The WiggleZ Dark Energy Survey: Survey Design and First Data Release

Abstract

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 target galaxies are selected using ultraviolet photometry from the GALEX satellite, with a flux limit of NUV<22.8 mag. The redshift range containing 90% of the galaxies is 0.2<z<1.0. The primary aim of the survey is to precisely measure the scale of baryon acoustic oscillations (BAO) imprinted on the spatial distribution of these galaxies at look-back times of 4-8 Gyrs. Detailed forecasts indicate the survey will measure the BAO scale to better than 2% and the tangential and radial acoustic wave scales to approximately 3% and 5%, respectively. This paper provides a detailed description of the survey and its design, as well as the spectroscopic observations, data reduction, and redshift measurement techniques employed. It also presents an analysis of the properties of the target galaxies, including emission line diagnostics which show that they are mostly extreme starburst galaxies, and Hubble Space Telescope images, which show they contain a high fraction of interacting or distorted systems. In conjunction with this paper, we make a public data release of data for the first 100,000 galaxies measured for the project.

Accepted by MNRAS; this has some figures in low resolution format. Full resolution PDF version (7MB) available at http://www.physics.uq.edu.au/people/mjd/pub/wigglez1.pdf The WiggleZ home page is at http://wigglez.swin.edu.au/

References in corpus (11)

• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Dark Energy and the Accelerating Universe
• New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
• Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
• Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
• The 2dF-SDSS LRG and QSO (2SLAQ) Luminous Red Galaxy Survey
• The Vimos VLT Deep Survey: Global properties of 20000 galaxies in the I_AB<=22.5 WIDE survey
• Hot DB White Dwarfs from the Sloan Digital Sky Survey
• Multi-Object Spectroscopy Field Configuration by Simulated Annealing
• Spectroscopic follow-up of a cluster candidate at z = 1.45
• The WiggleZ Dark Energy Survey: small-scale clustering of Lyman Break Galaxies at z < 1

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• Cosmological surveys with multi-object spectrographs
• The effects of peculiar velocities on the morphological properties of large-scale structure
• The GALAH Survey: Relative throughputs of the 2dF fibre positioner and the HERMES spectrograph from stellar targets
• The SDSS Coadd: Cross-Correlation Weak Lensing and Tomography of Galaxy Clusters
• Giga-z: A 100,000 Object Superconducting Spectrophotometer for LSST Follow-up
• The WiggleZ Dark Energy Survey: Star-formation in UV-luminous galaxies from their luminosity functions
• Stacked reverberation lags at high redshift
• Weak Lensing Trispectrum and Kurt-Spectra
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• Impact of photometric redshifts on the galaxy power spectrum and BAO scale in the LSST survey
• Optimising Spectroscopic and Photometric Galaxy Surveys: Efficient Target Selection and Survey Strategy
• Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
• Improved Tomographic Binning of 3x2pt Lens Samples: Neural Network Classifiers and Optimal Bin Assignments
• Deficit of Luminous and Normal Red Galaxies in Cosmic Voids
• Enhancing Photometric Redshift Catalogs Through Color-Space Analysis: Application to KiDS-Bright Galaxies
• Reconstructing thawing quintessence with multiple datasets
• The H$\alpha$ and [O III] $\lambda 5007$ Luminosity Functions of $1.2<z<1.9$ Emission-Line Galaxies from HST Grism Spectroscopy
• The WiggleZ Dark Energy Survey: Galaxy Evolution at 0.25 < z < 0.75 Using The Second Red-Sequence Cluster Survey (RCS-2)
• Bayesian large-scale structure inference and cosmic web analysis
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Kinetic properties of fractal media
• Photometric IGM tomography with Subaru/HSC: the large-scale structure of Ly$\alpha$ emitters and IGM transmission in the COSMOS field at $z\sim 5$
• HI Intensity Mapping with the MIGHTEE Survey: First Results of the HI Power Spectrum
• Position-Dependent Correlation Function of Weak Lensing Convergence
• The Low Redshift survey at Calar Alto (LoRCA)
• The establishment of the Standard Cosmological Model through observations
• Dust Properties of Clumpy Disc Galaxies at z~1.3 with Herschel-SPIRE
• Spectroscopic observations of the machine-learning selected anomaly catalogue from the AllWISE Sky Survey
• Determining accurate measurements of the growth rate from the galaxy correlation function in simulations
• Averaged universe confronted with cosmological observations: A fully covariant approach
• A search for HI absorption in distant star-forming galaxies with ASKAP-FLASH -- I. Selection and analysis of the radio sample
• Luminosity function of luminous compact star-forming galaxies
• Simulations and Observations of the Microwave Universe
• Symmetries, Invariants and Generating Functions: Higher-order Statistics of Biased Tracers
• The h-index in Australian Astronomy
• Direct Determination of Expansion History Using Redshift Distortions
• UNITSIM-Galaxies: data release and clustering of emission-line galaxies
• The Jet Paths of Radio AGN and their Cluster Weather
• On the Origin of the Strong Optical Variability of Emission-line Galaxies
• Foreground removal and angular power spectrum estimation of 21 cm signal using harmonic space ILC method
• Selecting Clusters and Protoclusters via Stellar Mass Density: II. Application to HSC-SSP Observations
• Baryon Acoustic Oscillations from galaxy surveys
• HI Intensity Mapping cross-correlation with thermal SZ fluctuations: forecasted cosmological parameters estimation for FAST and Planck
• Panchromatic properties of galaxies in wide-field optical spectroscopic and photometric surveys
• Characterising Improvements in Photometric Redshift Probability Density Functions with Galaxy Morphology
• Long-wavelength gravitational waves and cosmic acceleration
• A New Estimator for Phase Statistics
• Obtaining non-linear galaxy bias constraints from galaxy-lensing phase differences
• Perspectives for studying the dark energy at z>2 with galaxy surveys
• Propagation of gravitational waves in a universe with slowly-changing equation of state
• Stable Clustering Ansatz, Consistency Relations and Gravity Dual of Large-Scale Structure
• Using a Neural Network Classifier to Select Galaxies with the Most Accurate Photometric Redshifts
• Investigation of homogeneity and matter distribution on large scales using large quasar groups
• UV bright red-sequence galaxies: a comparative study between UV upturn and UV weak systems
• Testing Large-Scale Structure Measurements Against Fisher Matrix Predictions
• An emulation-based model for the projected correlation function
• A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
• Highly Efficient Selection of High-Redshift Emission-Line Galaxies for future DESI-like surveys with Deep Multi-band Imaging
• Catalogs of optically-selected clusters and photometric luminous red galaxies from the Hyper Suprime-Cam Subaru Strategic Program final year dataset