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

Open Access

Fig. 5.

Relation between DM $_{host}^{direct}$ $_{\mathrm{host}}^{\mathrm{direct}}$ and DM $_{host}^{Macquart}$ $_{\mathrm{host}}^{\mathrm{Macquart}}$ (dark points), with error bars showing the statistical uncertainties on DM $_{host}^{direct}$ $_{\mathrm{host}}^{\mathrm{direct}}$ (we did not estimate the uncertainties of our DM $_{host}^{Macquart}$ $_{\mathrm{host}}^{\mathrm{Macquart}}$ values). The dashed line corresponds to the identity line (i.e., the 1:1 relation). The golden star corresponds to the average values of DM $_{host}^{direct}$ $_{\mathrm{host}}^{\mathrm{direct}}$ and DM $_{host}^{Macquart}$ $_{\mathrm{host}}^{\mathrm{Macquart}}$ , with the error bars being their corresponding standard deviation.

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