Background-subtracted, exposure-corrected Chandra mosaic of PLCKG287 in the [0.5–7.0] keV band smoothed with a kernel of 4 pixels (1 ACIS pixel = 0.492″). The detected point sources (shown with green ellipses in the right panel of Fig. 1) have been subtracted. The green circle indicates R₅₀₀ = 1541 kpc. Overlaid in white are the GMRT radio contours at 330 MHz (levels start at ±3σ and increase by a factor of 2, where σ = 0.1 mJy/beam, beam = 12.9″ × 7.9″). The radio data shows two prominent radio relics to the NW and SE at distances of ∼500 kpc and ∼2.8 Mpc kpc from the cluster center. The bright X-ray core region is coincident with a giant radio halo. See Bonafede et al. (2014) for more details on the radio features.