Retorne
Título               : Clustering at high redshift  
Conferencista: Leopoldo Infante, PUC-Chile  
Data                  : Quarta-feira, 16/05/01, 14H00M  
Local                 : Auditório L.B.F. Clauzet - Água Funda  
Sumário           :
I will give a brief introduction on why clustering is expected at z>3. I will talk about "bias", the Halo Occupation Function (HOF) to describe the structure and describe statistical methods to study clustering and its evolution. I will then discuss how galaxies, groups, clusters and superclusters cluster at low redshifts. We'll also look at the measured and expected clustering evolution. Finally, I will describe current efforts in understanding clustering at high z (z=>3), qso clustering and surveys.