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E0a — orientation-lifted vs Hessian filament extraction (Voronoi toy, exact truth)

E0a — orientation-lifted vs Hessian filament extraction (Voronoi toy, exact truth)

Question (H1): does lifting a galaxy density field to the position–orientation manifold R³×S² recover filament spines better than the quadratic (Hessian) orientation response, at identical post-processing and matched skeleton length?

Setup. Voronoi filament model in a 128³ box (1 voxel = 1 h⁻¹Mpc at the nominal L=128 h⁻¹Mpc): filaments are Voronoi-cell edges (straight variant) or Bézier-bent edges (curved variant, sag ≈ 15% of length); galaxies = arclength-uniform points with transverse Gaussian scatter σ=0.8 vox + 15% node clumps + 25% uniform background; field = CIC deposit → log(1+δ) → Gaussian smooth σ=1. Exact truth: the generating curves and vertices.

Protocol. Each method gets 3 candidate configs; the best on calibration seed 1 (mean C+P+jF1 over sampling levels) is frozen, then evaluated on held-out seeds. Both methods share hysteresis thresholding, matched-length skeletonization (mask volume bisection, tube area 9 vox²), speckle pruning ≥4 vox, and junction clustering.

Metric definitions

Straight filaments

Chosen configs — lift: {'sig_par': 6.0, 'sig_perp': 1.5, 'diff_iter': 2}, hessian: {'sigma': 2.0}.

Per-method summary

n_gal method completeness mean ± sd median (p10–p90) purity junction F1
1200 se3_lift 0.813 ± 0.032 0.812 (0.780–0.852) 0.685 ± 0.059 0.383 ± 0.056
1200 hessian 0.811 ± 0.029 0.812 (0.777–0.843) 0.695 ± 0.034 0.455 ± 0.051
2500 se3_lift 0.867 ± 0.037 0.871 (0.823–0.904) 0.847 ± 0.052 0.464 ± 0.065
2500 hessian 0.912 ± 0.023 0.908 (0.887–0.945) 0.758 ± 0.054 0.469 ± 0.057
5000 se3_lift 0.886 ± 0.038 0.892 (0.837–0.929) 0.919 ± 0.029 0.512 ± 0.060
5000 hessian 0.938 ± 0.018 0.939 (0.913–0.960) 0.913 ± 0.049 0.541 ± 0.066
20000 se3_lift 0.890 ± 0.038 0.896 (0.838–0.930) 0.937 ± 0.022 0.530 ± 0.076
20000 hessian 0.943 ± 0.025 0.949 (0.910–0.973) 0.974 ± 0.012 0.592 ± 0.057
80000 se3_lift 0.882 ± 0.037 0.886 (0.829–0.930) 0.932 ± 0.023 0.523 ± 0.073
80000 hessian 0.939 ± 0.024 0.943 (0.906–0.968) 0.973 ± 0.012 0.591 ± 0.054

Paired differences (the H1 evidence)

n_gal n seeds ΔC mean ΔC median (p10–p90) lift wins Wilcoxon p (ΔC) ΔjF1 mean Wilcoxon p (ΔjF1)
1200 50 +0.003 +0.002 (-0.029–+0.035) 27/50 0.47 -0.071 5.9e-10
2500 50 -0.045 -0.041 (-0.083–-0.018) 3/50 2.5e-14 -0.005 0.5
5000 50 -0.053 -0.050 (-0.096–-0.016) 0/50 1.8e-15 -0.028 0.00065
20000 50 -0.053 -0.050 (-0.087–-0.028) 0/50 1.8e-15 -0.062 5e-11
80000 50 -0.057 -0.054 (-0.083–-0.036) 0/50 1.8e-15 -0.068 5.6e-11

E0a straight: box plots with per-seed points of paired delta completeness and delta junction F1 vs galaxy count; positive favours the lift

E0a straight: completeness, purity, junction F1 vs galaxy count, both methods, mean ± sd over held-out seeds

E0a straight: 6-voxel slab of the galaxy field with truth (red) and extracted skeletons (blue) for both methods

Curved filaments

Chosen configs — lift: {'sig_par': 6.0, 'sig_perp': 1.5, 'diff_iter': 2}, hessian: {'sigma': 1.5}.

