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2010

Trumpeting the Vuvuzela: UltraDeep HI observations with MeerKAT

Holwerda, B. W., Blyth, S-L.

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The MeerKAT UltraDeep HI Survey aims to observe the 21 cm emission line of neutral hydrogen gas out to a redshift of z=1 and beyond.

From both direct detections and stacked signal, we will address the HI mass function, the cosmic neutral gas density of the Universe (Omega_HI) and their evolution over cosmic times, as well as galaxy evolution via e.g., the Tully-Fisher relation, the relation between HI mass and Hubble Type or stellar mass, and the Schmidt-Kennicutt star-formation law.
We propose to observe two fields, the COSMOS and Chandra Deep Field South (CDF-S) for 1000 hours each, adding an additional 4000 hours to one of these fields in 2015 when the full instantaneous bandwidth of MeerKAT (0.58-2.5 GHz) will be realised.

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de Blok, W. J. G. et al. 2009, in Conference Proceedings of the ”Panoramic Radio Astronomy: Wide-field 1-2 GHz research on galaxy evolution”, June 02 - 05, 2009 Groningen, the Netherlands
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