CARMA aims at determining the age of Milky Way globular clusters with unprecedented homogeneity and precision.
The combination of this chronological information with the cluster dynamical properties has the ambition of pushing the current knowledge on the assembly history of our Galaxy (and beyond) to uncharted grounds.
The updated chrono/dynamical information about the “Origin of the systems of globular clusters in the Milky Way” can be found at:
Table of GC ages and associations
Latest update: Gaia eDR3 / CARMA-I
If you use these data, please cite both these papers: