Microwave haze at WMAP and Planck frequencies using a full-sky template fit to the data. The morphology of the haze is remarkably consistent from band to band and between data sets, implying that the spectrum of the haze does not vary significantly with position. Furthermore, the ν^2.5 scaling again yields about equal-brightness residuals, indicating that the haze spectrum is roughly T_ν ∝ ν^-2.5 through both the Planck and WMAP channels. In addition, while striping is negligible at low frequencies, above ~40 GHz it becomes comparable with, or brighter than, the haze emission (see text).