Multi-wavelength view of the merging cluster ClG 0217+70. The color image is the NXB subtracted, vignetting corrected, and adaptively smoothed 1–3 keV Chandra flux map. The white contours are compact source subtracted VLA L-band D configuration radio intensities at 3σ_rms × [1, 2, 4, 8] levels, where σ_rms = 70 μJy. Individual diffuse radio sources are labeled following the terms of Brown et al. (2011), where source A is the giant radio halo and B–G are relic candidates. The dashed circle represents r₂₀₀. The northern and southern X-ray surface brightness discontinuities and the western “channel” are indicated by cyan arcs and an annulus sector.