Fig. 13
Best-fit value of Ωm for XCS-DR1, with its 3σ uncertainty and the number of clusters in each region. Different uncertainty magnitudes for similar numbers of clusters are caused by the different scatter of the LX –T relation. Leftpanel: for Groups A and B. The rest of the sky has Ωm = 0.318 ± 0.071. Right panel:for the four “usual” quarters of the Galactic sky.
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