Comparison between the structures of the MARCS to 〈3D〉 Stagger models. The top two panels show temperature as a function of optical depth at 5000 Å for model atmospheres of four types of stars. The open (giant stars) and solid (dwarf stars) black circles and squares show the MARCS model atmospheres for the parameters given in the legend (low metallicity to the left, solar metallicity to the right). The corresponding 〈3D〉 Stagger models are shown as cyan dots. The bottom two panels show the difference between the MARCS model and the 〈3D〉 Stagger model for each case, following the same convention for open and solid circles or squares as in the top panels.