X-ray flux–mass relation for z ≳ 0.7 galaxy clusters

Open Access

Fig. 4.

ACT masses $M_{500 c}^{UPP}$ $M^{\mathrm{UPP}}_{\mathrm{500c}}$ for the subsample of the ACT DR5 clusters with 0° < l < 180° vs. eROSITA 0.5−2.0 keV fluxes extracted from a circle of R = 2′ arcmin centered at a cluster. The dashed, solid, and dotted lines show the F_X − M_500c relation (Eq. 3) with η = 1.0, 0.8 and 0.6, correspondingly. Cluster redshifts are shown with colors.

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