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Most cosmological data analysis today relies on the Friedmann-Lemaitre-Robertson-Walker (FLRW) metric, providing the basis of the current standard cosmological model.
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H. J. Macpherson and A. Heinesen, Erratum: Luminosity distance and anisotropic sky-sampling at low redshifts: A numerical relativity study [Phys. Rev. D 104, 023525 (2021)], Phys. Rev. D 104
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