Figure 11 from X-Ray Phase-resolved Spectroscopy of PSRs B0531+21, B1509–58, and B0540

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X-Ray Phase-resolved Spectroscopy of PSRs B0531+21, B1509–58, and B0540–69 with RXTE

Ge et al. 2012 The Astrophysical Journal Supplement Series 199 32.

Caption: Figure 11.

Similar to Figure 10, but the fitted model is log-parabola with E ₀ fixed at 1 keV. The reduced χ ² is 0.93 with the degree of freedom 85.