Fully cleaned (as in Fig. 1), CXB-subtracted, combined XMM-Newton-Suzaku mosaic image in the 0.5−2 keV band. The Suzaku data were calibrated to the XMM-Newton/MOS count rate. The emission from the cluster outskirts and the AGN residuals was removed from the Suzaku images, thus what is shown here is pure filamentary emission as detected by Suzaku. At the Suzaku's masked areas, the underlying XMM-Newton image is shown instead.