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K.S. Lee (Johns Hopkins University), M. Giavalisco, M.E. Dickinson (Space Telescope Science Institute), GOODS Team
The Great Observatories Origins Deep Survey includes both very deep ACS mluticolor images that covers relatively large area as well as relatively shallower that covers yet even larger area in the sky. This data set is very useful for studying clustering properties of high-redshift galaxies in general, especially for studying their dependence of clustering strength on luminosity class since our sample contains galaxies at the very faint end as well as the bright end, which would imply the relationship between star formation rate and the underlying mass distribution of dark matter haloes. Here we present angular correlation function measurement of galaxies with z~3,4,5 and 6 along with implied spatial correlation lengths on GOODS North(HDF-N) and South field(CDF-S).
The author(s) of this abstract have provided an email address for comments about the abstract: soolee@stsci.edu
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Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.