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The Galactic halo has a complex assembly history, which can be seen in itswealth of kinematic and chemical substructure. Globular clusters lose starsthrough tidal interactions with the Galaxy and cluster evaporation processes,meaning that they are inevitably a source of halo stars. These "migrants" fromglobular clusters can be recognized in the halo field by the characteristiclight element abundance anticorrelations that are commonly observed only inglobular cluster stars, and the number of halo stars that can be chemicallytagged to globular clusters can be used to place limits on the formationpathways of those clusters.

Rediscovering the origins of the stellar halo with chemical tagging