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Gerrit Schellenberger is leading a project whereby the HIFLUGCS cluster sample The Mass Function of an X-Ray Flux-limited Sample of Galaxy Clusters (Reiprich , T. H. & Böhringer, H. 2002, ApJ, 567, 716) is used to examine the effective area cross-calibration uncertainties between Chandra/ ACIS and XMM-Newton/EPIC instruments.

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