EMU: Evolutionary map of the universe

Ray P. Norris; A. M. Hopkins; J. Afonso; S. Brown; J. J. Condon; L. Dunne; I. Feain; R. Hollow; M. Jarvis; M. Johnston-Hollitt; E. Lenc; E. Middelberg; P. Padovani; I. Prandoni; L. Rudnick; N. Seymour; G. Umana; H. Andernach; D. M. Alexander; P. N. Appleton; D. Bacon; J. Banfield; W. Becker; M. J.I. Brown; P. Ciliegi; C. Jackson; S. Eales; A. C. Edge; B. M. Gaensler; G. Giovannini; C. A. Hales; P. Hancock; M. T. Huynh; E. Ibar; R. J. Ivison; R. Kennicutt; Amy E. Kimball; A. M. Koekemoer; B. S. Koribalski; R. Lpez-Snchez; M. Y. Mao; T. Murphy; H. Messias; K. A. Pimbblet; A. Raccanelli; K. E. Randall; T. H. Reiprich; I. G. Roseboom; H. Rttgering; D. J. Saikia; R. G. Sharp; O. B. Slee; Ian Smail; M. A. Thompson; J. S. Urquhart; J. V. Wall; G. B. Zhao

doi:10.1071/AS11021

EMU: Evolutionary map of the universe

Ray P. Norris^*, A. M. Hopkins, J. Afonso, S. Brown, J. J. Condon, L. Dunne, I. Feain, R. Hollow, M. Jarvis, M. Johnston-Hollitt, E. Lenc, E. Middelberg, P. Padovani, I. Prandoni, L. Rudnick, N. Seymour, G. Umana, H. Andernach, D. M. Alexander, P. N. AppletonD. Bacon, J. Banfield, W. Becker, M. J.I. Brown, P. Ciliegi, C. Jackson, S. Eales, A. C. Edge, B. M. Gaensler, G. Giovannini, C. A. Hales, P. Hancock, M. T. Huynh, E. Ibar, R. J. Ivison, R. Kennicutt, Amy E. Kimball, A. M. Koekemoer, B. S. Koribalski, R. Lpez-Snchez, M. Y. Mao, T. Murphy, H. Messias, K. A. Pimbblet, A. Raccanelli, K. E. Randall, T. H. Reiprich, I. G. Roseboom, H. Rttgering, D. J. Saikia, R. G. Sharp, O. B. Slee, Ian Smail, M. A. Thompson, J. S. Urquhart, J. V. Wall, G. B. Zhao

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

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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 ∼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 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.

Original language	English
Pages (from-to)	215-248
Number of pages	34
Journal	Publications of the Astronomical Society of Australia
Volume	28
Issue number	3
DOIs	https://doi.org/10.1071/AS11021
Publication status	Published - 2011
Externally published	Yes

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Norris, R. P., Hopkins, A. M., Afonso, J., Brown, S., Condon, J. J., Dunne, L., Feain, I., Hollow, R., Jarvis, M., Johnston-Hollitt, M., Lenc, E., Middelberg, E., Padovani, P., Prandoni, I., Rudnick, L., Seymour, N., Umana, G., Andernach, H., Alexander, D. M., ... Zhao, G. B. (2011). EMU: Evolutionary map of the universe. Publications of the Astronomical Society of Australia, 28(3), 215-248. https://doi.org/10.1071/AS11021

@article{c8909cd3513640a99fb785f91af70e9a,

title = "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 ∼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 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 = "cosmology: observations, galaxies: evolution, galaxies: formation, radio continuum: general, stars: activity, surveys, telescopes",

author = "Norris, {Ray P.} and Hopkins, {A. M.} and J. Afonso and S. Brown and Condon, {J. J.} and L. Dunne and I. Feain and R. Hollow and M. Jarvis and M. Johnston-Hollitt and E. Lenc and E. Middelberg and P. Padovani and I. Prandoni and L. Rudnick and N. Seymour and G. Umana and H. Andernach and Alexander, {D. M.} and Appleton, {P. N.} and D. Bacon and J. Banfield and W. Becker and Brown, {M. J.I.} and P. Ciliegi and C. Jackson and S. Eales and Edge, {A. C.} and Gaensler, {B. M.} and G. Giovannini and Hales, {C. A.} and P. Hancock and Huynh, {M. T.} and E. Ibar and Ivison, {R. J.} and R. Kennicutt and Kimball, {Amy E.} and Koekemoer, {A. M.} and Koribalski, {B. S.} and R. Lpez-Snchez and Mao, {M. Y.} and T. Murphy and H. Messias and Pimbblet, {K. A.} and A. Raccanelli and Randall, {K. E.} and Reiprich, {T. H.} and Roseboom, {I. G.} and H. Rttgering and Saikia, {D. J.} and Sharp, {R. G.} and Slee, {O. B.} and Ian Smail and Thompson, {M. A.} and Urquhart, {J. S.} and Wall, {J. V.} and Zhao, {G. B.}",

