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\subsection{Stellar parameters}\label{parameters}  We use the radiative transfer code MOOG \citep{sne73} to derive $T_{\rm{eff}}$, $\log g$, and metallicity for the two red giants.  \begin{itemize}  \item Identify metallicity-sensitive Fe lines in each disentangled spectrum with ARES \citep{Sousa_2007}.  \item Then, run MOOG  \end{itemize}