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Kinematically isolating intracluster light in AS1063: a distinct stellar population tracing the dark matter core
We present a technique using integral-field spectroscopy to kinematically isolate intracluster light (ICL) from the brightest cluster galaxy (BCG), enabling insights into their contrasting stellar populations and the inner dark matter halo profile. Applying this technique to MUSE data of Abell S1063
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