  On 22 September 2017, IceCube reported a high-energy neutrino event which was
found to be coincident with a flaring blazar, TXS 0506+056. This
multi-messenger observation hinted at blazars contributing to the observed
high-energy astrophysical neutrinos and raised a need for extensive correlation
studies. Recent work shows that the internal absorption of gamma rays, and
their interactions intrinsic to the source and with the extragalactic
background, will cause a lack of energetic gamma-ray and neutrino correlation
while hinting towards a correlation between neutrinos and lower photon energy
observations in the X-ray and radio bands. Studies based on published IceCube
alerts and radio observations report a possible radio-neutrino correlation in
both gamma-ray bright and gamma-ray dim active galactic nuclei (AGN). However,
they have marginal statistical significance due to limited available data. We
present a correlation analysis between 15 GHz radio observations of AGN
reported in the MOJAVE XV catalog and 10 years of IceCube detector data and
discuss the results derived from a time-averaged stacking analysis.
