
The photons are polarized in the horizontal plane with equal amounts of "s" and "p" light. The strong angular dependence is due to the coupling between emission direction, crystalline azimuthal orientation, and photon polarization. This is explained in the tight-binding calculation conducted by Gary Mankey and shown to the right of the data.
This data set shows that in any interpretation of photoemission data that does not integrate over a LARGE solid angle one must understand the
By the way, notice how much information is located in normal-emission photoemission (the center of each image) at this binding energy? Not much, eh? Imaging the full angular distribution provides much more information.