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We study the possibility that Υ-ray loud active galactic nuclei (AGNs) are the sources of ultrahigh-energy cosmic rays (UHECRs) by using a correlation analysis of their locations and the arrival directions of UHECR. We use data for Υ-ray loud AGN with d ≤ 100Mpc from the second Fermi Large-area Telescope AGN catalog and UHECR data with E ≥ 55EeV observed by the Pierre Auger Observatory. The distribution of arrival directions expected from the Υ-ray loud AGN is compared with that of the observed UHECR by using the correlational angular distance distribution and the Kolmogorov-Smirnov test. We conclude that the hypothesis that the Υ-ray loud AGN are the dominant sources of UHECR is disfavored unless there is a large smearing effect due to intergalactic magnetic fields.