Positions in (ϕ₁, ϕ₂) of stars with a membership probability larger than 50% and parallax < 0.8 mas displayed as a scatter plot (top) and a smoothed density map (bottom). Jhelum clearly stands out as an overdensity and has a clumpy morphology with multiple gaps. Possible narrow-component members are contained within the red region in the top panel. Below this region, the extended broad component stands out, while above it, between ϕ₁ ≈ 0–5 degrees, a thus far unreported third component can be seen.