Category: News

White dwarf binary provides unique natural laboratory for extreme physics

An international team led by astronomers at the University of Sydney has uncovered the clearest evidence yet for the origin of an unusual class of cosmic signals. In doing so, they have identified a rare stellar system that is providing scientists with a natural laboratory to study extreme physics.

Using CSIRO’s ASKAP radio telescope, the team discovered a small, dense star, called a white dwarf, shredding material from its larger, but less dense, companion star. As this material spirals in, it produces powerful bursts of radio waves and X-rays in a cycle that repeats every 1.4 hours.

The findings are published in Nature Astronomy.

Lead author and PhD student Kovi Rose from the University of Sydney’s School of Physics and CSIRO said this provides the first confirmed identification of what astronomers call ‘long-period radio transients’: cosmic pulses discovered from just a few remote regions of our galaxy.

“For the first time we have pinpointed the origin of these signals, confirming the source to be a ‘cataclysmic variable’, or an accreting white dwarf star,” said Mr Rose.

“Long-period radio transients have puzzled astronomers for years,” Mr Rose said. “We’ve only found about a dozen, and their origins have been unclear. Now, we’ve been able to show that the source for one of these transients comes from a white dwarf actively pulling material from a companion star.”

A rare and revealing system

The newly identified system, named ASKAP J1745−5051, consists of a white dwarf – a dense stellar remnant roughly the size of Earth but with the mass close to that of the Sun – paired with a larger but lower-mass red dwarf star of about one-tenth the Sun’s mass. The two stars orbit each other extremely closely, completing a full orbit in just over an hour.

As material from the less massive star is drawn towards the white dwarf, it heats up and emits X-rays. At the same time, interactions between the stars’ magnetic fields generate regular radio bursts, meaning the signal occurs at specific intervals.

“These emissions are all tied to the orbital motion of the system,” Mr Rose said. “But interestingly, the radio and X-ray signals don’t peak at the same time, which tells us they’re being produced in different regions of the system.”

The team found that the radio emission likely originates where the magnetic fields of the two stars meet and interact with the charged material being ripped from the companion star, producing tightly beamed bursts of radiation.

Solving a cosmic mystery

Long-period radio transients were initially thought to be slow-spinning neutron stars, known as pulsars. However, current models suggest neutron stars rotating this slowly should not be able to produce such signals.

The new discovery strengthens an alternative explanation: that at least some of these mysterious bursts come from systems of two stars, involving white dwarfs.

“Some similar objects had been linked to binary systems before, but this is the first one where we can clearly see both stars and the accretion process in action,” said Professor Murphy, Head of School at the University of Sydney School of Physics and Chief Investigator at the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav).

The system is also only the second known long-period radio transient to emit regular X-rays – and the first where the cause of the regularity has been confirmed.

A ‘Rosetta stone’ for future discoveries

This unique system was discovered using the ASKAP radio telescope, owned and operated by CSIRO, Australia’s national science agency. ASKAP’s mix of coverage, resolution, and sensitivity is unparalleled in radio astronomy, allowing for such unusual signals to be detected that would otherwise be missed.

The researchers say that ASKAP J1745-5051 could act as a reference point for understanding other long-period radio transients.

“This system gives us a way to decode these signals. It could help us determine whether other long-period transients are more like pulsars or like white dwarf systems, acting like a stellar Rosetta stone,” said Mr Rose, referring to the archaeological object discovered in Egypt that helped translate ancient hieroglyphics.

The discovery also provides a unique opportunity to study extreme plasma physics and magnetic interactions under conditions that cannot be replicated on Earth.

“These systems are natural laboratories,” Mr Rose said. “They allow us to test our understanding of how matter behaves in strong magnetic fields and under intense gravitational forces.”

Future research

The team plans further observations combining radio, optical and X-ray telescopes to better understand how these emissions are generated and whether similar mechanisms can explain the full population of long-period radio transients.

“Each new discovery is helping us piece together the bigger picture,” Mr Rose said. “We’re only just beginning to understand this new class of cosmic events.”

