Stellar evolution tracks from Dartmouth models, from the zero age main sequence stage to 25 Gyr age, in the luminosity-effective temperature plane for [Fe/H] = 0.15. The results from the photodynamical modelling using stellar models are denoted by the grey contours corresponding to 39.3%, 86.5%, and 98.9% joint confidence regions. The mass in solar masses is annotated at the beginning of the main sequence of each track.