Specific angular momentum for the 182 galaxies in the MUSE UDF mosaic fields with a max S/N ≳ 3. Left: total specific angular momentum (SFR weighted) as a function of stellar mass M_⋆. The points are color-coded as a function of V/σ_t. The right-axis shows the corresponding j_⋆ according to the 0.25dex offset found in Fig. 7. The blue (red) dashed line show the sequence for late (early) type galaxies at z = 0 from Fall & Romanowsky (2018, FR18). The dotted line (solid squares) show the z = 0 sAM j_⋆ − M_⋆ sequence from Posti et al. (2018a) (Lapi et al. 2018), respectively. The dotted line show the sequence for z = 0 disk galaxies of Posti et al. (2018a). The solid black line shows the expected j_⋆ − M_⋆ relation from Eq. (8). The solid blue and red lines show the fitted fiducial model from Eq. (9) and the gray band represents the 95% confidence interval. Right: normalized AM sequence as a function of (V/σ_t)_toz1 (normalized to z = 1 see text), i.e. after taking into account for the redshift evolution of σ_t(z), where the points are color-coded with redshift. In the inset, we show the redshift evolution of the sAM relation at M_⋆ = 10¹⁰ M_⊙ (solid line) at fixed (V/σ_t)_toz1 (=5) along with the 95% predictive interval (gray band), with the z = 0 ZP from Fall & Romanowsky (2018) (red square), the Swinbank et al. (2017) binned data (see text), and the expected (1 + z)^−0.5 evolution (dotted line) from Eq. (8).