Using MUSE H-alpha emission and halo modeling, the authors estimate rest-frame host DM for 12 FRBs, finding an average of 80 +/- 11 pc cm^-3 and correlations with stellar mass and star formation rate.
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Empirical estimation of host galaxy dispersion measure towards well localized fast radio bursts
Using MUSE H-alpha emission and halo modeling, the authors estimate rest-frame host DM for 12 FRBs, finding an average of 80 +/- 11 pc cm^-3 and correlations with stellar mass and star formation rate.