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Fig. 7

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Left panel: RGS 1 and 2 first order and ASTRO-H SXS effective area. Right panel: ASTRO-H SXS 100 ks simulations for the bright Perseus cluster and three groups of galaxies zoomed in the RGS energy band (see Sect. 5.4). We adopted the 3.4′ RGS models as a template (see Fig. A.7).

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