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Bursts before Burst: A Comparative Study on FRB 200428-associated and FRB-absent X-Ray Bursts from SGR J1935+2154

  • Authors: Yu-Han Yang, Bin-Bin Zhang, Lin Lin, Bing Zhang, Guo-Qiang Zhang, Yi-Si Yang, Zuo-Lin Tu, Jin-Hang Zou, Hao-Yang Ye, Fa-Yin Wang, and Zi-Gao Dai

2021 The Astrophysical Journal Letters 906 L12.

  • Provider: AAS Journals

Caption: Figure 3.

Correlation plots for time-integrated spectral fitting. The same method of linear regression is imported from Tu & Wang (2018). The black solid lines represent the best-fitting results. The red and yellow dotted lines represent 1σv and 2σv regions of extra variability, respectively (D’Agostini 2005), and the gray areas mark the 95% confidence interval of fitting uncertainties. The black dashed line in the top-left panel is Tbb = T90. The red, green, and yellow data points in the bottom panels are the same as the corresponding value with identical color in Figure 2. The purple dashed lines indicate upper/lower limits of several times of σv region that can contain the red points.

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