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Figure S1. A movie of the unsharp-masked X-ray emission of the simulated galaxy cluster. The X-ray emission was computed using an APEC thermal, collisionally ionized plasma, folded through the Chandra ACIS-I response. Colours are as follows: red = 0.5–2 keV, green = 2–5 keV, blue = 5–10 keV. QuickTime is required to view this MPEG-4 (h264 codec) movie. Figure S2. (a) A synthetic low-frequency radio synchrotron movie of the simulated galaxy cluster. The radio emission was computed assuming equipartition between particles and magnetic field pressure and neglected radiative losses on the electron population, appropriate for very low-frequency radiation. QuickTime is required to view this MPEG-4 (h264 codec) movie. Figure S2. (b) A movie of the X-ray emission of the simulated galaxy cluster.?The X-ray emission was computed using an APEC thermal,?collisionally ionized plasma, folded through the Chandra ACIS-I?response. Colours are as follows: red = 0.5–2 keV, green = 2–5 keV,?blue = 5–10 keV. QuickTime is required to view this MPEG-4 (h264 codec)?movie. Please note: Blackwell Publishing is not responsible for the content or functionality of any supplementary materials supplied by the authors. Any queries (other than missing material) should be directed to the corresponding author for the article.

FilenameFormatSizeDescription
mnl0243_suppfig1.zip2506KSupporting info item
mnl0243_suppfig2a.zip1535KSupporting info item
mnl0243_suppfig2b.zip764KSupporting info item

Please note: Wiley Blackwell is not responsible for the content or functionality of any supporting information supplied by the authors. Any queries (other than missing content) should be directed to the corresponding author for the article.