The international team included astronomers from the United States, China, Canada, Spain, Israel and Australia. The team used CSIRO’s Australia Telescope Compact Array and ASKAP radio telescopes in Australia, the MeerKAT radio telescope in South Africa, the SOAR and Magellan optical telescopes in Chile, and the space-based Swift (UV/X-ray) and Einstein Probe (X-ray) telescopes.

MEDIA ENQUIRIES: media.office@sydney.edu.au

Media Release prepared by Ivy Shih, Media and PR Adviser | University of Sydney

RESEARCH: Rose, K. et al ‘Periodic radio and X-ray emission from an accreting white dwarf binary’ (Nature Astronomy 2026). DOI: 0.1038/s41550-026-02882-x

Watch the explainer video below:

The LIGO-Virgo-KAGRA (LVK) Collaboration has today released its latest catalog of gravitational-wave detections. The data analysed for this update were collected by the twin Laser Interferometer Gravitational-wave Observatory (LIGO) detectors and the Virgo detectors. They are the world’s premier observatory of gravitational waves, ripples in the fabric of spacetime.

This catalog aggregates hundreds of cosmic collisions between pairs of black holes, each producing a new, heavier black hole. These distant events provide a rich dataset for scientists to map out how the Universe builds black hole systems.

Using the new data, compiled in the Gravitational-Wave Transient Catalog (GWTC-5.0), scientists from the LVK collaboration and  the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav) at Monash University, have identified clear evidence that black hole binaries are born in distinct sub-populations. Effectively, different cosmic assembly lines that operate in unique environments.

Project lead, Sharan Banagiri, a Research Fellow from Monash University’s School of Physics and Astronomy and OzGrav, used this data to observe the shared characteristics of colliding black holes and neutron stars.

“This set of nearly 400 gravitational-wave detections from LIGO and Virgo provides us with a clear indication that the binary black hole mergers we see are forming in several different ways. Some might form as one giant cloud of gas that collapses to give two massive stars that then become black holes. Others might be black holes that wander into each other in dense environments called clusters that are packed with stars. While others are the product of a previous generation of mergers between two black holes,” Dr Banagiri said.

The paper, released as a preprint, found that there is a presence of multiple sub-populations of merging black holes that can potentially arise from different formation pathways.

Assistant Professor of physics at Princeton University, Sylvia Biscoveanu, co-author of the study and previously a Fulbright postgraduate scholar at Monash University, commented on the unprecedented scale of the catalog update.

“GWTC-5 represents the largest single increase in the size of the gravitational-wave catalog, including events with remarkable properties such as GW241127, which contains BHs of very different masses with clearly wobbling orbits due to tilted spins. The new catalog also contains the event with the best localisation on the sky to date, GW240615.”

The researchers also found that some of these black holes are spinning very rapidly. These fast spinning black holes have two different sets of masses; the first set are between 10-20 times the sun’s mass and the second set have masses greater than 45 times the sun’s mass.

“One of the most fascinating things we’ve discovered about these new black holes is that they are spinning very fast. The sun rotates once every 25 days. If it became a black hole and started spinning as quickly as the ones we discovered, it would be rotating several thousand times every second. So where do these rapidly-spinning black holes come from? One leading explanation is that they are ‘hierarchical’ products of a previous generation of merger between two black holes,” Dr Banagiri said.

The paper identified that black holes which are hierarchical in origin, are more massive than other black holes nearby. By analysing the new data set, the researchers found that the black holes more massive than 45 times the sun, are more likely to merge with lower mass black holes.

The new dataset will provide rich new information about black holes for astronomers and scientists to research.

Chief Investigator at OzGrav and Professor of Physics and Astronomy at Monash University, Eric Thrane, said this is a milestone as gravitational-wave astronomy transitions from the discovery of individual events to the statistical profiling of cosmic population

“We are no longer just looking at individual anomalies, instead, we are seeing a true kaleidoscope of cosmic collisions. We are pushing the edges of what we know, seeing things that are more massive, spinning faster, and more unusual than ever before,” Professor Thrane said.

