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tokens: We thank the anonymous referee for comments which were beneficial to the final version of this paper. M.B.P. and S.E.Z. acknowledge support from NASA through the ADAP grant NNX11AG12G. B.D.L acknowledges support from NASA ADAP NNX16AG06G. The scientific results reported in this article are based on observations made by the Chandra X-ray Observatory . Support for this work was provided by NASA through Chandra Award numbers GO5-16084A (MBP) and GO5-16084B (AK) issued by the Chandra X-ray Observatory Center, which is operated by SAO for and on behalf of the NASA under contract NAS8-03060. Based on observations made with the NASA/ESA Hubble Space Telescope , obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program HST-GO-13942.001-A. Support for program number HST-GO-13942.001-A was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. This research has made use of NASA’s Astrophysics Data System (ADS) and the NASA/IPAC Extragalactic Database (NED). Facilities: CXO, HST , 2MASS. Software: SciPy, NumPy, matplotlib, pythonFSPS, TOPCAT, ds9.