Pulsar orientation angles based on the analysis of frequency-dependent component separation and the PA sweep rate versus the assumed value of the emission cone opening angle at 1 GHz, ρ_{1 GHz}. The black lines show α(ρ_{1 GHz}) and β(ρ_{1 GHz}) for R_PA = −2.9°/°. Shaded regions mark a ± 0.5°/° uncertainty in R_PA, where the lower edge corresponds to a lower absolute value of R_PA. The stars mark the DR01 geometry solutions corresponding to the inner and outer cone ρ_{1 GHz} (white and black, respectively). The angles were converted into the EW01 notation according to Table 2.