Empirical estimation of host galaxy dispersion measure toward well-localized fast radio bursts

Open Access

Fig. 3.

Distribution of DM $_{host}^{halo}$ $_{\mathrm{host}}^{\mathrm{halo}}$ for FRB20191001A. The vertical solid black line represents the median value and the dashed black lines the corresponding 16th and 84th percentiles.

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