Ratio of 0.3–10 keV X-ray flux at 11 hr, F_X,11, to the 15–150 keV gamma-ray fluence, ϕ_γ, vs. the projected physical offset from the GRB host galaxy. We highlight the events in our sample, divided by their gamma-ray duration into sGRB-KNe (blue) and LGRB-KNe (magenta), and compare them to a population of short and long GRBs (orange and gray, respectively). We note that some events in our sample (GRBs 150101B and 170817A) are not shown as they lack X-ray data at 11 hr. The black line is shown to guide the eye. The figure is reproduced from B. O’Connor et al. (2022) and Y.-H. Yang et al. (2024).