One Galaxy, Two Telescopes: How to Separate Physics from Distortions express

Original: "Learning What's Real: Disentangling Signal and Measurement Artifacts in Multi-Sensor Data, with Applications to Astrophysics"
arXiv:2604.09787 · 2026-04-10 · CC BY 4.0 · 1 min
Scientists taught a neural network to separate the true light of distant galaxies from the interference caused by different cameras.

If you photograph the same mountain with a film camera and a modern smartphone, you get different images: colors are brighter in one, details are blurrier in the other. The same goes for telescopes: each instrument sees the sky in its own way, adding its own distortions to the true light of galaxies, like a filter through which we look.

This new work offers a way to remove that 'filter.' The scientists collected pairs of images of the same galaxies taken by two large sky surveys: DESI Legacy Imaging Survey and Hyper Suprime-Cam. The neural network was trained as follows: it receives two images and must reconstruct one from the other, but taking into account that the cameras are different. During training, the network itself finds what is common to the two images (that is the real galaxy) and what differs (that is the distortion of a particular telescope).

The method is similar to how a person learns to understand accented speech: hearing the same word from different people, they pick out the essential and stop noticing the peculiarities of pronunciation.

As a result, the neural network outputs a 'clean' representation of the galaxy — without the noise and distortions of a specific instrument. This allows, for example, searching for similar galaxies in the archives of different telescopes without fear that their similarity is spoiled by different cameras. This approach is useful not only for astronomy: it provides a general recipe for training neural networks on data from different instruments — from medical scanners to sensors in cars.

Both telescopes whose data the scientists used are on Earth, but one of them (Hyper Suprime-Cam) is installed in Hawaii, while the other (DESI Legacy) scans the sky from an observatory in Arizona. The distance between them is about 4,800 km, but they see the same galaxies.

Scientists
Fritz ZwickySubrahmanyan ChandrasekharAdam RiessJohn Archibald WheelerGalileo GalileiWilliam Herschel
Concepts
artifact astrophysical signal detection degeneracy signal averaging medical imaging artifact detection data cleaning dataset labeled data overfitting false positive learning ai astrophysics astrophysics Contrastive Learning background statistics sensor distance statistical analysis Reinforcement Learning