A search for the young and energetic pulsar in G328.4+0.2

The pulsarpowered nebula G328.4+0.2 is one of the largest and most luminoussuch sources known, its properties implying the presence of a very young,energetic and rapidlyspinning pulsar within. We here propose to search forpulsations from this unseen pulsar using EPICpn. We expect this source to beat the extreme of phase space for young pulsars, and its discovery would thusmake an important contribution towards understanding the birth properties ofthese objects.