The purpose of this document is to generate a reliable primary beam
model for AARTFAAC-6. This is necessary to compensate for the primary
beam response in all-sky images, whose effect is to attenuate sources
away from the pointing center. The AARTFAAC system piggybacks on the
LOFAR antennae in 12 stations including the 6 superterp stations and the
first ring of station surrounding it.