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A Likelihood Based Approach to Distribution Regression Using Conditional Deep Generative Models

ICML 2025 · Probabilistic and scientific modeling › Variational and generative sampling · approach: Score-based generative modeling analysis · 0 citations (OpenAlex)

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Theoretical analysis of a likelihood-based sieve MLE for conditional deep generative models in distribution regression, giving Hellinger and Wasserstein convergence rates that depend only on intrinsic dimension and smoothness, plus small numerical validation on synthetic and MNIST data.

Problem

Estimating conditional distributions of a high-dimensional response that concentrates near a lower-dimensional manifold (with full-dimensional noise), and understanding why conditional deep generative models avoid the curse of dimensionality statistically.

Approach

Models the response as a conditional pushforward of a latent seed through a deep ReLU generator plus Gaussian noise, and analyzes a sieve MLE over sparse or fully connected networks; rates depend on intrinsic dimension and smoothness, and small noise injection (data perturbation) is proposed to handle near-singular supports.</1-2 sentences>

Key results

Measured effects reported in the paper

What was changedWhereMeasuredEffect
Use Sieve MLE instead of CKDE or FlexCodeconditional mean estimation · FD1, FD2, and FD3mean MSE: FD1: 0.0379 ± 0.0170 vs 1.0053 ± 0.1004 and 1.1660 ± 0.1076; FD2: 0.1943 ± 0.0427 vs 0.2640 ± 0.0515 and 0.3954 ± 0.0571Helped
Use Sieve MLE instead of CKDE or FlexCodeconditional standard deviation estimation · FD1 and FD2SD MSE: FD1: 0.0280 ± 0.0045 vs 0.9887 ± 0.0347 and 1.2000 ± 0.0126; FD2: 0.2843 ± 0.0093 vs 0.2853 ± 0.0213 and 5.8278 ± 0.1607Helped
Use Sieve MLE instead of CKDE for standard deviation estimationconditional distribution estimation · FD3SD MSE: 1.6394 ± 0.0861 vs 0.6334 ± 0.0460Hurt
Increase training sample sizeSieve MLE standard deviation estimation · FD3SD MSEHelped
Add Gaussian noise to MNIST training data (ablation)sparse and fully connected architectures · MNIST test imagesW1: Sparse: 1.9555 ± 0.7182 at 0 to 4.0880 ± 0.7518 at 0.5; fully connected: 1.8859 ± 0.7355 at 0 to 4.0995 ± 0.7633 at 0.5Hurt
Use sparse rather than fully connected architecture (ablation)conditional MNIST generation · MNIST test imagesW1: Noise 0: 1.9555 ± 0.7182 vs 1.8859 ± 0.7355; noise 0.005: 1.9478 ± 0.7329 vs 1.8663 ± 0.6251; noise 0.01: 1.9503 ± 0.729Mixed
Increase sample size (ablation)Sieve MLE on manifold data · Two Moon and Ellipse (σ* = 0.01)W1 median: 4000: 0.251 and 0.295; 10000: 0.196 and 0.251Helped

Surprising findings

Limitations

Experimental setup

Datasets: MNIST synthetic FD1-FD3 synthetic manifold M1 (two moons) synthetic manifold M2 (ellipses)

Benchmarks: MNIST synthetic FD1-FD3 synthetic manifolds M1 and M2

Metrics: MSE of conditional mean MSE of conditional standard deviation W1 distance

Baselines: CKDE FlexCode

Builds on: sieve MLE noise outsourcing lemma FlexCode conditional kernel density estimation

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