Modelling and interpreting the dependence of clustering on the spectral energy distributions of galaxies

Monthly Notices of the Royal Astronomical Society

Volumn 377, Issue 4, 2007, Pages 1419-1430

  Wang, Lan ^a,b   Li, Cheng ^b,c,d   Kauffmann, Guinevere ^b   De Lucia, Gabriella ^b  

^a PEKING UNIVERSITY   (China)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c CHINESE ACADEMY OF SCIENCES   (China)

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

Author keywords

Cosmology: theory; Dark matter; Galaxies: distances and redshifts; Galaxies: fundamental parameters; Galaxies: haloes; Large scale structure of Universe

Indexed keywords

GALAXIES; SATELLITES; SPECTROSCOPY; SURVEYS;

CLUSTERINGS; COSMOLOGY: THEORY; DARK MATTER; GALAXIES DISTANCES AND REDSHIFTS; GALAXIES: FUNDAMENTAL PARAMETERS; GALAXY:HALO; LARGE SCALE STRUCTURE OF UNIVERSE; SPECTRAL ENERGY DISTRIBUTION; STARS FORMATION; STELLAR MASS;

STARS;

EID: 34249747386     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11737.x     Document Type: Article

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