From AAS NOVA: “ASKAP Finds a Real-Time Radio Burst, but No Glow”

AASNOVA

From AAS NOVA

16 November 2020
Susanna Kohler

Australian Square Kilometre Array Pathfinder (ASKAP) is a radio telescope array located at Murchison Radio-astronomy Observatory (MRO) in the Australian Mid West. ASKAP consists of 36 identical parabolic antennas, each 12 metres in diameter, working together as a single instrument with a total collecting area of approximately 4,000 square metres.

As powerful millisecond bursts of radio emission continue to light up our detectors from across the universe, the hunt for the origins of these fast radio bursts continues. It’s the search for light before and after the burst, however, that might prove key to unraveling their mystery.

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Artist’s impression of the ASKAP radio telescope finding a fast radio burst. Other observatories are shown joining in follow-up observations. Credit:CSIRO/Andrew Howells.

An Extragalactic Puzzle

Since the first discovery of fast radio bursts (FRBs) more than a decade ago, we’ve found ~100 of them, including more than 20 that have been observed to repeat. Despite this growing sample — and though we’ve now localized repeating and non-repeating FRBs to distant host galaxies — we still don’t know with certainty what causes them.

Many of the leading origin theories for FRBs come with predictions of other emission that should complement the radio flash. The birth of a magnetized neutron star, for instance, should produce not only an FRB, but also a radio afterglow — steadier radio emission that appears after the burst and then slowly fades over time.

The fact that we haven’t yet found any radio afterglows definitively associated with FRBs means one of three things: 1) they don’t happen, 2) they’re fainter than we can detect, or 3) they evolve on quicker timescales than we’ve been surveying, so they’ve already faded by the time we look. A new radio array enterprise is focusing on ruling out the third of these possibilities.

Real-Time Eyes on the Skies

To catch a quickly evolving afterglow, we need real-time observations of FRBs — allowing us to monitor the source for radio emission before, during, and immediately after the burst. To this end, a new survey was begun in mid-2019 with the The Australian Square Kilometre Array Pathfinder (ASKAP): the Commensal Real-time ASKAP Fast Transients Survey (CRAFT).

CRAFT runs continuous low-time-resolution observations of the sky while ASKAP is being used for other survey science projects. When an FRB is spotted, the survey automatically saves the data from before and after the FRB itself, so that the survey team can search it for radio precursor and afterglow emission.

In a new study, a team of scientists led by Shivani Bhandari (Australia Telescope National Facility, CSIRO (AU) reports the first detection of an FRB in this mode: FRB 191001.

The Verdict: No Glow

From the CRAFT data, the authors were able to localize FRB 191001 to the outskirts of a star-forming spiral galaxy at a redshift of z = 0.234 (that’s nearly 3 billion light-years away!). The CRAFT data revealed neither a persistent, compact radio source before the burst, nor a slowly varying radio afterglow after the burst.

What does this mean? The lack of detectable afterglow for FRB 191001 alone doesn’t yet rule out any formation scenarios — but it does demonstrate that the afterglow was either fainter than our detection thresholds, or it didn’t occur at all.

And this CRAFT detection is just the start! With more observations like this one — especially of closer FRBs that would be expected to appear with correspondingly brighter afterglows — we may soon be able to narrow down the options of what causes these mysterious flashes.

Citation

“Limits on Precursor and Afterglow Radio Emission from a Fast Radio Burst in a Star-forming Galaxy,” Shivani Bhandari et al 2020 ApJL 901 L20.

https://iopscience.iop.org/article/10.3847/2041-8213/abb462

See the full article here .


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