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Scientific Showcase

Physics-Informed Super-Resolution for Strong Lensing

Vision & Motivation

Strong gravitational lensing provides a unique probe into dark matter substructure and the mass distribution of foreground lenses. However, observations from upcoming surveys like LSST (Rubin Observatory) and Euclid will be limited by resolution and point spread function (PSF) effects.

Traditional Super-Resolution (SR) relies on High-Resolution (HR) ground truth, which does not exist for real astronomical observations. We only have Low-Resolution (LR) images from telescopes. Therefore, relying solely on supervised learning on simulations is insufficient due to the domain gap.

Physics-Informed Approach

Our project implements a dual-strategy to bridge the gap between simulations and real survey data:

1. Physics Constraints

Enforcing that the Super-Resolved image, when degraded by the known telescope PSF and downsampling, matches the observed LR image ($L_{phy}$).

2. Domain Adaptation

Bridging the gap between synthetic training data and real observation noise signatures to enable zero-shot transfer.

Scientific Validation

We quantified the physical utility of Super-Resolution using domain-specific metrics beyond standard vision scores.

Method Arc Sharpness Ring Contrast
Bicubic Interpolation 221.96 ± 60.1 5.08 ± 3.06
SR Baseline (Supervised) 268.50 ± 79.5 4.97 ± 2.86
SR Hybrid (Physics-Informed) 267.41 ± 79.3 5.39 ± 3.27
HR Ground Truth 266.39 ± 77.8 5.14 ± 3.06

*Wilcoxon Signed-Rank Test: $p = 1.86 \times 10^{-9}$ for arc sharpness statistical significance.

Dark Matter Substructure Analysis

SR-enhanced images are used to feed downstream classifiers distinguishing between no_sub, vortex, and subhalo dark matter models.

ROC Comparison

ROC Comparison

Baseline classification performance on target samples.

Confusion Matrices

Confusion Matrices

Multi-class distribution and false positive rates.

Hard Mode ROC

Hard ROC

Performance under extreme PSF blur and low SNR.

Hard Mode Confusion

Hard Confusion

Misclassification patterns for faint substructures.