Figure 3 from Probabilistic Association of Transients to their Hosts (PATH)

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Probabilistic Association of Transients to their Hosts (PATH)

Authors: Kshitij Aggarwal, Tamás Budavári, Adam T. Deller, Tarraneh Eftekhari, Clancy W. James, J. Xavier Prochaska, and Shriharsh P. Tendulkar

2021 The Astrophysical Journal 911 95.

Provider: AAS Journals

Caption: Figure 3.

Three offset functions p(ω∣O_i) considered for the underlying angular distribution of FRBs relative to their host galaxies, normalized by the galaxy’s half-light radius ϕ. Each is normalized to have identical integrated area to a maximum assumed offset of ﹩{\theta }_{\max }=6\,\phi ﹩.

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