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The latest data from the Atacama Cosmology Telescope collaboration includes the clearest and most precise measurements yet of the universe’s earliest light.
Data and Pipeline Project Leader, Center for Computational Astrophysics
President, Simons Foundation
Over 17 years since it captured its first measurements of the universe’s earliest light, the Atacama Cosmology Telescope (ACT) collaboration has published the project’s final major data release. The latest data provide an even clearer view of what the universe was like 13 billion years ago, the universe’s composition, and the accuracy of the standard model of cosmology used to describe the universe’s structure and evolution.
The ACT researchers will present their new findings and data at a conference held by the American Physical Society on March 19 in Anaheim, California.
“It is great to see ACT retiring with this display of results,” says Erminia Calabrese, a professor of astrophysics at the University of Cardiff and a lead author on one of the new papers related to the data release. “The circle continues to close around our standard model of cosmology,” she says, with the latest results strongly backing the standard model and ruling out several proposed alternatives.
“Our standard model of cosmology has just undergone its most stringent set of tests. The results are in, and it looks very healthy,” says ACT collaboration member David Spergel, president of the Simons Foundation and previously ACT’s analysis lead. “We have tested it for new physics in many different ways and don’t see evidence for any novelties.”
From a site high in the Chilean Andes, ACT measured light from when the universe was 380,000 years old. This light is known as the cosmic microwave background (CMB). If the cosmos was now middle-aged, ACT’s images of the CMB would be the equivalent of hours-old baby pictures.
In the light, “we are seeing the first steps towards making the earliest stars and galaxies,” says Suzanne Staggs, director of ACT and the Henry deWolf Smyth Professor of Physics at Princeton University. “And we’re not just seeing light and dark, we’re seeing the polarization of light in high resolution.” That polarization provides crucial information about what happened during the universe’s first moments and how the cosmos has evolved since.
The new pictures of the CMB offer higher resolution than those made more than a decade ago by the Planck space-based telescope. “ACT measures the intensity and polarization of the light at five times the resolution of Planck and with around three times the sensitivity,” says Sigurd Naess, a researcher at the University of Oslo and lead author of the new papers related to the project. That detail enabled scientists to learn more about the cosmos, such as providing more precise measurements of the universe’s age.
The ACT collaboration’s dedication to open science has been an inspiration to the field, says ACT scientist Simone Aiola, a researcher at the Flatiron Institute’s Center for Computational Astrophysics in New York City. “ACT is one of the few ground-based experiments that has really committed to releasing as much of its data as it could.”
With the ACT project winding down, the scientific community is now excitedly looking to the Simons Observatory, which sits on the same site in Chile where ACT was based. Last year, the Simons Observatory began collecting some of the most precise measurements ever made of the CMB. With that level of precision, scientists hope to learn more about the universe and its history, such as what happened in the minuscule fraction of a second that followed the Big Bang.
“ACT demonstrated that you can do cosmology from Chile with high-resolution telescopes that capture really big patches of the sky,” Aiola says. “ACT was incredibly successful, and the Simons Observatory will do that even better.”
With ACT now winding down, the project’s researchers reflect on the unprecedented view of the universe their work has provided freely and openly to the scientific community. “We can see right back through cosmic history,” says Jo Dunkley, the Joseph Henry Professor of Physics and Astrophysical Sciences at Princeton University and the ACT analysis leader. “From our own Milky Way, out past distant galaxies hosting vast black holes and huge galaxy clusters, all the way to that time of infancy.”
