Free Access

Fig. 4

thumbnail

Colourmagnitude diagram displaying the selection of sources considered stars (selected as explained in Sect. 2.2). The plume on the red side (g − r ≈ 1.2) is composed of the nearby M-dwarfs, whereas the main sequence on the bluer side (0.18 < g − r < 0.6) corresponds to a halo overdensity located at a particular well-defined distance. The cloud of sources at faint magnitudes are faint galaxies that enter the star selection. Left: CMD derived from an image that has not been PSF-corrected. Right: CMD derived from a PSF-corrected image. After homogenizing the PSF, the galaxy contamination decreases markedly below r ≈ 22.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.