keV, $1985.6 \pm 1.3$ keV, $2062.3 \pm 1.5$ keV and $2145 \pm 5$ keV are attributed to the $\beta$-$\gamma$ decay of $^{22}Al$. In fact, four $\gamma$-ray transitions at $1246.98 \pm 0.03$ keV, $1984.8 \pm 0.1$ keV, $2061.09 \pm 0.05$ keV and $2143.5 \pm 0.6 $ keV were previously established in $^{22}Mg$ (see [@firestone96], [@firestone05]). The $\gamma$ rays 6 and 10 should correspond to these known transitions. However, according to the reference [@firestone96], a known $\gamma$ ray at 1984 keV should be accompanied by another $\gamma$ ray at 891 keV with a relative branching ratio of 67%. From 657 counts observed in the $\gamma$ peak at 1985.6 keV we would expect 837 counts at 891 keV. This is not the case. We deduce therefore that the $\gamma$ ray 9 measured at 1985.6 keV is compatible with the new adopted $\gamma$ transition in reference [@firestone05] with 100% relative branching ratio. From our measurement, this $\gamma$ ray is most likely emitted from a level situated at $5.294 \pm 0.003$ MeV in $^{22}Mg$. This assumption is in agreement with the adopted value of $5.29311 \pm 0.00015$ MeV and supported by theoretical calculations (see section \[sec:6\] below). The weak $\gamma$-ray labelled 11 in fig. \[fig:gamma\] 