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Fast Optical Variability of the TeV Blazar PKS 1725+123 Observed by SVOM-VT and Insights from Multiwavelength Follow-up Observations

  • Authors: Shuo-Yu Liu, Yu-Wei Yu, Ji-Shun Lian, Xin-Ke Hu, Alexis Coleiro, Zhu-Heng Yao, Li-Ping Xin, Jing Wang, Hua-Li Li, Zi-Qi Wang, Jin Zhang, Floriane Cangemi, Bertrand Cordier, Antoine Foisseau, Olivier Godet, Andrea Goldwurm, Diego Götz, Sébastien Guillot, Xu-Hui Han, Ning Jiang, Cyril Lachaud, Sébastien Le Stum, En-Wei Liang, Pierre Maggi, Yu-Lei Qiu, Jérôme Rodriguez, Lian Tao, Jian-Yan Wei, Chao Wu, Liang Zhang, Shuang-Nan Zhang, Shi-Jie Zheng

Shuo-Yu Liu et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 4.

Swift-XRT observations for PKS 1725+123. Light curves of F0.3−10 (black points in the first panels), F0.3−2 (red points in the second panels), F2−10 (blue points in the second panels), Γγ (green points in the third panels), and the HR (orange points in the fourth panels) are respectively depicted. The gray shaded area indicates the quasi-simultaneous observations (on August 19 and 21) corresponding to the TeV detections. The left panels show the three historical Swift-XRT observations, while the right panels display the Swift-XRT follow-up observations of the TeV detection for the source. MJD 60755 corresponds to 2025 March 21.

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