Kinematic maps from NIRSpec. From left to right: maps of the stellar velocity and velocity dispersion, gas velocity from the binned data, and Paα velocity from the spaxel-wise analysis. Velocities are relative to the assumed systematic velocity of 1068 km s⁻¹. The black contours are flux contours of the F360M image to guide the eye and the crosses mark the positions of the three clusters. Only bins with velocity uncertainties < 10 km s⁻¹ or velocity dispersion uncertainties < 15 km s⁻¹ are shown. For the unbinned Paα maps, only spaxels with S/N > 10 are shown.