The dependence of galaxy formation on cosmological parameters: Can we distinguish between the WMAP1 and WMAP3 parameter sets?

Monthly Notices of the Royal Astronomical Society

Volumn 384, Issue 4, 2008, Pages 1301-1315

  Wang, Jie ^a   De Lucia, Gabriella ^a   Kitzbichler, Manfred G ^a   White, Simon D M ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Cosmology: theory; Galaxies: evolution; Galaxies: formation; Methods: N body simulations

Indexed keywords

FORECASTING; GALAXIES; POPULATION STATISTICS; SUPERNOVAE; UNCERTAINTY ANALYSIS;

COSMOLOGICAL PARAMETERS; COSMOLOGY: THEORY; GALAXY EVOLUTION; GALAXY FORMATIONS; METHODS:N-BODY SIMULATIONS; N-BODY SIMULATION; PARAMETER SET; PHYSICAL MODELLING; PROPERTY; REDSHIFT GALAXIES;

COSMOLOGY;

EID: 40249111978     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12797.x     Document Type: Article

References (72)