4 papers
Evidence for Galaxy Formation at High Redshift
T. Shanks, N. Metcalfe, R. Fong +3
We have shown previously that galaxy counts from the UV to the near-IR are well-fitted by simple evolutionary models where the space density of galaxies remains constant with look-…
Galaxy Number Counts
Ana Campos
In these Lectures Notes I re-visit the problem of the deep number counts as a viable method to (1) study the evolution of the galaxy population in the past and (2) determine the va…
Faint Field Galaxies: A Population of Intrinsically Faint Objects at Low Redshift?
Ana Campos
To distinguish between the different models proposed to understand the excess of faint field counts over the predictions from non-evolving models, a number of redshift surveys have…
The Angular Correlation Function of Galaxies in CDM and CHDM Models
G. Yepes, A. Klypin, A. Campos +1
We estimate the angular correlation function for the standard CDM, tilted CDM and hybrid (CHDM) models, and compare with observations. When compared with the APM observatio…