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Since the first detection of intracluster planetary nebulae in 1996, imagingand spectroscopic surveys identified such stars to trace the radial extent andthe kinematics of diffuse light in clusters. This topic of research is tightlylinked with the studies of galaxy formation and evolution in dense environment,as the spatial distribution and kinematics of planetary nebulae in theoutermost regions of galaxies and in the cluster cores is relevant for settingconstraints on cosmological simulations. In this sense, extragalactic planetarynebulae play a very important role in the near-field cosmology, in order tomeasure the integrated mass as function of radius and the orbital distributionof stars in structures placed in the densest regions of the nearby universe.

Extended halos and intracluster light using Planetary Nebulae as tracers in nearby clusters