Characterizing the X-ray properties of the earliest magnetic stars

The recent detection of magnetic fields in massive stars has profoundly changedour understanding of the structure and evolution of these objects. In addition,detailed modelling shows that intense magnetic fields can have a strong impacton the Xray emission. Currently, only a few tens of magnetic hot stars areknown, and much fewer have been observed at high energies. The observeddiversity of behaviours and the small sample size actually prevent us fromrecognizing the overall trends. By doubling the sample size with a smallinvestment of time, we will be able to undertake such a systematic study of theXray properties of magnetic massive stars, which will help us better understandwhich parameters govern their highenergy emission. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]