Proper motions of the optically visible open clusters based on the UCAC4 catalog

By W. Dias, H. Monteiro, T. C. Caetano, J. Lépine, M. Assafin, A. F. Oliveira. 2014

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A Gaia DR2 view of the open cluster population in the Milky Way (2018, background): “This was noted for instance by Dias et al. (2014) and Netopil et al. (2015).”
FIRST RESULTS FROM HIGH ANGULAR RESOLUTION ALMA OBSERVATIO NS TOWARD THE HL TAU REGION (2015, methodology): “For comparison, the weighted average of optical and infrared proper motions for HL Tau listed in Vizier22 since 2000 (e.g. Dias et al. 2014; Zacharias et al. 2013; Roeser et al. 2010) isvR.”
On the metallicity of open clusters. III. Homogenised sample (2015, methodology): “For the few remaining objects we used the additional literature (e.g. proper motion membership by Dias et al. 2014).”
BANYAN. XI. The BANYAN Σ Multivariate Bayesian Algorithm to Identify Members of Young Associations with 150 pc (2018, background): “In order to identify more members, the Dias et al. (2014) list of 4 102 XFOR candidates was cross-matched with the Gaia-DR1.”