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The WiggleZ Dark Energy Survey - Berkeley Cosmology Group

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<strong>Survey</strong> design<br />

• Follow up UV-selected sources<br />

from GALEX imaging<br />

• Colour cuts select highredshift<br />

galaxies<br />

• Star-forming galaxies : redshifts<br />

from emission lines, SFR<br />

10-100 solar masses per year<br />

•<br />

Short 1-hr exposures -<br />

maximize numbers with 70%<br />

redshift completeness

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