HIGHLIGHTS
- What: The aim of this work is to understand what the authors can learn if the authors include these new objects into the Milky Way globular cluster (GC) system that the authors know today. The authors compare the new sample compilation with previously published ones finding that the distributions are in good general agreement. The authors selected the clusters depending on their mean cluster PMs (where available), and the authors compare the sample with well-known Galactic GCs studied by Vasiliev and amp; Baumgardt . The authors investigate this to see how the known MW GC LF changes . . .

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