Fig. 6
P(k) 21 cm LSS power spectrum at redshift z = 1 with fHI = 2% and the noise power spectrum for several interferometer configurations ((a), (b), (c), (d), (e), (f), (g)) with 121, 128, 129, 400, and 960 receivers. The noise power spectrum has been computed for all configurations assuming a survey of a quarter of the sky over one year, with a system temperature Tsys = 50 K.
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