Image Details

Choose export citation format:

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 2.

Distributions of characteristic timescales, time-integrated spectral fitting parameters, and other derived parameters. Flux, fluence, and energy are calculated in the energy band of 8–200 keV. The dotted curves are the best Gaussian fits to the histograms. The red/green/yellow vertical lines and corresponding shadow areas represent the parameter values and errors of the FRB-associated burst obtained with HXMT/INTEGRAL/Konus-Wind (Li et al. 2020; Mereghetti et al. 2020; Ridnaia et al. 2020).

Other Images in This Article
Copyright and Terms & Conditions