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The 14N(p,γ)15O reaction controls the rate of CNO cycle hydrogen burning in various astrophysical sites and it is therefore one of the most important reactions in nuclear astrophysics. An experimental program is in progress to measure the 14N(p,γ)15O cross section in a wide energy range using a novel approach. A crucial quantity for the cross section determination is the number of N atoms in the target. In this paper the results of different experiments used for N target characterization are presented

Target characterizations for a 14N(p,γ)15O cross section measurement

Target characterizations for a ¹⁴N(p,γ)¹⁵O cross section measurement