  We present the results of our search for Lyman continuum (LyC) emitting AGN
at redshifts 2.3$\lesssim$z$\lesssim$4.9 from HST WFC3 F275W observations in
the UVCANDELS fields. We also include LyC emission from AGN using HST WFC3
F225W, F275W, and F336W found in the ERS and HDUV data. We performed exhaustive
queries of the Vizier database to locate AGN with high quality spectroscopic
redshifts. In total, we found 51 AGN that met our criteria within the UVCANDELS
and ERS footprints. Of these 51, we find 12 AGN had $\geq$4$\sigma$ detected
LyC flux in the WFC3/UVIS images. Using space- and ground-based data from X-ray
to radio, we fit the multi-wavelength photometric data of each AGN to a CIGALE
SED and correlate various SED parameters to the LyC flux. KS-tests of the SED
parameter distributions for the LyC-detected and non-detected AGN showed they
are likely not distinct samples. However, we find that X-ray luminosity,
star-formation onset age, and disk luminosity show strong correlations relative
to their emitted LyC flux. We also find strong correlation of the LyC flux to
several dust parameters, i.e., polar and toroidal dust emission, 6 $\mu m$
luminosity, and anti-correlation with metallicity and $A_{FUV}$. We simulate
the LyC escape fraction ($f_{esc}$) using the CIGALE and IGM transmission
models for the LyC-detected AGN and find an average $f_{esc}$$\simeq$18%,
weighted by uncertainties. We stack the LyC flux of subsamples of AGN according
to the wavelength continuum region in which they are detected and find no
significant distinctions in their LyC emission, although our $sub-mm\ detected$
F336W sample shows the brightest stacked LyC flux. These findings indicate that
LyC-production and -escape in AGN is more complicated than the simple
assumption of thermal emission and a 100% escape fraction. Further testing of
AGN models with larger samples than presented here is needed.
