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June 2025

Director's note

Douglas Bock is wearing a smart blue-green shirt and smiling at the camera.
Douglas Bock, Director of the Australia Telescope National Facility (ATNF).

Welcome to the ATNF News. This edition aligns with a reminder that proposals for the coming semester (OCT25) are due Tuesday, 17 June (next week). As we have a dual-anonymisation process, please ensure you’ve taken all steps to keep your proposal anonymous. Tips are below.

It’s an exciting time for our facility. We have the CryoPAF available for shared-risk time on Murriyang, our Parkes radio telescope, as well as a second semester of CRACO. Meanwhile, the ongoing works for BIGCAT on the Australia Telescope Compact Array add to the promise of great science to come.

Much of this was covered in April’s Australia Telescope User Committee (ATUC) meeting, which includes an open session for the community. We also had an ATCA science day prior to the ATUC meeting, which was a chance for the astronomy community to consider opportunities for the telescope into the coming future, as infrastructure priorities change with the incoming SKA telescopes.  You can find more information on this and the ATUC meeting on the website.

More recently, we held the first Bolton Symposium in five years. The Symposium provides a platform for the ATNF’s early-career research staff to showcase their research, develop collaborations, and engage in career development activities. The intention is for this to become a regular occurrence.

Upcoming is the ASA Annual Scientific Meeting. As part of this, on Wednesday, 9 July, ATNF will host a Town Hall to provide updates and an open forum for discussion.

Lastly, I’d like to welcome the new members of our Australia Telescope Steering Committee, including new Chair, Professor Lister Staveley-Smith. I’d like to thank the outgoing members and outgoing Chair, Professor Tara Murphy, for their exceptional work and support of the ATNF. Read more on our website.

Many thanks for being a part of our community.

Douglas Bock, ATNF Director

Image: Ziteng Wang, ICRAR

LPT discovered with matching X-ray signal

Discovered in ASKAP and Chandra data, a long period transient has been discovered to also emit matching x-ray pulses for the first time. The research, published in Nature, concedes that there is no clear explanation for such long, regular intervals though theories include a magnetar or binary star system.

Read more

Updates and upgrades

A crane and a cherry picker gentle manoeuvre a large gear box from under a dish telescope
Removing the gears on Murriyang, our Parkes radio telescope

Murriyang gears up for another decade

Every twenty years or so, Murriyang, our Parkes radio telescope undergoes maintenance on its ball bearings and six-tonne gear boxes. This month, the gears were removed to be cleaned and machined ready for the next two decades.

The 1000-tonne dish structure sits on the tower’s azimuth track, from where it can be driven around. Then separate gears and motors drive the dish in zenith from its natural resting point (stowed). Because the dish’s counterweight is heavier than the dish itself, the stowed position is when the dish is pointing straight up. 

Inbuilt hydraulics systems lift the dish millimetres off the track, enabling our site management team to remove the gears.

This is being done within our five-week scheduled shutdown, of which we are currently into the second week. The gearbox work will take up about four weeks, including testing and commissioning, to make sure Murriyang continues to move smoothly.

BIGCAT commissioning underway

Commissioning of the BIGCAT upgrade for ATCA is progressing well, with system testing currently underway. While early results are promising, further validation of different observing modes is still ongoing, and BIGCAT is not yet ready for general use. Once we have verified different observing modes, BIGCAT will be made available in shared-risk mode, and the observing schedule for the current semester will be released.

Users who submitted proposals at the last proposal deadline and are awaiting the current schedule may request pre-graded status for the next semester (2025OCTS). This means that the grade awarded last semester will be carried over for 2025OCTS, for up to the same time request. To request this, email the ATNF Time Assignment Committee Executive Officer, Elizabeth Mahony. A cover sheet and observation table (with the same proposal code) must still be submitted in OPAL, but no science justification is required. Please see the call for proposals for further details.

The BIGCAT RF upgrade, expanding the bandwidth to 8 GHz, is scheduled for later this year.

Image: Z. Li et al.

Redefining our galaxy's structure

Recent research led by our post-doc, Jayender Kumar has changed our understanding of the Milky Way's inner structure. This part of the galaxy is notoriously hard to study, but these new insights are redefining the shape of our home galaxy. Rather than spiral arms radiating from the centre, there is instead an elliptical orbit of stars and gas about the Milky Way Bar.

Read more

People and culture

Man sits at a computer with a mess of buttons and cables behind him.
Lawrence Toomey in the observing room of Murriyang, our Parkes radio telescope.

