Extended Data Fig. 6: Constraints on the RVM α, β parameter phase space for different assumed duty cycles of FRB 20221022A.
From: A pulsar-like polarization angle swing from a nearby fast radio burst

For each panel, the beaming angle, ρ, is determined from equation (4) and is represented by a logarithmic (base 10) colour map. The 1σ (solid line) & 3σ (dotted line) contour lines for best-fit α, β values indicate a general trend toward smaller inferred beaming angles for smaller assumed duty cycles.