BINARY QUASARS AT HIGH REDSHIFT I 24 NEW QUASAR PAIRS AT

The evolution of the redshift-space correlation function of quasars in the 2dF survey has been measured by Croom et al (2001b) Their study shows that the clustering of quasars in the survey is very comparable to that ofL galaxies at low-redshift, and that the correlation length R0 remains approximately constant out to z ˘ 2

The Structure and Evolution of Galaxies - GBV

8 6 1 Evolution again 267 8 6 2 Faint blue galaxies 270 8 6 3 Radio source counts 270 8 6 4 Quasars 271 8 7 The night sky brightness 272 8 7 1 Metal production 274 8 7 2 QSO absorption lines 274 8 8 The star formation history of the universe 276 8 8 1 Star formation models 277 8 8 2 Star formation at high z 279 8 9 Reionisation and the first

Clustering of high-redshift(z>29) quasars from SDSS

Just as galaxies, quasars are biased tracers of the Evolution of quasar clustering at z

Clustering of quasars in SDSS-IV eBOSS : study of potential

2 Clustering of quasars in SDSS-IV 3 eBOSS : study of potential 4 systematics and bias determination Pierre Laurent,a Sarah Eftekharzadeh,b Jean-Marc Le Goff,a;1 5 Adam Myers,b Etienne Burtin,a Martin White,c ;d e Ashley J Ross,f 6 Jeremy Tinker,g Rita Tojeiro,h Julian Bautista,i Jonathan 7 Brinkmann,j Johan Comparat,k Kyle Dawson,i Hélion

Vol 435 2 June 2005 ARTICLES

Simulations of the formation, evolution and clustering of galaxies and quasars Volker Springel1, Simon D M White1, Adrian Jenkins2, Carlos S Frenk2, Naoki Yoshida3, Liang Gao1, Julio Navarro4, Robert Thacker5, Darren Croton1, John Helly2, John A Peacock6, Shaun Cole2, Peter Thomas7, Hugh Couchman5, August Evrard8,Jo¨rg Colberg9 & Frazer