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In the standard (classic) approach, galaxy clustering measurements from spectroscopic surveys are compressed into baryon acoustic oscillations and redshift space distortions measurements, which in turn can be compared to cosmological models.
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A.G. Sanchez et al., Cosmological parameters from CMB measurements and the final 2dFGRS power spectrum , Mon. Not. Roy. Astron. Soc. 366
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S. Vagnozzi et al., Bias due to neutrinos must not uncorrect’d go , JCAP 09
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