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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 6.

Pulsed spectrum of PSR J2021+4026 as observed by the XMM-Newton PN camera with the best-fit BB model illustrated (upper panel) and the contributions to the χ2 fit statistic (lower panel).

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