normalized to full occupancy. In addition, for the JLab data sets we fit a normalization factor for the independent particle shell model (IPSM) to the inclusive data in the range $10 \leq E_m \leq 80$ MeV according to $$\label{eq:NIPSM}
\sigma_\text{red} = N_\text{IPSM} 
\left( \sigma_\text{red}(1p) +  \sigma_\text{red}(1s) \right)$$ Calculations will be shown for the entire $p_m$ range measured for each data set, but only data in the range $|p_m| \leq 200$ MeV$c$ will used to fit the normalization factors because larger $p_m$ may be susceptible to increasing corrections for effects not contained in the RDWIA model based upon single-nucleon current operators.

We also require a model of the $1s$ energy distribution to obtain the spectroscopic factor from the normalization $N_{1s}(E_\text{min},E_\text{max})$ fit to limited and variable intervals of $E_m$. One often employs a Lorentzian distribution $$\label{eq:L}
L_{1s}(E_m) = \frac{1}{2\pi} \frac{\Gamma(E_m)}
{(E_m-E_{1s})^2 + (\Gamma(E_m)/2)^2}$$ whose energy-dependent width is given by the Brown-Rho parametrization [@Brown81] $$\label{eq:BR}
\Gamma(E_m) = \frac{ a (E_m - E_F)^2 }{(E_m-E_F)^2+b}$$ where $E_F$ is the Fermi energy and $a$,$b$ are constants. For the present purposes it suffices to use the parameters $a=24$ MeV and $b=500$ MeV$^2$ originally proposed by Brown and Rho [@Brown81] with $E_F = 15.96$ MeV and $E_{1s} = 