Figure 2 from Searching for the Transit of the Earth-mass Exoplanet Proxima Centauri b in Antarctica: Preliminary Result

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Searching for the Transit of the Earth-mass Exoplanet Proxima Centauri b in Antarctica: Preliminary Result

Authors: Hui-Gen Liu, Peng Jiang, Xingxing Huang, Zhou-Yi Yu, Ming Yang, Minghao Jia, Supachai Awiphan, Xiang Pan, Bo Liu, Hongfei Zhang, Jian Wang, Zhengyang Li, Fujia Du, Xiaoyan Li, Haiping Lu, Zhiyong Zhang, Qi-Guo Tian, Bin Li, Tuo Ji, Shaohua Zhang, Xiheng Shi, Ji Wang, Ji-Lin Zhou, and Hongyan Zhou

2018 The Astronomical Journal 155 12.

Provider: AAS Journals

Caption: Figure 2.

Candidate transit event in the detrended light curve. It is in the 1σ window of interest of T_IC = 2,457,640.74 ± 0.67 HJD for the 86th epoch. The best-fitted model, with T_C = 2,457,640.1983 ± 0.0020 HJD, T_d = 82 ± 6 minutes, and D = 5.5 ± 1.1 mmag, is overplotted (the red solid curve).

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