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The 6dF Galaxy Survey: baryon acoustic oscillations and the local Hubble constant
- F. Beutler, C. Blake, F. Watson
- Physics
- 16 June 2011
We analyse the large-scale correlation function of the 6dF Galaxy Survey (6dFGS) and detect a baryon acoustic oscillation (BAO) signal at 105h −1 Mpc. The 6dFGS BAO detection allows us to constrain…
KiDS-450: cosmological parameter constraints from tomographic weak gravitational lensing
- H. Hildebrandt, M. Viola, L. Waerbeke
- Physics
- 16 June 2016
We present cosmological parameter constraints from a tomographic weak gravitational lensing analysis of ~450deg$^2$ of imaging data from the Kilo Degree Survey (KiDS). For a flat $\Lambda$CDM…
The WiggleZ Dark Energy Survey: joint measurements of the expansion and growth history at z < 1
We perform a joint determination of the distance–redshift relation and cosmic expansion rate at redshifts z = 0.44, 0.6 and 0.73 by combining measurements of the baryon acoustic peak and…
The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations
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. We combine our…
The WiggleZ Dark Energy Survey: survey design and first data release
- M. Drinkwater, R. Jurek, H. Yee
- Physics
- 22 November 2009
The WiggleZ Dark Energy Survey is a survey of 240 000 emission-line galaxies in the distant Universe, measured with the AAOmega spectrograph on the 3.9-m Anglo-Australian Telescope (AAT). The primary…
The DESI Experiment Part I: Science,Targeting, and Survey Design
- Desi Collaboration Amir Aghamousa, J. Aguilar, Y. Zu
- Physics
- 31 October 2016
DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through redshift-space…
The WiggleZ Dark Energy Survey: testing the cosmological model with baryon acoustic oscillations at z= 0.6
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 emission-line…
Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlation
- K. Masui, E. Switzer, T. Voytek
- Physics
- 1 August 2012
In this Letter, 21 cm intensity maps acquired at the Green Bank Telescope are cross-correlated with large-scale structure traced by galaxies in the WiggleZ Dark Energy Survey. The data span the…
The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9
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…
CFHTLenS: the Canada–France–Hawaii Telescope Lensing Survey – imaging data and catalogue products
- T. Erben, H. Hildebrandt, M. Velander
- Physics
- 30 October 2012
We present data products from the Canada–France–Hawaii Telescope Lensing Survey (CFHTLenS). CFHTLenS is based on the Wide component of the Canada–France–Hawaii Telescope Legacy Survey (CFHTLS). It…
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