A new crowded-field light-profile fitting method yields light, kinematics, and stellar mass constraints for 289 cluster members plus the BCG and intra-cluster light in Abell S1063, feeding a future dark matter/baryon separation model.
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A comprehensive separation of dark matter and baryonic mass components in galaxy clusters I: Mass constraints from Abell S1063
A new crowded-field light-profile fitting method yields light, kinematics, and stellar mass constraints for 289 cluster members plus the BCG and intra-cluster light in Abell S1063, feeding a future dark matter/baryon separation model.