Revealing the radio continuum and X-ray properties of the Galactic supernova remnant G5.9+3.1 with Murchison Widefield Array and XMM-Newton

We will present the radio continuum and X-ray analysis of Galactic supernova remnant G5.9+3.1. The radio spectral energy distribution obtained with the Murchison Widefield Array, together with the surveys at other radio continuum frequencies is discussed. In addition, we have also examined an archival XMM-Newton observation which allowed us to detect an X-ray emission from this remnant for the first time. Finally, a detailed X-ray spectral analysis will be presented.