\begin{document}${\cal{O}}(1)$\end{document} TeV. The LHAASO sensitivity to the DM decay lifetime reaches \begin{document}${\cal{O}} (10^{26}) \sim {\cal{O}} (10^{28})$\end{document} s for several decay channels at the DM mass scale from 1 TeV to 100 TeV."> Expected LHAASO sensitivity to decaying dark matter signatures from dwarf galaxies gamma-ray emission -
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