# Generative Adversarial Networks recover features in astrophysical images of galaxies beyond the deconvolution limit

## TL;DR

This paper demonstrates that a trained GAN can recover detailed galaxy features from degraded astrophysical images, surpassing traditional deconvolution methods and enhancing analysis of current and future astronomical data.

## Contribution

The study introduces a GAN-based method for recovering galaxy features from noisy, low-resolution images, exceeding the capabilities of conventional deconvolution techniques.

## Key findings

- GAN outperforms traditional deconvolution in feature recovery
- Method effectively enhances low-signal-to-noise galaxy images
- Applicable to data from LSST, Hubble, and James Webb telescopes

## Abstract

Observations of astrophysical objects such as galaxies are limited by various sources of random and systematic noise from the sky background, the optical system of the telescope and the detector used to record the data. Conventional deconvolution techniques are limited in their ability to recover features in imaging data by the Shannon-Nyquist sampling theorem. Here we train a generative adversarial network (GAN) on a sample of $4,550$ images of nearby galaxies at $0.01<z<0.02$ from the Sloan Digital Sky Survey and conduct $10\times$ cross validation to evaluate the results. We present a method using a GAN trained on galaxy images that can recover features from artificially degraded images with worse seeing and higher noise than the original with a performance which far exceeds simple deconvolution. The ability to better recover detailed features such as galaxy morphology from low-signal-to-noise and low angular resolution imaging data significantly increases our ability to study existing data sets of astrophysical objects as well as future observations with observatories such as the Large Synoptic Sky Telescope (LSST) and the Hubble and James Webb space telescopes.