Clustering of simulated galaxies at redshift 4

Details Clustering of simulated galaxies at redshift 4 Clustering of simulated galaxies at redshift 4

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005assl..329p..22h&link_type=abstract

Starbursts: From 30 Doradus to Lyman Break Galaxies, Held in Cambridge, UK, 6-10 September 2004. Edited by R. de Grijs and R.M.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We have investigated the structures formed in our hydrodynamic cosmological simulation of reionization and its aftermath. We have identified dark matter haloes and peaks of I-band luminosity. We relate the clustering of these structures to the observed angular correlation of galaxies at redshift 4. The observed correlation is best modelled by the multiple occurrence of luminosity peaks in individual dark matter haloes. Examination of earlier stages of the simulation suggests the importance of disruptive interactions between dark matter haloes.

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