Meet Lawrence Toomey

So much of the work we do at the ATNF involves managing data and making it accessible for researchers around the world. From fast radio bursts to odd radio circles, a lot of great discoveries would not be possible without these pipelines, catalogues and archives. One of the people working behind the scenes on these is Lawrence Toomey, our senior research technician.

A furniture maker and joiner for 20 years, Lawrence undertook a dramatic career change into astronomy where he now focuses on the pipelines that archive data from Murriyang, our Parkes radio telescope and manages the ATNF pulsar catalogue, PSRCAT.

"I love supporting astronomers to do cutting edge science with our instruments, something I've done across my 12 years at CSIRO."

Last year had a particular highlight, with the publication of Lawrence’s first paper. The paper outlines SDHDF, a file format he led the development on, which solves the problem of storing massive datasets from telescope receivers with multiple beams, such as our CryoPAF receiver. 

Tips on ensuring your proposal is anonymous 

A dual-anonymous peer review (DAPR) process has become standard for many observatories and research facilities around the world, including the ATNF. The process aims to reduce instances of unconscious bias affecting the acceptance outcomes. This means that proposals should not identify any team member. The names and affiliations are also removed from the cover sheets when reviewed by the Time Assignment Committee (TAC).

Since this has been in place for several semesters, the TAC now has the ability to penalise proposals that identify authors in two ways:

  • through outright rejection of the proposal (for blatant breaches of anonymity),
  • or by a reduction of the final grade. 

Here are some examples of what would be penalised: 

  • Self-citations or inclusions that could lead the TAC to identify the proposal authors. 
    e.g. “In [NAME] (2018), we showed x,y,z”,
    “In our previous observations (C1234, PI: Smith)”
  • Listing initials when detailing team contributions.
  • Listing PI or author names/collaborators within the proposal document.
  • Repeated breaches of the DAPR policy.

To ensure you don’t get caught out, here are some ways to provide this information in line with ATNF’s anonymity guidelines: 

  • Avoid use of “we”, “I”, “our”
  • “Data from C1234 shows that…”
  • “It has been shown in [1] that x=y”
  • To support these observations, we have compiled a team of XX people. In our team there are 3 members who are experienced observers and 5 who have contributed to our data reduction pipeline and are expert [telescope] users. The remaining YY members will contribute to the scientific analysis.

More examples and guidance can be found on other observatory websites, such as for the Hubble Space Telescope, and European Space Observatory

If you have any further questions about the DAPR process, contact George Hobbs or TAC Executive Officer, Elizabeth Mahony.

Five large radio telescope dishes face into a starry sky where a fuzzy cloud of a nearby galaxy is visible.
The Australia Telescope Compact Array and the Large Magellanic Cloud

National and international engagement

We are involved or participate in regular meetings around the world as part of the international astronomy community to share our great science and gather information on how we can be a valuable radio astronomy facility.    

Recent meetings we were involved in:

  • SKAO PI26 (March)
  • EuCAP (March)
  • ICTS (April)
  • IAUS 397 (June)

Upcoming key meetings:

  • SKAO general scientific meeting (June)
  • ASA Annual  Scientific Meeting (July)
  • The Dynamic Radio Sky 2025 (July)
  • URSI AP-RASC (August)
  • MWA Project Meeting and Phase 3 Launch (August)
  • Pulsar Conference 2025 (September)
  • IAC 2025 (September)

ATNF flashback

Wavelengths ahead: Ruby Payne-Scott

One of the first radio astronomers, Ruby Payne-Scott, was recognised last week with a Sydney ferry named in her honour. Ruby was part of the team who made the first interferometry measurements of a Sunspot and had a lasting impact on CSIRO beyond research. Image of CSIRO staff with Ruby's daughter at the ferry launch: Ron Ekers, Fiona Hall (Ruby's daughter), Vanessa Moss, Elizabeth Mahony and Douglas Bock.

Acknowledgement

We acknowledge the Traditional Owners of the lands of all our sites and pay respect to their Elders past and present.

  • The Radiophysics Lab, Marsfield, Wallumattagal
  • Paul Wild Observatory, Narrabri, Gomeroi People
  • Parkes Observatory, Parkes, Wiradjuri People
  • Mopra Observatory, Coonabarabran, Gamilaroi People
  • ARRC, Kensington, Whadjuk People of the Noongar Nation
  • Murchison Support Facility, Geraldton, Nhanhangardi, Naaguja, Wilunyu and Amangu Peoples
  • Inyarrimanha Ilgari Bundara, our Murchison Radio-astronomy Observatory, Wajarri Yamaji