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\section{Conclusions}  \begin{itemize}  Understanding the pre-explosion eruption is a major topic of the Scialog 2015 meeting, and one of the emerging themes is to measure the mass-loss history before explosion. We propose to measure the mass-loss history for a large sample of core-collapse SNe. Raffaella Margutti will orchestrate the observations, Jeremiah Murphy will simulate the shock-CSM interaction, and Matteo Cantiello will use these results to constrain mass-loss in stellar evolution  theory. \end{itemize}