FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION

@article{Komatsu2008FIVEYEARWM,
  title={FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION},
  author={Eiichiro Komatsu and K. M. Smith and Jo Dunkley and Charles L. Bennett and Benjamin Gold and Gary F. Hinshaw and Norman Jarosik and David L. Larson and Michael R. Nolta and Lyman A. Page and David N. Spergel and Mark Halpern and Robert S. Hill and Alan Kogut and Michele Limon and Stephan S. Meyer and N. Odegard and Gregory S. Tucker and Janet L. Weiland and Edward J. Wollack and E. L. Wright},
  journal={The Astrophysical Journal Supplement Series},
  year={2008},
  volume={180},
  pages={330 - 376}
}
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References

SHOWING 1-10 OF 815 REFERENCES
First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
WMAP precision data enable accurate testing of cosmological models. We find that the emerging standard model of cosmology, a flat Λ-dominated universe seeded by a nearly scale-invariant adiabatic
First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications For Inflation
We confront predictions of inflationary scenarios with the Wilkinson Microwave Anisotropy Probe (WMAP) data, in combination with complementary small-scale cosmic microwave background (CMB)
WMAP five-year constraints on lepton asymmetry and radiation energy density: implications for Planck
In this paper we set bounds on the radiation content of the Universe and neutrino properties by using the WMAP (Wilkinson microwave anisotropy probe) five-year CMB (cosmic microwave background)
First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity
We present limits to the amplitude of non-Gaussian primordial fluctuations in the WMAP 1 yr cosmic microwave background sky maps. A nonlinear coupling parameter, fNL, characterizes the amplitude of a
PROBING DYNAMICS OF DARK ENERGY WITH SUPERNOVA, GALAXY CLUSTERING AND THE THREE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS
Using the Markov chain Monte Carlo (MCMC) method, we perform a global analysis constraining the dynamics of dark energy in light of the supernova (Riess "gold" samples), galaxy clustering (SDSS 3D
Bounds on cold dark matter and neutrino isocurvature perturbations from CMB and LSS data
Early universe models for the origin of structure typically produce a spectrum of initial fluctuations with a mixture of adiabatic and isocurvature perturbations. Using the observed anisotropies of
FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: LIKELIHOODS AND PARAMETERS FROM THE WMAP DATA
This paper focuses on cosmological constraints derived from analysis of WMAP data alone. A simple ΛCDM cosmological model fits the five-year WMAP temperature and polarization data. The basic
SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: POWER SPECTRA AND WMAP-DERIVED PARAMETERS
The WMAP mission has produced sky maps from seven years of observations at L2. We present the angular power spectra derived from the seven-year maps and discuss the cosmological conclusions that can
Cosmological parameters from SDSS and WMAP
We measure cosmological parameters using the three-dimensional power spectrum P(k) from over 200,000 galaxies in the Sloan Digital Sky Survey (SDSS) in combination with WMAP and other data. Our
Wilkinson Microwave Anisotropy Probe Constraints on the Intracluster Medium
We devise a Monte Carlo-based, optimized filter match method to extract the thermal Sunyaev-Zel'dovich (SZ) signature of a catalog of 116 low-redshift X-ray clusters from the first-year data release
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