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Fig. 14

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1D projection of the power spectrum for one simulation. The HI power spectrum is divided by an envelop curve P(k)ref corresponding to the power spectrum without baryonic oscillations. The dots represents one simulation for a “packed” array of dishes with a system temperature, Tsys = 50 K, an observation time, Tobs =  1 year, a solid angle of 1πsr, an average redshift, z = 1.5 and a redshift depth, Δz = 0.5. The solid line is the result of the fit to the data.

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