Fig. 22.

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Expected contribution to scattering at 1370 MHz for different lens DMs from an FRB host galaxy at zH = 1 and an intervening galaxy halo within the line of sight. The solid lines show the expected host galaxy contribution for different electron density variations and a geometric boost factor Gsc = 1. The dashed lines show the expected contribution from an intervening galaxy halo with a thickness L = 30 kpc and pc−2/3 km−1/3 located at different redshifts. The orange shaded region represents the observed Apertif τsc range.
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