A possible new interpretation of the results of from QSO absorption lines
arXiv:astro-ph/0502191 · doi:10.1016/j.physletb.2005.04.070
Abstract
The measurement of from the QSO absorption lines of Fe_II taken at two different redshifts (Quast et al, Levshakov et al) is compared with the result based on the 23 data points also obtained from VLT/UVES (Chand et al), to demonstrate that the apparent oscillatory time-dependence fitting the latter taken at face value is reinforced by the former claimed to be of much better accuracy.
5 pages, 2 figures
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