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Discovery of Short-term γ-Ray Pulsed Radiation Variations Following a Glitch in PSR J0205+6449

  • Authors: Wen-Tao Ye, Ming-Yu Ge, Shi-Jie Zheng, Xiang Ma, Yu-Jia Zheng, Han-Long Peng, Xue-Zhi Liu, Li-Ming Song, Shuang-Nan Zhang, Fang-Jun Lu

Wen-Tao Ye et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 1.

The left panel shows the timing results for the glitch at MJD 54904. Panels (a) and (b) show the residuals of ν and ﹩\dot{\nu }﹩ of partial-timing results that subtract the preglitch spin-down trend, respectively. The solid lines represent the glitch model listed in Table 1. Panel (c) displays the TOA residuals fitted with the glitch model listed in Table 1. The right panel shows short-term variations in the pulse profile, and the vertical dashed lines in the left panel mark their epochs. Panels (d), (e), and (f) show the three successive pulse profile variations during MJD 54905–54940, MJD 54940–55000, and MJD 55000–55160, respectively. The black profile represents the short-term pulse profile, and the red profile represents the template profile accumulated from full data.

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