From CSIROscope (AU): “ASKAP searches for afterglow of gravitational wave”

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From CSIROscope (AU)


CSIRO (AU)-Commonwealth Scientific and Industrial Research Organisation

24 Jun, 2020 [Just found this anchored to another article in social media]
Annabelle Young

Scientists have made a new gravitational waves discovery. Image credit: C. Knox/ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav).

Scientists are puzzled by a new gravitational waves discovery. Have they discovered the heaviest neutron star or the lightest black hole ever observed?

More than a century ago, Albert Einstein predicted massive objects like neutron stars and black holes produce ripples in space as they orbit one another and eventually merge in a violent clash.

Gravitational waves from a black hole merger were first detected in 2015. Two years later researchers found not only gravitational waves but gamma-rays, light and radio waves from the merger of a pair of neutron stars.

The Laser Interferometer Gravitational-Wave Observatory (LIGO) discovered these gravitational waves or ‘ripples’ in space. It bagged three of its founders the 2017 Nobel prize in physics.

October 3, 2017
The LIGO Laboratory, comprising LIGO Hanford, LIGO Livingston, Caltech, and MIT are excited to announce that LIGO’s three longest-standing and greatest champions have been awarded the 2017 Nobel Prize in Physics: Barry Barish and Kip Thorne of California Institute of Technology (US) and Rainer Weiss of Massachusetts Institute of Technology (US).

The announcement was made this morning by the Nobel Committee in Stockholm Sweden. First broadcast live, you can watch the recording here: Nobel Prize in Physics Announcement.


Caltech /MIT Advanced aLigo .


LIGO’s system of lasers, mirrors and vacuum tubes make it the most precise ‘ruler’ on Earth. It’s capable of detecting these previously invisible ripples in space, which are smaller than the diameter of a proton.

In August 2019, astronomers received an alert that LIGO had detected gravitational waves from a new type of event. The long-awaited merger of a suspected neutron star and a black hole!

ASKAP on patrol for a gravitational waves discovery.

Within minutes of receiving the alert, a team led by Professor Tara Murphy at The University of Sydney (AU) activated plans to use our ASKAP radio telescope [below]. They were searching for the afterglow produced by the merger.

Because gravitational waves are so hard to detect, LIGO can’t pinpoint where these mergers occur. So, they send the astronomy community a ‘sky map’ indicating a region where the event happened. Often these maps cover as much as a quarter of the sky. This takes hundreds of hours to search using a regular telescope.

ASKAP is equipped with novel receivers that give it a wide-angle lens on the sky. In one pointing, ASKAP can view an area of sky about the size of the Southern Cross.

Coincidentally, the sky map sent by LIGO for the detection of this merger was about the same size as ASKAP’s field of view. This allowed Tara’s team to observe almost the whole area of the map at once.

Nine days after the merger, the ASKAP team found a source known as AT2019osy that had nearly doubled in brightness over the course of a week. The smoking gun of a radio afterglow?

“We immediately alerted thousands of astronomers involved in the gravitational wave follow-up effort, and telescopes across the world, and in space, began slewing to observe our candidate,” team member Dougal Dobie, a co-supervised PhD student at The University of Sydney and CSIRO said.

False start but the tide’s rising.

“Unfortunately, these observations suggested AT2019osy was produced by normal activity from the black hole at the centre of a galaxy and unrelated to the merger,” Dougal said.

Continued ASKAP searches didn’t find any other candidates. This might seem disappointing but the ASKAP team say the effort was not wasted. A non-detection rules out several scenarios and helps place limits on the energy released during the merger.

Hints of a deeper mystery

Ongoing analysis of the LIGO data has shown the lack of a radio counterpart may even support the idea something unexpected is happening. The signal received by LIGO when a merger occurs depends on the mass of the two objects involved. Initial analysis suggested the merger of a neutron star and a black hole. But a recent announcement suggests this may not be the entire story.

In August of 2019, the LIGO-Virgo gravitational-wave network witnessed the merger of a black hole with 23 times the mass of our sun and a mystery object 2.6 times the mass of the sun. Scientists do not know if the mystery object was a neutron star or black hole, but either way it set a record as being either the heaviest known neutron star or the lightest known black hole. Image credit: R. Hurt (Caltech IPAC-Infrared Processing and Analysis Center (US)) Caltech/ MIT Advanced aLIGO (US)/California Institute of Technology (US)/Massachusetts Institute of Technology (US).

“We may have discovered either the heaviest neutron star or the lightest black hole ever observed. If it really is a heavy neutron star, this will radically alter our understanding of nuclear matter in the densest, most extreme environments in the Universe,” Rory Smith from OzGrav-Monash University said.

The presence or absence of a radio counterpart may help tip the balance one way or another.

Catching the next wave

The era of gravitational wave research is still young. As the sensitivity of LIGO improves, it will detect more mergers at even greater distances.

“This is just the tip of the iceberg. ASKAP’s fast survey capability will enable us to probe the sky deeper and wider than ever before, playing a key role in understanding these mergers,” Tara said.

We acknowledge the Wajarri Yamatji as the traditional owners of the Murchison Radio-astronomy Observatory site.

See the full article here .


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CSIRO (AU)-Commonwealth Scientific and Industrial Research Organisation , is Australia’s national science agency and one of the largest and most diverse research agencies in the world.

CSIRO works with leading organisations around the world. From its headquarters in Canberra, CSIRO maintains more than 50 sites across Australia and in France, Chile and the United States, employing about 5,500 people.

Federally funded scientific research began in Australia 104 years ago. The Advisory Council of Science and Industry was established in 1916 but was hampered by insufficient available finance. In 1926 the research effort was reinvigorated by establishment of the Council for Scientific and Industrial Research (CSIR), which strengthened national science leadership and increased research funding. CSIR grew rapidly and achieved significant early successes. In 1949 further legislated changes included renaming the organisation as CSIRO.

Notable developments by CSIRO have included the invention of atomic absorption spectroscopy; essential components of Wi-Fi technology; development of the first commercially successful polymer banknote; the invention of the insect repellent in Aerogard and the introduction of a series of biological controls into Australia, such as the introduction of myxomatosis and rabbit calicivirus for the control of rabbit populations.

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CSIRO Pawsey Supercomputing Centre AU)

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SKA- Square Kilometer Array