Read the research paper: https://dcc.ligo.org/LIGO-P2600045/public

MEDIA Release prepared by Monash University.

An international team of scientists from the LIGO, Virgo, and KAGRA collaborations, including researchers from the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav), has completed one of the most sensitive searches yet for continuous gravitational waves from young supernova remnants. 

 Neutron stars (NSs) are among the most exotic objects in the Universe. They are born when massive stars die in energetic explosions called core-collapse supernovae. These explosions rip the star apart and leave behind a beautiful diffuse nebula called a supernova remnant.  

“These objects are incredibly extreme environments,” said Dr Ornella Piccinni, from the University of the Balearic Islands and Associate Investigator at OzGrav, who led the study while at the Australian National University. “They give us a way to test physics in conditions we can’t reproduce on Earth.” 

NSs are also the strongest magnets in the Universe and can rotate astonishingly fast, with some rotating hundreds of times per second. Astrophysical estimates suggest that millions of NS may have formed in our Galaxy. However, only a fraction of neutron stars are observed as pulsars (they emit pulses of light). This lack of observation may be either because their emission beams do not intersect the Earth or because they have become too weak to detect. As a result, most neutron stars remain electromagnetically silent, and their internal properties are largely inaccessible even to the most sensitive telescopes. 

“Gravitational-wave signals from neutron stars are incredibly faint, which makes them difficult to detect,” said Dr Ling (Lilli) Sun. “But they carry unique information about the structure of neutron stars.” 

Continuous gravitational waves (CWs) provide a new tool to discover previously missed pulsars and unobserved NSs and probe their exotic interiors. 

In a recent paper, the team searched for continuous gravitational waves from 15 young to middle-aged supernova remnants, ranging from approximately 40 years old (SN 1987A) to tens of thousands of years old, 14 of which are in our galaxy and one in our neighbouring galaxy, the Large Magellanic Cloud. 

The search used eight months of data from May 2023 to Jan 2024 during the first phase of the detectors’ fourth observing run (O4a). 

While transient bursts of gravitational waves are now regularly observed, CWs are much harder to detect because these signals are expected to be far weaker than the bursts seen from neutron star or black hole mergers, often weaker by several orders of magnitude. 

But no detection does not mean there are no results. 

By measuring how sensitive the search was, the team was able to place the strongest limits so far on how strong these signals could be, improving on previous observing runs. These limits help narrow what scientists think neutron stars can look like, including how “bumpy” they are and how matter behaves under the most extreme conditions in the Universe. 

“Even when we don’t see a signal, we’re still learning,” said Yutong (Tracy) Bu from the University of Melbourne, who worked on the analysis. “We can place stronger constraints on what these neutron stars are doing.” 

These systems may host young neutron stars where the rotation frequency is still unknown. Their relatively young age implies that the neutron star candidates are more likely to have non-uniform deformations than older ones and emit stronger continuous gravitational waves. 

“We’re pushing the sensitivity of these searches further than ever before,” said Dr Piccinni. “Each step brings us closer to a detection.” 

These results are the most sensitive broadband frequency searches so far for continuous gravitational waves from supernova remnants. 

As data collection continues and sensitivity improves, researchers are closing in on the first detection of continuous gravitational waves — a breakthrough that would open an entirely new way of studying neutron stars. 

Watch the explainer video below:

An international team of scientists from the LIGO, Virgo, and KAGRA collaborations, including researchers from the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav), has shown for the first time that gravitational waves, ripples in space and time produced by some of the most violent events in the Universe, such as the collision of two black holes, can be used to measure and correct the calibration of the detectors that observe them.

The breakthrough comes from the study of two exceptionally strong gravitational-wave signals, known as GW240925 and GW250207, produced by the collisions of pairs of black holes and detected by the twin detectors of the US National Science Foundation Laser Interferometer Gravitational-wave Observatory (NSF LIGO). These events were so strong that they allowed researchers not only to study the black holes that created them, but also to check how accurately the detectors were recording the signals.

