\begin{document}$ \alpha $\end{document}, the shadow aligns within \begin{document}$ 2\sigma $\end{document}uncertainty for homogeneous plasma and within \begin{document}$ 1\sigma $\end{document} for nonhomogeneous plasma. Next, we determine the energy emission rate for the Kerr MOG BH and analyze the influence of parameters α, \begin{document}$ k_o $\end{document}, \begin{document}$ k_\theta $\end{document}, and \begin{document}$ k_r $\end{document}on particle emissions in the BH vicinity. We further analyze the deflection angle in the presence of homogeneous and nonhomogeneous plasma profiles. The findings indicate notable differences from the vacuum scenario, underscoring the importance of accounting for plasma effects in examining light propagation around compact objects."> Shadow cast by the Kerr MOG black hole under the influence of plasma and constraints from EHT observations -
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