Light curve and sky map of the AGN CAZJ2114+8204 which is spatiotemporally associated with the neutrino IC190629A (W_T = 0.003). For plot details, see description of Fig. 3. We note that around the neutrino arrival time, the quality of the merged CAZ light curve is poor (i.e., the filters exhibit substantial discrepancies in contemporaneous flux densities). However, it appears that the identified BBHOP, whose peak is the BB95 which coincides with the neutrino arrival, reliably traces the overall behavior of optical emission. We caution that, unlike all other such plots, the x- and y-axis of the sky map are not equal in scale. This blazar has another neutrino association (IC140410A; W_T = 0.003) which arrives before the CAZ light curve starts.