“In a way, we are using black holes to help check the accuracy of our detectors. How cool is that!” said Dr Ling (Lilli) Sun from the Australian National University.

Three OzGrav researchers from three different Australian universities played key scientific roles in the study. Dr Ling (Lilli) Sun from the Australian National University provided scientific leadership on the paper, while Mallika Sinha, a PhD student at Monash University, and Dr Yi Shuen Christine Lee, a Postdoctoral researcher at the University of Melbourne, made important contributions to the analysis and interpretation of the results.

The LIGO–Virgo–KAGRA collaboration has now confidently detected more than 200 gravitational-wave signals from merging black holes and neutron stars. Each signal carries information about its source and the extreme physics governing these collisions. Extracting that information requires the detectors to measure gravitational waves with extraordinary precision and to carefully account for any uncertainties in those measurements.

Gravitational waves stretch and squeeze spacetime as they pass through Earth. The detectors measure this by sending laser light down two perpendicular arms and looking for tiny differences in the time it takes the light to travel back and forth. A typical gravitational wave changes the arm length by about one ten-billionth of a billionth of a metre, smaller than the width of a proton.

“Thanks to major upgrades over the past decade, our detectors are now so sensitive that signals from colliding black holes come through loud and clear,” said Dr Sun. “If Einstein’s theory of general relativity is correct, those signals should follow a very specific pattern.”

Turning those minute measurements into a physical gravitational-wave signal requires a detailed model of the detector’s response. This includes accounting for the complex control systems used to keep the instruments stable. Normally, calibration uncertainties are measured and estimated using auxiliary lasers, sensors, and engineering data. However, during the detections of GW240925 and GW250207, the LIGO Hanford detector happened to have a larger calibration error than usual.

According to Dr Sun, “by comparing the predicted signal with what we actually record, we can spot tiny mismatches that sometimes reveal the detector wasn’t perfectly calibrated at the time.”

Because both signals were exceptionally loud, the researchers were able to disentangle the true gravitational-wave signal from the detector’s calibration error, a process known as astrophysical calibration. GW240925 served as a verification case, allowing the team to compare results from astrophysical calibration with data that was later corrected using standard methods.

GW250207, meanwhile, is the second-loudest gravitational-wave event ever observed and provides a unique window into extreme physics. For this event, astrophysical calibration was essential to ensure the data could be trusted at all.

Accurate calibration is critical because even small errors can bias estimates of key source properties, such as the masses of the black holes, whether they are spinning, and where the signal originated in the sky.

“It was simply bad luck that such a loud event was observed while LIGO Hanford was in an unsettled state,” said Mallika Sinha. “As our detectors become more sensitive and we observe more events, situations like this will only become more common. Without astrophysical calibration, we might not be able to reliably analyse these interesting events and miss out on some nifty science.”

The researchers found that GW240925 was produced by black holes around nine and seven times the mass of the Sun, while GW250207 involved black holes roughly 35 and 30 times the Sun’s mass.

“Using three detectors instead of two helps us pinpoint the location of gravitational-wave sources much more precisely, which also means we can better understand the physical properties of the sources themselves,” said Dr Yi Shuen Christine Lee.

“This successful astrophysical calibration using GW240925 and GW250207 is an exciting step forward for gravitational-wave astronomy. It improves our chances for extracting important astrophysical information from gravitational-wave sources, even when traditional detector calibration methods are not accurate or feasible!”

Because of its strength and position in the sky, GW250207 is considered one of the most promising gravitational-wave signals for future measurements of the Hubble constant, although many such “dark siren” events, gravitational-wave signals from black hole mergers that produce no visible light, will be needed to resolve the long-standing tension between different cosmological measurements.

Together, GW240925 and GW250207 mark the first successful tests of astrophysical calibration, a technique that could allow scientists to trust gravitational-wave data even when detectors are in an unsettled state.

