Cosmological parameters after WMAP5: Forecasts for Planck and future galaxy surveys

Monthly Notices of the Royal Astronomical Society

Volumn 398, Issue 4, 2009, Pages 1621-1637

  Colombo, L P L ^a   Pierpaoli, E ^a   Pritchard, J R ^b  

^a UNIVERSITY OF SOUTHERN CALIFORNIA   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Cosmic microwave background; Cosmological parameters; Galaxies: Statistics; Large scale structure of Universe

Indexed keywords

DATA HANDLING; GALAXIES; INFORMATION ANALYSIS; POLARIZATION; PROBES; SURVEYS; TENSORS;

'CURRENT; COSMIC MICROWAVES BACKGROUND; COSMOLOGICAL PARAMETERS; GALAXIES: STATISTICS; LARGE SCALE STRUCTURE OF UNIVERSE; MEASUREMENTS OF; PERFORMANCE; PLANCK SATELLITES; SPECTRAL INDICES; WILKINSON MICROWAVE ANISOTROPY PROBE;

COSMOLOGY;

EID: 70349194883     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14802.x     Document Type: Article

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