Fig. 1.

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Characteristics of the GOG simulated samples. Top left and middle: distribution of proper motions in right ascension and declination, respectively. In orange and blue: LMC and the MW training samples. Top right: parallax distribution. Bottom left: magnitude G distribution of the simulated samples. Bottom middle and right: colour-magnitude diagram of the LMC and MW, respectively. Colors represent relative stellar density, with darker colors meaning higher densities.
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