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The $^{22}$Ne($\alpha,n$)$^{25}$Mg reaction is an important source ofneutrons for the s-process. Due to the difficulty in directly measuring thecross section of this reaction and the competing$^{22}$Ne($\alpha,\gamma$)$^{26}$Mg reaction, indirect methods are frequentlyused to try to instead calculate the relevant reaction rates. Uncertainty,however, persists in the number and properties of the pertinent excited statesof $^{26}$Mg.  In this paper, the results of proton and deuteron scattering from $^{26}$Mgare presented, giving a list of levels in $^{26}$Mg. In addition, levelassignments in $^{26}$Mg are discussed, including some possible changes to thepreviously accepted assignments in $^{26}$Mg.

A high-resolution study of levels in the astrophysically important nucleus $^{26}$Mg and resulting updated level assignments