Aerial shot of field with special telescopes

CHIME telescope detects more than 500 mysterious fast radio bursts in its first year of operation

account_circle By Jennifer Chu, MIT News Office
Observations quadruple the number of known radio bursts and reveal two types: one-offs and repeaters.

To catch sight of a fast radio burst is to be extremely lucky in where and when you point your radio dish. Fast radio bursts, or FRBs, are oddly bright flashes of light, registering in the radio band of the electromagnetic spectrum, that blaze for a few milliseconds before vanishing without a trace.

These brief and mysterious beacons have been spotted in various and distant parts of the universe, as well as in our own galaxy. Their origins are unknown, and their appearance is unpredictable. Since the first was discovered in 2007, radio astronomers have only caught sight of around 140 bursts in their scopes.

Now, a large stationary radio telescope in British Columbia has nearly quadrupled the number of fast radio bursts discovered to date. The telescope, known as CHIME, for the Canadian Hydrogen Intensity Mapping Experiment, has detected 535 new fast radio bursts during its first year of operation, between 2018 and 2019.

Scientists with the CHIME Collaboration, including researchers at Perimeter, have assembled the new signals in the telescope’s first FRB catalog, which they will present this week at the American Astronomical Society Meeting.

The new catalog significantly expands the current library of known FRBs, and is already yielding clues as to their properties. For instance, the newly discovered bursts appear to fall in two distinct classes: those that repeat, and those that don’t. Scientists identified 18 FRB sources that burst repeatedly, while the rest appear to be one-offs. The repeaters also look different, with each burst lasting slightly longer and emitting more focused radio frequencies than bursts from single, nonrepeating FRBs.

These observations strongly suggest that repeaters and one-offs arise from separate mechanisms and astrophysical sources. With more observations, astronomers hope soon to pin down the extreme origins of these curiously bright signals.

“By adapting the existing CHIME telescope and software and adding the custom-built CHIME/FRB computer cluster, we were able continuously search huge patches of sky for FRBs and transform the field from occasional, one-off detections to a continuous stream of discoveries,” says Dustin Lang, a computational scientist at Perimeter.

“One of the really powerful aspects of the CHIME/FRB survey is that we're observing 24/7, so we're surveying the sky in a uniform way. Importantly, we know how sensitive we are to FRBs with different properties. As we build up a large collection of FRBs observed in this uniform way, we can start to understand the whole population, which is the key to unraveling the origins of FRBs," Lang says.

 

Seeing flashes

CHIME comprises four massive cylindrical radio antennas, roughly the size and shape of snowboarding half-pipes, located at the Dominion Radio Astrophysical Observatory in British Columbia, Canada. CHIME is a stationary array, with no moving parts. The telescope receives radio signals each day from half of the sky as the Earth rotates.

While most radio astronomy is done by swiveling a large dish to focus light from different parts of the sky, CHIME stares, motionless, at the sky, and focuses incoming signals using a correlator — a powerful digital signaling processor that can work through huge amounts of data, at a rate of about 7 terabits per second, equivalent to a few percent of the world’s internet traffic.

“The CHIME telescope has 1000 times the sensitivity of a traditional radio telescope, but it also generates 1000 times more data,” says Kendrick Smith, who holds the Daniel Family James Peebles Chair at Perimeter. “A few years ago, searching a CHIME-sized dataset for FRBs looked computationally impossible, but the Perimeter team made breakthroughs in algorithms and software which made the CHIME/FRB search possible."

Over the first year of operation, CHIME detected 535 new fast radio bursts. When the scientists mapped their locations, they found the bursts were evenly distributed in space, seeming to arise from any and all parts of the sky. From the FRBs that CHIME was able to detect, the scientists calculated that bright fast radio bursts occur at a rate of about 800 per day across the entire sky — the most precise estimate of FRBs overall rate to date.

“That’s kind of the beautiful thing about this field — FRBs are really hard to see, but they’re not uncommon,” says Kiyoshi Masui, assistant professor of physics at MIT and a member of MIT’s Kavli Institute for Astrophysics and Space Research. “If your eyes could see radio flashes the way you can see camera flashes, you would see them all the time if you just looked up.”

 

Mapping the universe

As radio waves travel across space, any interstellar gas, or plasma, along the way can distort or disperse the wave’s properties and trajectory. The degree to which a radio wave is dispersed can give clues to how much gas it passed through, and possibly how much distance it has traveled from its source.

For each of the 535 FRBs that CHIME detected, Masui and his colleagues measured its dispersion, and found that most bursts likely originated from far-off sources within distant galaxies. The fact that the bursts were bright enough to be detected by CHIME suggests that they must have been produced by extremely energetic sources. As the telescope detects more FRBs, scientists hope to pin down exactly what kind of exotic phenomena could generate such ultrabright, ultrafast signals.

Scientists also plan to use the bursts, and their dispersion estimates, to map the distribution of gas throughout the universe.

“This data release enables us to answer key questions about FRBs as a population,” says Masoud Rafiei-Ravandi, a PhD student at Perimeter. “In one of the companion papers, we describe a detailed analysis on the correlation between CHIME FRBs and galaxies. Intriguingly, we found statistically that CHIME/FRB sources populate the same dark matter halos that galaxies inhabit. It's just one of the ways in which this dataset is going to help us answer deep questions about FRBs – what they are, and how they can help us understand the large-scale structure of the universe.”

“We're releasing the catalog publicly so that other scientists can explore this huge dataset to hunt for clues toward the origin of FRBs. It will be exciting to see what discoveries emerge,” Smith says.

This research was supported by various institutions including the Canada Foundation for Innovation, the Dunlap Institute for Astronomy and Astrophysics at the University of Toronto, the Canadian Institute for Advanced Research, McGill University and the McGill Space Institute via the Trottier Family Foundation, and the University of British Columbia.

 

Media contacts:

Mike Brown, Perimeter Institute for Theoretical Physics
[email protected]; 519-591-5099

Abby Abazorius, MIT News Office
[email protected]; 617-253-2709
Read the MIT news release.