The14 N(p, γ) 15 O reaction regulates the power generated by the CN cycle and thus impacts the structure and evolution of every star at some point in its life. The lowest positive-energy resonance in this reaction is located at E c.m. r = 259 keV, too high in energy to strongly influence quiescent stellar burning. However, the strength of this resonance is used as a cross-section normalization for lower-energy measurements of this reaction. We report on new measurements of the energy, strength and γ-ray branching ratios for the 259-keV resonance, using different detection and dataanalysis schemes. We have also re-evaluated previous results, where possible. Our new recommended strength of ωγ = 12.6(3) meV is in agreement with the previous value of 13.1(6) meV, but is more precise and thus provides a more reliable normalization for low-energy (p,γ) measurements.