Quasar-Galaxy Clustering through Projected Galaxy Counts at z=0.6-1.2 [PDF]
Shao-Hua Zhang, Ting-Gui Wang, Hui-Yuan Wang, Hongyan ZhouWe investigate the spatial clustering of galaxies around quasars at redshifts from 0.6 to 1.2 using the photometric data from Sloan Digital Sky Survey (SDSS) Stripe 82. The quasar and galaxy cross-correlation functions are measured through the projected galaxy number density n(r_p) on scales $0.05View original: http://arxiv.org/abs/1307.1951
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