Planet formation maps with and without the thermal torque from Masset (2017) using the Jiménez & Masset (2017) formula for the other torque components. Simulations were performed with an increased pebble flux of , i.e. about 950 M_E over 3 Myr. The plot should be read just like Fig. 2. Planets in the inner disk are significantly affected by the thermal torque due to the larger amount of pebbles. Planets that are inserted in the outer disk are not noticeably influenced by the thermal torque.