Fig. 7.
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2 × 2 degrees image showing a combination of the X-ray residuals (red, see Fig. 4) and radio emission by LOFAR from van Weeren et al. (2024). The radio image (blue-cyan colors) is itself composed from the 7″ (blue) and 80″ (green) resolution data. NGC 1275 mini-halo (and NGC 1272) dominates the center. The two most prominent off-center (tailed) galaxies are IC310 and NGC 1265 (see Gendron-Marsolais et al. 2020; van Weeren et al. 2024, for recent high-quality radio images of the Perseus cluster).
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