The VMC survey - XLV. Proper motion of the outer LMC and the impact of the SMC

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Fig. C.1.

Proper motion differences between Gaia EDR3 and VMC as a function of: parallax (ω), J − K_s colour, G magnitude, K_s magnitude, right ascension, and declination (from top to bottom) for both components of motion (from left to right).

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