Comparison of our membership determination in NGC 6380 to that of S24. Diagrams and point descriptions as in Figure 1, but with yellow points indicating members selected by S24, and green pentagons showing duplications in their selection. The typical error in PM is about 0.01 mas yr⁻¹ for both pmRa and pmDec, and in the RV versus metallicity plot, typical errors are shown in red. S24 included a number of stars that do not satisfy our more stringent membership requirements.