  Active Galactic Nuclei (AGN) are prime candidate sources of the high-energy,
astrophysical neutrinos detected by IceCube. This is demonstrated by the
real-time multi-messenger detection of the blazar TXS 0506+056 and the recent
evidence of neutrino emission from NGC 1068 from a separate time-averaged
study. However, the production mechanism of the astrophysical neutrinos in AGN
is not well established which can be resolved via correlation studies with
photon observations. For neutrinos produced due to photohadronic interactions
in AGN, in addition to a correlation of neutrinos with high-energy photons,
there would also be a correlation of neutrinos with photons emitted at radio
wavelengths. In this work, we perform an in-depth stacking study of the
correlation between 15 GHz radio observations of AGN reported in the MOJAVE XV
catalog, and ten years of neutrino data from IceCube. We also use a
time-dependent approach which improves the statistical power of the stacking
analysis. No significant correlation was found for both analyses and upper
limits are reported. When compared to the IceCube diffuse flux, at 100 TeV and
for a spectral index of 2.5, the upper limits derived are $\sim3\%$ and
$\sim9\%$ for the time-averaged and time-dependent case, respectively.
