Observational Validation of the Chronometric Cosmology: The Redshift-Magnitude Relation for Quasi-Stellar Objects

Details Observational Validation of the Chronometric Cosmology: The Redshift-Magnitude Relation for Quasi-Stellar Objects Observational Validation of the Chronometric Cosmology: The Redshift-Magnitude Relation for Quasi-Stellar Objects

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pnas...75..535n&link_type=abstract

Proceedings of the National Academy of Sciences of the United States of America, Volume 75, Issue 2, pp. 535-539

Computer Science

6

Scientific paper

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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