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Fig. 3


Comparison between the KMOS data cubes (thin blue contours, upper panels) and the 3DBarolo best-fit model-cubes (thick red contours, lower panels) for the high-mass galaxy zcos_z1_202 at z = 0.84 (top) and the low-mass galaxy zmus_z1_125 at z = 0.99 (bottom). Negative contours are shown as thin grey lines in the data. Cyan crosses represent the centre of the galaxies. We show five representative channel maps: the central panels represent the channel closest to the systemic velocity of the galaxy, the rightmost and leftmost panels indicate the extreme velocities, and the second and fourth panels indicate the intermediate velocities. Boxes have sizes of about 3′′ × 3′′, the PSFs are 0.72′′ for zcos_z1_202 and 0,79′′ for zmus_z1_125.

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