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
The evolution of galaxy clustering from z=0 to z≃4.5 is analysed using the angular correlation function and the photometric redshift distribution of galaxies brighter than IAB 28.5 in the Hubble Deep Field North. The reliability of the photometric redshift estimates is discussed on the basis of the available spectroscopic redshifts, …