Fig. 2

Examples of two galaxies, zcos_z1_202 and zmus_z1_125, used in this work. From the left to the right: HST images in the F814W filter (roughly corresponding to I) from the CANDELS survey, total Hα intensity maps, Hα velocity fields, and the comparison between model and data through position-velocity diagrams (P-Vs) taken along the kinematic major axis. Moment maps and P-Vs are extracted from the KMOS data cubes used in this paper. For the maps: white and black crosses are the adopted centres, the grey thick line is the adopted kinematic position angle. Empty circles denote the PSFs. For the P-Vs: the x-axis represents the offset along the major axis from the galaxy centre, the y-axis the line-of-sight velocity in km s-1 centred at the systemic velocity of the galaxy. Data are shown as blue and grey (negatives) thin lines, our best models as thick red lines. The green dots denote the 3DBarolo’s rotation velocities. An equivalent figure for the full galaxy sample is available in .
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