期刊名称：Proceedings of the National Academy of Sciences
印刷版ISSN：0027-8424
电子版ISSN：1091-6490
出版年度：1978
卷号：75
期号：2
页码：535-539
DOI：10.1073/pnas.75.2.535
语种：English
出版社：The National Academy of Sciences of the United States of America
摘要：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 {Lambda} of the expansion theory, provides an excellent fit to the observed relation. The expansion theory does not provide an empirically meaningful fit.
