Probing the Epoch of Reionization with the Hubble Ultra Deep Field

Details Probing the Epoch of Reionization with the Hubble Ultra Deep Field Probing the Epoch of Reionization with the Hubble Ultra Deep Field

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.3808s&link_type=abstract

American Astronomical Society Meeting 205, #38.08; Bulletin of the American Astronomical Society, Vol. 36, p.1406

Astronomy and Astrophysics

Astronomy

Scientific paper

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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