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In addition to this, our collaborators have provided high-resolution spectra from the Fred Lawrence Whipple Observatory (FLWO) 1.5 m telescope in Arizona using the Tillinghast Reflector Echelle Spectrograph (TRES) from 2012 March through 2013 April for KIC 9246715. These spectra are being used together with those from ARCES to derive an orbital solution in \citet{raw14}. Rawls et al. 2014 (in prep).  High-resolution spectra are essential to extract radial velocities for each system, and if the signals from the two stars can be disentangled they can be modeled to determine atmospheric parameters such as $T_{\rm{eff}}$, $\log g$, and metallicity. This is explored in more detail in Section \ref{specanal2}. \subsection{Ground-based Photometry}