Table 3

Properties observed by eROSITA and HSC of the eight clusters in the supercluster; see Fig. 1.

Cluster λ Tcin Lcin Tcex Lcex R500 M500 Mg,500 Counts
[keV] [1044 erg s−1] [keV] [1044 erg s−1] [arcmin] [1014M] [1014M]
eFEDS J093501.1+005418 143 ± 12 276
eFEDS J093510.7+004910 62 ± 9 125
eFEDS J093513.3+004746 208 ± 15 935
eFEDS J093520.8+003445 30 ± 6 106
eFEDS J093612.6+001651 32 ± 7 127
eFEDS J093546.4-000115 41 ± 7 147
eFEDS J093543.9-000334 41 ± 7 101
eFEDS J093432.2-002303 58 ± 8 231

Notes. We show the richness, best-fitting temperatures, and luminosity in units of keV and 1044 erg s−1, respectively,both core included and excluded, the masses and the gas masses both in units of 1014 M and the cluster counts in the [0.5–2.0] keV energy band. We remind the reader that the masses are computed using Bulbul et al. (2019) scaling relations, and the uncertainties reported refer to the sum in quadrature of the statistical uncertainty and the intrinsic scatter present in the scaling relations.

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