Add to ORKGThe high ionization level and universal metallicity (1% solar) of the intergalactic gas at redshifts z10 and damps the amplitude of anisotropies on angular scales 5. The cumulative Bremsstrahlung emission from these star clusters yields a measurable distortion to the spectrum of the microwave background
The exploration of the end of the Dark Ages will be one of the most exciting field of the next decad...
We present results on the evolution of dark matter halos and reionization. Dark matter halos enshro...
A simple scenario of cosmological reionization is presented. In hierarchical clustering models of st...
The first light from stars and quasars ended the ``dark ages'' of the universe and led to the reioni...
We show that the cosmic star formation rate per comoving volume should exhibit a distinct drop aroun...
Motivated by the recent detection by the Wilkinson Microwave Anisotropy Probe of a large optical dep...
The intergalactic medium was reionized before redshift z ∼ 6, most likely by starlight which escaped...
We compare model results from a semi-analytic (merger-tree based) framework for high-redshift (z ' 5...
We simulate a plausible cosmological model in considerable physical and numerical detail through the...
We present a self-consistent, semi-analytical LCDM model of star formation and reionization. For the...
The intergalactic medium was reionized before redshift z similar to 6, most likely by starlight whic...
We study the inhomogeneous reionization in a critical density CDM universe due to stellar sources, i...
Various observations suggest that the universe is reionized at z< 5 after the recombination at z ...
We have modelled the process of reionization in the high redshift Universe to determine the epoch of...
We have modelled the process of reionization of the intergalactic medium (IGM) by photoionization by...
The exploration of the end of the Dark Ages will be one of the most exciting field of the next decad...
We present results on the evolution of dark matter halos and reionization. Dark matter halos enshro...
A simple scenario of cosmological reionization is presented. In hierarchical clustering models of st...
The first light from stars and quasars ended the ``dark ages'' of the universe and led to the reioni...
We show that the cosmic star formation rate per comoving volume should exhibit a distinct drop aroun...
Motivated by the recent detection by the Wilkinson Microwave Anisotropy Probe of a large optical dep...
The intergalactic medium was reionized before redshift z ∼ 6, most likely by starlight which escaped...
We compare model results from a semi-analytic (merger-tree based) framework for high-redshift (z ' 5...
We simulate a plausible cosmological model in considerable physical and numerical detail through the...
We present a self-consistent, semi-analytical LCDM model of star formation and reionization. For the...
The intergalactic medium was reionized before redshift z similar to 6, most likely by starlight whic...
We study the inhomogeneous reionization in a critical density CDM universe due to stellar sources, i...
Various observations suggest that the universe is reionized at z< 5 after the recombination at z ...
We have modelled the process of reionization in the high redshift Universe to determine the epoch of...
We have modelled the process of reionization of the intergalactic medium (IGM) by photoionization by...
The exploration of the end of the Dark Ages will be one of the most exciting field of the next decad...
We present results on the evolution of dark matter halos and reionization. Dark matter halos enshro...
A simple scenario of cosmological reionization is presented. In hierarchical clustering models of st...