The Damping Wing of the Gunn-Peterson Absorption and Lyman-Alpha Emitters in the Pre-Reionization Era
arXiv:astro-ph/0403345 · doi:10.1086/422390
Abstract
We use a numerical simulation of cosmological reionization to estimate the likelihood of detecting Lyman-alpha emitting galaxies during the pre-reionization era. We show that it is possible to find galaxies even at z~9 that are barely affected by the dumping wing of the Gunn-Peterson absorption from the neutral IGM outside of their HII regions. The damping wing becomes rapidly more significant at z>9, but even at z>10 is it not inconceivable (although quite hard) to see a Lyman-alpha emission line from a star-forming galaxy.
submitted to ApJ
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- Secondary anisotropies of the CMB
- Improved Constraints on The Neutral Intergalactic Hydrogen Surrounding Quasars at Redshifts z>6
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- Constraining Reionization with the Evolution of the Luminosity Function of Lyman Alpha mitting Galaxies
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- The Strömgren sphere, the environment and the reionization in the local universe of the highest redshift QSOs
- Stellar populations and Lya emission in two lensed z>~6 galaxies
- 21 cm Tomography of the High-Redshift Universe with the Square Kilometer Array
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- Hubble Advanced Camera for Surveys Observations of the z=6.42 Quasar SDSS 1148+5251: A Leak in the Gunn-Peterson Trough
- Narrow-band surveys for very high redshift Lyman-alpha emitters
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- The cosmological free-free signal from galaxy groups and clusters
- Implications of the Lyman alpha Emission Line from a Candidate z=10 Galaxy
- Constraining Reionization with Lyman Alpha Emitting Galaxies
- Observations of Ly Emitters at High Redshift
- Lyman- Emitting Galaxies (LAEs) at Cosmic Dawn: Implications and Predictions