Overproduction factors ⟨F_i⟩ (Eq. (1)) mass-averaged over all PPLs for all p-nuclides when considering the ¹⁷O(α,γ)²¹Ne rate of Best et al. (2013, top panel), Best et al. (2013) divided by 10 (middle), and Taggart et al. (2019, bottom panel). The filled symbols highlight the n_pp-nuclides (Table 2) that have the highest overabundances, i.e. those with ⟨F_i⟩ higher than the highest value divided by an arbitrary factor of 20. The green curves show the velocity-averaged yields over the three 25 M_⊙ models assuming they follow the rotational distribution of observed young B stars from Huang et al. (2010, their Fig. 6). See text for more details.