Measuring and Modelling the Redshift Evolution of Clustering: the Hubble Deep Field North

Details Measuring and Modelling the Redshift Evolution of Clustering: the Hubble Deep Field North Measuring and Modelling the Redshift Evolution of Clustering: the Hubble Deep Field North

1999-02-19

arxiv.org/abs/astro-ph/9902290v2

Mon.Not.Roy.Astron.Soc. 310 (1999) 540-556

Astronomy and Astrophysics

Astrophysics

23 pages, Latex using MN style, figures enclosed. Version accepted for publication in MNRAS

Scientific paper

10.1046/j.1365-8711.1999.02978.x

(abridged) The evolution of galaxy clustering from z=0 to z=4.5 is analyzed using the angular correlation function and the photometric redshift distribution of galaxies brighter than I_{AB}\le 28.5 in the HDF North. The reliability of the photometric redshift estimates is discussed on the basis of the available spectroscopic redshifts, comparing different codes and investigating the effects of photometric errors. The redshift bins in which the clustering properties are measured are then optimized to take into account the uncertainties of the photometric redshifts. The results show that the comoving correlation length has a small decrease in the range 0

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