Per-method summary

n_gal method completeness mean ± sd median (p10–p90) purity junction F1
1200 se3_lift 0.813 ± 0.030 0.815 (0.775–0.849) 0.677 ± 0.050 0.376 ± 0.047
1200 hessian 0.810 ± 0.024 0.806 (0.784–0.841) 0.707 ± 0.036 0.435 ± 0.039
2500 se3_lift 0.869 ± 0.032 0.874 (0.835–0.895) 0.828 ± 0.055 0.459 ± 0.061
2500 hessian 0.919 ± 0.017 0.921 (0.899–0.936) 0.778 ± 0.034 0.484 ± 0.042
5000 se3_lift 0.891 ± 0.036 0.899 (0.846–0.930) 0.909 ± 0.029 0.508 ± 0.053
5000 hessian 0.956 ± 0.013 0.953 (0.944–0.975) 0.866 ± 0.050 0.510 ± 0.052
20000 se3_lift 0.892 ± 0.043 0.902 (0.834–0.941) 0.933 ± 0.026 0.520 ± 0.071
20000 hessian 0.956 ± 0.021 0.960 (0.932–0.982) 0.971 ± 0.017 0.593 ± 0.058
80000 se3_lift 0.884 ± 0.046 0.888 (0.817–0.931) 0.927 ± 0.028 0.519 ± 0.069
80000 hessian 0.950 ± 0.024 0.951 (0.919–0.977) 0.974 ± 0.013 0.600 ± 0.053

Paired differences (the H1 evidence)

n_gal n seeds ΔC mean ΔC median (p10–p90) lift wins Wilcoxon p (ΔC) ΔjF1 mean Wilcoxon p (ΔjF1)
1200 50 +0.004 +0.010 (-0.037–+0.044) 30/50 0.36 -0.059 8.9e-10
2500 50 -0.050 -0.049 (-0.074–-0.016) 0/50 1.8e-15 -0.025 0.0054
5000 50 -0.064 -0.062 (-0.104–-0.029) 0/50 7.6e-10 -0.003 0.75
20000 50 -0.064 -0.059 (-0.101–-0.028) 0/50 1.8e-15 -0.073 3.1e-12
80000 50 -0.066 -0.062 (-0.104–-0.033) 0/50 1.8e-15 -0.081 1.8e-15

E0a curved: box plots with per-seed points of paired delta completeness and delta junction F1 vs galaxy count; positive favours the lift

E0a curved: completeness, purity, junction F1 vs galaxy count, both methods, mean ± sd over held-out seeds

E0a curved: 6-voxel slab of the galaxy field with truth (red) and extracted skeletons (blue) for both methods

Verdict on H1 (toy-level)

Not supported (CORRECTED result). An earlier version of this report claimed a sparse-regime lift win (+0.07 completeness at n_gal=2500). That was an evaluation artifact: the original extractor targeted mask volume, and realized skeleton lengths differed systematically between methods (lift ~19% longer at sparse levels) — longer skeletons buy completeness mechanically. With skeleton length enforced (iterative correction to the target), the Hessian matches or beats the lift at every sampling level on both variants; the lift’s best case is a statistical tie at the ultra-sparse level (n_gal=1200, p≈0.4). Junction F1 favours the Hessian at essentially all levels. The diffusion component remains rejected by calibration (weak diffusion shows a small positive only at n_gal=1200 in the E0b sweep, +0.01). Detection of the artifact: an instrument change made for E1 (connected-web extraction) retroactively changed E0 parent scores; the n_est fields in the archived E0 results confirmed the length mismatch.

Open questions / next tests

  1. Why doesn’t diffusion help? Candidates: bend level too mild (sag 15%); diffusion parameters not co-calibrated with filter scales; matched-length extraction absorbing its benefit. Next: sweep bend_frac ∈ {0.15, 0.3, 0.5} × diffusion strength, and score curvature-binned completeness (does diffusion win specifically on high-curvature arcs?).
  2. Junctions: node clumps make junctions easy for both methods. Re-run with node_frac=0 — the lift should shine when junctions are only implied by filament continuity.
  3. Gravity realism (E1): port the benchmark to a Zel’dovich / N-body field where filaments are tidal-sheared, not tubular — the regime the physics prior (tidal-modulated coefficients, H2) targets.
  4. Tier B: the current extraction skeletonises the ridgeness; true SR geodesic tracing on the lifted graph is not yet exercised and is where curvature penalties enter explicitly.