Notes.The F- and M-model name in the first column refers to the nomenclature of Valle et al. (2017), Tables 2 and 3. The G-I to G-III models refer to our additional tests. The Δ age column shows the minimal age difference between the secondary and the primary, determined from the age-radius evolution (see text). Columns 6 and 7 specify the primary’s He-core mass at the end of the main sequence and the maximum radius at the tip of the RGB, respectively. In Col. 7 a value over 46 R_⊙ indicates that Roche-lobe overflow would happen during the red giant phase. Columns 8 to 10 give the radius, effective temperature, and luminosity of our best-fit models in the form “primary/secondary”. The final column contains comments, if the calculations deviated from the default specification.