Euclid on Sky
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Fig. 2

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Measured galaxy power spectrum multipoles calculated from dedicated mocks (Pezzotta et al. in prep.) based on the Flagship simulation (see Sect. 6.1) of the Euclid emission-line sample for a redshift bin 1.3 < z < 1.5, compared to a best-fit model based on effective field theory (EFT, also called EFTofLSS, see Sect. 8.2.2 for further discussion) assuming kmax = 0.25 h Mpc−1. Error bars here correspond to the Euclid full mission volume for this redshift bin prior to observational effects.

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