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Article << Previous     |     Next >>   Contents Vol 28(3)

EMU: Evolutionary Map of the Universe

Ray P. Norris A AM, A. M. Hopkins B AJ, J. Afonso C, S. Brown A, J. J. Condon D, L. Dunne E, I. Feain A, R. Hollow A, M. Jarvis F AL, M. Johnston-Hollitt G, E. Lenc A, E. Middelberg H, P. Padovani I, I. Prandoni J, L. Rudnick K, N. Seymour L, G. Umana M, H. Andernach N, D. M. Alexander U, P. N. Appleton O, D. Bacon P, J. Banfield A, W. Becker Q, M. J. I. Brown R, P. Ciliegi S, C. Jackson A, S. Eales T, A. C. Edge U, B. M. Gaensler V AJ, G. Giovannini J, C. A. Hales A V, P. Hancock V AJ, M. T. Huynh W, E. Ibar X, R. J. Ivison X Y, R. Kennicutt Z, Amy E. Kimball D, A. M. Koekemoer AA, B. S. Koribalski A, Á. R. López-Sánchez B AK, M. Y. Mao A B AB, T. Murphy V AJ, H. Messias C, K. A. Pimbblet R, A. Raccanelli P, K. E. Randall A V, T. H. Reiprich AE, I. G. Roseboom AE, H. Röttgering AG, D. J. Saikia AH, R. G. Sharp AG, O. B. Slee A, Ian Smail U, M. A. Thompson F, J. S. Urquhart A, J. V. Wall AI and G.-B. Zhao P

A CSIRO Astronomy & Space Science, Epping, NSW 1710, Australia
B Australian Astronomical Observatory, Epping, NSW 1710, Australia
C Centro de Astronomia e Astrofísica da Universidade de Lisboa, Observatório Astronómico de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal
D National Radio Astronomy Observatory, Charlottesville, VA 22903, USA
E School of Physics & Astronomy, University of Nottingham, Nottingham, NG7 2RD, UK
F Centre for Astrophysics Research, University of Hertfordshire, Hatfield, Hertfordshire, AL10 9AB, UK
G School of Chemical & Physical Sciences, Victoria University of Wellington, Wellington 6140, New Zealand
H Astronomisches Institut, Ruhr-Universität Bochum, 44801 Bochum, Germany
I European Southern Observatory, D-85748 Garching bei München, Germany
J INAF-IRA, 40129 Bologna, Italy
K Department of Astronomy, University of Minnesota, Minneapolis, MN 55455, USA
L University College London, Mullard Space Science Laboratory, Dorking, Surrey, RH5 6NT, UK
M INAF-Catania Astrophysical Observatory, 95123 Catania, Italy
N Depto. de Astronomía, Universidad de Guanajuato, Guanajuato, C.P. 36000, GTO, Mexico
O NASA Herschel Science Center, Caltech, Pasadena, CA 91125, USA
P Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth, PO1 3FX, UK
Q Max-Planck Institut für extraterr. Physik, 85741 Garching, Germany
R School of Physics, Monash University, Clayton, VIC 3800, Australia
S INAF – OABO, 40127 Bologna, Italy
T School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, UK
U Department of Physics, Durham University, Durham, DH1 3LE, UK
V Sydney Institute for Astronomy, School of Physics, The University of Sydney, NSW 2006, Australia
W International Centre for Radio Astronomy Research, University of WA, Crawley, WA 6009, Australia
X UK Astronomy Technology Centre, Royal Observatory, Edinburgh EH9 3HJ, UK
Y Institute for Astronomy, University of Edinburgh, Edinburgh, EH9 3HJ, UK
Z Institute of Astronomy, University of Cambridge, Cambridge, CB3 0HA, UK
AA Space Telescope Science Institute, Baltimore MD 21218, USA
AB School of Mathematics & Physics, University of Tasmania, Hobart, TAS 7001, Australia
AD Argelander Institute for Astronomy, Bonn University, 53121 Bonn, Germany
AE Dept of Physics and Astronomy, University of Sussex, Falmer, East Sussex, BN1 9RH, UK
AF Leiden Observatory, Leiden University, 2300 RA Leiden, The Netherlands
AG National Centre for Radio Astrophysics, TIFR, Pune 411 007, India
AH Mount Stromlo Observatory, Canberra, ACT 2611, Australia
AI Dept. of Physics and Astronomy, University of British Columbia, Vancouver, B.C. V6T 1Z1, Canada
AJ ARC Centre of Excellence for All-sky Astrophysics, University of Sydney, Sydney, NSW 2006, Australia
AK Department of Physics and Astronomy, Macquarie University, North Ryde, NSW 2109, Australia
AL Physics Department, University of the Western Cape, Cape Town 7535, South Africa
AM Corresponding author. Email: ray.norris@csiro.au

Publications of the Astronomical Society of Australia 28(3) 215-248 http://dx.doi.org/10.1071/AS11021
Submitted: 19 May 11  Accepted: 15 June 11   Published: 30 August 2011


 
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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 μJy/beam) radio continuum survey of the entire Southern sky at 1.3 GHz, extending as far North as +30° 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 active galactic nuclei 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.

Keywords: telescopes — surveys — stars: activity — galaxies: evolution — galaxies: formation — cosmology: observations — radio continuum: general


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