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Radiative Transfer Modeling of Lyman Alpha Emitters. I. Statistics of Spectra and Luminosity
Zheng Zheng, Renyue Cen, Hy Trac +1
We combine a cosmological reionization simulation with box size of 100Mpc/h on a side and a Monte Carlo Lyman-alpha (Lya) radiative transfer code to model Lyman Alpha Emitters (LAE…
Probing the Epoch of Reionization with the Lyman Alpha Forest at z~4-5
Renyue Cen, Patrick McDonald, Hy Trac +1
The inhomogeneous cosmological reionization process leaves tangible imprints in the intergalactic medium down to z=4-5. The Lyman-alpha forest flux power spectrum provides a potent…
The 21 cm Forest as a Probe of the Reionization and the Temperature of the Intergalactic Medium
Yidong Xu, Xuelei Chen, Zuhui Fan +2
Using high redshift radio sources as background, the 21cm forest observations probe the neutral hydrogen absorption signatures of early structures along the lines of sight. Directl…
Crawling the Cosmic Network: Exploring the Morphology of Structure in the Galaxy Distribution
Nicholas Bond, Michael Strauss, Renyue Cen
Although coherent large-scale structures such as filaments and walls are apparent to the eye in galaxy redshift surveys, they have so far proven difficult to characterize with comp…
First Light Sources at the End of the Dark Ages: Direct Observations of Population III Stars, Proto-Galaxies, and Supernovae During the Reionization Epoch
Jeff Cooke, Asantha Cooray, Ranga-Ram Chary +16
The cosmic dark ages are the mysterious epoch during which the pristine gas began to condense and ultimately form the first stars. Although these beginnings have long been a topic…
Cosmology from the Highly-Redshifted 21 cm Line
Steven Furlanetto, Adam Lidz, Abraham Loeb +26
One of the next decade's most exciting prospects is to explore the cosmic "dark ages," during which the first stars in the Universe formed, with the 21 cm line of neutral hydrogen.…