The Cosmic Star Formation Rate History at z > 1

Details The Cosmic Star Formation Rate History at z > 1 The Cosmic Star Formation Rate History at z > 1

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..259g&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

I will give a critical assessment of the observational determination of the cosmic SFR history at z > 1 from UV/IR/submm deep fields. It turns out that the UV extinction of star forming high-z galaxies is high and induces large corrections. The hybrid (N-body + semi-analytic) implementation of hierarchical galaxy formation predicts the overall statistical properties of high-z galaxies in the UV and IR/submm. The observational facilities in forthcoming years should offer exciting opportunities to understand the high-z galaxy and star formation histories.

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