Fig. 2

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Projected locations of the 1178 galaxy groups in the primary catalog in the eROSITA and Legacy Survey DR9N and DR10 13,116 deg2 common footprints. The redshift confirmed by the follow-up algorithm eROMaPPer is color coded (Kluge et al. 2024), while the sizes of the detections are scaled with the angular sizes (r500c) of the groups (see Sect. 3.3 for the r500c estimation procedure). The inhomogeneity of the source density in this figure is due to the exposure variation across the eROSITA-DE X-ray sky (see Fig. 2 in Bulbul et al. 2024).
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