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2015

HI intensity mapping with FAST

Bigot-Sazy, Marie-Anne, Ma, Yin-Zhe, Battye, Richard A. et al.

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We discuss the detectability of large-scale HI intensity fluctuations using the FAST telescope.

We present forecasts for the accuracy of measuring the Baryonic Acoustic Oscillations and constraining the properties of dark energy.
The FAST $19$-beam L-band receivers ($1.05$--$1.45$ GHz) can provide constraints on the matter power spectrum and dark energy equation of state parameters ($w_{0},w_{a}$) that are comparable to the BINGO and CHIME experiments.
For one year of integration time we find that the optimal survey area is $6000\,{\rm deg}^2$.

HI intensity mapping with FAST · Around

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