Astronomers search distant galaxies for giant star-forming clumps — cradles of stars that were furiously born billions of years ago. Manually sifting through hundreds of thousands of images is like a mushroom forager combing an endless forest. But machine learning gives the forager-program an atlas of examples.
First, thousands of volunteers labeled galaxies — this is the ABCs. Then the neural network examined every patch of sky in six bands — from ultraviolet to infrared. Ultraviolet, by the way, added discoveries: young stars shine there like tiny lanterns. To weed out mistakes, scientists sprinkled in computer-generated fakes — and the program spotted them.
The result: one and a half million candidates in 710,000 galaxies. By evaluating the reddening of light (galaxies are racing apart), heavy-element impurities, and interstellar gas, scientists will reconstruct galaxy growth. Meanwhile, splitting light will tell the stellar life story.
To train the program, scientists labeled over three thousand images, marking all the "impostors" — stars and background galaxies that can easily be mistaken for clumps.