  Makemake is one of the brightest known trans-Neptunian objects, as such, it
has been widely observed. Nevertheless, its visible to near-infrared spectrum
has not been completely observed in medium resolving power, aimed at studying
in detail the absorption features of CH$_4$ ice. In this paper we present the
spectrum of Makemake observed with X-Shooter at the Very Large Telescope
(Chile). We analyse the detected features, measuring their location and depth.
Furthermore, we compare Makemake's spectrum with that of Eris, obtained with
the same instrument and similar setup, to conclude that the bands of the CH$_4$
ice in both objects show similar shifts.