As gravitational-wave astronomy moves from discovery to precision science, using the Universe itself to help calibrate our instruments may become an increasingly powerful tool.

Watch the explainer video below:

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Media Enquiries

Researchers from the study are available for interview.

For interview requests, additional information, or media enquiries, please contact:

Diana Haikal
Senior Communications and Engagement Advisor
ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav)
ozgrav.comms@swin.edu.au

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DOI: https://doi.org/10.1103/gzrj-mwv3

Physical Review Letters journal link:  https://journals.aps.org/prl/accepted/10.1103/gzrj-mwv3

 

 

 

An awe-inspiring new chapter in science engagement has begun, with Professor Matthew Bailes, Director of the ARC Centre of Excellence for Gravitational Wave Discovery, officially launching Swinburne Virtual Universe.

The space is exactly what it sounds like. A fully immersive room wrapped in more than 100 square metres of high-contrast LED screens, where you’re not just looking at the Universe, you’re inside it.

Visitors can move through a virtual solar system, guided in real time, with 3D visuals built from supercomputer simulations and real astrophysics data. It’s designed to make complex science feel intuitive, and honestly, a bit magical.

“It’s hard to describe that moment,” Professor Bailes said, reflecting on seeing Saturn’s rings stretch across the entire space. “You feel like you can walk along them and look out into infinity. That’s the feeling I want people to experience when they come in here.”

The idea for the Virtual Universe goes back much further. For Bailes, it traces all the way back to watching the Moon landing as a child and the sense of wonder that came with it. That same feeling is what this space is trying to recreate, not just for students, but for anyone who walks through the door.

Early reactions suggest it’s working.

From school students reaching out to grab floating moons, to adults completely absorbed in the experience, the Virtual Universe is already doing what it set out to do, connecting people to science in a way that sticks.

Built in partnership with OzGrav, the facility brings together research, technology and storytelling in one place. It also opens up new opportunities, not just for outreach, but for research translation and creative industries.

Now open, the Virtual Universe is already bringing in schools and the wider community, turning curiosity about space into something people can actually step inside and feel.

To learn more, visit www.svu3d.ai

Watch Professor Matthew Bailes speaking about SVU below:
Professor Matthew Bailes speaking about SVU

An international team of scientists led by the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav) at Monash University has uncovered evidence of a rare form of exploding star, helping to shed light on one of the most cataclysmic events in the Universe.

At the end of their lives, most massive stars collapse into black holes – objects with gravity so strong that not even light can escape.

Some very massive stars, however, are expected to become so hot that they are blown apart in a pair-instability supernova – an explosion so intense that the star is completely disrupted, leaving behind no black hole.

First predicted in the 1960s, pair-instability supernovae are challenging to distinguish from more common stellar explosions that leave behind black holes.

In a study published in Nature, researchers found that by using gravitational waves – ripples in the fabric of spacetime detected by the LIGO-Virgo-KAGRA observatory network – they were able to measure the properties of black holes and found a “forbidden range” of black-hole masses.

Black holes with masses more than 45 times the mass of the sun are rare because the stars that might otherwise have made them exploded in pair-instability supernovae.

Project lead, Hui Tong, a PhD candidate from OzGrav at Monash University’s School of Physics and Astronomy, said the research found a forbidden mass range where stars seemingly don’t make black holes.

“The observation is well explained by pair instability; there are no stellar-origin black holes in the forbidden zone because stars are undergoing pair-instability supernovae. The only black holes in this mass range are made from merging smaller black holes, rather than directly from stars,” Mr Tong said.

Confirming the existence of this gap would help settle a major question about how the most massive stars live and die, and the origin of black holes.

Project collaborator, Professor Maya Fishbach from the University of Toronto and CITA said the study highlights the potential of gravitational waves to probe the lives, deaths and afterlives of the most massive stars in our Universe.

