Consistency study of high- and low-accreting Mg ii quasars: No
  significant effect of the Fe ii to Mg ii flux ratio on the radius-luminosity
  relation dispersion
  We use observations of 66 reverberation-measured \Mgii\ quasars (QSOs) in the
redshift range $0.36 \leq z \leq 1.686$ -- a subset of the 78 QSOs we
previously studied that also have \rfe\ (flux ratio parameter of UV \Feii\ to
\Mgii\ that is used as an accretion-rate proxy) measurements -- to
simultaneously constrain cosmological model parameters and QSO 2-parameter and
3-parameter radius-luminosity ($R-L$) relation parameters in six different
cosmological models. We find that these QSO $R-L$ relation parameters are
independent of the assumed cosmological model and so these QSOs are
standardizable through the $R-L$ relations. Also: (1) With the 2-parameter
$R-L$ relation, we find that the low-\rfe\ and high-\rfe\ data subsets obey the
same $R-L$ relation within the error bars. (2) Extending the 2-parameter $R-L$
relation to a 3-parameter one does not result in the hoped-for reduction in the
intrinsic dispersion of the $R-L$ relation. (3) Neither of the 3-parameter
$R-L$ relations provide a significantly better fit to the measurements than
does the 2-parameter $R-L$ relation. These are promising results for the
on-going development of \Mgii\ cosmological probes. The first and third of
these results differ significantly from those we found elsewhere from analyses
of reverberation-measured \hb\ QSOs.
