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We discuss the impact of the uncertainty ( keV) in the excitation energy of the astrophysically important 6.356 MeV state of O on the precision with which the Coulomb reduced ANC () for the $\left<^{17}(1/2^+_2) \mid \protect{^{13}} + \alpha \right>$ overlap can be extracted from direct reaction data. We find a linear dependence of on the binding energy, the value extracted varying by a factor of 4 over the range – MeV. This represents an intrinsic limit on the precision with which can be determined which cannot be improved unless or until the uncertainty in is reduced.

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