“We are seeing indirect evidence of one of the most titanic blasts in the cosmos: pair-instability supernovae. At the same time, we are finding that once they are born, black holes can grow via repeated mergers,” said Professor Maya Fishbach.

“It’s a cool result because we are using black holes to learn about the nuclear reactions inside stars,” said Professor Eric Thrane, Chief Investigator at OzGrav.

Read the research paper: https://doi.org/10.1038/s41586-026-10359-0

Watch our explainer video below:

Australia may be far from the world’s seismic hotspots, but a team from the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav) at the Australian National University (ANU) is leading a breakthrough that could transform how earthquakes and tsunamis are detected worldwide. With $671,000 in new funding from the Australian Research Council’s (ARC) Discovery Projects (DP) scheme, Professor Bram Slagmolen and colleagues are developing technology capable of detecting earthquakes almost as soon as they happen at the speed of light.

When earthquakes strike, devastation can unfold in minutes or even seconds. Current early warning systems, such as those in Japan, rely on networks of seismometers to detect seismic waves. While effective, these systems can only provide limited notice, as seismic waves travel comparatively slowly through the Earth.

Professor Slagmolen explained the stakes “Our work focuses on creating early warning systems that could provide precious seconds for earthquakes and valuable minutes for tsunamis, allowing more time to safeguard lives, halt hazardous activities, and protect vital infrastructure such as power stations and gas pipelines.”

Those seconds matter. Extra lead time could allow high-speed trains to decelerate safely, surgeons to pause delicate procedures, or operators to shut down power grids in controlled ways. For tsunamis, additional minutes could mean entire coastal communities have time to evacuate.

So how does it work? The key lies in detecting prompt elasto-gravity signals, tiny changes in gravity generated the instant a fault ruptures in the Earth. Unlike seismic waves, which move at the speed of sound in rock, gravitational changes propagate at the speed of light.

Professor Robert Ward, OzGrav node leader at ANU, likens it to watching someone swing an axe across a field: you see the movement instantly, but the sound of the strike takes seconds to reach you. The gravitational “signal” arrives first, and with the right sensors, it can be measured before the destructive shaking begins. “Much of this system has been designed and fabricated here at ANU, it’s a huge engineering effort, and now we’re entering the phase of commissioning and testing.”

The team has already built and tested a prototype sensor. Now, they are installing it on a sophisticated seismic isolation platform, similar to those used in gravitational-wave observatories like Virgo in Italy and KAGRA in Japan, to filter out local vibrations and allow the sensor to focus only on gravitational changes.

Although Australia is not earthquake-prone, its scientists are global leaders in gravitational-wave detection, a field that requires ultra-sensitive instruments capable of measuring minuscule distortions in space-time. That expertise provides a unique advantage for tackling the challenge of gravitational earthquake detection.

“Australia may not experience major earthquakes, but we have world-class expertise in gravitational-wave detection, and that makes us uniquely placed to lead this research,” said Ward.

International collaboration is essential to the project’s success. Researchers in Japan and Switzerland are already testing smaller-scale versions of the sensor for both earthquake research and fundamental physics experiments. These partnerships ensure that the technology is not only refined in Australia but also tested in regions where earthquakes are more frequent, accelerating its path toward real-world deployment.

The coming years will focus on commissioning the upgraded sensor system and validating its performance. If successful, the technology could become an integral part of next-generation early warning systems, providing unprecedented speed and reliability.

For Ward, the ultimate goal is clear: “Ultimately, this technology could help solve a global problem: giving communities precious time to prepare before an earthquake or tsunami strikes.”

By uniting physics, engineering, and international cooperation, the ANU-led team is charting a path toward safer, more resilient societies. Their work demonstrates the power of fundamental research to address urgent global challenges.

OzGrav Annual Awards

Our Annual Awards celebrate the people and teams who embody OzGrav’s values — excellence in research, collaboration, service, equity, and community. From scientific leadership to mentoring, outreach, and care for others, these awards recognise the many ways our members strengthen both our science and our culture.

We thank the judging panel for their time and thoughtful consideration.

