Most radio astronomical observations are affected to some degree by ma
n-made and natural interference. There are a few avoidance techniques
that can reduce the impact of interference an the survey, but we must
make quite significant advances in the understanding of our antennas a
nd receivers and the interference itself before a substantial improvem
ent can be expected. A major increase in the efficiency of future surv
eys will likely come from phased-array feeds, which have the potential
for much closer beam spacings, greater antenna efficiency, and wider
fields of view than current independent-feed arrays.