This article has 2 errata:
[https://doi.org/10.1051/0004-6361/202039217]
[https://doi.org/10.1051/0004-6361/201832698e]
Fig. A.10
Parallaxes and residual PMs of sources in the LMC. The lines show the median value as a function of coordinate position x for all LMC sources within 0.2° stripes centred at y = −0.5, 0 or 0.5°. Residual PMs are calculated after subtraction of a model disc with parameters determined using only sources within 3° of the centre. The non-zero values are due to both the systematic errors in the Gaia data and the differences between the simple disc model and the true dynamics of the LMC.
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