Stellar velocity (top row), velocity dispersion (second row), h₃ (third row), and h₄ (fourth row) for GECKOS galaxy IC1711 calculated over the wavelength ranges of Hβ and Mgb (4750–5500 Å; first column), and the CaT (8458–8935Å, middle column) binned to SN = 100. The right column shows the difference between the two. The most obvious feature is seen at the centres of the V_⋆ and h₃ maps; evidence for a nuclear disc is seen in the CaT maps, but is absent (and presumably hidden by the dust lane) in the Hβ maps.