Observational validation of the chronometric cosmology: The redshift—magnitude relation for quasi-stellar objectsa

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RESUMO

A statistical study is made of the redshift—magnitude relation for a recent comprehensive catalogue of quasi-stellar objects. The chronometric theory, although devoid of free parameters such as the q0 and Λ of the expansion theory, provides an excellent fit to the observed relation. The expansion theory does not provide an empirically meaningful fit.

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