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Abstract We measure the redshift-space correlation function from a spectroscopic sample of 2783 emission line galaxies from the FastSound survey. The survey, which uses the Subaru Telescope and covers a redshift range of 1. 19 z 1. 55, is the first cosmological study at such high redshifts. We detect clear anisotropy due to redshift-space distortions (RSD) both in the correlation function as a function of separations parallel and perpendicular to the line of sight and its quadrupole moment. RSD has been extensively used to test general relativity on cosmological scales at z 1. Adopting a ΛCDM cosmology with the fixed expansion history and no velocity dispersion (σv = 0), and using the RSD measurements on scales above 8 h−1 Mpc, we obtain the first constraint on the growth rate at the redshift, f (z) σ8 (z) = 0. 482 ± 0. 116 at z ∼ 1. 4 after marginalizing over the galaxy bias parameter b (z) σ8 (z). This corresponds to 4. 2 σ detection of RSD. Our constraint is consistent with the prediction of general relativity fσ8 ∼ 0. 392 within the 1 σ confidence level. When we allow σv to vary and marginalize over it, the growth rate constraint becomes f ₈=0. 494^+0. 126-₀. ₁₂₀. We also demonstrate that by combining with the low-z constraints on fσ8, high-z galaxy surveys like the FastSound can be useful to distinguish modified gravity models without relying on CMB anisotropy experiments.
Okumura et al. (Tue,) studied this question.