The Evolution of the UV Luminosity Function of Star-Forming Galaxies at 2.5<z<6.5

Details The Evolution of the UV Luminosity Function of Star-Forming Galaxies at 2.5<z<6.5 The Evolution of the UV Luminosity Function of Star-Forming Galaxies at 2.5<z<6.5

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.9412g&link_type=abstract

American Astronomical Society Meeting 205, #94.12; Bulletin of the American Astronomical Society, Vol. 36, p.1497

Astronomy and Astrophysics

Astronomy

Scientific paper

The history of the cosmic star-formation activity is a key observable to compare against theoretical predictions. The contribution by star-forming galaxies at high redshifts with moderate amount of dust obscuration (and reddening) is relatively easily estimated from optical and near-infrared data. Observations at longer wavelengths are necessary to identify those with more severe dust obscuration. Using multi-wavelength imaging data from the Great Observatories Origins Deep Survey (GOODS) we report on the evolution of the rest-frame UV luminosity function of relatively unobscured star-forming galaxies at redshifts 2.5

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