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We test both the FLRW geometry and $\Lambda$CDM cosmology in a model independent way by reconstructing the Hubble function $H(z)$, the comoving distance $D(z)$ and the growth of structure $f\sigma_8(z)$ using the most recent data available.
1902
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2015
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C. Escamilla-Rivera and J. C. Fabris, “Nonparametric reconstruction of the O m
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2017
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F. Montanari and S. Rasanen, “Backreaction and FRW consistency conditions,” JCAP
2017
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