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 WiggleZ Dark Energy Survey. Our results, which have a precision of around 1
Higher order statistics are a useful and complementary tool for measuring the clustering of galaxies...
We measure the imprint of baryon acoustic oscillations (BAOs) in the galaxy clustering pattern at th...
We present measurements of the baryon acoustic peak at redshifts z= 0.44, 0.6 and 0.73 in the galaxy...
We present precise measurements of the growth rate of cosmic structure for the redshift range 0.1 < ...
We present precise measurements of the growth rate of cosmic structure for the redshift range 0.1 < ...
We present cosmological results from the nearly-completed WiggleZ Dark Energy Survey at the AAT. We ...
The growth history of large-scale structure in the Universe is a powerful probe of the cosmological ...
We report one of the most accurate measurements of the three-dimensional large-scale galaxy power sp...
The WiggleZ Dark Energy Survey on the Anglo-Australian Telescope has measured redshifts for 220,000 ...
We report one of the most accurate measurements of the three-dimensional large-scale galaxy power sp...
Measurements of the growth rate of structure f at different redshifts can discriminate the origin of...
Astronomical observations suggest that today's Universe is dominated by a dark energy of unknown phy...
Astronomical observations suggest that today’s Universe is dominated by a dark energy of unknown phy...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift ultraviole...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift ultraviole...
Higher order statistics are a useful and complementary tool for measuring the clustering of galaxies...
We measure the imprint of baryon acoustic oscillations (BAOs) in the galaxy clustering pattern at th...
We present measurements of the baryon acoustic peak at redshifts z= 0.44, 0.6 and 0.73 in the galaxy...
We present precise measurements of the growth rate of cosmic structure for the redshift range 0.1 < ...
We present precise measurements of the growth rate of cosmic structure for the redshift range 0.1 < ...
We present cosmological results from the nearly-completed WiggleZ Dark Energy Survey at the AAT. We ...
The growth history of large-scale structure in the Universe is a powerful probe of the cosmological ...
We report one of the most accurate measurements of the three-dimensional large-scale galaxy power sp...
The WiggleZ Dark Energy Survey on the Anglo-Australian Telescope has measured redshifts for 220,000 ...
We report one of the most accurate measurements of the three-dimensional large-scale galaxy power sp...
Measurements of the growth rate of structure f at different redshifts can discriminate the origin of...
Astronomical observations suggest that today's Universe is dominated by a dark energy of unknown phy...
Astronomical observations suggest that today’s Universe is dominated by a dark energy of unknown phy...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift ultraviole...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift ultraviole...
Higher order statistics are a useful and complementary tool for measuring the clustering of galaxies...
We measure the imprint of baryon acoustic oscillations (BAOs) in the galaxy clustering pattern at th...
We present measurements of the baryon acoustic peak at redshifts z= 0.44, 0.6 and 0.73 in the galaxy...