Two-point correlation functions of high-redshift objects on a light-cone

Details Two-point correlation functions of high-redshift objects on a light-cone Two-point correlation functions of high-redshift objects on a light-cone

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..470..176y&link_type=abstract

The 9th astrophysics conference: After the dark ages, when galaxies were young (the Universe at 2<Z<5). AIP Conference Proceedi

Astronomy and Astrophysics

Astrophysics

Relativity And Gravitation

Scientific paper

A theoretical formulation for a two-point correlation function of high-redshift objects is investigated. While all the cosmological observations are carried out on a light-cone, the null hypersurface of an observer at z=0, the clustering statistics has been properly defined only on the constant-time hypersurface. We develop the theoretical formulation for the two-point correlation function on the light-cone, and derive a simple approximate expression relevant to the discussion of clustering of high-redshift objects. As an example, we present a prediction of the two-point correlation function for the SDSS quasar catalogue.

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