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New type of Fast Radio Burst discovered in Green Bank Telescope data

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New type of Fast Radio Burst discovered in Green Bank Telescope data

Green Bank Telescope with artist rendering of microsecond Fast Radio Bursts above the antenna's dish.

Artist’s impression of the discovery of microsecond Fast Radio Bursts being observed by the Green Bank Telescope. Incoming radio waves are shown as white, red, and orange streaks that follow each other in rapid succession. The long red streaks are the previously known millisecond flashes. (c) Daniëlle Futselaar/www.artsource.nl

An international team of researchers have discovered radio pulses from the distant universe that last only millionths of a second. They found these microsecond bursts after a meticulous examination of archival data from the National Science Foundation’s Green Bank Telescope. It’s unclear how the ultrafast bursts were created. The researchers published their findings in Nature Astronomy.

Fast radio bursts (FRBs) are unpredictable, extremely short flashes of radio waves far beyond our Milky Way. They are possibly caused by magnetic neutron stars, also known as magnetars. The first bursts were discovered in 2007. So far, most bursts last longer than a thousandth of a second and emit as much energy as our sun generates in a day.

In 2022, researchers at the University of Amsterdam and ASTRON hypothesized that there might be bursts that would last not thousandths, but only millionths of a second. “During our group meetings, we often talked about it”, says Mark Snelders, PhD candidate at ASTRON and the University of Amsterdam (the Netherlands), who was in charge of the research that uncovered the ultra-fast radio bursts. “By coincidence, I found out that there was a public dataset that we could use for this.”

Watch a presentation by Mark for the Green Bank Observatory about this science.

Five hours of data – and millions of images

The researchers accessed the public data archive from the Breakthrough Listen project, which uses the Green Bank Telescope to search for extraterrestrial life. They focused on five hours of data from FRB 20121102A, located some three billion light years away, towards the Auriga constellation.

The researchers divided each second of the first thirty minutes of data into half a million individual images. Next, they used software filters and machine learning to search for outliers. Through this meticulous process, they discovered eight ultra-fast bursts that lasted only ten millionths of a second or less.
Now that the first ultra-fast microsecond source has been detected, researchers expect to find more. However, finding them may be easier said than done, as some data files are not detailed enough to cut into half a million pieces per second.

The Green Bank Observatory is supported by the National Science Foundation and is operated by Associated Universities, Inc.

Read more at the Netherlands Research School for Astronomy.

Media Contact:
Jill Malusky, NRAO & GBO News & Public Information Manager
[email protected]

This news article was originally published on the GBO website on October 19, 2023.

Recent News

Next-Generation Very Large Array Antenna Design to be Used By German Astronomers

The U.S. National Science Foundation National Radio Astronomy Observatory has announced a significant collaboration with the Bavarian State Government to construct a cutting-edge radio telescope atop Germany’s highest mountain. This radio telescope will use the design of the proposed NSF NRAO’s Next Generation Very Large Array (ngVLA).

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High-energy transient signals are most often determined to be gamma-ray burst events, but the recently-launched Einstein Probe has expanded astronomers’ ability to quickly respond to similar signals occurring at X-ray wavelengths. Now, a multi-wavelength study of EP240408a concludes that while many of the signal’s characteristics might lead to the conclusion that it is a gamma-ray burst, the non-detection at radio wavelengths precludes that possibility.

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The flexible observing setup of the Green Bank Observatory’s 20-meter telescope enabled frequent, long-duration observations of eight pulsars, spanning two and a half years for a student-driven study carried out by students in the Pulsar Science Collaboratory program.