Luminosity Function at the End of Reionization

Details Luminosity Function at the End of Reionization Luminosity Function at the End of Reionization

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21541012s&link_type=abstract

American Astronomical Society, AAS Meeting #215, #410.12; Bulletin of the American Astronomical Society, Vol. 42, p.236

Astronomy and Astrophysics

Astronomy

Scientific paper

Deep photometric fields, such as GOODS and HUDF, have been extensively and successfully investigated for the high-redshift galaxies and quasars by dropout technique. The UV luminosity function (LF), a key factor to the study of the universe at the end of reionization, remains, however, not well constrained, particularly at the faint end. We present here a derivation of LF at redshift six by a new application of the maximum likelihood method by exploring the deepest available fields, including the first analysis of HUDF NICP34.

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