Abstract
We review recent observations that suggest that the global star formation rate density of UV-bright galaxies is declining monotonically with redshift over 3 < z < 7 and illustrate the challenges that a continuation of this decline poses in explaining the assembled stellar mass in several z ∼ 6 galaxies deduced from recent Spitzer data. A plausible conclusion is a vigorous period of yet 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 10 lensing clusters for 8.5 < z < 10 Ly α emitters using NIRSPEC on Keck. We demonstrate this survey is achieving an (unlensed) sensitivity equivalent to a star formation rate of 0.1 M⊙ yr-1. A companion survey, now beginning with HST and Spitzer, will target lensed z and J-band drop-outs and probe a ≃ 1 arcmin2 region 1 magnitude deeper than the UDF/NICMOS observations. In combination, both surveys will provide the first constraints on the contribution of early, low luminosity, sources to cosmic reionization.
Original language | English (US) |
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Pages (from-to) | 46-52 |
Number of pages | 7 |
Journal | New Astronomy Reviews |
Volume | 50 |
Issue number | 1-3 SPEC. ISS. |
DOIs | |
State | Published - Mar 2006 |
Externally published | Yes |
Keywords
- Cosmology: observations
- Galaxies: high redshift
- Gravitational lensing
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science