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Probing the Intergalactic Turbulence with Fast Radio Bursts

  • Authors: Siyao Xu, and Bing Zhang

2020 The Astrophysical Journal Letters 898 L48.

  • Provider: AAS Journals

Caption: Figure 4.

(a) DME distribution for the entire FRB sample. The thick solid line shows the kernel density estimate of the distribution. The peak of the distribution at ﹩{\mathrm{DM}}_{{Ep}}=306.3﹩ pc cm−3 is indicated by the vertical dashed line. (b) DMIGM–z relation (solid line). The dashed line marks ﹩z\approx 0.36﹩ corresponding to DMEp.

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