2004A&A...419..269W

We present XMM-Newton MOS imaging and PN timing data of the faint millisecond pulsars PSR J0751+1807 and PSR J1012+5307. We find 46 sources in the MOS field of view of PSR J0751+1807 searching down to an unabsorbed flux limit of 3x10^–15ergs/cm²/s (0.2-10.0keV). We present, for the first time, the X-ray spectra of these two faint millisecond pulsars. We find that a power law model best fits the spectrum of PSR J0751+1807, Γ=1.59±0.20, with an unabsorbed flux of 4.4x10^–14ergs/cm²/s (0.2-10.0keV). A power law is also a good description of the spectrum of PSR J1012+5307, Γ=1.78±0.36, with an unabsorbed flux of 1.2x10^–13ergs/cm²/s (0.2-10.0keV). However, a blackbody model cannot be excluded as the best fit to this data. We present some evidence to suggest that both of these millisecond pulsars show pulsations in this X-ray band. We find some evidence for a single broad X-ray pulse for PSR J0751+1807 and we discuss the possibility that there are two pulses per spin period for PSR J1012+5307.