This article has 2 errata:
[https://doi.org/10.1051/0004-6361/201527565]
[https://doi.org/10.1051/0004-6361/201423481e]
Fig. 10
Top left: profiles of the flux density of the NSC in 45 degree-wide wedges perpendicular to the Galactic plane (GP). Top right: profiles parallel to the GP. Bottom left: profiles at intermediate angles. The profile at 225° is systematically lower at 5−15 pc because of the dark cloud southwest of the NSC. Bottom right: mean profiles parallel and perpendicular to the GP. Angles increase east of north, with 0° corresponding to Galactic north.
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