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tokens: J.L.D. acknowledges support for this work provided by NASA through Hubble Fellowship grant HF-51303.01 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. B.D.S. acknowledges support from the National Aeronautics and Space Administration (NASA) through Einstein Postdoctoral Fellowship Award Number PF5-160143 issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of NASA under contract NAS8-03060. C.L. acknowledges support from NSF grant AST-1004583. Finally, we thank the anonymous referee for discussions and comments that improved the paper.