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WFST Follow-up of S251112cm: Searching for an Optical Counterpart to a Subsolar-mass Compact-binary Merger Candidate

  • Authors: Zhengyan Liu, Zelin Xu, Ji-an Jiang, Wen Zhao, Zhiping Jin, Zigao Dai, Dezheng Meng, Yefei Yuan, Xuefeng Wu, Lulu Fan, Xu Kong, Xander J. Hall, Antonella Palmese, Feng Li, Ming Liang, Binyang Liu, Zhen Wan, Hairen Wang, Jian Wang, Tinggui Wang, Hongfei Zhang, Xianzhong Zheng, Qingfeng Zhu

Zhengyan Liu et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure 6.

Constraints on the ejecta masses and viewing angle, with other parameters (vej, Ye) fixed to the best-fit values of AT 2017gfo. The color scale indicates the grid excluded fraction of the parameter space. Red stars mark the inferred ejecta masses and viewing angle for AT 2017gfo, shown for comparison.

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