The WiggleZ Dark Energy Survey - Berkeley Cosmology Group

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Page 1 and 2: The WiggleZ Dark Energy Survey •
Page 3 and 4: The WiggleZ Survey (observational)
Page 5 and 6: Survey comparison
Page 7 and 8: Survey design • Follow up UV-sele
Page 9 and 10: Survey design
Page 11 and 12: Target Galaxy selection targets (Cr
Page 13 and 14: The baryon acoustic peak in WiggleZ
Page 15 and 16: BAO Hubble diagram arXiv:1108.2635
Page 17 and 18: The Comparison dark energy of BAO p
Page 19 and 20: Cosmological parameter fits arXiv:1
Page 21 and 22: Cosmological parameter fits Spatial
Page 23 and 24: Redshift-space distortions 4 • Do
Page 25 and 26: Redshift-space distortions in Wiggl
Page 27: Growth rate measurements from Wiggl
Page 31 and 32: Alcock-Paczynski measurement in Wig
Page 33 and 34: Alcock-Paczynski measurement in Wig
Page 35 and 36: Non-parametric expansion history ar
Page 37 and 38: Non-parametric expansion history ar
Page 39 and 40: Transition to cosmic homogeneity Sc
Page 41: Summary of results from WiggleZ •

The WiggleZ Dark Energy Survey - Berkeley Cosmology Group

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