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M. Stiavelli, S.M. Fall (STScI), N. Panagia (STScI and ESA)
We derive the expected properties of reionization sources with very low metallicity and show how the z=6 galaxies identified as i-band dropouts in the Hubble Ultra Deep Field and in the GOODS survey would be capable of reionizing the Universe provided their metallicity is very low and/or their mass function is top heavy. We discuss possible alternatives to that of a very low metallicity and how some of these alternatives could be tested with observations.
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Bulletin of the American Astronomical Society, 36 5
© 2004. The American Astronomical Society.