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2000MNRAS.318..913M - Mon. Not. R. Astron. Soc., 318, 913-924 (2000/November-1)
Galaxy clustering in the Herschel Deep Field.
McCRACKEN H.J., SHANKS T., METCALFE N., FONG R. and CAMPOS A.
Abstract (from CDS):
If our luminosity evolution models provide a correct description of the underlying redshift distributions (and comparisons to available observations at brighter magnitudes suggest they do), then our measurements in all bandpasses are consistent with a rapid growth of galaxy clustering (0<ε<2 in the normal parametrization) on the sub-Mpc scales which our survey probes. We demonstrate that this rapid growth of clustering is consistent with the predictions of biased models of galaxy formation, which indicate that a rapid rate of clustering growth is expected for the intrinsically faint galaxies which dominate our survey.
Abstract Copyright: 2000, Royal Astronomical Society
Journal keyword(s): galaxies: evolution - galaxies: statistics - cosmology: observations - large-scale structure of Universe
Simbad objects: 3
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