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Scientists pinpoint distance to fast radio burst

For the first time a team of scientists has tracked down the location of a fast radio burst (FRB), confirming that these short but spectacular flashes of radio waves originate in the distant universe.
RELATED TOPICS: RADIO ASTRONOMY
FRB
This image shows the field of view of the Parkes radio telescope on the left. On the right are successive zoom-ins in on the area where the signal came from. The image at the bottom right shows the Subaru Telescope's image of the FRB galaxy, with the elliptical regions showing the location of the fading 6-day afterglow seen with ATCA.
D. Kaplan (UWM), E. F. Keane (SKAO)

The breakthrough, published in the journal Nature, was made using the Commonwealth Scientific and Industrial Research Organization (CSIRO) radio telescopes in eastern Australia and the National Astronomical Observatory of Japan’s Subaru telescope in Hawaii.

“Our discovery opens the way to working out what makes these bursts,” said Simon Johnston, Head of Astrophysics at CSIRO and a member of the research team.

Fast radio bursts (FRBs) emit as much energy in one millisecond as the sun emits in 10,000 years, but the physical phenomenon that causes them is unknown. This, and their apparently huge distances, have tantalized scientists since their discovery in 2007. Only 16 bursts have ever been found but astronomers estimate that they might occur 10,000 times a day across the entire sky.

The recent paper in Nature records a burst from a host galaxy around 6 billion light-years away. Importantly, it also confirms that FRBs can be used to find matter in the universe that had ‘gone missing’.

Astronomers think the contents of the universe are 70 percent dark energy, 25 percent dark matter, and 5 percent ordinary matter. But when they add up the matter they can see in stars, galaxies and hydrogen gas, they still only find half as much ordinary matter as should be there — the rest has not been seen directly and so has been described as ‘missing’.

Using the burst (FRB 150418) as a tool, the team was able to ‘weigh’ the universe, or at least the normal matter it contains.

"The good news is our observations and the model match — we have found the missing matter," explained  Evan Keane from the SKA Organisation, lead author on the Nature paper. "It's the first time a fast radio burst has been used to conduct a cosmological measurement."

Most FRBs have been found by sifting through recorded data months or even years after it was taken, by which time it was too late for follow-up observations. To remedy this, Keane and his international team developed a system to detect FRBs within seconds, immediately alerting other telescopes with a view to pinpointing their location.

The Parkes telescope detected the new FRB on April 18, 2015, and two hours later, CSIRO’s Compact Array telescope, 250 miles (400 kilometers) north of Parkes, homed in on the patch of sky the flash had come from. It saw a radio source that lasted for six days before fading — the FRB’s radio afterglow. This let the researchers zoom in on the FRB about 1,000 times more precisely than any of the 16 previously detected bursts.

Meanwhile, in Hawaii, the 8.2-meter optical Subaru telescope was also at work. Looking at the FRB field, it found a galaxy that could be matched with the radio source seen by the Compact Array. More sleuthing showed that this object was an elliptical galaxy — a huge football-shaped mass of stars. Its redshift (0.492) means that it is about 6 billion light-years away. The galaxy is old, well past its prime period for star formation.

“This is not what we expected,” Johnston said. “It might mean that the FRB resulted from, say, two neutron stars colliding rather than anything to do with recent star birth.”

But there could be more than one road to an FRB, he added. “In the near future, using CSIRO’s Australian SKA Pathfinder (ASKAP) should be ideal and ASKAP will be able to start looking for FRBs this year,” he said. “We expect to find several a week, and really clean up.”

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