Notes. Since no uncertainty on the effective temperature of the primary component of KIC 5193386 was available, we computed the error bar on its ν_max parameter using σ_Teff = 100 K, which is the typical order of magnitude of the uncertainty for this parameter. We note that the APOGEE DR14 rather suggests an uncertainty of 70 K (Abolfathi et al. 2018; Pinsonneault et al. 2018). However, given the low luminosity of this system (visible magnitude of 14.7, while the typical value for the rest of the sample is 13), its high luminosity ratio (L₂/L₁ = 0.33), and the uncertainties for the other binaries studied in this work (typically 150 K), we suspect this value to be underestimated. For the other stars, we used the uncertainty provided in Table 1.