EMU: Evolutionary Map of the Universe

Raymond Norris, Andrew Hopkins, J Afonso, S Brown, J Condon, L Dunne, I Feain, R Hollow, M Jarvis, Melanie Johnston-Hollitt, E Lenc, E Middelberg, P Padovani, I Prandoni, L Rudnick, N Seymour, G Umana, H Andernach, D Alexander, P AppletonD Bacon, J Banfield, W Becker, Michael Brown, P Ciliegi, C Jackson, S Eales, Alastair Edge, Bryan Gaensler, G Giovannini, Christopher Hales, Paul Hancock, M Huynh, E Ibar, R Ivison, R Kennicutt, Amy Kimball, A Koekemoer, B Koribalski, Angel Lopez-Sanchez, M Mao, Tara Murphy, H Messias, Kevin Pimbblet, A Raccanelli, Karen Randall, T Reiprich, Isaac Roseboom, H Rottgering, D Saikia, Robert Sharp, O Slee, Ian Smail, M Thompson, J Urquhart, J Wall, G Zhao

    Research output: Contribution to journalArticleResearchpeer-review

    290 Citations (Scopus)


    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 a??10Jy/beam) radio continuum survey of the entire Southern sky at 1.3GHz, extending as far North as +30 declination, with a resolution of 10arcsec. EMU is expected to detect and catalogue about 70million galaxies, including typical star-forming galaxies up to za??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.
    Original languageEnglish
    Pages (from-to)215 - 248
    Number of pages34
    JournalPublications of the Astronomical Society of Australia
    Issue number3
    Publication statusPublished - 2011

    Cite this