Statistics
Scientific paper
Jan 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21330201l&link_type=abstract
American Astronomical Society, AAS Meeting #213, #302.01; Bulletin of the American Astronomical Society, Vol. 41, p.270
Statistics
Scientific paper
Our improved understanding of dark-matter halo statistics can be effectively used to extract useful physical information directly from the observed galaxy statistics commonly measured from large galaxy surveys, such as luminosity function and clustering properties (luminosity-dependent trend and overall shape) of galaxies. We apply a simple formalism to constrain the scaling laws between UV luminosity and halo mass (local gravity), and the typical duration of star-formation at z 4 and 5. From these results, we discuss possible dominant mechanisms of star-formation for the majority of galaxies (L
Conroy Charlie
Dickinson Mark Everett
Ferguson Henry C.
Giavalisco Mauro
Lee Kyoungsoo
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