Two eclipses of pulsar A detected with MeerKAT using the UHF (left) and L-band (right) receiver systems. These light curves were generated after averaging over the full receiver bandpasses. We have inflated the flux uncertainties by the median recovered EQUAD for each eclipse. The orange traces correspond to the median a posteriori light-curve models recovered from fitting the observations. Bottom panels show the residuals after subtracting the median model.