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We explore the variation in stellar population ages for Coma cluster galaxies as a function of projected cluster‐centric distance, using a sample of 362 red‐sequence galaxies with high signal‐to‐noise ratio spectroscopy. The sample spans a wide range in luminosity (0.02–4 L*) and extends from the cluster core to near the virial radius. We find a clear distinction in the observed trends of the giant...
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