Synthetic synchrotron specific flux maps displaying the expected radio emission from IGR J11014–6103 in the 0.9–1.7 GHz band in which MeerKAT operates, convolved with an instrument beam of 15″ × 15″ (Jonas & MeerKAT Team 2016). The contribution from particles injected all along the IGR J11014–6103’s lifetime, which escaped the nebula and diffused into the ISM (B_ISM = 5μG), is displayed in the left panel, and that from the JET region (B_ISM = 30μG) is shown in the right panel. A white star indicates the position of the pulsar, which is assumed to move leftwards along the horizontal dashed-line.