Clustering at High Redshift

Details Clustering at High Redshift Clustering at High Redshift

1999-05-25

arxiv.org/abs/astro-ph/9905314v1

Astronomy and Astrophysics

Astrophysics

8 pages Latex, with 3 PostScript figures. To appear in the Proceedings of the VLT Opening Symposium, Antofagasta, Chile 1-4 Ma

Scientific paper

10.1007/10720961_24

Together with the CMB, the three sources of information that astronomers have at high redshift as probes of the formation and evolution of the LSS are QSOs, galaxies and absorbers observed in the spectrum of distant background objects. In this contribution I try to give a hint of historical perspective, following how the technological advances have driven the emphasis from one class to another, in order to show what are the likely forthcoming milestones.

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