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Learning What's Real: Disentangling Signals and Measurement Artifacts in Multi-Sensor Data, with Applications to Astrophysics
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Proposes a dual-encoder conditional flow-matching model that separates physics and instrument latents from overlapping multi-instrument galaxy images (HSC and Legacy), using counterfactual generation as the training objective.
Problem
Observations are confounded by instrument-specific artifacts, which hinder extracting physical signals and combining heterogeneous multi-instrument data; standard foundation models treat instruments as independent modalities without disentangling them.
Approach
Train two ResNet-18 encoders (physics encoder on the same source from another instrument; instrument encoder on other sources from the same instrument) whose latents condition a flow-matching decoder that reconstructs an anchor observation never fed to the encoders, so disentanglement emerges from the counterfactual generation objective rather than contrastive or hand-designed losses.
Key results
- Physics latents match AION-1 within a few percentage points on most physics targets (e.g., redshift R^2 0.801 vs 0.857 for AION-1-B) while instrument latents outperform AION-1 on instrument properties (galaxy depth R^2 0.682 vs 0.426).
- Outliers from the physics latent are free of instrument artifacts and show mergers, while AION-1 and instrument-latent outliers are dominated by saturation and noise patterns.
- Counterfactual HSC images from Legacy inputs yield ellipticity R^2 of 0.81 with a frozen HSC-trained ResNet, versus 0.82 on real HSC images.
Surprising findings
- Physics latents retain instrument-related information only near the random-baseline level, while a randomly initialized ResNet exceeds the trained instrument encoder on some physical properties.
- Cross-predict baseline outperforms the instrument latent on extinction-like quantities.
Limitations
- Requires overlapping observations across instruments, limiting applicability to shared sky regions.
- Generated counterfactuals reflect statistical expectation and cannot recover information absent from the input; mild posterior overconfidence (~15% variance underestimate).
- Evaluated only on galaxy imaging with two instruments; a simplified codebase is released but not the full pipeline.
Experimental setup
Datasets: Multimodal Universe cross-matched HSC and DESI Legacy Imaging Survey galaxy images PROVABGS catalogue HSC shape catalog
Benchmarks: Multi-instrument galaxy probe tasks (MLP R^2 on physics and instrument properties) Outlier detection on HSC galaxies Cross-instrument reconstruction MSE
Metrics: R^2 MSE log-likelihood (outlier score) power spectral density agreement pixel-wise Z-score calibration
Baselines: AION-1 AstroCLIP randomly initialized ResNet-18 cross-predict ResNet
Builds on: flow matching beta-VAE AION-1 UNet2DConditionModel ResNet
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