X-ray identification of the high magnetic field pulsar B1727-47

We propose first Xrays observations of the high magnetic field middleage radiopulsar B172747. Models predict that high magnetic field pulsars are hotter thanpulsars with lower magnetic field. However, current Xray data on highlymagnetized pulsars are scarce to confidently confirm this. Analysis of the radiotiming and interferometry data suggest that B172747 has a significant propermotion, which points on the association with the nearby (<1 kpc) evolvedsupernova remnant RCW 114. Potential proximity, high Galactic latitude (b7.69deg) and thus low absorption (Nh<2e21 cm2) make PSR B172747 a good Xraytarget to study magnetic field impact on the thermal emission properties ofrotation powered pulsars. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]