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+ ---
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+ license: mit
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+ task_categories:
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+ - other
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+ tags:
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+ - point-cloud
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+ - geometry
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+ - topology
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+ - benchmark
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+ - higher-dimensions
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+ - synthetic
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+ pretty_name: HyperShadow
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+ size_categories:
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+ - 10K<n<100K
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+ ---
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+
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+ # HyperShadow
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+
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+ A benchmark for one question: given a 3D point cloud, can you tell whether
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+ it is an ordinary 3D object or the 3D projection (the "shadow") of an
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+ object from a higher spatial dimension?
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+
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+ Most datasets that say "4D" mean 3D plus time. Here the extra dimensions
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+ are spatial: label 1 clouds are projections of objects living in R^4, R^5
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+ or R^6 (hyperspheres, tesseracts, Clifford tori, duocylinders, hypertori,
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+ random smooth manifolds), rotated randomly in their ambient space before
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+ projection. Label 0 clouds are native 3D shapes given the same rotation
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+ and corruption treatment, so nothing in the preprocessing separates the
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+ classes.
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+
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+ ## Why this is an interesting task
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+
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+ A shadow is still at most 3-dimensional data, so intrinsic-dimension
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+ estimation cannot solve this. On this benchmark, TwoNN and the
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+ Levina-Bickel MLE reach about 71-73% accuracy. What actually separates
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+ the classes are the traces the projection map leaves behind: density
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+ folds, volumes filled with a particular radial profile, changed topology.
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+ A small PointNet (190k parameters) picks these up at 96.6%, and still
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+ detects shape families it was never trained on (79-91%).
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+
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+ The temporal track has the strongest result, and it needs no learning at
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+ all. A rigid 3D object in rigid motion can be aligned frame to frame by a
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+ rigid 3D transform with near-zero residual. The shadow of a rigidly
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+ rotating 4D object cannot: no rigid 3D motion explains it. The mean
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+ Kabsch alignment residual, one number per sequence, separates the classes
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+ at AUROC 0.982.
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+
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+ ## Files
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+
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+ | file | contents |
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+ |---|---|
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+ | `static.npz` | `points`: float32 (10800, 1024, 3); `labels`: int64 (10800,) |
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+ | `static_meta.json` | per-sample shape name, ambient dimension, corruption tier, projection type |
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+ | `temporal.npz` | `points`: float32 (1800, 16, 512, 3), rigid-rotation sequences; `labels` |
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+ | `temporal_meta.json` | per-sequence metadata |
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+
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+ Labels: 0 = native 3D, 1 = projection of a higher-dimensional object.
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+ Classes are balanced across corruption tiers. All clouds are centred,
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+ scaled to unit mean radius, and resampled to a fixed point count.
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+
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+ Corruption tiers (cumulative): 0 clean; 1 Gaussian jitter (2% of scale);
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+ 2 plus random half-space occlusion; 3 plus heavier jitter and
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+ distance-dependent dropout.
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+
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+ ## Loading
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+
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+ ```python
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+ import numpy as np
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+
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+ d = np.load("static.npz")
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+ x, y = d["points"], d["labels"] # (10800, 1024, 3), (10800,)
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+
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+ t = np.load("temporal.npz")
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+ seq = t["points"] # (1800, 16, 512, 3)
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+ ```
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+
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+ ## Baseline numbers to beat
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+
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+ | Method | Accuracy (static) |
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+ |---|---|
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+ | intrinsic dimension, best threshold | 0.732 |
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+ | persistent homology + GBT | 0.904 |
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+ | geometric features + GBT | 0.956 |
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+ | PointNet-lite, 190k params | 0.966 |
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+
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+ Temporal track: Kabsch rigidity residual threshold, AUROC 0.982.
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+
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+ ## Reproducing or extending
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+
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+ The generator is plain seeded NumPy, no GPU needed. Code, tests, and all
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+ baseline implementations are in the GitHub repository (link in the
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+ citation section once the paper is up). Regenerating with the published
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+ seeds reproduces these exact files. New shape families can be added with
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+ a single sampler function.
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+
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+ ## Limitations
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+
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+ Everything here is simulated, under specific choices of sampling measure,
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+ projection model and noise. Results on this data say nothing about
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+ physical reality. The intended uses are: benchmarking point-cloud models
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+ on a task where the ground truth is known and the shortcut routes have
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+ been closed off, studying out-of-distribution detection with a
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+ mathematically defined "out", and comparing machine performance against
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+ the human 4D-rigidity perception results reported by He, Bi and Zaidi
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+ (2023).
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+
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+ ## Citation
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+
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+ ```bibtex
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+ @misc{hypershadow2026,
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+ title = {HyperShadow: A Benchmark for Detecting 3D Projections of
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+ Higher-Dimensional Spatial Objects},
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+ author = {Sasi, Akshay},
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+ year = {2026},
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+ }
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+ ```