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High-redshift galaxy populations

Author

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  • Esther M. Hu

    (Institute for Astronomy, University of Hawaii)

  • Lennox L. Cowie

    (Institute for Astronomy, University of Hawaii)

Abstract

We now see many galaxies as they were only 800 million years after the Big Bang, and that limit may soon be exceeded when wide-field infrared detectors are widely available. Multi-wavelength studies show that there was relatively little star formation at very early times and that star formation was at its maximum at about half the age of the Universe. A small number of high-redshift objects have been found by targeting X-ray and radio sources and most recently, γ-ray bursts. The γ-ray burst sources may provide a way to reach even higher-redshift galaxies in the future, and to probe the first generation of stars.

Suggested Citation

  • Esther M. Hu & Lennox L. Cowie, 2006. "High-redshift galaxy populations," Nature, Nature, vol. 440(7088), pages 1145-1150, April.
    • Handle: RePEc:nat:nature:v:440:y:2006:i:7088:d:10.1038_nature04806
    DOI: 10.1038/nature04806
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