Fig. 1.
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uGMRT Band 4 (550–850 MHz) image of the galaxy cluster Abell 2256 with an angular resolution of 12″, highlighting the spectacular central halo emission, the filamentary relic, and radio galaxies in the field. The beam size is indicated in the bottom left corner of each image. The image is created with Briggs weighting using robust = −0.5. The rms is 14 μJy beam−1.
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