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2009

Exploring the HI Universe with ASKAP

Meyer, Martin

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The survey speed of ASKAP makes it a prime instrument with which to survey the HI universe, enabling it to carry out both wide surveys of the entire sky, as well as deep surveys covering cosmologically representative volumes.

Here, the use of ASKAP to study deep HI fields is discussed as proposed by the Deep Investigation of Neutral Gas Origins (DINGO) survey.
This ASKAP science survey project anticipates observing in excess of 10^5 sources out to redshift z~0.4.
Key science goals include: Omega_HI and its evolution, the cosmic web as traced by distributions such as the HI mass function and the 2pt correlation function, and the formation and evolution of galaxies.

Exploring the HI Universe with ASKAP · Around

Built on

M. J. Meyer et. al
2004
Earlier work this paper cites.
M. A. Zwaan, M. J. Meyer, L. Staveley-Smith, and R. L. Webster, The HIPASS Catalogue: Ω HI \Omega_{\rm HI} and environmental effects on the HI mass function of galaxies
2005
Earlier work this paper cites.
S. M. Rao, D. A. Turnshek, and D. B. Nestor, Damped Ly α \alpha systems at z¡1.65: The expanded sloan digital sky survey hubble space telescope sample
2006
Earlier work this paper cites.
P. Lah et. al
2007
Earlier work this paper cites.

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2009
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Then

I. Feain, S. Johnston, and R. Braun, The Australian Square Kilometre Array Pathfinder (ASKAP) an SKA pre-cursor
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S. Driver, P. Norberg, I. Baldry, S. Bamford, A. Hopkins, J. Liske, J. Loveday, and J. Peacock, GAMA: towards a physical understanding of galaxy formation
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S. Wyithe, M. J. I. Brown, M. A. Zwaan, and M. J. Meyer, The Halo Occupation Distribution of HI Galaxies
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