EPIC spectra of the three new Be/X-ray binary pulsars (MOS1: black, MOS2: red, pn: green). The best-fit models are plotted as histogram and the bottom panels show the residuals. For eRASSU J050810.4–660653 and eRASSt J044811.1–691318 an absorbed power law yielded an acceptable fit; however, for RX J0501.6–7034, an additional black-body component was included (individual components are indicated by dotted lines). See Table 3, for the model parameters.