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Fig. 2
One of largest tile-to-tile magnitude zero-point variations in the T0005 data. The position of the stellar sequence in the (g − r) vs. (u − g) plane is compared for tile #9 and tile #11 in the W4 VIPERS area (see Appendix C), showing an offset of ~ 0.15 mag in (g − r) and ~ 0.06 in (u − g) between the two tiles.
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