Shrestha et al. performed a detailed analysis of five distant interplanetary shocks observed by the Solar Wind Around Pluto instrument on board New Horizons, which exhibit the signature of a suprathermal H⁺ pickup ion (PUI) tail in the downstream distribution. These shocks were observed with a PUI data cadence of approximately 24 hr, covering a heliocentric distance range of 23.71–36.75 au. They found that the H⁺ PUI density and temperature show a gradual increase across the shock, while the H⁺ solar wind density shows erratic behavior without a distinct downstream compression. The H⁺ PUI cooling index variation across the shock displays different characteristics in each shock. Their study demonstrated, for the first time, the variation of the number density of downstream H⁺ PUI tails with the shock compression ratio, revealing an increase in tail density with stronger shocks. Additionally, their theoretical estimates of reflected PUI number densities derived from the electrostatic cross-shock potential agree very well with the observed H⁺ PUI tail densities for stronger shocks.