The glow of axion quark nugget dark matter - II. Galaxy clusters

Open Access

Fig. A.2

Radial profiles of $\tilde{J} (r)$ $\mathop J\limits^ \left( r \right)$ (see Eq. 38) for cross-correlated galaxy clusters that showed a thermal AQN emission excess in the spectral features. Galaxy clusters with high $\tilde{J}$ $\mathop J\limits^$ in Fig. 7 exhibit higher $\tilde{J} (r)$ $\mathop J\limits^ \left( r \right)$ in central regions of the galaxy cluster.

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