deletions | additions       diff --git a/Stellar atmosphere model.tex b/Stellar atmosphere model.tex  index e0c8ac3..3d8f006 100644  --- a/Stellar atmosphere model.tex  +++ b/Stellar atmosphere model.tex 
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\section{Stellar atmosphere model}\label{atm}  % Yeah, so this needs to happen We use the radiative transfer code MOOG \citep{sne73} to derive $T_{\rm{eff}}$, $\log g$, and metallicity for the two red giants. This is tricky because we have \begin{itemize}  \item First, disentangle spectra using FDBinary  \item Next, identify metallicity-sensitive Fe  lines from two stars, but hey, they're similar, so that's good, right? in each disentangled spectrum with ARES  \item Finally, run MOOG  \end{itemize}  IN PROGRESS