Extended Data Fig. 1: Observed radio emission in our high-z galaxy cluster sample.
From: Fast magnetic field amplification in distant galaxy clusters
In colorscale we show the full-resolution LOFAR images. Low- resolution source-subtracted radio contours, displayed at the [-2,2,3,4,5,8,16]xσrms level, are shown only for clusters that host diffuse radio emission (with σrms the individual map noise; the negative contour levels are indicated with a short- dashed line style). The full- and low-resolution LOFAR beams are displayed in the bottom left corner (in pink and grey colors, respectively). In the header of each image, the galaxy cluster name, mass and redshift are reported. The dashed black circle in each map shows the R = 0.5RSZ,500 region, obtained from MSZ,500.
