deletions | additions       diff --git a/Discussion.tex b/Discussion.tex  index ffa4bad..9bbeca5 100644  --- a/Discussion.tex  +++ b/Discussion.tex 
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\begin{equation}  \left( \frac{M}{M_\odot} \right) \simeq \left( \frac{\nu_{\rm{max}}}{\nu_{\rm{max,\odot}}} \right)^3 \left( \frac{\Delta \nu}{\Delta \nu_\odot} \right)^{-4} \left( \frac{T_{\rm{eff}}}{T_{\rm{eff,\odot}}} \right)^{1.5}.  \end{equation}\subsection{Stellar Activity}  \begin{itemize}  \item Discuss how different light curve ``chunks'' give different model results  \item Talk about any other weird or interesting things  \end{itemize}  \subsection{Results}\label{results}  \begin{itemize}  \item Quantitatively compare the Section \ref{model} results with the \citet{gau14} results described in Section \ref{seismo}  \item Make a clear figure that shows masses and radii from seismology vs. binary modeling  \end{itemize}  \subsection{Future Work}\label{future}  Model ALL the RG/EBs!