Add to ORKGWe study the luminosity functions of high-redshift galaxies in detailed hydrodynamic simulations of cosmic reionization, which are designed to reproduce the evolution of the Lyman-alpha forest between z=5 and z=6. We find that the luminosity functions and total stellar mass densities are in agreement with observations when plausible assumptions about reddenning at z=6 are made. Our simulations support the conclusion that stars alone reionized the universe
The reionization of intergalactic hydrogen in the universe’s first billion years was likely driven b...
Near-infrared observations of Lyman-break galaxies at redshifts z~3 are beginning to provide constra...
We investigate the properties of the galaxies that reionized the Universe and the history of cosmic ...
We present a self-consistent, semi-analytical LCDM model of star formation and reionization. For the...
We present a self-consistent, semi-analytical ΛCDM model of star formation and reionization. F...
We present a self-consistent, semi-analytical ΛCDM model of star formation and reionization. F...
We use high-resolution simulations of cosmological volumes to model galaxy forma-tion at high-redshi...
We show that the cosmic star formation rate per comoving volume should exhibit a distinct drop aroun...
Cosmological hydrodynamic simulations have significantly improved over the past several years, and w...
Reionization is thought to have occurred in the redshift range of 6 6 that matches the measured gal...
Cosmological hydrodynamic simulations have significantly improved over the past several years, and w...
We use high-resolution simulations of cosmological volumes to model galaxy formation at high-redshif...
© 2018 Dr. Yuxiang QinHow galaxies form at high redshift remains a puzzle due to our limited observa...
We combine observational data on a dozen independent cosmic properties at high-z with the informatio...
We combine observational data on a dozen independent cosmic properties at high-z with the informatio...
The reionization of intergalactic hydrogen in the universe’s first billion years was likely driven b...
Near-infrared observations of Lyman-break galaxies at redshifts z~3 are beginning to provide constra...
We investigate the properties of the galaxies that reionized the Universe and the history of cosmic ...
We present a self-consistent, semi-analytical LCDM model of star formation and reionization. For the...
We present a self-consistent, semi-analytical ΛCDM model of star formation and reionization. F...
We present a self-consistent, semi-analytical ΛCDM model of star formation and reionization. F...
We use high-resolution simulations of cosmological volumes to model galaxy forma-tion at high-redshi...
We show that the cosmic star formation rate per comoving volume should exhibit a distinct drop aroun...
Cosmological hydrodynamic simulations have significantly improved over the past several years, and w...
Reionization is thought to have occurred in the redshift range of 6 6 that matches the measured gal...
Cosmological hydrodynamic simulations have significantly improved over the past several years, and w...
We use high-resolution simulations of cosmological volumes to model galaxy formation at high-redshif...
© 2018 Dr. Yuxiang QinHow galaxies form at high redshift remains a puzzle due to our limited observa...
We combine observational data on a dozen independent cosmic properties at high-z with the informatio...
We combine observational data on a dozen independent cosmic properties at high-z with the informatio...
The reionization of intergalactic hydrogen in the universe’s first billion years was likely driven b...
Near-infrared observations of Lyman-break galaxies at redshifts z~3 are beginning to provide constra...
We investigate the properties of the galaxies that reionized the Universe and the history of cosmic ...