deletions | additions       diff --git a/subsection_Line_fitting_We_perform__.tex b/subsection_Line_fitting_We_perform__.tex  index bcb3519..dd894bf 100644  --- a/subsection_Line_fitting_We_perform__.tex  +++ b/subsection_Line_fitting_We_perform__.tex 
...
\subsection{Line fitting}  We perform Voigt profile fitting of the calcium II H \& K lines after dividing out the continuum spectrum and, in the case of the calcium II H lines, dividing out the Sersi\'c fit to the strong H$\epsilon$ line, which is centered at 230 km/s LSR in the calcium II H frame. The Milky Way rest and high-velocity lines are each best fit with two components in each of the the two Ca II lines  \begin{table}[ht]  \centering