Fig. 3
Rest-frame PDFs of relative likelihood against DMhost for multiple FRB progenitor scenarios. From top left to bottom right: sources follow stellar distributions (OB stars, YPSRs, OPSRs, MSPs) in spiral galaxies; homogeneous distributions (within spheres of radius H kpc) in spiral galaxies; elliptical distributions (confined to multiples of the galaxy effective radius, Re = 3.2 kpc) in elliptical galaxies; and homogeneous distributions (within spheres of radius H kpc) in elliptical galaxies.
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