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| In this paper, using the theory and formula of cosmological redshift as the validation technique in determining distances to high-redshift supernovae, we present the results of 43 high-redshift (0.172 $leq z leq$ 1.755) type Ia supernovae. The results show that the distances determined by the cosmological redshift formula and the Standard Candle Method have a good match within the measurement uncertainties. This cosmological redshift formula can not only describe the universe beyond the boundary of Hubble's Law, but also evolve back to Hubble's Law in low-redshift scale. All these results have nothing to do with the assumption of dark energy and the average density of the universe. |
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| Keywords: Dark energy, Cosmological redshift, Cosmological redshift formula, Nonlinear redshift, Hubble's law, Type Ia supernovae |
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