Notes. Columns log ϵ(B)...v sin i present empirical parameters based on the mentioned references. The typical 1-σ error for T_eff (log g) of 1000 K (0.1cm/s²) is adopted when not provided. If v_eq is available, it is shown in parenthesis in the v sin i column. In some occasions, v sin i is larger than v_eq since the former reflects the total line broadening which may include turbulence, pulsations, and rotation (Morel et al. 2008). Columns Mass...P_ev / P_T,L / P_T,g / Π are the results from our Bayesian analysis (see text). In particular, columns Mass, Age, v_{rot, i} are the results for the mixing efficiency f_c which leads to the maximum probability Π. Values of P_ev, P_T,L, P_T,g, and Π that are smaller than 0.05, 0.1, 0,1, and 0.6, respectively, are marked in red. The last column presents information about the longitudinal magnetic field strengths (preceded by ^m) and binary properties (preceded by ^b), if known, with their references. Magnetic field values are given in Gauss, where boldface values highlight stars in which all the corresponding references report field detection, while the plane values highlight stars in which not all the corresponding references report field detection. When multiple measurements exist, we show the value with the highest significance. “Non-det.” means that no magnetic field was detected, while “N/A” implies that spectropolarimetric data was taken but a magnetic field measurement was not attempted (Wade et al. 2016). Binary properties show binary type / P_orb / e / (R/R_RL)_max, with binary type as SB1, SB2, or EB (eclipsing binary), and (R/R_RL)_max denoting the maximum possible ratio of the stellar radius over the Roche lobe radius (see text). Most of the orbital periods (P_orb) and eccentricities (e) are obtained via SB9: The ninth catalog of spectroscopic binary orbits (Pourbaix et al. 2004). Stars in NGC 3293 are marked in bold (except for the last column).

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