  In this review we address the progress that has been made toward the
understanding the population of Magellanic Cloud planetary nebulae since the
last Magellanic Cloud Symposium. Planetary nebulae in the Clouds are not only
important as key probes of stellar and ISM evolution in these galaxies, but
also reflect the evolution of AGB stars and beyond in low-metallicity
environments. We present the recent surveys results, including the wide fields
ground-based search for PNe, the {\it HST} study of the resolves ejecta and
their central stars, and the {\it Spitzer} analysis of the gas contents of
these ejecta. Finally, we show how Magellanic Cloud PNe can be used to
constraint the distance scale of galactic PNe.
