Image Details
Caption: Figure 1.
DMhost for all localized FRBs with z < 0.2 at the time of writing plotted against potential indicators of DMhost,ISM: host galaxy inclination i, scattering timescale τexc, RM, and impact parameter b⊥. The colored points are the five FRBs selected for our analysis. Light gray points are the poorly localized (approximately arcminute) FRBs.
© 2026. The Author(s). Published by the American Astronomical Society.