This article has 2 errata:
[https://doi.org/10.1051/0004-6361/201527565]
[https://doi.org/10.1051/0004-6361/201423481e]
Fig. 2
CMD resulting from our work (left) compared to the results of Ramírez et al. (2008). The green line connects the mean colours in given magnitude intervals and the red line shows the unreddened giant sequence. The red arrow indicates the reddening law used in this work. The dashed blue lines indicate magnitude and colour cuts applied to the detected stars.
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