The WMAP "haze" is an extended region of excess microwaves towards the
Galactic Center relative to known ISM
emissions. I will first present the results of our analysis of the morphological
and spectral features of the haze.
From there, I will show that they are consistent with synchrotron emission from
an injection of high energy
electrons/positrons sourced by ~500 GeV neutralino DM annihilations with
thermal relic cross section in the galactic
DM halo with a rho~r^-1.2 density profile and no boost factor. Further, I will
show that they are inconsistent with
a point source injection from massive explosions such as GRBs, SNe, etc. Halo
annihilations of this type have
significant consequences for present and future indirect observations such as
Planck, PAMELA, and GLAST.