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A Detailed X-Ray Investigation of PSR J2021+4026 and the γ-Cygni Supernova Remnant

  • Authors: C. Y. Hui, K. A. Seo, L. C. C. Lin, R. H. H. Huang, C. P. Hu, J. H. K. Wu, L. Trepl, J. Takata, Y. Wang, Y. Chou, K. S. Cheng, and A. K. H. Kong

Hui et al. 2015 The Astrophysical Journal 799 76.

  • Provider: AAS Journals

Caption: Figure 7.

Pulse profile of PSR J2021+4026 as observed by the XMM-Newton PN camera in 0.7–2.0 keV (see Figure 1 in Lin et al. 2013) and the best-fit simulated profile (solid curve) with the effects of gravitational light-bending incorporated. Error bars indicate the 1σ uncertainty. Two rotation cycles are shown for clarity.

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