Illustration of the inclinations of host galaxies and the projected distance of FRBs from the center of the host galaxy (b_offset), showed for face-on, inclined, and edge-on galaxies. The observer is on the left side. The total angular momentum vector of the host galaxy (L) is perpendicular to the plane of its disk. The inclination (i) is the angle between the line of sight and L. The filled circles indicate the positions of the FRBs.