Lyman Break Galaxies and Reionization of the Universe

Abstract

We present the star formation histories, luminosities, colors, mass to light ratios, and halo masses of "galaxies" formed in a simulation of cosmological reionization. We compare these galaxies with Lyman Break Galaxies observed at high redshift. While the simulation is severely limited by the small box size, the simulated galaxies do appear as fainter cousins of the observed ones. They have similar colors, and both simulated and observed galaxies can be fitted with the same luminosity function. This is significant to the process of reionization since in the simulation the stars alone are responsible for reionization at a redshift consistent with that of the Gunn-Peterson trough seen in the absorption spectra of QSO's. The brightest galaxies at z = 4 are indeed quite young in accord with observational studies. But these brightest galaxies are free riders - they contributed only about 25% to the reionization of the universe at z > 6. Instead, the bulk of the work was done by dimmer galaxies, those that fall within the 28 < I < 30 magnitude range at z = 4. These dimmer galaxies are not necessarily less massive than the brightest ones.

submitted to ApJ

References in corpus (5)

• Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization
• The Evolution of the Global Stellar Mass Density at 0 < z < 3
• The Discovery of Two Lyman$\alpha$ Emitters Beyond Redshift 6 in the Subaru Deep Field
• Luminous Lyman Break Galaxies at z>5 and the Source of Reionization
• Lyman Break Galaxies at z~5: Luminosity Function

Cited by in corpus (9)

• Faint Lyman-Break galaxies as a crucial test for galaxy formation models
• Probing the Dark Ages with the Square Kilometer Array
• Photometric Properties of Lyman-break Galaxies at z=3 in Cosmological SPH Simulations
• Lyman Break Galaxies at z = 4 - 6 in cosmological SPH Simulations
• Photometric Properties of the Most Massive High-Redshift Galaxies
• Physical Properties of Local Star-Forming Analogues to z~5 Lyman Break Galaxies
• Intergalactic baryon-rich regions at high redshift
• Radio observations confirm young stellar populations in local analogues to $z\sim 5$ Lyman break galaxies
• Star Formation in a Cosmological Simulation of Reionization