Identification of a dwarf galaxy stream in Gaia, and its possible association with the vast polar structure

Open Access

Fig. B.1.

The distribution of the member stars in the color magnitude diagram, B_P − R_P versus G within different longitude ϕ₁ ranges. The common stars with LAMOST and DESI are marked with red and magenta dots, respectively. The horizontal dashed line in each panel represents G = 17.6 for testing the distance gradient.

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