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Fig. 9.
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Total intensity map of Abell 3376 at a resolution of 8″ × 8″, with five example spectra from the cluster relics and two from the bright AGNs. Each spectrum has been shifted by local estimates of the Galactic Faraday rotation. The spectra are color-coded as in Figs. 4 and 5, together with the magnitude shown in red.
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