Galaxy Luminosity Function & Star-forming Sequence vs. Redshift

Details Galaxy Luminosity Function & Star-forming Sequence vs. Redshift Galaxy Luminosity Function & Star-forming Sequence vs. Redshift

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21543503l&link_type=abstract

American Astronomical Society, AAS Meeting #215, #435.03; Bulletin of the American Astronomical Society, Vol. 42, p.379

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Scientific paper

We measure the galaxy luminosity function (LF) at FUV band ( effective wavelength 1516 Angstrom ) from z 0 to 1.2 based on GALEX data and CFHTLS observations. We present the evolution of its slope and other parameters through redshift. From the measured LF we select a sub-sample of the bright galaxies as extreme star-forming galaxies and study their properties.

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