The WiggleZ Dark Energy Survey - Berkeley Cosmology Group

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Neutrino mass limit from WiggleZ P(k) Riemer-Sorensen et al. arXiv:1112.4940 Combined WiggleZ power spectrum dataset compared to various models : Probability histogram for the k 1.6 k Pconv(k) 1.6 Pconv(k) Relative probability 140 120 100 80 60 40 0.25 0.20 0.15 0.05 0.1 0.2 0.3 0.4 0.5 k [h Mpc −1 0.1 0.2 0.3 0.4 0.5 k [h Mpc ] −1 ] WiggleZ+WMAP+H0+SDSS-BAO: 0.29 eV (95% limit) sum of neutrino masses : 0.10 WiggleZ + WMAP7 : 0.60 eV (95% limit) 0.00 0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 !m " [eV]
Transition to cosmic homogeneity Scrimgeour et al. (submitted) Measurement of the correlation dimension N(
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 and 28: Growth rate measurements from Wiggl
Page 29 and 30: Density and velocity power spectra
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: Non-parametric expansion history ar
Page 41: Summary of results from WiggleZ •

The WiggleZ Dark Energy Survey - Berkeley Cosmology Group

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