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Fig. 8.

image

Upper panel: RVs differences for 71 common clusters between SC18 and our catalog. Bottom panel: RVs differences for 36 common clusters between DJ20 and our catalog. The solid circles and their corresponding error bars represent the mean RVs and dispersion of each cluster in our catalog, respectively. The color of the data points represents the number of stars used to estimate the average in our catalog. As a comparison of the results of overall RVs of OCs, the average difference for LAMOST-Gaia and LAMOST-APOGEE is −5.1 ± 6.4 km s−1 and −5.5 ± 5.4 km s−1, respectively.

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