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