EMU: Evolutionary Map of the Universe

Abstract

EMU is a wide-field radio continuum survey planned for the new Australian Square Kilometre Array Pathfinder (ASKAP) telescope. The primary goal of EMU is to make a deep (rms ~ 10 microJy/beam) radio continuum survey of the entire Southern Sky at 1.3 GHz, extending as far North as +30 degrees declination, with a resolution of 10 arcsec. EMU is expected to detect and catalogue about 70 million galaxies, including typical star-forming galaxies up to z~1, powerful starbursts to even greater redshifts, and AGNs to the edge of the visible Universe. It will undoubtedly discover new classes of object. This paper defines the science goals and parameters of the survey, and describes the development of techniques necessary to maximise the science return from EMU.

Accepted by PASA; see http://www.atnf.csiro.au/people/rnorris/papers/n252.pdf for higher-resolution figures

References in corpus (60)

• The Cosmic Evolution Survey (COSMOS) -- Overview
• Heating Hot Atmospheres with Active Galactic Nuclei
• The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
• The GALEX Ultraviolet Atlas of Nearby Galaxies
• Turbulence and Magnetic Fields in the Large Scale Structure of the Universe
• The VLA Galactic Plane Survey
• Hot and cold gas accretion and feedback in radio-loud active galaxies
• Particle Acceleration on Megaparsec Scales in a Merging Galaxy Cluster
• Photometric redshift and classification for the XMM-COSMOS sources
• Radio sources in the 6dFGS: Local luminosity functions at 1.4 GHz for star-forming galaxies and radio-loud AGN
• Multiwavelength study of massive galaxies at z~2. II. Widespread Compton thick AGN and the concurrent growth of black holes and bulges
• On the connection between giant radio halos and cluster mergers
• The VLA-COSMOS Survey: II. Source Catalog of the Large Project
• AGN-controlled cooling in elliptical galaxies
• An Imprint of Super-Structures on the Microwave Background due to the Integrated Sachs-Wolfe Effect
• Compressed sensing imaging techniques for radio interferometry
• Science With The Australian Square Kilometre Array Pathfinder
• Confirmation of the Electron Cyclotron Maser Instability as the Dominant Source of Radio Emission from Very Low Mass Stars and Brown Dwarfs
• The Molonglo Galactic Plane Survey (MGPS-2): Compact Source Catalogue
• Signals from the Noise: Image Stacking for Quasars in the FIRST Survey
• Integrated Sachs-Wolfe effect from the cross correlation of WMAP3 year and the NRAO VLA sky survey data: New results and constraints on dark energy
• Radio imaging of the Subaru/XMM-Newton Deep Field - I. The 100-microJy catalogue, optical identifications, and the nature of the faint radio source population
• The X-ray nuclei of intermediate-redshift radio sources
• Deep ATLAS radio observations of the CDFS-SWIRE field
• Photometric redshifts in the SWIRE Survey
• The Star Formation History of the Universe as Revealed by Deep Radio Observations
• The First Appearance of the Red Sequence of Galaxies in Proto-Clusters at 2<~z<~3
• The dependence of Star Formation on Galaxy Stellar Mass
• The star-formation history of K-selected galaxies
• Cosmological Shocks in Adaptive Mesh Refinement Simulations and the Acceleration of Cosmic Rays
• Spitzer Reveals Hidden Quasar Nuclei in Some Powerful FR II Radio Galaxies
• The Spiderweb galaxy: a forming massive cluster galaxy at z~2
• A new method to separate star forming from AGN galaxies at intermediate redshift: The submillijansky radio population in the VLA-COSMOS survey
• The Deep SWIRE Field I. 20cm Continuum Radio Observations: A Crowded Sky
• Simulating cosmic rays in clusters of galaxies - I. Effects on the Sunyaev-Zel'dovich effect and the X-ray emission
• The VLA 1.4GHz Survey of the Extended Chandra Deep Field South: First Data Release
• The Southern Galactic Plane Survey: Polarized Radio Continuum Observations and Analysis
• Probing radio source environments via HI and OH absorption
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• A reassessment of the evidence of the Integrated Sachs-Wolfe effect through the WMAP-NVSS correlation
• First Detection of Cosmic Structure in the 21-cm Intensity Field
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• The Chandra, HST, and VLA View of the Circumnuclear Extended Emission in the Narrow Emission Line Galaxy NGC 2110
• VLBI detection of an Infrared-Faint Radio Source
• Deep 610-MHz Giant Metrewave Radio Telescope observations of the Spitzer extragalactic First Look Survey field - III. The radio properties of Infrared-Faint Radio Sources
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• Diffuse cluster-like radio emission in poor environments
• CMB-Galaxy correlation in Unified Dark Matter Scalar Field Cosmologies
• The Coherent Radio Emission from the RS CVn Binary HR 1099

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