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The $^{22}\rm{Ne}(\alpha,\gamma)^{26}\rm{Mg}$ is an important reaction instellar helium burning environments as it competes directly with one of themain neutron sources for the s-process, the$^{22}\rm{Ne}(\alpha,n)^{25}\rm{Mg}$ reaction. The reaction rate of the$^{22}\rm{Ne}(\alpha,\gamma)^{26}\rm{Mg}$ is dominated by the low energyresonances at $E_{\alpha}^{lab}$ = 650 and 830 keV respectively. The$E_{\alpha}^{lab}$ = 830 keV resonance has been measured previously, but thereare some uncertainties in the previous measurements. We confirmed themeasurement of the $E_{\alpha}^{lab}$ = 830 keV resonance using implanted$^{22}$Ne targets. We obtained a resonance strength of $\omega\gamma$ = 35$\pm$ 4 $\mu eV$, and provide a weighted average of the present and previousmeasurements of $\omega\gamma$ = 35 $\pm$ 2 $\mu eV$ with reduced uncertaintiescompared to previous studies. We also attempted to measure the strength of thepredicted resonance at $E_{\alpha}^{lab}$ = 650 keV directly for the first timeand found an upper limit of $\omega\gamma$ $\mathrm{<0.15}$ $\mu eV$ for thestrength of this resonance. In addition, we also studied the $E_{P}^{lab}$= 851keV resonance in $^{22}\rm{Ne}(p,\gamma)^{23}\rm{Na}$, and obtained a resonancestrength of $\omega\gamma$ = 9.2 $\pm$ 0.7 eV with significantly loweruncertainties compared to previous measurements.

Direct measurement of the low energy resonances in $^{22}\rm{Ne}(\alpha,\gamma)^{26}\rm{Mg}$ reaction