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The WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies
Signe Riemer-Sørensen, Chris Blake, David Parkinson +25
The absolute neutrino mass scale is currently unknown, but can be constrained from cosmology. The WiggleZ high redshift star-forming blue galaxy sample is less sensitive to systema…
The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae
Chris Blake, Karl Glazebrook, Tamara Davis +22
Astronomical observations suggest that today's Universe is dominated by a dark energy of unknown physical origin. One of the most notable consequences in many models is that dark e…
The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations
Chris Blake, Eyal Kazin, Florian Beutler +26
We present measurements of the baryon acoustic peak at redshifts z = 0.44, 0.6 and 0.73 in the galaxy correlation function of the final dataset of the WiggleZ Dark Energy Survey. W…
The WiggleZ Dark Energy Survey: High Resolution Kinematics of Luminous Star-Forming Galaxies
Emily Wisnioski, Karl Glazebrook, Chris Blake +24
We report evidence of ordered orbital motion in luminous star-forming galaxies at z~1.3. We present integral field spectroscopy (IFS) observations, performed with the OH Suppressin…
The WiggleZ Dark Energy Survey: testing the cosmological model with baryon acoustic oscillations at z=0.6
Chris Blake, Tamara Davis, Gregory Poole +23
We measure the imprint of baryon acoustic oscillations (BAOs) in the galaxy clustering pattern at the highest redshift achieved to date, z=0.6, using the distribution of N=132,509…
The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9
Chris Blake, Sarah Brough, Matthew Colless +22
We present precise measurements of the growth rate of cosmic structure for the redshift range 0.1 < z < 0.9, using redshift-space distortions in the galaxy power spectrum of the Wi…