Abstract The reactions 13C(p,γ1,2)14N and 13C(p, p', γ(3.09, 3.68, 3.85))13C have been studied for Ep = 3.0 to 18 MeV, covering the giant dipole resonance in 14N. Below Ep = 7.0 MeV resonances in the γ0 yield were found at Ep = 3.771 MeV (Γc.m.≦ 2keV), 4.53 (115 ± 10), 5.32 (48 ± 7) and 6.2 (1000 ± 150), corresponding to excitation energies of 11.049, 11.74, 12.485 and 13.3 MeV, respectively. From the angular distribution, Jπ = 2+, 3+ was established for the 11.049 MeV state, which is thus a newly found excited state of 14N. In all other cases cross correlations exist with states reported in other reactions. The 13.3 MeV state is thought to be part of the giant dipole resonance. Above 7 MeV bombarding energy the (p, γo) yield shows broad structure and the giant dipole resonance with two peaks at 22.5 and 23.0 MeV excitation energy. All peaks can be related to structure observed in the inverse photonuclear (γ, po) reaction. The inverted (p, γo) cross section exhausts 18 % of the classical dipole sum-rule between 12 and 24 MeV. Angular distributions indicate that most of the GDR up to 24 MeV is related to Jπ = 2− states, in accordance with theoretical predictions. The (p,γ1) yield to the Jπ = 0+, T = 1 state in 14N averages only 1 5 of the γ0 yield and no giant resonance structure is evident up to 24 MeV. The expectations for the T = 0 GDR based on the 2.31 MeV state are discussed. It is suggested that two narrow resonances seen at excitation energies of Ex = 23.7 MeV (Γc.m.≈ 500 keV) and 24.2 MeV (Γc.m.≈ 100 keV) are the lowest Jπ = 1−, T = 2 states in 14N.