We study the correlation between compact radio quasars or 3EG gamma-ray bla
zars and the arrival direction of cosmic rays above 10(19) eV using an upda
ted list of air shower detections. Our Monte Carlo simulations reveal no si
gnificant correlations above random results, and some previous positive res
ults appear to be an effect of the small sample size. Consequently, there i
s no evidence for ultrahigh energy cosmic ray primaries being new particles
or particles with new interactions beyond the electroweak scale, produced
in high-redshift active galactic nuclei.