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We discuss the predicted performance of the HARMONI spectrograph and the ELTin the context of two specific science cases: resolved stellar populations ofLocal Volume galaxies and Galactic archaeology in dense environments. We haveproduced and analysed a set of simulated data-cubes using the HSIM software,mimicking observations across the giant elliptical galaxy Centaurus A and inthe nuclear bulge of the Milky Way. We use our results to demonstrate theinstruments capabilities to perform stellar absorption line spectroscopy in alarge number of stars which will allow us to study the detailed kinematics andstellar population characteristics of these high density regions

From the inner Milky Way to Local Volume galaxies: resolved stellar populations with ELT-HARMONI