Figure 9 from A Detailed X-Ray Investigation of PSR J2021+4026 and the γ-Cygni Supernova Remnant

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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 9.

Upper panel: X-ray energy spectrum of the southeastern region of G78.2+2.1 as observed by MOS1/2 (cf. Figure 1), which is simultaneously fitted to an absorbed non-equilibrium ionization plasma model. Additional PL components have been applied to account for the residual soft proton contamination in the individual camera. Lower panel: contributions to the χ² fit statistic.

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