Comparison with the results of other WG13 nodes. Left panels: differences between the stellar parameters expressed as this study minus other node. In each panel, fast rotators for which we estimate V sin i above 150 km s⁻¹ are indicated by lighter colours. Only one colour is used for the ON node because only slow rotators below that threshold were analysed. Right panels: position of each sub-sample in a Kiel diagram based on our parameters. Theoretical evolutionary tracks at solar metallicity and with ω_init = 0.8 (see Sect. 6 for definition) are overlaid (Georgy et al. 2013). The initial stellar mass (in solar units) is indicated.