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The origin of the "wiggles" in the distribution of galaxiesTime goes from top to bottom. The "bullseyes" show where there have been two sources of pressure waves in the early universe, the waves travelling outwards like the ripples on a pond. Galaxies prefer to grow at the centre and edge of the bullseye. Their preferred separation is the radius of the bullseye (the scale bar). Image: Sam Moorefield, Swinburne University. Larger image6.1MB jpeg; 21cm wide at 300dpi |
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The 3.9-m Anglo-Australian TelescopePhoto: Fred Kamphues Larger image1.8MB jpeg; 36cm wide at 300dpi
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The 3.9-m Anglo-Australian TelescopePhoto: Fred Kamphues Larger image2.6MB jpeg; 24cm wide at 300dpi |
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The 3.9-m Anglo-Australian TelescopePhoto: Fred Kamphues Larger image2.1MB jpeg; 36cm wide at 300dpi |
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The dome of the Anglo-Australian Telescope at Siding Spring Observatory, NSW, AustraliaPhoto: Fred Kamphues Larger image1.7MB jpeg; 36cm wide at 300dpi |
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The dome of the Anglo-Australian Telescope at Siding Spring Observatory, NSW, AustraliaPhoto: Fred Kamphues Larger image1.9MB jpeg; 36cm wide at 300dpi |
Researcher contact
Dr Sarah Brough, Anglo-Australian Observatory
Office: 02 9372 4854
Mob: 0449-505-219
sb@aao.gov.au
Publication
Michael J. Drinkwater et al. “The WiggleZ Dark Energy Survey: Survey Design and First Data Release.” Accepted for publication in the Monthly Notices of the Royal Astronomical Society. On astro-ph at http://xxx.lanl.gov/abs/0911.4246.





