Figure 1 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

Authors: M. Y. Ge, F. J. Lu, J. L. Qu, S. J. Zheng, Y. Chen, and D. W. Han

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

Provider: AAS Journals

Caption: Figure 1.

Timing result of the Crab pulsar. Panel (a) shows the frequency evolution, panel (b) shows the frequency residuals of the fit with Equation (1), and panel (c) shows the differences between the frequencies measured by X-ray observations and those calculated from the radio ephemeris.

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