Abstract
We outline the case for a comprehensive wide and deep survey ultimately
targeted at obtaining 21-cm HI line emission spectroscopic observations
of more than a billion galaxies to redshift z=1.5 and greater over half
the sky. This survey provides a database of galaxy redshifts, HI gas
masses, and galaxy rotation curves that would enable a wide range of
science, including fundamental cosmology and studies of Dark Energy.
This science requires the next generation of radio arrays, which are
being designed under the umbrella of the Square Kilometer Array (SKA)
project. We present a science roadmap, extending to 2020 and beyond,
that would enable this ambitious survey. We also place this survey in
the context of other multi-wavelength surveys.
Original language | English |
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Journal | Astro2010: The Astronomy and Astrophysics Decadal Survey, Science White Papers |
Volume | 2010 |
Publication status | Published - 2010 |