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This article has 2 errata:
[https://doi.org/10.1051/0004-6361/202039217]
[https://doi.org/10.1051/0004-6361/201832698e]
Fig. 5
Density distribution on the sky of the stars selected as members of the LMC (left) and SMC (right). Positions are shown in the (x, y) coordinatesdescribed in the text (Eq. (2)). In all figures that use this coordinate system, the x-axis has been inverted so that it corresponds to the usual inversion of right ascension.
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