year = "2011",

doi = "10.1071/AS11021",

language = "English",

volume = "28",

pages = "215--248",

journal = "Publications of the Astronomical Society of Australia",

issn = "1323-3580",

publisher = "Cambridge University Press",

number = "3",

}

Norris, RP, Hopkins, AM, Afonso, J, Brown, S, Condon, JJ, Dunne, L, Feain, I, Hollow, R, Jarvis, M, Johnston-Hollitt, M, Lenc, E, Middelberg, E, Padovani, P, Prandoni, I, Rudnick, L, Seymour, N, Umana, G, Andernach, H, Alexander, DM, Appleton, PN, Bacon, D, Banfield, J, Becker, W, Brown, MJI, Ciliegi, P, Jackson, C, Eales, S, Edge, AC, Gaensler, BM, Giovannini, G, Hales, CA, Hancock, P, Huynh, MT, Ibar, E, Ivison, RJ, Kennicutt, R, Kimball, AE, Koekemoer, AM, Koribalski, BS, Lpez-Snchez, R, Mao, MY, Murphy, T, Messias, H, Pimbblet, KA, Raccanelli, A, Randall, KE, Reiprich, TH, Roseboom, IG, Rttgering, H, Saikia, DJ, Sharp, RG, Slee, OB, Smail, I, Thompson, MA, Urquhart, JS, Wall, JV & Zhao, GB 2011, 'EMU: Evolutionary map of the universe', Publications of the Astronomical Society of Australia, vol. 28, no. 3, pp. 215-248. https://doi.org/10.1071/AS11021

TY - JOUR

T1 - EMU

T2 - Evolutionary map of the universe

AU - Norris, Ray P.

AU - Hopkins, A. M.

AU - Afonso, J.

AU - Brown, S.

AU - Condon, J. J.

AU - Dunne, L.

AU - Feain, I.

AU - Hollow, R.

AU - Jarvis, M.

AU - Johnston-Hollitt, M.

AU - Lenc, E.

AU - Middelberg, E.

AU - Padovani, P.

AU - Prandoni, I.

AU - Rudnick, L.

AU - Seymour, N.

AU - Umana, G.

AU - Andernach, H.

AU - Alexander, D. M.

AU - Appleton, P. N.

AU - Bacon, D.

AU - Banfield, J.

AU - Becker, W.

AU - Brown, M. J.I.

AU - Ciliegi, P.

AU - Jackson, C.

AU - Eales, S.

AU - Edge, A. C.

AU - Gaensler, B. M.

AU - Giovannini, G.

AU - Hales, C. A.

AU - Hancock, P.

AU - Huynh, M. T.

AU - Ibar, E.

AU - Ivison, R. J.

AU - Kennicutt, R.

AU - Kimball, Amy E.

AU - Koekemoer, A. M.

AU - Koribalski, B. S.

AU - Lpez-Snchez, R.

AU - Mao, M. Y.

AU - Murphy, T.

AU - Messias, H.

AU - Pimbblet, K. A.

AU - Raccanelli, A.

AU - Randall, K. E.

AU - Reiprich, T. H.

AU - Roseboom, I. G.

AU - Rttgering, H.

AU - Saikia, D. J.

AU - Sharp, R. G.

AU - Slee, O. B.

AU - Smail, Ian

AU - Thompson, M. A.

AU - Urquhart, J. S.

AU - Wall, J. V.

AU - Zhao, G. B.

PY - 2011

Y1 - 2011

N2 - 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 ∼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 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.

AB - 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 ∼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 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.

KW - cosmology: observations

KW - galaxies: evolution

KW - galaxies: formation

KW - radio continuum: general

KW - stars: activity

KW - surveys

KW - telescopes

UR - http://www.scopus.com/inward/record.url?scp=80053408029&partnerID=8YFLogxK

U2 - 10.1071/AS11021

DO - 10.1071/AS11021

M3 - Article

SN - 1323-3580

VL - 28

SP - 215

EP - 248

JO - Publications of the Astronomical Society of Australia

JF - Publications of the Astronomical Society of Australia

IS - 3

ER -

EMU: Evolutionary map of the universe

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