6.7k citations · 18.2k across the 85 of their papers we have counts for
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Dynamics of Linear Perturbations in f(R) Gravity
Rachel Bean, David Bernat, Levon Pogosian +2
We consider predictions for structure formation from modifications to general relativity in which the Einstein-Hilbert action is replaced by a general function of the Ricci scalar.…
The impact of neutrino masses on the determination of dark energy properties
Axel De La Macorra, Alessandro Melchiorri, Paolo Serra +1
Recently, the Heidelberg-Moscow double beta decay experiment has claimed a detection for a neutrino mass with high significance. Here we consider the impact of this measurement on…
Constraining Isocurvature Initial Conditions with WMAP 3-year data
Rachel Bean, Joanna Dunkley, Elena Pierpaoli
We present constraints on the presence of isocurvature modes from the temperature and polarization CMB spectrum data from the WMAP satellite alone, and in combination with other da…
Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles, Data Processing, Radiometer Characterization and Systematic Error Limits
N. Jarosik, C. Barnes, M. R. Greason +18
The WMAP satellite has completed 3 years of observations of the cosmic microwave background radiation. The 3-year data products include several sets of full sky maps of the Stokes…
Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
G. Hinshaw, M. R. Nolta, C. L. Bennett +19
We present new full-sky temperature maps in five frequency bands from 23 to 94 GHz, based on the first three years of the WMAP sky survey. The new maps, which are consistent with t…
Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
L. Page, G. Hinshaw, E. Komatsu +20
The Wilkinson Microwave Anisotropy Probe WMAP has mapped the entire sky in five frequency bands between 23 and 94 GHz with polarization sensitive radiometers. We present three-year…
Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
D. N. Spergel, R. Bean, O. Doré +19
A simple cosmological model with only six parameters (matter density, Omega_m h^2, baryon density, Omega_b h^2, Hubble Constant, H_0, amplitude of fluctuations, sigma_8, optical de…