A new three-parameter fit to the comoving distance gives a dark-energy-model-independent spatial curvature constraint of Ω_K = -0.01 ± 0.09, consistent with flatness.
Guth, Inflationary universe: A possible solution to the horizon and flatness problems , Physical Review D 23 (1981) 347
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A dark energy parameterization independent constraint of the spatial curvature $\Omega_K$
A new three-parameter fit to the comoving distance gives a dark-energy-model-independent spatial curvature constraint of Ω_K = -0.01 ± 0.09, consistent with flatness.