Searching for the Sources Responsible for Cosmic Reionization: Probing 7 < z < 10 and Beyond
arXiv:astro-ph/0508123 · doi:10.1016/j.newar.2005.11.012
Abstract
(Abridged) We review recent observations that suggest the star formation rate density is declining over 37 and illustrate the challenges that this poses in explaining the assembled stellar mass in z6 galaxies deduced from Spitzer data. A plausible conclusion is a vigorous period of earlier star formation. Prior to JWST and TMT, strong lensing offers a unique probe of the extent of this earlier activity. We discuss the first results of a blind spectroscopic survey of lensing clusters for 8.510 Ly emitters using NIRSPEC which is achieving a limiting star formation rate of 0.1 yr. A companion HST/IRAC survey is targeting lensed and -band dropouts and probes a 1 arcmin region 1 magnitude deeper than the UDF/NICMOS observations. Both surveys will constrain the contribution of early, low luminosity, sources to cosmic reionization.
12 pages, 6 figures, to appear in "First Light & Reionization", eds. E. Barton & A. Cooray, New Astronomy Reviews, in press
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- A galaxy at a redshift z = 6.96
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- The Physical Properties and Detectability of Reionization-Epoch Galaxies
- Unveiling the oldest and most massive galaxies at very high redshift
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- Dwarf Galaxy Formation Was Suppressed By Cosmic Reionization
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- Observations of the High Redshift Universe