The dynamical evolution tracks (M_p and a) of all large planets in IGM16 simulation 1 around a 0.49 M_⊙ star. The coloured solid lines represent different planets. The transparent dashed lines represent large planetesimals that merged with the planets. Only planets with masses > 0.01 M_E are included. The cyan shaded region indicates the habitable zone. In the 0.49 M_⊙ simulations, the planets that form at a late stage in the disc (t ≳ 1 Myr) form outside the HZ and remain too small to migrate into it.