AI finds hidden data of galactic evolution in over 100 galaxies. Here’s how

The interstellar clouds of distant, ancient galaxies are often filled with carbon. That means, if astronomers can track down and detect these bits of carbon, which they call neutral carbon absorbers, they can learn a lot about how galaxies evolve.

However, actually detecting neutral carbon absorbers—a process that usually involves finding the signature fingerprint of carbon absorption lines in the spectrum of light emitted by a galaxy—is tedious. It is also very difficult. Out of millions of galaxies, astronomers know only a few dozen that contain these absorbers.

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