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Advancing Equity Award

Winner: Kirsten Banks
Kirsten is recognised for her outstanding leadership in championing First Nations astronomy. Through mentoring Indigenous high school students and creating meaningful pathways into STEM, she has made a lasting contribution to equity, diversity, and inclusion within OzGrav and the broader astronomical community.

Runner-up: Sparrow Roch
Sparrow is recognised for generously sharing their cultural heritage and sky stories, fostering deeper understanding and appreciation of Indigenous perspectives in astronomy and strengthening inclusive engagement across the Centre.

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Cross-Nodal Collaboration Award

Winner: Liana Rauf
Liana is recognised as an exemplar of cross-nodal leadership, consistently leading and supporting initiatives that strengthen collaboration across OzGrav. Her work has elevated gravitational-wave cosmology research within the Centre and internationally.

Runner-up: Terry McRae
Terry is commended for his calm, proactive leadership in aligning the efforts of multiple research groups across OzGrav nodes, helping to build strong and sustained collaborations.

Highly Commended:

• The MeerKAT PTA Team

• The Arm-Length Stabilisation Team

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Mentor Award

Winner: Yeshe Fenner
Yeshe is recognised for her exceptional mentoring, providing thoughtful guidance and support that enables members of the OzGrav community to grow both personally and professionally.

Runner-up: Daniel Reardon
Daniel is commended for his approachability and for fostering a welcoming learning environment that builds confidence and supports students’ aspirations.

Highly Commended:
Ryosuke Hirai, Simon Stevenson, Khaled Said, Terry McRae, Bram Slagmolen, Paul Lasky, Andrés Vargas, Eric Thrane

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Professional Resilience Award

Winner: Sparrow Roch
Sparrow is recognised for consistently embodying professional resilience, demonstrating a willingness to take risks, embrace uncertainty, and openly learn from setbacks in pursuit of continued growth.

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Research Translation Pioneer Award

Winner: Diana Haikal
Diana is recognised for proposing, designing, and leading the establishment of the Australian Research Translation and Innovation Consortium (ARTIC), creating a new pathway for industry–research collaboration.

Runner-up:
Bram Slagmolen, Robert Ward, Sheon Chua, Avanish Kulur Ramamohan, Lane Scheel
For groundbreaking work developing speed-of-light earthquake and tsunami early-warning technology.

Highly Commended:
Emily Rose Rees, Andrew Wade, Kirk McKenzie
For developing a novel laser-stabilisation technique to improve long-term measurements on the GRACE missions.

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Discovery Theme Award

Winner: Teagan Clarke
Teagan is recognised for combining creativity, technical rigour, and a fearless approach to challenging assumptions in multimessenger astronomy. Their work has raised OzGrav’s profile within the LIGO–Virgo–KAGRA community and beyond.

Runner-up: Joshua Lee
Joshua is commended for his role in the discovery and analysis of a long-period radio transient, delivering results with significant implications for neutron star physics.

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Instrumentation Theme Award

Joint Winner: Kar Meng Kwan
Recognised for pioneering work on optical squeezing for gravitational-wave detectors, demonstrating deep technical understanding and innovative problem-solving.

Joint Winner: Thomas Rooke
Recognised for outstanding initiative in developing the QOSEM sensor, a major OzGrav contribution to identifying sources of excess low-frequency noise in LIGO detectors.

Runner-up: Jian Liu
Commended for significant contributions to advanced configuration and control techniques for future detectors.

Highly Commended:

• Quantum Efficiency Team

• Coatings Team

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Physics Theme Award

Joint Winners: Lilli Sun, Dana Jones, Fulin Li, Neil Lu, Ornella Piccinni, Aswathi Subhash
Recognised for leading analyses underpinning major LIGO collaboration papers and for developing new methods to search for ultralight bosonic dark matter using gravitational-wave data.

Runner-up: Neil Lu
Commended for key contributions to multiple LVK papers and for advancing OzGrav’s Gravity Key Program.

