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Clustering at High Redshift

Name: Clustering at High Redshift
Creator: Stefano Cristiani
Keywords: Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Preprint , Other literature type 10 Feb 2006Embargo end date: 01 Jan 1999 English Publisher:Springer Science and Business Media LLC

Authors: Stefano Cristiani;

doi: 10.1007/10720961_24 , 10.48550/arxiv.astro-ph/9905314

arXiv: http://arxiv.org/abs/astro-ph/9905314

Clustering at High Redshift

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Abstract

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.

8 pages Latex, with 3 PostScript figures. To appear in the Proceedings of the VLT Opening Symposium, Antofagasta, Chile 1-4 March 1999

Related Organizations

University of Padua
Italy

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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Related to Research communities

NEANIAS Space Research Community