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We report on X-ray studies of the gamma-ray pulsar PSR J1418$-$6058 in theRabbit pulsar wind nebula (PWN) carried out using archival Chandra andXMM-Newton observations. A refined timing analysis performed with the 120-ksXMM-Newton data finds significant ($p\approx10^{-7}$) pulsation at$P\approx110$ ms which is consistent with that measured with the Fermi largearea telescope (LAT). In the Chandra image, we find extended emission aroundthe pulsar similar to those seen around other pulsars in young PWNe, whichfurther argues for association between PSR J1418$-$6058 and the Rabbit PWN. TheX-ray spectrum of the pulsar is hard and similar to those of soft-gammapulsars. Hence PSR J1418$-$6058 may add to the list of soft-gamma pulsars.

Characterizing X-ray properties of the gamma-ray pulsar PSR J1418$-$6058 in the Rabbit pulsar wind nebula