However, the three year WMAP data returned a different result, with reionization beginning at " z " = 11 and the universe ionized by " z " = 7.
42.
It is unusual because it has hints of an early spiral structure, which is normally only found in satellite galaxy of the Milky Way, recently discovered to be a potential relic of the epoch of reionization.
43.
Improved constraints were put on the redshift of reionization, which is, the redshift of decoupling, ( as well as age of universe at decoupling, ) and the redshift of matter / radiation equality,.
44.
His later research includes the study of non-Gaussianity in the cosmic microwave background anisotropy, Lyman alpha forest, application of wavelet in cosmology, turbulence in intergalactic medium, and the 21cm radiation during the Reionization.
45.
Despite the fact that the ratio of neutral hydrogen to ionized hydrogen may not have been particularly high, the low flux observed past the Lyman-alpha limit indicates that the universe was in the final stages of reionization.
46.
These massive stars triggered the reionization process and are believed to have created many of the heavy elements in the early Universe, which, through nuclear decay, create lighter elements, allowing the cycle of nucleosynthesis to continue longer.
47.
LyC leakage is crucial to the process known as Reionization which is theorised to have occurred between redshift z = 11 and z = 7, that is to say within the first 10 % of the age of the Universe.
48.
Following the first release of data from the WMAP spacecraft in 2003, the determination by Becker that the end of reionization occurred at z H " 6 appeared to conflict with estimates made from the WMAP measurement of the electron column density.
49.
Reionization, or The Epoch of Reionization ( EofR ), is a term used to describe the period during which the gas in the early Universe went from being almost completely neutral to a state in which it became almost completely ionized.
50.
Reionization, or The Epoch of Reionization ( EofR ), is a term used to describe the period during which the gas in the early Universe went from being almost completely neutral to a state in which it became almost completely ionized.
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