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Fig. 10.
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Power spectra of the LORELI simulations at k = 0.1 h/cMpc as a function of z. These are compared to recent upper limits of various instruments (Patil et al. 2017; Mertens et al. 2020; Trott et al. 2020; Abdurashidova et al. 2023) as well as theoretical thermal noise power of 1000 h observations with NenuFAR and LOFAR.
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