Output from the simulation of a star-forming disk galaxy as it would appear at z = 2 before it was beam smeared. Shown are the distribution of the star-formation rate intensity (left panel), Hα velocity field (center panel) and Hα dispersion map (right panel). The galaxy is projected at an inclination angle of 45° relative to face-on. The scale on the axes is in kpc and the kinematic axis is horizontal. Despite the different units (kpc vs. arcsec), we note that the sizes of these panels and those in Fig. 6 are similar, for ease of direct comparison.