  We study the correlation between compact radio quasars or 3EG gamma-ray
blazars and the arrival directions of cosmic rays above 10^19 eV using an
updated list of air shower detections. Our Monte Carlo simulations reveal no
significant correlations above random and some previous positive results appear
to be an effect of the small sample size. Consequently, unless somehow severely
deflected, there is no evidence for ultra-high energy cosmic ray primaries
being new particles or particles with new interactions beyond the electroweak
scale, produced in high-redshift active galactic nuclei.
