Understanding the results of galaxy-galaxy lensing using galaxy-mass correlation in numerical simulations

Monthly Notices of the Royal Astronomical Society

Volumn 339, Issue 2, 2003, Pages 387-396

  Yang, Xiao Hu ^a,b,c   Mo, H J ^a   Kauffmann, Guinevere ^a   Chu, Yao Quan ^b,c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

^c CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

Dark matter; Galaxies: haloes; Gravitational lensing; Largescale structure of universe; Methods: statistical

Indexed keywords

GRAVITATION; LUMINANCE; NUMERICAL METHODS;

CROSS-CORRELATIONS; DARK MATTER; GALAXIES-GALAXIES; GALAXY:HALO; GRAVITATIONAL LENSING; HALO MASS; LARGE SCALE STRUCTURE OF UNIVERSE; MASS CORRELATION; METHODS:STATISTICAL; VIRIAL MASS;

GALAXIES;

EID: 0142041960     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06217.x     Document Type: Article

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