Three‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Implications for Cosmology
The Astrophysical Journal Supplement Series2007Vol. 170(2), pp. 377–408
Citations Over TimeTop 1% of 2007 papers
David N. Spergel, Rachel Bean, Olivier Doré, M. R. Nolta, C. L. Bennett, J. Dunkley, G. Hinshaw, N. Jarosik, Eiichiro Komatsu, Lyman A. Page, Hiranya V. Peiris, Licia Verde, M. Halpern, Ryley Hill, A. Kogut, M. Limon, S. S. Meyer, N. Odegard, Gregory S. Tucker, J. L. Weiland, Edward J. Wollack, E. L. Wright
Abstract
A simple cosmological model with only six parameters (matter density,mh 2, baryon density,bh 2, Hubble con-stant, H0, amplitude of fluctuations, 8, optical depth, , and a slope for the scalar perturbation spectrum, ns) fits not only the 3 yearWMAP temperature and polarization data, but also small-scale CMB data, light element abundances, large-scale structure observations, and the supernova luminosity/distance relationship.UsingWMAP data only, the best-fit values for cosmological parameters for the power-law flat cold dark matter (CDM) model are (mh
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