We present the analysis of the archival Suzaku and Swift X-ray observations of the young γ-ray pulsar J1932+1916 field. The data revealed a point-like object at the γ-ray position of the pulsar and diffuse X-ray emission around it. Spectra of the point-like source and diffuse emission are well-described by absorbed power-law models with spectral parameters typical for pulsar plus pulsar wind nebula systems. Therefore we suggest that Suzaku and Swift detected the X-ray counterpart of PSR J1932+1916. Assuming this interpretation, we constrain the distance to the pulsar in the range of 2-6 kpc. We also suggest possible association of the pulsar with the nearby supernova remnant G54.4-0.3 and discuss its implications for the pulsar proper motion, age and distance.
@article{arxiv.1612.03647,
title = {Observations of the $\gamma$-ray pulsar J1932+1916 in X-rays},
author = {A. Karpova and P. Shternin and D. Zyuzin and A. Danilenko and Yu. Shibanov},
journal= {arXiv preprint arXiv:1612.03647},
year = {2017}
}