Joint Winner: Paul Disberg
Recognised for an exceptional publication record during his PhD, including a standout paper on neutron star kick velocities.

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Service Award

Winner: Liana Rauf
Liana is recognised for her exceptional service to OzGrav, including leadership roles on committees, cross-nodal coordination, and program scientist responsibilities.

Runner-up: Karl Wette
Karl is commended for his sustained dedication to the Centre through EDI committee work and broader OzGrav initiatives.

Highly Commended:
Diana Haikal, Neil Lu

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Superstars of Outreach Award

Winner: Yi Shuen (Christine) Lee
Christine is recognised for outstanding leadership in outreach, from coordinating major events and developing educational resources to representing OzGrav internationally.

Joint Runners-up:
Chris Flynn — for leadership of the ASTRAL program
Olivia Vidal Velazquez — for consistently exceeding expectations with creativity, professionalism, and enthusiasm

Highly Commended:
The Einstein First Team, OzGrav Outreach Ambassadors

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Special Recognition Awards

• Community Care & Support: Jackie Bondell
  For consistently supporting the wellbeing, comfort, and sense of belonging of OzGrav members.

• Positive Attitude: Saurav Mishra
  For fostering a welcoming and supportive environment through kindness and positivity.

• Workshop Organisation:
  10th Anniversary Workshop Team
  For the successful delivery of OzGrav’s milestone event.

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Rising Star Award

Winner: Teagan Clarke
Recognised for bold, original science, leadership in collaboration, and a deep commitment to positive research culture.

Runner-up: Paul Disberg
Commended for prolific publications across a wide range of astrophysical topics.

Highly Commended:
Emily Rose Rees, Neil Lu

Last week, the Australian gravitational-wave community gathered at Swinburne University to celebrate a landmark moment in science, the 10-year anniversary of the first direct detection of gravitational waves (GW150914). This discovery, announced in 2016 from data recorded on 14 September 2015, confirmed Einstein’s prediction and opened an entirely new window on the Universe.

The two-day workshop, hosted by the Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav), brought together more than 80 students, researchers, and leaders from across the country. The workshop was more than just a commemoration of GW150914, it was a chance to reflect on Australia’s pivotal role in that discovery, to celebrate the remarkable advances of the past decade, and to look forward to what the next decade of gravitational-wave science will bring.

OzGrav’s Director, Professor Matthew Bailes, reflected on the impact of that first signal: “When the first detection happened in 2015, it completely transformed the landscape. Suddenly, gravitational-wave astronomy was real, and Australia needed a Centre of Excellence dedicated to it and that’s how OzGrav was born in 2017.” He added, “Since then, we’ve captured neutron star mergers in both gravitational waves and light, pushed quantum noise limits, and pioneered squeezed-light technology.”

For many in the room, it was collaboration that defined the journey. As Distinguished Professor Susan Scott, from the Australian National University, reminded the audience, “The first detection was only possible through collaboration and that spirit continues to drive gravitational-wave science forward.”

The workshop program reflected that spirit, spanning technical advances, new discoveries, and emerging projects, while also acknowledging the teamwork and persistence that made it all possible.

The celebration was about the future as much as the past. Day two highlighted the next generation of detectors and discoveries with Professor Paul Lasky from Monash University summing up the mood with optimism, “The gravitational-wave future is loud, much louder than GW150914. Every increase in sensitivity lets us hear further into the universe.” He also issued a call to action: “If we want an observatory in Australia, we will need ambition and collaboration to make it happen.”

Over coffee breaks, panel discussions, and even a celebratory cake, there was a palpable sense of both gratitude and anticipation. The workshop marked not only ten years since a signal that changed the world but also the strength of a community that has grown around it, a community ready to take the next bold steps into the cosmos.

Thank you to the local organising committee:

• Jade Powell, Diana Haikal, Kirsten Banks, Jackie Bondell, Carl Knox (Swinburne University of Technology)

• Susan Scott (ANU)

• Christine Lee (University of Melbourne)