tokens: We thank Chris Belczynski for providing tabulated data to map between ZAMS stellar masses and final compact remnant masses, and Tod Lauer for assistance in interpreting the Nuker data sets. We thank Iair Arcavi and Suvi Gezari for providing useful data on the peak luminosities of observed TDEs. We thank Brad Cenko, Jacqueline van Gorkum, Morgan MacLeod, Jeremiah Ostriker, Greg Snyder, Linda Strubbe, and Sjoert van Velzen for helpful conversations. Finally, we also thank the anonymous referee for many useful suggestions. BDM gratefully acknowledges support from the NSF grant AST-1410950 and the Alfred P. Sloan Foundation. This work was supported in part by the National Science Foundation under Grant No. PHYS-1066293 and the hospitality of the Aspen Center for Physics.
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