deletions | additions       diff --git a/Conclusion.tex b/Conclusion.tex  index 59b0118..81f4086 100644  --- a/Conclusion.tex  +++ b/Conclusion.tex 
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\section{Conclusions}\label{conclude}  {\textbf{You should say somewhere thata second paper,  we will try in a second paper  to disentangle oscillations modes of both stars, based on accurate peak bagging using Bayesian methods, and invert the measured frequency to unambiguously model the systems with the help of MESA + GYRE}}. We have characterized the double red giant eclipsing binary KIC 9246715 with a combination of dynamical modeling, stellar atmosphere modeling, and global asteroseismology, and have investigated the roles of magnetic activity, tidal forces, and stellar evolution in creating the system we observe today. KIC 9246715 represents a likely future state of similar-mass RG/EB systems and raises interesting questions about the interactions among stellar activity, tides, and solar-like oscillations. 
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Red giants are ideal tools for probing the Milky Way Galaxy via asteroseismology, so it is crucial that we understand the accuracy and precision of asteroseismically-derived physical parameters. Along the same lines, more than half of cool stars should be in binary or multiple systems, so galactic studies must be done carefully due to external influences of binarity on solar-like oscillations. Detailed studies of the handful of known RG/EBs are crucial to ensure we understand these galactic beacons. Future work will characterize the other known oscillating RG/EBs as well as several non-oscillating RG/EBs. These have the potential to become some of the best-studied stars while simultaneously helping us better understand the structure of the Milky Way.