XMM-Newton EPIC-pn spectrum of SNR J0533−7202, shown alone for clarity. The best-fit model is given by the solid black line. The red dashed line indicates the vsedov component corresponding to the SNR emission, the magenta dash-dot lines mark the AXB components, the blue dash-dot-dot-dot line shows the combined contributions of the QPB, residual SPs, instrumental fluorescence lines, and electronic noise. The source fit parameters are given in Table 1.