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We investigate the use of next generation radio telescopes such as the SquareKilometre Array (SKA) to detect axion two-photon coupling in the astrophysicalenvironment. The uncertainty surrounding astrophysical magnetic fields presentsnew challenges, but with a frequency range corresponding to axions of mass$1.7-57\mu$eV and a spectral profile with a number of distinguishing features,SKA-mid offers a tantalising opportunity to constrain axion dark matterproperties. To determine the sensitivity of SKA-mid to an axion signal, weconsider observations of the Galactic centre and interstellar medium, and findthat this new telescope could allow us to probe axion couplings$\gtrsim10^{-16}$GeV$^{-1}$.

Searching for Axion Dark Matter using Radio Telescopes