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The integrated properties of young star clusters are subject to largecluster-to-cluster variations because they depend directly on small numbers ofbright stars. At ages at which red supergiants are expected to exist, theseluminous but rare stars can be blamed for most of the variations. If unresolvedclusters are to be used to constrain red supergiant models, methods must bedeveloped that take these stochastic fluctuations into account. We discussprospects and open issues in this field, based on recent work on high massclusters in M82, and on first experiments towards a Bayesian study of clusterpopulations.

Constraining the evolution of red supergiants with the integrated light of star clusters