Fig. 2.

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Xray-uGMRT (550−850 MHz) overlay Abell 2744. The intensity in red shows the radio emission observed with uGMRT Band 4 at a central frequency of 675 MHz. The intensity in blue shows Chandra X-ray emission in the 0.5−2.0 keV band (Pearce et al. 2017), smoothed to 3″. The image properties are given in Table 2, IM10. The presence of four relics and the halo suggests a complex, multiple mergers.
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