Orbital decompositions of NGC 1380 and NGC 1427. Panel a-1: probability density distribution of the stellar orbits p(r, λ_z) in the phase space of time-averaged radius r versus circularity λ_z in units of stellar mass per unit area in the phase space. We show the model within 140 arcsecs (or ∼14 kpc) for NGC 1380. The stellar masses are normalized such that they sum to unity within the data coverage. Panels b-1 and c-1: stellar age t(r, λ_z) and metallicity Z(t, λ_z) distribution of the orbits in the same phase space. All distributions p(r, λ_z), t(r, λ_z), and Z(t, λ_z) are averages of multiple best fitting models that fall within the 1σ confidence level of the model hyperparameters. The dashed lines indicate our orbit-based division into four components: disk, warm, bulge, and hot inner stellar halo. Panels a-2, b-2, c-2: same but for NGC 1427, which does not have an extended disk.