High-Resolution Imaging and Timing of 3FGL J1016.5-6034

We propose to followup an interesting Xray source discovered in the field ofan unidentified 3FGL Fermi source. Ther 3FGL source has GeV propertiesconsistent with those of young pulsars and PWNe. This Xray source showsextended emission on small and large scales and is likely to be a new bright PWNwith a yet to be discovered pulsar. However, the existing snapshot exposuresare too short to study the extended emission, morphology, spectrum, and timingproperties. In the proposed Chandra observation we aim to resolve the morphologyand measure the spectra on different scales, confirm the PWN nature of thissource, constrain the orientation of the pulsar.s spin axis, and search forXray pulsations using a joint XMMNewton observation. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]