,{\sigma}), and log10(fmean,{\sigma}). Lastly, we find marginalevidence for a correlation between line-profile shape, when using theroot-meansquare spectrum, log10(FWHM/{\sigma})rms, and the virial coefficient,log10(frms,{\sigma}), and investigate how BLR properties might be related toline-profile shape using caramel models.

What Does the Virial Coefficient of the \Hb Broad-Line Region Depend On?