Keck Observatory astronomers win prestigious science prize

  • O’Meara

  • The Milky Way Galaxy stretches above the core group of CSIRO’s Australian Square Kilometre Array Pathfinder radio telescope (CSIRO/Alex Cherney)

  • The W.M. Keck Observatory’s twin 10-meter telescopes open for a night of observation. Along with the Very Large Telescope and Gemini South telescopes, the Keck Observatory aided follow-up optical observations to image the host galaxy of a fast radio burst. (Ethan Tweedie/Special to West Hawaii Today)

  • An artist’s impression of CSIRO’s Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope finding a fast radio burst and determining its precise location. The W.M. Keck Observatory, Very Large Telescope and Gemini South telescopes joined ASKAP with follow-up optical observations to image the host galaxy (CSIRO/Andrew Howells)

A historic feat — successfully zeroing in on the precise location of a non-repeating fast radio burst — has earned the highest recognition from the American Association for the Advancement of Science.

The international team that made the breakthrough discovery has won the prestigious 2020 AAAS Newcomb Cleveland Prize, which goes to the most impactful research paper published in the journal Science.


“Given the robust research AAAS publishes across a variety of scientific fields, it’s a great honor to have this work selected for the Newcomb Cleveland Prize,” said W. M. Keck Observatory Chief Scientist John O’Meara, a co-author of the study. “There was a global team of astronomers involved in this work, and it’s wonderful to see such a large collaboration earn this distinction for an exciting science result.”

AAAS made the announcement on Tuesday at its 187th AAAS Annual Meeting; authors will receive the award today during a virtual ceremony.

The winning paper, “A single fast radio burst localized to a massive galaxy at cosmological distance,” was published in Science on Aug. 9, 2019, and includes key data obtained using Keck Observatory on Maunakea.

“Keck’s world-leading instrument and the nimbleness of its Target of Opportunity program let us measure the galaxy’s distance within hours after the fast radio burst was localized,” said co-author J. Xavier Prochaska of University of California, Santa Cruz, who coordinated the team that used the Keck Cosmic Web Imager on the Keck II telescope to measure the distance of the FRB’s home.

They traced it back to a galaxy called DES J214425.25−405400.81, located 3.6 billion light-years away from Earth.

FRBs are extremely bright, powerful flashes of radio waves that disappear in the blink of an eye, lasting less than a millisecond. This makes it a challenge detecting these signals, let alone pinpointing their source to then accurately measure their distance.

To catch one, the team, led by Keith Bannister of the Commonwealth Scientific and Industrial Research Organization, developed a new detection method using the Australian Square Kilometre Array Pathfinder radio telescope, which consists of an array of 36 dish antennas. Because they’re spread across about 4,000 square meters, FRB 180924’s radio waves traveled to each antenna at very slightly different times, just a fraction of a billionth of a second. Bannister’s team was able to replay the data from each dish and triangulate the FRBs source. Follow-up observations using Keck Observatory as well as the Very Large Telescope and Gemini South, both in Chile, then revealed the burst’s birthplace.

Astronomers can now further probe and characterize its host galaxy to investigate what might have generated the intensely energetic FRB.


Bannister and his team’s award-winning discovery is the first one-and-done deep-space radio signal to have its location characterized.

The paper was chosen out of 687 papers published in the Research Articles or Reports sections of Science between June 2019 and May 2020. Newcomb Cleveland Prize winners receive a medal and $25,000.

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