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Fig. 9

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Comparison of the 21 cm LSS power spectrum at z = 0.6 with fHI ≃ 1.3% (red, orange) with the radio foreground power spectrum. The radio sky power spectrum is shown for the GSM (Model-I) sky model (dark blue), as well as for our simple model based on Haslam+NVSS (Model-II, black). The curves with circle markers show the power spectrum as observed by a perfect instrument with a 25 arcmin (FWHM) Gaussian beam.

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