A new home-grown instrument based on bundles of optical fibres is giving Australian astronomers the first ‘Google street view’ of the cosmos—incredibly detailed views of huge numbers of galaxies.
Developed by researchers at the University of Sydney and the Australian Astronomical Observatory, the optical-fibre bundles can sample the light from up to 60 parts of a galaxy, for a dozen galaxies at a time.
By analysing the light’s spectrum astronomers can learn how gas and stars move within each galaxy, where the young stars are forming and where the old stars live. This will allow them to better understand how galaxies change over time and what drives that change.
“It’s a giant step,” said Dr James Allen of the ARC Centre of Excellence for All-sky Astrophysics (CAASTRO), which funded many of the researchers involved.
“Before, we could study one galaxy at a time in detail, or lots of galaxies at once but in much less detail. Now we have both the numbers and the detail.” The Australian team is now a year or two ahead of its international competition in this field. In just 64 nights it has gathered data on 1000 galaxies, twice as many as the previous largest project, and over the next two years it will study another 2000. CAASTRO funding was crucial in helping the team gain its lead. “They had a great idea but it was going to take time to pull the resources together,” said CAASTRO Director Professor Bryan Gaensler. “CAASTRO was able to get it happening fast.”
Called SAMI (the Sydney-AAO Multi-Object Integral field spectrograph), the optical-fibre instrument was installed on the 4-m Anglo-Australian Telescope at Siding Spring Observatory in northwest NSW last year.
The technological leap in SAMI is the ‘hexabundle’, sixty or more optical fibres close-packed and fused together, developed by the University of Sydney’s astrophotonics group led by Professor Joss Bland-Hawthorn.
Using SAMI, astronomers from the Australian National University and the University of Sydney have already spotted ‘galactic winds’—streams of matter travelling at many hundreds of kilometres a second—flowing from the centre of two galaxies (ESO 185-G031 and SDSS J090005.05+000446.7).
“We’ve seen galactic winds in other galaxies, but we have no idea how common they really are, because we’ve never had the means to look for them systematically. But with SAMI we now do,” said the University of Sydney’s Associate Professor Scott Croom, a Chief Investigator with CAASTRO who leads the SAMI team.
Another study with SAMI is uncovering the formation history of galaxies by looking to see if they are rotating in a regular way or if the movement of their stars is random and disordered.
“There are hints that galaxies with random motions sit at the centres of groups of galaxies, where many smaller galaxies may have fallen into them,” said Dr Lisa Fogarty, a CAASTRO researcher at the University of Sydney, who led this work.
On Thursday 24 July the SAMI team will release the first set of data from the instrument to the worldwide astronomical community. On the same day Dr Allen will give a presentation about SAMI at the annual scientific meeting of the Astronomical Society of Australia, being held at Macquarie University in Sydney during 20-25 July.
CAASTRO is a collaboration between Curtin University, The University of Western Australia, the University of Sydney, the Australian National University, the University of Melbourne, Swinburne University of Technology and the University of Queensland. It is funded under the Australian Research Council Centre of Excellence program and receives additional funding from the seven participating universities and the NSW State Government Science Leveraging Fund.