Protoplanetary disc lifetimes and characteristic sizes for stellar masses between 0.6 M_⊙ and 1.4M_⊙. The disc masses were calculated from the scaling law of Appelgren et al. (2020) while the lifetimes were set to the time when all gas had either been lost due to X-ray photoevaporation or accreted onto the star. The disc lifetime increases with stellar mass where the maximum lifetime is 3 Myr for M_* = 1.4 M_⊙, in line with observations of young stars (Ribas et al. 2015).