Welcome to SKA

 
Slideshow

Australia and New Zealand SKA project

The Square Kilometre Array, or SKA, is a global next-generation radio telescope project involving institutions from over 20 countries. The SKA will be the largest and most capable radio telescope ever constructed. During its 50+ year lifetime, it will expand our understanding of the universe and drive technological development worldwide. Australia and southern Africa will each host different SKA components.



July 2016


The SKA has been called the ultimate Big Data project – its antennas producing a data stream several times greater than today’s entire global internet traffic. So how do you get that volume of information all the way from Australia’s remote SKA site to the supercomputers needed to process it? More..

 

Website Survey 

 

How can we make it easier for you to use our website? Take part in a 5 minute survey and let us know what you think.

 

Follow the Australian SKA Office on Twitter

 
 

The Australian Square Kilometre Array Twitter page aims to provide you with the latest updates, multimedia and communications about the SKA project and its Australian stakeholders, and the opportunity to connect international partners, astronomers, researchers, industry members and the general public in an online conversation about this transformational project.

 

 

 
 
 
 

MWA Completes Technicolour Radio Survey of the Sky

 

The Murchison Widefield Array (MWA) has produced one of the largest radio surveys of the sky ever.

The GaLactic and Extragalactic All-sky MWA, or ‘GLEAM’ survey is a large-scale, high resolution survey of the sky that will be used to explore remnants of explosions from ancient stars, the beginning and end of supermassive black holes, and what happens when clusters of galaxies collide. While previous radio surveys have been performed in a narrow frequency band, GLEAM has observed the sky across a much wider band. By viewing such an exceptionally broad spectrum of ‘radio colours’, astronomers will be able to discern and explore new features of the sky.

As well as being an extremely valuable resource for scientists, completion of the GLEAM survey is a big step towards SKA-Low. Lessons learned from the survey will help fine-tune the development of SKA-Low which will be capable of making even deeper observations into the universe. You can read more about the survey here.

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A ‘radio colour’ view of the sky above a ‘tile’ of the MWA. Credit: Radio image by Natasha Hurley-Walker (ICRAR/Curtin) and the GLEAM Team. MWA tile and landscape by Dr John Goldsmith / Celestial Visions.

 
 

News and Updates


Featured News

 

The First Pietro Baracchi Conference: Italo-Australian Radio Astronomy in the Era of the SKA

 

The First Pietro Baracchi Conference, entitled ‘Italo-Australian Radio Astronomy in the Era of the SKA’ will be held in Perth on 1-4 November 2016. The conference will bring together Italian and Australian researchers from all areas of radio astronomy to boost research collaboration between the countries.

The conference is the first in a series of meetings planned to alternate between Australia and Italy. These meetings illustrate the strong relationship between the Australian and Italian scientific communities, and our collaborative efforts on the SKA. Read more about the conference here.


Pietro Baracchi

 

March 2017 SKA-Low Meeting

 

The ‘Realising SKA-­Low: new technologies & techniques for imaging and calibration of low frequency arrays’ conference will be held in Perth in March 2017.

A large body of knowledge has been accumulated in the field of low frequency radio astronomy in recent years. The conference is to share this information and assess how lessons learned from the SKA pathfinders and precursors and other low frequency arrays can benefit the final design stages of SKA-Low.

You can read more about the event at the conference website.


 

 

 

 

 

 

 

 

 

 


 

 

 

 


 

 


 



 
  

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