\begin{document}$\theta_{\infty}$\end{document} and relative magnification \begin{document}$r_m$\end{document} decrease while deflection angle \begin{document}$\alpha(\theta)$\end{document} and image separation s increase. The results will degenerate to that of the Kerr case, RN case with magnetic charge and Schwarzschild case when we take some specific values for the black hole parameters. The results also show that, due to the small influence of magnetic charge and EYM parameters, it is difficult for current astronomical instruments to tell this black hole apart from a General Relativity one."> Strong gravitational lensing of rotating regular black holes in non-minimally coupled Einstein-Yang-Mills theory -
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