XL-Calibur measurements of polarised hard X-ray emission from the Crab

Abstract

We report measurements of the linear polarisation degree (PD) and angle (PA) for hard X-ray emission from the Crab pulsar and wind nebula. Measurements were made with the XL-Calibur ($\sim$15-80 keV) balloon-borne Compton-scattering polarimeter in July 2024. The polarisation parameters are determined using a Bayesian analysis of Stokes parameters obtained from X-ray scattering angles. Well-constrained ($\sim$8.5$\sigma$) results are obtained for the polarisation of the $\sim$19-64 keV signal integrated over all pulsar phases: PD=(25.1$\pm$2.9)% and PA=(129.8$\pm$3.2)${}^{\circ }$. In the off-pulse (nebula-dominated) phase range, the PD is constrained at $\sim$4.5$\sigma$ and is compatible with the phase-integrated result. The PA of the nebular hard X-ray emission aligns with that measured by IXPE in the 2-8 keV band for the toroidal inner region of the pulsar wind nebula, where the hard X-rays predominantly originate. For the main pulsar peak, PD=(32.8${}_{-28.5}^{+18.2}$)% and PA=(156.0 $\pm$ 21.7)${}^{\circ }$, while for the second peak (inter-pulse), PD=(0.0${}_{-0.0}^{+33.6}$)% and PA=(154.5 $\pm$ 34.5)${}^{\circ }$. A low level of polarisation in the pulsar peaks likely does not favour emission originating from the inner regions of the pulsar magnetosphere. Discriminating between Crab pulsar emission models will require deeper observations, e.g. with a satellite-borne hard X-ray polarimeter.

arXiv comment8 pages, 4 figures. Accepted for publication in Monthly Notices of the Royal Astronomical Society; Stokes _uncertainties_ in Table 2 updated

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