Image Details
Caption: Figure 7.
A histogram of the Galactocentric velocities of APOGEE stars at (l,b) = (5.°5,0°) (bottom) and the APOGEE+AAT stars at (l,b) = (−5.°5,0°) (top). The best-fit curve to the histogram from a k-means clustering algorithm and a GMM is overlaid. The mean and standard deviations of these distributions are given in Table 3.
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