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.