Distribution of the sample stars in the R − z plane (top left) as well as the three actions J_R − J_z (top right), J_R − J_ϕ = L_z (bottom left), and J_z − L_z (bottom right). With exception of the top left panel (coloured by parallax precision), colour indicates the number of stars per bin in each panel, with a lower limit of five stars per bin. Individual stars outside the bins are shown as black dots. Top left panel: increasing distance from the Sun, the parallax precision decreases. It also shows that with the exception of two special pointings, the Galactic plane (|b| < 10 deg) is neglected by GALAH. The individual action angle plots show that most of the stars move on circular orbits with solar Galactocentric orbit and angular momentum. Top right corner: decreasing density with a diagonal pattern up to a line which intercepts with J_R at 150 kpc km s⁻¹ and J_z at 20 kpc km s⁻¹ and with only few stars with larger actions. The J_R − L_z shows trends of a minority of stars to be on eccentric orbits which have their apocentre in the solar neighbourhood (sub-solar L_z and increased J_R) or eccentric orbits with pericentres in the solar vicinity (super-solar L_z and increased J_R). While stars do not show increased vertical actions in the J_z − L_z plane (bottom right), an increase vertical actions can be seen for stars with solar angular momentum.