  The $^{20}$Ne$(p, \gamma)^{21}$Na reaction is the starting point of the NeNa
cycle, which is an important process for the production of intermediate mass
elements. The $E_{\text{cm}} = 1113$ keV resonance plays an important role in
the determination of stellar rates for this reaction since it is used to
normalize experimental direct capture yields at lower energies. The commonly
accepted strength of this resonance, $\omega \gamma = 1.13 \pm 0.07$ eV, has
been misinterpreted as the strength in the center-of-mass frame when it is
actually the strength in the laboratory frame. This has motivated a new
measurement of the $E_{\text{cm}} = 1113$ keV resonance strength in
$^{20}$Ne$(p, \gamma)^{21}$Na using the DRAGON recoil mass spectrometer. The
DRAGON result, $0.972 \pm 0.11$ eV, is in good agreement with the accepted
value when both are calculated in the same frame of reference.
